## JPL Publication 02-25



# Chemical Kinetics and Photochemical Data for Use in Atmospheric Studies

Evaluation Number 14

NASA Panel for Data Evaluation:

S. P. Sander R. R. Friedl Jet Propulsion Laboratory Pasadena, California A. R. Ravishankara NOAA Environmental Research Laboratory Boulder, Colorado

D. M. Golden Stanford University Stanford, California C. E. Kolb Aerodyne Research, Inc. Billerica, Massachusetts

M. J. Kurylo R. E. Huie V. L. Orkin National Institute of Standards and Technology Gaithersburg, Maryland M. J. Molina Massachusetts Institute of Technology Cambridge, Massachusetts

G. K. Moortgat Max-Planck Institute for Chemistry Mainz, Germany B. J.Finlayson-Pitts University of California, Irvine Irvine, California

National Aeronautics and Space Administration

Jet Propulsion Laboratory California Institute of Technology Pasadena, California



## February 1, 2003

### ii The research described in this publication was carried out by the Jet Propulsion Laboratory, California Instit ute of Technology, under a c ontract with the National Aeronautics and Space Administration.

Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or ot herwise, does not constitute or imply its endorsement by the United States Government or the Jet Propulsion Laboratory, Calif ornia Institute of Technology

### iii ABSTRACT

This is the fourteenth in a series of evaluated se ts of rate constants and photochemical cross sections compiled by the NASA Panel for Data Evaluation. The data are used primarily to model stratospheri c and upper tropospheric processes, with particular emphasis on the ozone layer and its possible pert urbation by anthropogenic and natural phenomena. Copies of this evaluation are available in electronic form and may be printed from the following Internet URL: 

### http://jpldataeval.jpl.nasa.gov/

### iv TABLE OF CONTENTS

INTRODUCTION viii I.1 Basis of the Recommenda tions................................................................................................... ................ix I.2 Scope of the Evalua tion........................................................................................................ ......................ix I.3 Format of th e Evalua tion ....................................................................................................... ......................x I.4 Computer Access................................................................................................................ .........................x I.5 Data Formats ................................................................................................................... ............................x I.6 Units .......................................................................................................................... ..................................x I.7 Noteworthy Changes in This Evaluation.......................................................................................... ...........x I.8 Acknowledgements ............................................................................................................... .................. xiii I.9 References ..................................................................................................................... .......................... xiii

SECTION 1. BIMOLECULAR REACTIONS 1-1 1.1 Introduction ............................................................................................................... .............................. 1-1 1.2 Uncertaint y Estima tes...................................................................................................... ........................ 1-2 1.3 Notes to Table 1........................................................................................................... .......................... 1-31 1.4 References ................................................................................................................. ............................ 1-93

SECTION 2. TERMOLECULAR REACTIONS 2-1 2.1 Introduction................................................................................................................... .............................2-1
2.2 Low–Pressure-Limiting Rate Constant, 

## ( ) x

o 

### k T ..................................................................................... 2-1

2.3 Temperature Dependence of Low–Pressure Limiting Rate Constants: T n ............................................... 2-2 2.4 High-Pressure-Limit Rate Constants, k
∞ (T) ............................................................................................ 2-2 2.5 Temperature Dependence of High-Pressure-Limiting Rate Constants: T m .............................................. 2-3 2.6 Uncertainty Estimates.......................................................................................................... .................... 2-3 2.7 Notes to Table 2............................................................................................................... ........................ 2-8 2.8 References .................................................................................................................... ...........................2-16

SECTION 3. EQUILIBR IUM CONSTANTS 3-1 3.1 Format ......................................................................................................................... ............................ 3-1 3.2 Definitions .................................................................................................................... ........................... 3-1 3.3 Notes to Table 3............................................................................................................... ........................ 3-3 3.4 References ..................................................................................................................... .......................... 3-5

SECTION 4. PHOTOCHEMICAL DATA 4-1 4.1 Format and E rror Estim ates..................................................................................................... ................ 4-3 4.2 Halocarbon Absorption Cross Sec tions and Quantum Yields ................................................................. 4-3 4.3 References ..................................................................................................................... ...................... 4-102

SECTION 5. HETEROGEN EOUS CHEMISTRY............................................................................................. ...... 5-1 5.1 Introduc tion ................................................................................................................... .......................... 5-1 5.2 Surface Types—Acid/Water, Liquids, an d Solids.................................................................................. . 5-2 5.3 Surface Types—Soot and Alumina ................................................................................................. ........ 5-2 5.4 Surface Composition and Morphology............................................................................................. ....... 5-3 5.5 Surface Po rosity............................................................................................................... ........................ 5-4 5.6 Temperature Dependences of Parameters.......................................................................................... ...... 5-4 5.7 Solubility Li mitations......................................................................................................... ..................... 5-4 5.8 Data Orga nization.............................................................................................................. ...................... 5-4 5.9 Parameter Definitions.......................................................................................................... .................... 5-5 5.10 Mass Accommodation Coefficients fo r Surfaces Other Than Soot ......................................................... 5-8 5.11 Notes to Table 5-1 ............................................................................................................. ...................... 5-9 5.12 Gas/Surface Reaction Probab ilities for Surfaces Ot her Than Soot........................................................ 5-16 5.13 Notes to Table 5-2 ............................................................................................................. .................... 5-19

### v 5.14 Soot Surface Uptake Coefficients............................................................................................... ........... 5-32 5.15 Notes to Table 5-3 ............................................................................................................. .................... 5-32 5.16 Henry’s Law Constant s for Pure Water........................................................................................... ...... 5-35 5.17 Notes to Table 5-4 ............................................................................................................. .................... 5-36 5.18 Henry’s Law Consta nts for Acids................................................................................................ .......... 5-40 5.19 Notes to Table 5-5 ............................................................................................................. .................... 5-40 5.20 References ..................................................................................................................... ........................ 5-44

APPENDIX A. THERMODY NAMIC PARA METERS ..........................................................................................A -1 A.1 Gas-phase entropy and enthalpy values...................................................................................... .............A-1 A.1 References ................................................................................................................. ..............................A-8



### TABLES

Table I-1. Editions of this Pub lication........................................................................................ ................................. viii Table I-2. Panel Members and their Major Re sponsibilities for the Current Ev aluation........................................... .. viii

Table 1-1. Rate Constants for Second-Order Reactions........................................................................... ....................1-5

Table 2–1. Rate Constants for Termolecular Reactions........................................................................... ....................2-4

Table 3-1. Equilib rium Constants............................................................................................... ............................... 3-2

Table 4-1. Photoc hemical Reactions ............................................................................................. ............................ 4-4 Table 4-2. Combined Uncertainties for Cross Sections a nd Quantum Yields........................................................ ... 4-6 Table 4-3. Absorption Cross Sections of O 2 Between 205 an d 240 nm .................................................................... 4-7 Table 4-4. Absorption Cross Sections of O 3 at 273 K ............................................................................................... 4-8 Table 4-5. Parameters for the Calculation of O( 1 D) Quantum Yields ....................................................................... 4-9 Table 4-6. Absorption Cross Sections of HO 2 ......................................................................................................... 4-10 Table 4-7. Absorption Cross Sections of H 2 O Vapor.............................................................................................. 4-11 Table 4-8. Absorption Cross Sections of H 2 O 2 Vapor............................................................................................. 4-11 Table 4-9. Mathematical Expression for Absorption Cross Sections of H 2 O 2 as a Function of Temperature......... 4-12 Table 4-10. Absorption Cross Sections of NO 2 ....................................................................................................... 4-13 Table 4-11. Quantum Yields for NO 2 Photolysis .................................................................................................... 4-14 Table 4-12. Absorption Cross Sections of NO 3 at 298 K ........................................................................................ 4-16 Table 4-13. Mathematical Expression for Absorption Cross Sections of N 2 O as a Function of Temperature * ....... 4-16 Table 4-14. Absorption Cross Sections of N 2 O at 298 K ........................................................................................ 4-17 Table 4-15. Absorption Cross Sections of N 2 O 5 ...................................................................................................... 4-18 Table 4-16. Absorption Cr oss Sections of HONO .................................................................................. ................ 4-19 Table 4-17. Absorption Cross Sections and Temperature Coefficients of HNO 3 Vapor......................................... 4-20 Table 4-18. Absorption Cross Sections of HO 2 NO 2 Vapor..................................................................................... 4-20 Table 4-19. Absorption Cross Sections and Quantum Yields for Photolysis of CH 2 O ........................................... 4-21 Table 4-20. Absorption Cross Sections of CH 3 O 2 , C 2 H 5 O 2 , and CH 3 C(O)O 2 ......................................................... 4-22 Table 4-21. Absorption Cross Sections of CH 3 OOH............................................................................................... 4-23 Table 4-22. Absorption Cr oss Sections of PAN................................................................................... ................... 4-25 Table 4-23. Absorption Cr oss Sections of FNO................................................................................... ................... 4-26 Table 4-24. Absorption Cross Sections of CCl 2 O, CClFO, and CF 2 O at 298 K...................................................... 4-27 Table 4-25. Absorption Cross Sections of Cl 2 ......................................................................................................... 4-28 Table 4-26. Absorption Cr oss Sections of ClOO .................................................................................. .................. 4-29 Table 4-27. Absorption Cross Sections of OClO at th e Band Peaks ................................................................ ....... 4-30 Table 4-28. Absorption Cross Sections of Cl 2 O...................................................................................................... 4-32 Table 4-29. Absorption Cross Sec tions of ClOOCl at 200–25 0 K ................................................................... ....... 4-33 Table 4-30. Absorption Cross Sections of Cl 2 O 3 ..................................................................................................... 4-34 Table 4-31. Absorption Cross Sections of Cl 2 O 4 ..................................................................................................... 4-34 Table 4-32. Absorption Cross Sections of Cl 2 O 6 ..................................................................................................... 4-34

### vi Table 4-33. Absorption Cros s Sections of HCl Vapor ............................................................................. ............... 4-35 Table 4-34. Absorption Cr oss Sections of HOCl .................................................................................. .................. 4-36 Table 4-35. Absorption Cr oss Sections of ClNO .................................................................................. .................. 4-37 Table 4-36. Absorption Cross Sections of ClNO 2 ................................................................................................... 4-37 Table 4-37. Absorption Cross S ections of ClON O at 231 K........................................................................ ........... 4-38 Table 4-38. Absorption Cross Sections of ClONO 2 ................................................................................................ 4-39 Table 4-39. Absorption Cross Sections of CCl 4 at 295–298 K................................................................................ 4-41 Table 4-40. Absorption Cross Sections of CH 3 OCl ................................................................................................ 4-42 Table 4-41. Absorption Cross Sections of CHCl 3 at 295–298 K............................................................................. 4-43 Table 4-42. Absorption Cross Sections of CH 2 Cl 2 at 295–298 K ........................................................................... 4-44 Table 4-43. Absorption Cross Sections of CH 3 Cl at 295 –298 K............................................................................. 4-46 Table 4-44. Absorption Cross Sections of CH 3 CCl 3 at 295–298 K ......................................................................... 4-47 Table 4-45. Absorption Cross Sections of CH 3 CH 2 Cl at 298 K.............................................................................. 4-47 Table 4-46. Absorption Cross Sections of CH 3 CHClCH 3 at 295 K ........................................................................ 4-48 Table 4-47. Absorption Cross Sections of CFCl 3 at 295–298 K ............................................................................. 4-49 Table 4-48. Absorption Cross Sections of CF 2 Cl 2 at 295–298 K ............................................................................ 4-50 Table 4-49. Absorption Cross Sections of CF 3 Cl at 295 K ..................................................................................... 4-51 Table 4-50. Absorption Cross Sections of CF 2 ClCFCl 2 at 295–298 K.................................................................... 4-52 Table 4-51. Absorption Cross Sections of CF 2 ClCF 2 Cl at 295 K ........................................................................... 4-53 Table 4-52. Absorption Cross Sections of CF 3 CF 2 Cl at 295– 298 K ....................................................................... 4-53 Table 4-53. Absorption Cross Sections of CHFCl 2 at 295–298 K........................................................................... 4-54 Table 4-54. Absorption Cross Sections of CHF 2 Cl at 295–298 K........................................................................... 4-55 Table 4–55. Absorption Cross Sections of CH 2 FCl at 298 K.................................................................................. 4-55 Table 4-56. Absorption Cross Sections of CF 3 CHCl 2 at 295 K............................................................................... 4-56 Table 4-57. Absorption Cross Sections of CF 3 CHFCl at 295 K.............................................................................. 4-57 Table 4-58. Absorption Cross Sections of CF 3 CH 2 Cl at 298 K............................................................................... 4-58 Table 4-59. Absorption Cross Sections of CH 3 CFCl 2 at 295–298 K....................................................................... 4-59 Table 4–60. Absorption Cross Sections of CH 3 CF 2 Cl at 295–29 8 K...................................................................... 4-60 Table 4-61. Absorption Cross Sections of CF 3 CF 2 CHCl 2 and CF 2 ClCF 2 CFCl at 298 K ........................................ 4-61 Table 4-62. Absorption Cross Sections at the Peak of Various Bands in the A ← X Spectrum of BrO ................. 4-62 Table 4-63. Absorption Cr oss Sections of BrO ................................................................................... .................... 4-62 Table 4-64. Absorption Cr oss Sections of HOBr .................................................................................. .................. 4-65 Table 4-65. Absorption Cross Sections of BrONO 2 at 298 K ................................................................................. 4-66 Table 4-66. Absorption Cross S ections of BrCl at 298 K......................................................................... ............... 4-67 Table 4-67. Absorption Cross Sections of CH 3 Br at 295–29 6 K............................................................................. 4-69 Table 4-68. Absorption Cross Sections of CH 2 Br 2 at 295–298 K ........................................................................... 4-70 Table 4-69. Absorption Cross Sections of CHBr 3 at 295–296 K............................................................................. 4-71 Table 4-70. Absorption Cross Sections of CH 2 BrCH 2 Br at 295 K.......................................................................... 4-72 Table 4-71. Absorption Cross Sections of C 2 H 5 Br at 295 K ................................................................................... 4-72 Table 4-72. Absorption Cross Sections of CH 2 ClBr at 295 K................................................................................. 4-73 Table 4-73. Absorption Cross Sections of CHClBr 2 at 296 K................................................................................. 4-74 Table 4-74. Absorption Cross Sections of CHCl 2 Br at 298 K................................................................................. 4-75 Table 4-75. Absorption Cross Sections of CCl 3 Br at 298 K.................................................................................... 4-75 Table 4-76. Absorption Cross Sections of CHF 2 Br at 298 K .................................................................................. 4-76 Table 4-77. Absorption Cross Sections of CF 2 Br 2 at 295–296 K............................................................................ 4-78 Table 4-78. Absorption Cross Sections of CF 2 ClBr at 295– 298 K ......................................................................... 4-80 Table 4-79. Absorption Cross Sections of CF 3 Br at 295–29 8 K ............................................................................. 4-82 Table 4-80. Absorption Cross Sections of CF 3 CH 2 Br at 295 K .............................................................................. 4-82 Table 4-81. Absorption Cross Sections of CF 3 CHClBr at 295 –298 K.................................................................... 4-84 Table 4-82. Absorption Cross Sections of CF 3 CHFBr at 295 K ............................................................................. 4-84 Table 4-83. Absorption Cross Sections of CF 2 BrCF 2 Br at 296 K........................................................................... 4-86 Table 4-84. Absorption Cross Sections of CF 3 CF 2 Br at 298 K............................................................................... 4-87 Table 4-85. Absorption Cross Sections of CH 3 I at 296–298 K and Temper ature Coefficients............................... 4-88 Table 4-86. Absorption Cross Sections of CH 2 I 2 at 298 K...................................................................................... 4-89 Table 4-87. Absorption Cross Sections of C 2 H 5 I at 298 K and Temperat ure Coefficients ..................................... 4-90 Table 4-88. Absorption Cross Sections of CH 3 CHI 2 at 298 K ................................................................................ 4-91

### vii Table 4-89. Absorption Cross Sections of C 3 H 7 I at 298 K and Temperat ure Coefficients ..................................... 4-92 Table 4-90. Absorption Cross Sections of (CH 3 ) 3 CI at 298 K................................................................................. 4-93 Table 4-91. Absorption Cross Sections of CF 3 I at 295–300 K................................................................................ 4-95 Table 4-92. Absorption Cross Sections of CF 2 I 2 at 294 K ...................................................................................... 4-96 Table 4-93. Absorption Cross Sections of C 2 F 5 I at 323 K ...................................................................................... 4-96 Table 4-94. Absorption Cross Sections of 1-C 3 F 7 I at 295–298 K ........................................................................... 4-97 Table 4-95. Absorption Cross Sections of CH 2 ICl at 298 K and Temper ature Coefficients................................... 4-98 Table 4-96. Absorption Cross Sections of CH 2 BrI at 298 K and Temper ature Coefficients................................... 4-99 Table 4-97. Absorption Cr oss Sections of OCS ................................................................................... ................. 4-100 Table 4-98. Absorption Cross Secti ons of NaCl Va por at 300 K................................................................... ....... 4-101

Table 5-1. Mass Accommodation Coefficients ( α ) for Surfaces Other Than Soot. .................................................. 5-8 Table 5-2. Gas/Surface Reaction Probabilities ( γ ) for Surfaces Other Than Soot................................................... 5-16 Table 5-3. Soot Surface Uptake Coef ficients. ................................................................................... ...................... 5-32 Table 5-4. Henry’s Law Co nstants for Pure Water. ............................................................................... ................. 5-35 Table 5-5. Henry’s Law Constants for Acids ..................................................................................... ..................... 5-40

Table A-1. Gas-phase entropy and enthalpy values for selected species at 298.15 K and 100 kPa...........................A-1



### FIGURES

Figure 1-1. Symmetric and Asymmetric E rror Limits.............................................................................. ...................1-3

Figure 4-1. Absorption Spectrum of NO 3 ................................................................................................................ 4-15 Figure 4-2. Absorptio n Spectrum of ClO ......................................................................................... ....................... 4-29 Figure 4-3. Absorptio n Spectrum of OClO ........................................................................................ ..................... 4-31 Figure 4-4. Absorption Spectrum of BrO......................................................................................... ....................... 4-63

Figure 5-1. Recommended reactive uptake coefficients as a function of temperature for key stratospheric heterogeneous processes on sulfuric acid aerosols.............................................................................. ............. 5-7

### viii 

## INTRODUCTION

This compilation of kinetic and photochemical data is an update to the 13th evaluation prepared by the NASA Panel for Data Evaluation. The Panel was estab lished in 1977 by the NASA Upper Atmosphere Research Program Office for the purpose of providing a critical tabulation of the latest kinetic and photochemical data for use by modelers in computer simulations of stratospheric chemistry. Table I-1 lists this publication’s editions:

Table I-1. Editions of this Publication

Edition Reference 1 NASA RP 1010, Chapter 1 (Hudson [1]) 2 JPL Publication 79-27 (DeMore et al. [12]) 3 NASA RP 1049, Chapter 1 (Hudson and Reed [2]) 4 JPL Publication 81-3 (DeMore et al. [10]) 5 JPL Publication 82-57 (DeMore et al. [8]) 6 JPL Publication 83-62 (DeMore et al. [9]) 7 JPL Publication 85-37 (DeMore et al. [3]) 8 JPL Publication 87-41 (DeMore et al. [4]) 9 JPL Publication 90-1 (DeMore et al. [5]) 10 JPL Publication 92-20 (DeMore et al. [6]) 11 JPL Publication 94-26 (DeMore et al. [7]) 12 JPL Publication 97-4 (DeMore et al. [11]) 13 JPL Publication 00-3 (Sander et al. [14]) 14 JPL Publication 02-25 (Sander et al. [13])

In addition to the current edition, several of the previous editions are available for download from the website. Panel members, and their major responsibilities for the current evaluation are listed in Table I-2.

Table I-2. Panel Members and their Major Responsibilities for the Current Evaluation
Panel Members Responsibility S. P. Sander, Chairman Editorial Review, publication, website M. J. Kurylo V. L. Orkin OH reactions with halocarbons
D. M. Golden Three-body reac tions, equilibrium constants R. E. Huie Aqueous chemistry, thermodynamics B. J. Finlayson-Pitts C. E. Kolb M. J. Molina Heterogeneous chemistry

R. R. Friedl A. R. Ravishankara Upper Troposphere/Lower St ratosphere gas-phase chemistry G. K. Moortgat Photochemistry

As shown above, each Panel member concentrates his efforts on a given ar ea or type of data. Nevertheless, the Panel’s final recommendations represent a consensus of the entire Panel. Each member reviews the basis for all recommendations, and is cognizant of the final decision in every case.

Communications regarding particular reactions may be addressed to the appropriate panel member:

### ix S. P. Sander R. R. Friedl Jet Propulsion Laboratory M/S 183-901 4800 Oak Grove Drive Pasadena, CA 91109 stanley.sander@jpl.nasa.gov randall.friedl@jpl.nasa.gov D. M. Golden Department of Mechanical Engineering Stanford University Bldg 520 Stanford, CA 94305 david.golden@stanford.edu

R. E. Huie M. J. Kurylo V. L. Orkin National Institute of St andards and Technology Physical and Chemical Properties Division Gaithersburg, MD 20899 robert.huie@nist.gov michael.kurylo@nist.gov vladimir.orkin@nist.gov A. R. Ravishankara NOAA-ERL, R/E/AL2 325 Broadway Boulder, CO 80303 ravi@al.noaa.gov

C. E. Kolb Aerodyne Research Inc. 45 Manning Rd. Billerica, MA 01821 kolb@aerodyne.com M. J. Molina Department of Earth, Atmospheric, and Planetary Sciences and Department of Chemistry Massachusetts Institute of Technology Cambridge, MA 02139 mmolina@mit.edu G. K. Moortgat Max-Planck-Institut für Chemie Atmospheric Chemistry Division Postfach 3060 55020 Mainz Germany moo@mpch-mainz.mpg.de B. J. Finlayson-Pitts Department of Chemistry University of California, Irvine 516 Rowland Hall Irvine, CA 92697-2025 bjfinlay@uci.edu



### I.1 Basis of the Recommendations

The recommended rate data and cross sections are ba sed on laboratory measurements. In order to provide recommendations that are as up-to-date as possible, prep rints and written private comm unications are accepted, but only when it is expected that they will appear as published journal articles. Under no circumstances are rate constants adjusted to fit observations of atmospheric concentrations . The Panel considers the question of consistency of data with expectations based on the theory of reaction kinetics, a nd when a discrepancy appears to exist this fact is pointed out in the accompanying note. The major us e of theoretical extrapolation of da ta is in connection with three-body reactions, in which the required pressure or temperat ure dependence is sometimes unavailable from laboratory measurements, and can be estimated by use of appropriate theoretical treatment. In the case of important rate constants for which no experimental data are available, the panel may provide estimates of rate constant parameters based on analogy to similar reactions for which data are available.



### I.2 Scope of the Evaluation

In the past (releases 1-12 of this evaluation) it has been the practice of the Panel to reevaluate the entire set of reactions with individual Panel memb ers taking responsibility for specific chemi cal families or processes. In recent years, the upper troposphere and lower stratosphere (UT/LS ) have become the primary areas of focus for model calculations and atmospheric measuremen ts related to studies of ozone depl etion and climate change. Because the UT/LS is a region of relatively high chemical and dynamical complexity, a different approach has been adopted for future releases of the evaluation. Sp ecifically, the entire reaction set of th e data evaluation will no longer be reevaluated for each release. Instead, sp ecific subsets will be chosen for re-eva luation, with several Panel members working to develop recommendations for a given area. This approach will make it possible to treat each subset in

### x greater depth, and to expand the scope of the evaluation to ne w areas. It is the aim of the Panel to consider the entire set of kinetics, photochemical and thermodynamic paramete rs every three review cycles. Each release of the evaluation will contain not only the new evaluations, but also recommendations for every process that has been considered in the past. In this way, the tables for each release will constitu te a complete set of recommendations. It is recognized that important new laboratory data may be published that lie outside the specific subset chosen for re-evaluation. In order to ensure that these important data receive prompt consideration, each evaluation will also have a “special topics” category. Feedback from the atmospheric modeling community is solicited in the selection of reactions for this category. For the current evaluation, the speci fic subsets include the following:

• Hydrocarbon chemistry of the upper troposphere (C3 hydrocarbons and below).

• Reactions of OH and Cl with halocarbon species.

• Photochemistry of halocarbon species.

• Heterogeneous processes on liquid sulfuric acid and soot surfaces

• Thermodynamic parameters (entropy and enthalpy of formation)

• The special topics category in cludes the following reactions: O 3 + h ν , O + O 2 + M, OH + O 3 , HO 2 + O 3 , OH + NO 2 + M, HO 2 + NO 2 + M, OH + HNO 3 , OH + ClO, HO 2 + ClO and ClO + ClO + M.


### I.3 Format of the Evaluation

Changes or additions to the tables of data are indicated by shading. A new entry is completely shaded, whereas a changed entry is shaded onl y where it has changed. In some cases only the note has been changed, in which case the corresponding note number in the table is shaded.



### I.4 Computer Access

This document is available online in the form of individual chapters and as a complete document in Adobe PDF (Portable Data File) format. Files may be downloaded from http://jpldataeval.jpl.nasa.gov/ . This document is not available in printed form from JPL.

Individuals who wish to receive no tice when the web page is revised should submit email addresses in the appropriate reply box on the web page.
For more information, contact Stanley Sander ( Stanley.Sander@jpl.nasa.gov ).



### I.5 Data Formats

In Table 1 (Rate Constants for Bimolecular Reactions) the reactions are grouped into the classes O
x , HO x , NO x , Organic Compounds, FO
x , ClO
x , BrO x , IO x , SO x and Metal Reactions. The data in Table 2 (Rate Constants for Association Reactions) are presented in the same orde r as the bimolecular reactions. The presentation of photochemical cross section data follows the same sequence.



### I.6 Units

The rate constants are given in units of concentra tion expressed as molecule s per cubic centimeter and time in seconds. Thus, for first-, second-, and third-order reactions the units of k are s -1 , cm 3 molecule -1 s -1 , and

cm 6 molecule -2 s -1 , respectively. Cross sections are expressed as cm 2 molecule -1 , base e.


### I.7 Noteworthy Changes in This Evaluation

I.7.1 Bimolecular Reactions I.7.1.1 Hydrocarbon Reactions Im portant in the Upper Troposphere Atmospheric observations suggest that photochemistry in the upper troposphere has a much greater global significance than previously believed. The production of O 3 in this region is significant and is controlled by interaction of the HO

x and NO

x radical families. Increasingly, it has b een recognized that organic compounds (e.g. ketones, aldehydes, peroxides, and acids ) play an important role in supplying HO

x to the upper troposphere. NO

x sources in this region are numerous and long-lived reservoi r species such as peroxyacyl nitrates (e.g. PAN) and peroxynitric acid (PNA) serve to redistribute NO

x globally.

### xi In addition, there is renewed interest in the role of convective activity in lifting short-lived hydrocarbons and halocarbon species to levels near the tropopause. If the convection does not directly penetrate the stratosphere, the reactive organics and organo-halogens are likely to r eact in the upper troposphere. This would be a mechanism for the transport of aldehydes and peroxides noted above . In case of the organo-halogen compounds, releasing degradation products and/or chlorine and bromine ra dicals in the upper troposphere can be significant. The subsequent fate of the degradation products, especially whether they survive long enough to be transported from the upper troposphere into the stratosphere to affect the halogen budget, is an important open question. In this update we have considered a set of reactions of importance in upper tropospheric HO

x , NO

x and shortlived halocarbon chemistry. The set includes reactions of OH and Cl with selected alkyl pe roxides, organic acids, alkyl and acyl nitrates, aldehydes, and alcohols. It also includes reacti ons of Cl with various alkylhalides. We have also updated kinetics para meters for a number of alkylperoxy self- and cross-reactions of importance in upper tropospheric HO
x chemistry. The reactions of peroxy radicals have been studied in the laboratory for many years. However, there are some key difficulties associated with such studies. First, many of the peroxy radicals of interest to the atmosphere ar e radical-radical reactions that are inherently difficult to study in isolation. For example, many of the reactions of pe roxy radicals cannot be ca rried out under pseudo-first order conditions. Second, many peroxy radical r eactions produce reactive products that unavoidably lead to further reactions with the species being monitored. Third, most peroxy radicals do not fluoresce and none have been observed via a fluorescence technique. They also have weak, unstructured absorption spectra in the ultraviolet, which often overlap with those of other peroxy radicals. Therefor e, a sensitiveity and selectiveity method for the detection of peroxy radicals is missing. Lastly, in general, peroxy radical reactions often have more than one set of products. Previously, it was not always possible to perform a critical analysis using a self-consistent data base because (a) all the information about the experiments was not available, (b) it requi red re-analysis of previous data in light of new information such as absorption cross s ections and product yields, and (c) the knowledge of the interfering reactions and their rates was also uncertain. Therefore, a panel of scientists who have worked with the peroxy radicals of interest to the atmosphere and w hose data usually form the basis of recommendations was assembled as a part of the SPARC-IGAC initiative. This panel critically reevaluated the existing data, discarded some, and modified others to arrive at a self-consistent ev aluation of the rate coefficients and product yields in the reactions of RO 2 radicals. This effort resulted in a paper that was published in the Journal of Geophysical Research [15]. The current recommendation uses these evaluated data. Our consideration of upper tropospheric reactions has resulted in the add ition of 18 new reactions, most of which involve reactions of Cl with al kyl nitrates, alkyl halides and organi c peroxides and acids. Changes to the existing reactions mainly represent small refinements of the Arrhenius parameters and tightening of the uncertainty limits. One significant change involve s the OH + acetone reaction rate coe fficient which may exhibit curved Arrhenius behavior.

I.7.1.2 OH + Halocarbon Reactions A comprehensive review of the reactions of indus trial and naturally occurring halocarbons with the hydroxyl radical (OH) was conducted for this evaluation. In doing so, attempts were made to understand and reconcile apparent differences between the results of absolute and relative rate measurements for some of the reactions. Relative rate constants were “renormalized” usi ng the revised recommendations for the reference reactions. Thus, the re-evaluation procedure was an iterative one, since relative rate studies themselves were often included as the basis for the rate constant recommendations of these very reference reactions. Th e recommendations were then checked for self-consistency by seeing whether ratios of the recommended rate constant s were in agreement with published relative rate measurements. In some cases, disparities may seem to exist. However, it should be recognized that the focus of this reevaluation was the generation of recommended rate constant s over the temperature range of atmospheric importance (i.e., below 300 K). Many of the latest (o r relatively recent) ab solute rate studies have fo cused on this region but often extend to temperatures greater than 300 K Relative rate investigations, on the other hand, have been conducted predominantly above room temperature, with only limited extension below 300 K. This can lead to difficulties in evaluating the studies since many of the OH + halocarbon reactions exhibit pronounced Arrhenius curvature. This curvature has several possible causes incl uding multiple reaction pathways (differe nt types of abstractable H atoms), multiple reactant conformers (whose populations and reactivity differ with temperature), and tunneling. Of course, convincing evidence had to exist that such Arrhenius behavior was indeed real and not an artifact of the experimental procedure. For example, one of the common reasons for experimentally observed non-Arrhenius behavior is the

### xii presence of highly reactive impurities in the samples used in the absolute measurements. However, most recent absolute studies have involve d thorough reactant sample purification and anal ysis and curvature in the Arrhenius plot is not likely due to such impurities. Thus, in the presence of real Arrhenius curvature, a rate constant expression derived predominantly from absolute rate constant meas urements conducted below room temperature may not be appropriate for normalizing relative rate constant measur ements conducted above room temperature. More detail about these issues may be found in the notes for the r eactions of OH with HFC-152a and HFC-152 (reactions E7 and E8, respectively). For some reactions in this section, there have been significant revisions in the recommendations as a result of new and improved studies. For other reactions, only minor changes from earlier recommendations have been made. Nevertheless, in all cases, such changes were made so that the complete set of recommendations is completely current with the published literature and is self-consistent. Finally, several new reactions have been included and the rate constant uncertainty factors (f and g) have been caref ully reviewed in an attempt to narrow the range of rate constant uncertainties for modeling purposes. Previous uncerta inty limits were overly conservative in some cases. In the present evaluation, the 2 σ confidence limits derived from these factors were visually inspected together with the complete experimental database for consistency. I.7.1.3 Absorption Cross Sections and Quantum Yields The database for the evaluation of the absorption cr oss sections and quantum yields has been expanded considerably for all the halocarbon compounds. Whereas the previous evaluation JPL 97-4 reported only the absorption cross sections of a limited number of selected halocarbons, the present evaluation includes now a comprehensive review of most halocarbons of atmos pheric relevance investigated in recent years. The newly evaluated halocarbons are listed in Table 4. This list includes new entries for C 1 to C 4 chloroalkanes, C 1 to C 2 chlorofluoroalkanes (CFCs) and C 1 to C 3 hydrochlorofluorocarbons (HCFCs). For these species the database was expanded from 14 to 26 compounds. Mo reover, the database for the brominated hydro- and mixed halocarbons, including halons, was increased from 6 to 18 compounds. Finally, a large range of iodinecontaining compounds (total 32) has now been implemented in the present evaluation. Also new in this section is the incorporation of temperature-dependence data, including the parameters used to express the temperature varia tion of the absorption cross sections by a polynomial expansion formula. These expressions will allow the calculation of absorption cross sections in a wide range of stratospheric temperatures. Finally, quantum yield data have also been updated for many species. I.7.2 Heterogeneous Processes
New and/or updated evaluations in this document ha ve focused on uptake measurements on binary liquid sulfuric acid/water solutions, supplemented in a few cases by data on ternary liquid sulfuric acid/nitric acid/water solutions, on water ice, and on “soot” (see definitions in th e section on heterogeneous chemistry). No updates on solid acid/ice compositions are presented in this document, although evaluations for key nitrogen oxide sequestration and/or halogen activation reac tions on nitric acid trihydrate (NAT) surfaces were recently re-evaluated and presented in JPL 00-3 [14]. Uptake data on alumina, salt and aqueous salt solutions have not been updated since JPL 97-4 [11]. Henry’s law solubility data for reactive upper tropospheric/stratospheri c species in binary liqui d sulfuric acid/water, and, where available, in ternary liquid sulfuric acid/nitric acid/water solutions have also been updated and a much more extensive compilation of Henry’s law parameters for pure water has been added. I.7.3 Thermodynamic Parameters
The table in Appendix 1 contains selected entropy and enthalpy of formation values at 298 K for a number of atmospheric species. As much as possi ble, the values were taken from primary evaluations, that is, evaluations that develop a recommended value from the original studies. Othe rwise, the values were se lected from the original literature, which is referenced in the table. Often, the enthalpy of formation and the entropy values are taken from different sources, usually due to a more recent value for the enthalpy of formation. The cited error limits are from the original references and therefore reflect widely varying criteria. Some enthalpy values were corrected slightly to reflect the value of a reference compound selected for this table; these are indicated. Values that are calculated or estimated are also indicated in the table.

### xiii I.8 Acknowledgements

The Panel wishes to acknowledge Hannelore Keller-Rude k for her assistance preparing the evaluation of the photochemistry section and efforts updating the data base on absorption spectra of atmospheric relevant compounds. The new and updated evaluations presented in this hete rogeneous chemistry section were prepared by B.J. Finlayson-Pitts, R.E. Huie, C.E. Kolb and M.J. Molina. They would like to acknowledge valuable technical and editorial assistance from L.R. Williams, Q. Shi, L.T. Molina and D.M. Smith. They would also like to thank the members of the international heterogeneous research communities who provided copies of their reprints, preprints and written summaries of recent results fro m their laboratories.We gratefully ac knowledge the critical reading of this evaluation by Drs. W. B. DeMore and R. F. Hampson. We also appreciate the expert ed itorial assistance and website suppport provided by T. Wilson and L. Palkovic of the Jet Propul sion Laboratory. The typi ng skills of X. Sabounchi are also gratefully acknowledged.



### I.9 References

1. Chlorofluoromethanes and the Stratosphere. In NASA Reference Publication 1010 ; Hudson, R. D., Ed.; NASA: Washington, D.C, 1977. 2. The Stratosphere: Present and Future. In NASA Reference Publication 1049 ; Hudson, R. D., Reed, E. I., Eds.; NASA: Washington, D.C, 1979. 3. DeMore, W. B., D. M. Golden, R. F. Hampson, C. J. Howard, M. J. Kurylo, J. J. Margitan, M. J. Molina, A. R. Ravishankara and R. T. Watson “Chemical Kinetic s and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 7,” JP L Publication 85-37, Jet Propulsion La boratory, California Institute of Technology, Pasadena CA, 1985. 4. DeMore, W. B., D. M. Golden, R. F. Hampson, C. J. Howard, M. J. Kurylo, M. J. Molina, A. R. Ravishankara and S. P. Sander “Chemical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 8,” JP L Publication 87-41, Jet Propulsion La boratory, California Institute of Technology, Pasadena CA, 1987. 5. DeMore, W. B., D. M. Golden, R. F. Hampson, C. J. Howard, M. J. Kurylo, M. J. Molina, A. R. Ravishankara and S. P. Sander “Chemical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 9,” JP L Publication 90-1, Jet Propulsion La boratory, California Institute of Technology, Pasadena CA, 1990. 6. DeMore, W. B., D. M. Golden, R. F. Hampson, C. J. Howard, M. J. Kurylo, M. J. Molina, A. R. Ravishankara and S. P. Sander “Chemical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 10,” JP L Publication 92-20, Jet Propulsion La boratory, California Institute of Technology, Pasadena, CA, 1992. 7. DeMore, W. B., D. M. Golden, R. F. Hampson, C. J. Howard, M. J. Kurylo, M. J. Molina, A. R. Ravishankara and S. P. Sander “Chemical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 11,” JP L Publication 94-26, Jet Propulsion La boratory, California Institute of Technology, Pasadena, CA, 1994. 8. DeMore, W. B., D. M. Golden, R. F. Hampson, C. J. Howard, M. J. Kurylo, M. J. Molina, A. R. Ravishankara and R. T. Watson “Chemical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 5,” JP L Publication 82-57, Jet Propulsion La boratory, California Institute of Technology, Pasadena CA, 1982. 9. DeMore, W. B., D. M. Golden, R. F. Hampson, C. J. Howard, M. J. Kurylo, M. J. Molina, A. R. Ravishankara and R. T. Watson “Chemical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 6,” JP L Publication 83-62, Jet Propulsion La boratory, California Institute of Technology, Pasadena CA, 1983. 10. DeMore, W. B., D. M. Golden, R. F. Hampson, M. J. Ku rylo, J. J. Margitan, M. J. Molina, L. J. Stief and R. T. Watson “Chemical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 4,” JPL Publication 81-3, Jet Propulsion Laborat ory, California Institute of Technology, Pasadena CA, 1981. 11. DeMore, W. B., S. P. Sander, D. M. Golden, R. F. Hampson, M. J. Kurylo, C. J. Howard, A. R. Ravishankara, C. E. Kolb and M. J. Molina “Che mical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 12,” JPL Publication 97-4, Jet Propulsion Laboratory, California Institute of T echnology, Pasadena, CA, 1997.

### xiv 12. DeMore, W. B., L. J. Stief, F. Kaufman, D. M. Golden , R. F. Hampson, M. J. Kurylo, J. J. Margitan, M. J. Molina and R. T. Watson “Chemical Kinetics and Photoc hemical Data for Use in Stratospheric Modeling, Evaluation Number 2,” JPL Publication 79-27, Je t Propulsion Laboratory, California Institute of Technology, Pasadena, CA, 1979. 13. Sander, S. P., B. J. Finlayson-Pitts, R. R. Friedl, D. M. Golden, R. E. Huie, C. E. Kolb, M. J. Kurylo, M. J. Molina, G. K. Moortgat, V. L. Orkin and A. R. Ra vishankara “Chemical Kinetics and Photochemical Data for Use in Atmospheric Studies, Evaluation Number 14,” JPL Publication 02-25, Jet Propulsion Laboratory, Pasadena, 2002. 14. Sander, S. P., R. R. Friedl, W. B. DeMore, D. M. Go lden, M. J. Kurylo, R. F. Hampson, R. E. Huie, G. K. Moortgat, A. R. Ravishankara, C. E. Kolb and M. J. Molina “Chemical Kinetics and Photochemical Data for Use in Stratospheric Modeling, Evaluation Number 13,” JPL Publication 00-3, Jet Propulsion Laboratory, California Institute of T echnology, Pasadena, CA, 2000. 15. Tyndall, G. S., R. A. Cox, C. Granier, R. Lesclaux, G. K. Moortgat, M. J. Pilling, A. R. Ravishankara and T. J. Wallington, 2001, J. Geophys. Res., 106 , 12157-12182.

### 1-1 

## SECTION 1. BIMOLECULAR REACTIONS

Table of Contents

SECTION 1. BIMOLECULAR REACTIONS............................................................................................... .............. 1-1 1.1 Introduction ............................................................................................................... .................................. 1-1 1.2 Uncertainty Estim ates...................................................................................................... ............................ 1-2 1.3 Notes to Table 1........................................................................................................... .............................. 1-31 1.4 References ................................................................................................................. ................................ 1-93



### Tables Table 1-1. Rate Constants for Second-Order Reactions........................................................................... .....................1-5



### Figures Figure 1-1. Symmetric and Asymmetric E rror Limits.............................................................................. .....................1-3



### 1.1 Introduction

In Table 1 (Rate Constants for S econd-Order Reactions) the reactions are grouped into the classes O
x , O( 1 D), Singlet O 2 , HO x , NO x , Organic Compounds, FO
x , ClO
x , BrO x , IO x , SO x and Metals. Some of the reactions in Table 1-1 are actually more comple x than simple two-body reactions. To explain the pressure and temperature dependences occasionally seen in reactions of this type, it is necessary to consider the bimo lecular class of reactions in terms of two subcategories, direct (concer ted) and indirect ( nonconcerted) reactions.

A direct or concerted bimolecular r eaction is one in which the reactants A and B proceed to products C and D without the intermediate formation of an AB adduct that has appreciable bonding, i.e., there is no bound intermediate; only the transition state (AB) ≠ lies between reactants and products.

A + B → (AB) ≠ → C + D

The reaction of OH with CH 4 forming H 2 O + CH 3 is an example of a reaction of this class.
Very useful correlations between the expect ed structure of the transition state [AB] ≠ and the A-Factor of the reaction rate constant can be made, especially in reac tions that are constrained to follow a well-defined approach of the two reactants in order to minimize energy requirements in the ma king and breaking of bonds. The rate constants for these reactions are well represented by the Arrhenius expression k = A exp(–E/RT) in the 200–300 K temperature
range. These rate constants are not pressure dependent.

The indirect or nonconcerted class of bimolecular reactions is character ized by a more complex reaction path involving a potential well between reactants and products, leading to a bound adduct (or reaction complex) formed between the reactants A and B:

A + B ↔ [AB]* → C + D
The intermediate [AB]* is different from the transition state [AB] ≠ , in that it is a bound molecule which can, in principle, be isolated. (Of course, transition states are involved in all of the a bove reactions, both forward and backward, but are not explicitly shown.) An example of this reaction type is ClO + NO, which normally produces Cl + NO 2 . Reactions of the nonconcerted type can have a more complex temperature dependence and can exhibit a pressure dependence if the lifetime of [AB]* is compar able to the rate of collis ional deactivation of [AB]*. This arises because the relative rate at which [AB]* goes to products C + D vs. reactants A + B is a sensitive function of its excitation energy. Thus, in reactions of this type, the distinction between the bimolecular and termolecular classification becomes less meaningful, and it is especially necessary to study such reactions under the temperature and pressure conditions in which they are to be used in model calculation, or, alternatively, to develop a reliable theoretical basis for extrapolation of data.

The rate constant tabulation for second-order reactions (Table 1-1) is given in Arrhenius form: k(T) = A exp ((-E/R)(1/T)) and contains the following information:

### 1-2 1. Reaction stoichiometry and products (if known). The pressure dependences are included, where appropriate.
2. Arrhenius A-factor. 3. Temperature dependence and associated un certainty (“activation temperature” E/R±g).

4. Rate constant at 298 K. 5. Uncertainty factor at 298 K. 6. Note giving basis of recommendation and any other pertinent information. 

### 1.2 Uncertainty Estimates

For bimolecular rate constants in Table 1-1, an estimat e of the uncertainty at an y given temperature, f(T), may be obtained from the following expression:

1 1 f(T)=f(298 K)exp g T 298  

−    

Note that the exponent is an absolute value. An upper or lower bound (corresponding approximately to one standard deviation) of the rate constant at any temperature T can be obtained by multiplying or dividing the recommended value of the rate constant at that temperature by the factor f(T). The quantity f(298 K) is the uncertainty in the rate constant at T = 298 K. The quantity g has been de fined in this evaluation for use with f(298 K) in the above expression to obtain the rate constant uncertainty at diffe rent temperatures. It should not be interpreted as the uncertainty in the Arrhen ius activation temperature (E/R). Both uncertainty factors, f( 298 K) and g, do not necessarily result from a rigorous statistical analysis of the available data . Rather, they are chosen by the evaluators to construct the appropriate uncertainty factor, f(T), shown above. This approach is based on the fact that rate constants are almost always known with minimum uncertainty at room temperature. The overall uncerta inty normally increases at other temper atures, because there are usually fewer data at other temperatures. In addition, data obtained at temperatures far di stant from 298 K may be less accurate than at room temperature due to various experimental difficulties. The uncertainty represented by f(T) is normally symmetric; i.e., the rate constant may be greater than or less than the recommended value, k(T), by the factor f(T). In a few cases in Table 1-1 asymmetric uncertainties are given in the temperature coefficient. For these cases, the factors by which a rate constant is to be multiplied or divided to obtain, respectively, the upper and lower limits are not equal, except at 298 K where the factor is simply f(298 K). Explicit equations are given below for the case where g is given as (g +a, –b): For T > 298 K, multiply by the factor

1 1 a 298 T 

### f(298)e    

−    

   

and divide by the factor

1 1 b 298 T 

### f(298)e    

−    

   

For T < 298 K, multiply by the factor

1 1 b T 298 

### f(298)e    

−    

   

and divide by the factor

1 1 a T 298 

### f(298)e    

−    

   

Examples of symmetric and asymmetric error limits are shown in Figure 1-1.

### 1-3 Figure 1-1. Symmetric and Asymmetric Error Limits

The assigned uncertainties represent the subjective judgm ent of the Panel. They are not determined by a rigorous, statistical analysis of the database, which generally is too limited to permit such an analysis. Rather, the uncertainties are based on knowledge of the techniques, th e difficulties of the experiments, and the potential for systematic errors. There is obviously no way to quantify these “unknown” errors. The spread in results among different techniques for a given reaction may provide some basis for an uncertainty, but the possibility of the same, or compensating, systematic errors in all the studies must be recognized.

### 1-4 Furthermore, the probability distribution may not follow the normal Gaussian form. For measurements subject to large systematic errors, the true rate constant may be much further from the recommended value than would be expected based on a Gaussian distribution with the stated uncertainty. As an example, in the past the recommended rate constants for the reactions HO 2 + NO and Cl + ClONO 2 changed by factors of 30–50. These changes could not have been allowed for with any reasonable values of σ in a Gaussian distribution.

### 1-5 Table 1-1. Rate Constants for Second-Order Reactions

Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes



### O × 

### Reactions

O + O 2 M 

###  →

 O 3 (See Table 2-1)

O + O 3 → O 2 + O 2 8.0×10 –12 2060 8.0×10 –15 1.15 250 A1



### O( 1 

### D) Reactions

O( 1 D) + O 2 → O + O 2 3.2×10 –11 –70 4.0×10 –11 1.2 100 A2, A3

O( 1 D) + O 3 → O 2 + O 2 1.2×10 –10 0 1.2×10 –10 1.3 100 A2, A4

→ O 2 + O + O 1.2×10 –10 0 1.2×10 –10 1.3 100 A2, A4

O( 1 D) + H 2 → OH + H 1.1×10 –10 0 1.1×10 –10 1.1 100 A2, A5

O( 1 D) + H 2 O → OH + OH 2.2×10 –10 0 2.2×10 –10 1.2 100 A2, A6

O( 1 D) + N 2 → O + N 2 1.8×10 –11 –110 2.6×10 –11 1.2 100 A2

O( 1 D) + N 2 M 

###  →

 N 2 O (See Table 2-1)

O( 1 D) + N 2 O → N 2 + O 2 4.9×10 –11 0 4.9×10 –11 1.3 100 A2, A7

→ NO + NO 6.7×10 –11 0 6.7×10 –11 1.3 100 A2, A7

O( 1 D) + NH 3 → OH + NH 2 2.5×10 –10 0 2.5×10 –10 1.3 100 A2, A8

O( 1 D) + CO 2 → O + CO 2 7.4×10 –11 –120 1.1×10 –10 1.2 100 A2

O( 1 D) + CH 4 → products 1.5×10 –10 0 1.5×10 –10 1.2 100 A2, A9

O( 1 D) + HCl → products 1.5×10 –10 0 1.5×10 –10 1.2 100 A10

O( 1 D) + HF → OH + F 1.4×10 –10 0 1.4×10 –10 2.0 100 A11

O( 1 D) + HBr → products 1.5×10 –10 0 1.5×10 –10 2.0 100 A12

O( 1 D) + Cl 2 → products 2.8×10 –10 0 2.8×10 –10 2.0 100 A13

O( 1 D) + CCl 2 O → products 3.6×10 –10 0 3.6×10 –10 2.0 100 A2, A14

O( 1 D) + CClFO → products 1.9×10 –10 0 1.9×10 –10 2.0 100 A2, A14

O( 1 D) + CF 2 O → products 7.4×10 –11 0 7.4×10 –11 2.0 100 A2, A14
O( 1 D) + CCl 4 → products (CFC-10) 3.3×10 –10 0 3.3×10 –10 1.2 100 A2, A15

### 1-6 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

O( 1 D) + CH 3 Br → products 1.8×10 –10 0 1.8×10 –10 1.3 100 A15, A16

O( 1 D) + CH 2 Br 2 → products 2.7×10 –10 0 2.7×10 –10 1.3 100 A15, A17

O( 1 D) + CHBr 3 → products 6.6×10 –10 0 6.6×10 –10 1.5 100 A15, A18
O( 1 D) + CH 3 F → products (HFC-41) 1.5×10 –10 0 1.5×10 –10 1.2 100 A15, A19
O( 1 D) + CH 2 F 2 → products (HFC-32) 5.1×10 –11 0 5.1×10 –11 1.3 100 A15, A20
O( 1 D) + CHF 3 → products (HFC-23) 9.1×10 –12 0 9.1×10 –12 1.2 100 A15, A21
O( 1 D) + CHCl 2 F → products (HCFC-21) 1.9×10 –10 0 1.9×10 –10 1.3 100 A15, A22
O( 1 D) + CHClF 2 → products (HCFC-22) 1.0×10 –10 0 1.0×10 –10 1.2 100 A15, A23
O( 1 D) + CCl 3 F → products (CFC-11) 2.3×10 –10 0 2.3×10 –10 1.2 100 A2, A15
O( 1 D) + CCl 2 F 2 → products (CFC-12) 1.4×10 –10 0 1.4×10 –10 1.3 100 A2, A15
O( 1 D) + CClF 3 → products (CFC-13) 8.7×10 –11 0 8.7×10 –11 1.3 100 A15, A24
O( 1 D) + CClBrF 2 → products (Halon-1211) 1.5×10 –10 0 1.5×10 –10 1.3 100 A15, A25
O( 1 D) + CBr 2 F 2 → products (Halon-1202) 2.2×10 –10 0 2.2×10 –10 1.3 100 A15, A26
O( 1 D) + CBrF 3 → products (Halon-1301) 1.0×10 –10 0 1.0×10 –10 1.3 100 A15, A27
O( 1 D) + CF 4 → CF 4 + O (CFC-14) – – 2.0×10 –14 1.5 – A15, A28
O( 1 D) + CH 3 CH 2 F → products (HFC-161) 2.6×10 –10 0 2.6×10 –10 1.3 100 A15, A29
O( 1 D) + CH 3 CHF 2 → products (HFC-152a) 2.0×10 –10 0 2.0×10 –10 1.3 100 A15, A30
O( 1 D) + CH 3 CCl 2 F → products (HCFC-141b) 2.6×10 –10 0 2.6×10 –10 1.3 100 A15, A31
O( 1 D) + CH 3 CClF 2 → products (HCFC-142b) 2.2×10 –10 0 2.2×10 –10 1.3 100 A15, A32
O( 1 D) + CH 3 CF 3 → products (HFC-143a) 1.0×10 –10 0 1.0×10 –10 3.0 100 A15, A33
O( 1 D) + CH 2 ClCClF 2 → products (HCFC-132b) 1.6×10 –10 0 1.6×10 –10 2.0 100 A15, A34
O( 1 D) + CH 2 ClCF 3 → products (HCFC-133a) 1.2×10 –10 0 1.2×10 –10 1.3 100 A15, A35
O( 1 D) + CH 2 FCF 3 → products (HFC-134a) 4.9×10 –11 0 4.9×10 –11 1.3 100 A15, A36
O( 1 D) + CHCl 2 CF 3 → products (HCFC-123) 2.0×10 –10 0 2.0×10 –10 1.3 100 A15, A37
O( 1 D) + CHClFCF 3 → products (HCFC-124) 8.6×10 –11 0 8.6×10 –11 1.3 100 A15, A38

### 1-7 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

O( 1 D) + CHF 2 CF 3 → products ( HF C -12 5) 1.2×10 –10 0 1.2×10 –10 2.0 100 A15, A39
O( 1 D) + CCl 3 CF 3 → products (CFC-113a) 2×10 –10 0 2×10 –10 2.0 100 A15, A40
O( 1 D) + CCl 2 FCClF 2 → products (CFC-113) 2×10 -10 0 2×10 -10 2.0 100 A15, A41
O( 1 D) + CCl 2 FCF 3 → products (CFC-114a) 1×10 -10 0 1×10 -10 2.0 100 A15, A42
O( 1 D) + CClF 2 CClF 2 → products (CFC-114) 1.3×10 -10 0 1.3×10 -10 1.3 100 A15, A43
O( 1 D) + CClF 2 CF 3 → products (CFC-115) 5×10 -11 0 5×10 -11 1.3 100 A15, A44
O( 1 D) + CBrF 2 CBrF 2 → products (Halon-2402) 1.6×10 -10 0 1.6×10 –10 1.3 100 A15, A45
O( 1 D) + CF 3 CF 3 → O + CF 3 CF 3 (CFC-116) – – 1.5×10 –13 1.5 – A15, A46
O( 1 D) + CHF 2 CF 2 CF 2 CHF 2 → products (HFC-338pcc) 1.8×10 –11 0 1.8×10 –11 1.5 100 A15, A47

O( 1 D) + c-C 4 F 8 → products – – 8×10 –13 1.3 – A15, A48
O( 1 D) + CF 3 CHFCHFCF 2 CF 3 → products (HFC-43-10mee) 2.1×10 –10 0 2.1×10 –10 4 100 A15, A49
O( 1 D) + C 5 F 12 → products (CFC-41-12) – – 3.9×10 –13 2 – A15, A50
O( 1 D) + C 6 F 14 → products (CFC-51-14 ) – – 1×10 –12 2 – A15, A51

O( 1 D) + 1,2-(CF 3 ) 2 c-C 4 F 6 → products – – 2.8×10 –13 2 – A15, A52

O( 1 D) + SF 6 → products – – 1.8×10 –14 1.5 – A53



### Singlet O 2 

### Reactions

O 2 ( 1 ∆ ) + O → products – – <2×10 –16 – – A54

O 2 ( 1 ∆ ) + O 2 → products 3.6×10 –18 220 1.7×10 –18 1.2 100 A55

O 2 ( 1 ∆ ) + O 3 → O + 2O 2 5.2×10 –11 2840 3.8×10 –15 1.2 500 A56

O 2 ( 1 ∆ ) + H 2 O → products – – 4.8×10 –18 1.5 – A57

O 2 ( 1 ∆ ) + N → NO + O – – <9×10 –17 – – A58

O 2 ( 1 ∆ ) + N 2 → products – – <10 –20 – – A59

O 2 ( 1 ∆ ) + CO 2 → products – – <2×10 –20 – – A60

O 2 ( 1 Σ ) + O → products – – 8×10 –14 5.0 – A61

O 2 ( 1 Σ ) + O 2 → products – – 3.9×10 –17 1.5 – A62

### 1-8 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

O 2 ( 1 Σ ) + O 3 → products 2.2×10 –11 0 2.2×10 –11 1.2 200 A63

O 2 ( 1 Σ ) + H 2 O → products – – 5.4×10 –12 1.3 – A64

O 2 ( 1 Σ ) + N → products – – <10 –13 – – A65

O 2 ( 1 Σ ) + N 2 → products 2.1×10 –15 0 2.1×10 –15 1.2 200 A66

O 2 ( 1 Σ ) + CO 2 → products 4.2×10 –13 0 4.2×10 –13 1.2 200 A67



### HO × 

### Reactions

O + OH → O 2 + H 2.2×10 –11 –120 3.3×10 –11 1.2 100 B 1

O + HO 2 → OH + O 2 3.0×10 –11 –200 5.9×10 –11 1.1 50 B 2

O + H 2 O 2 → OH + HO 2 1.4×10 –12 2000 1.7×10 –15 2.0 1000 B 3

H + O 2 M 

###  →

 HO 2 (See Table 2-1)

H + O 3 → OH + O 2 1.4×10 –10 470 2.9×10 –11 1.25 200 B 4

H + HO 2 → products 8.1×10 –11 0 8.1×10 –11 1.3 100 B 5

OH + O 3 → HO 2 + O 2 1.7×10 –12 940 7.3×10 –14 1.2 80 B 6

OH + H 2 → H 2 O+ H 5.5×10 –12 2000 6.7×10 –15 1.1 100 B 7

OH + HD → products 5.0×10 –12 2130 4.0×10 –15 1.2 200 B 8

OH + OH → H 2 O + O 4.2×10 –12 240 1.9×10 –12 1.4 240 B 9

M 

###  →

 H 2 O 2 (See Table 2-1)

OH + HO 2 → H 2 O + O 2 4.8×10 –11 –250 1.1×10 –10 1.3 100 B10

OH + H 2 O 2 → H 2 O+ HO 2 2.9×10 –12 160 1.7×10 –12 1.15 50 B11

HO 2 + O 3 → OH + 2O 2 1.0×10 –14 490 1.9×10 –15 1.15 +160 –80 B12

HO 2 + HO 2 → H 2 O 2 + O 2 2.3×10 –13 –600 1.7×10 –12 1.3 200 B13

M 

###  →

 H 2 O 2 + O 2 1.7×10 –33 [M] –1000 4.9×10 –32 [M] 1.3 400 B13



### NO × 

### Reactions

O + NO M 

###  →

 NO 2 (See Table 2-1)

O + NO 2 → NO + O 2 5.6×10 –12 –180 1.0×10 –11 1.1 50 C1

### 1-9 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

O + NO 2 M 

###  →

 NO 3 (See Table 2-1)

O + NO 3 → O 2 + NO 2 1.0×10 –11 0 1.0×10 –11 1.5 150 C 2

O + N 2 O 5 → products <3.0×10 –16 C 3

O + HNO 3 → OH + NO 3 <3.0×10 –17 C 4

O + HO 2 NO 2 → products 7.8×10 –11 3400 8.6×10 –16 3.0 750 C 5

H + NO 2 → OH + NO 4.0×10 –10 340 1.3×10 –10 1.3 300 C 6

OH + NO M 

###  →

 HONO (See Table 2-1)

OH + NO 2 M 

###  →

 HNO 3 (See Table 2-1)

OH + NO 3 → products 2.2×10 –11 1.5 C 7

OH + HONO → H 2 O + NO 2 1.8×10 –11 390 4.5×10 –12 1.5 +200 –500 C 8

OH + HNO 3 → H 2 O + NO 3 (See Note) 1.2 C 9

OH + HO 2 NO 2 → products 1.3×10 –12 –380 4.6×10 –12 1.3 +270 –500 C10

OH + NH 3 → H 2 O + NH 2 1.7×10 –12 710 1.6×10 –13 1.2 200 C11

HO 2 + NO → NO 2 + OH 3.5×10 –12 –250 8.1×10 –12 1.15 50 C12

HO 2 + NO 2 M 

###  →

 HO 2 NO 2 (See Table 2-1)

HO 2 + NO 2 → HONO + O 2 (See Note) C13

HO 2 + NO 3 → products 3.5×10 –12 1.5 C14

HO 2 + NH 2 → products 3.4×10 –11 2.0 C15

N + O 2 → NO + O 1.5×10 –11 3600 8.5×10 –17 1.25 400 C16

N + O 3 → NO + O 2 <2.0×10 –16 C17

N + NO → N 2 + O 2.1×10 –11 –100 3.0×10 –11 1.3 100 C18

N + NO 2 → N 2 O + O 5.8×10 –12 –220 1.2×10 –11 1.5 100 C19

NO + O 3 → NO 2 + O 2 3.0×10 –12 1500 1.9×10 –14 1.1 200 C20

NO + NO 3 → 2NO 2 1.5×10 –11 –170 2.6×10 –11 1.3 100 C21

NO 2 + O 3 → NO 3 + O 2 1.2×10 –13 2450 3.2×10 –17 1.15 150 C22

### 1-10 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

NO 2 + NO 3 → NO + NO 2 +O 2 (See Note) C23

NO 2 + NO 3 M 

###  →

 N 2 O 5 (See Table 2-1)

NO 3 + NO 3 → 2NO 2 + O 2 8.5×10 –13 2450 2.3×10 –16 1.5 500 C24

NH 2 + O 2 → products <6.0×10 –21 C25

NH 2 + O 3 → products 4.3×10 –12 930 1.9×10 –13 3.0 500 C26

NH 2 + NO → products 4.0×10 –12 –450 1.8×10 –11 1.3 150 C27

NH 2 + NO 2 → products 2.1×10 –12 –650 1.9×10 –11 3.0 250 C28

NH + NO → products 4.9×10 –11 0 4.9×10 –11 1.5 300 C29

NH + NO 2 → products 3.5×10 –13 –1140 1.6×10 –11 2.0 500 C30

O 3 + HNO 2 → O 2 + HNO 3 <5.0×10 –19 C31

N 2 O 5 + H 2 O → 2HNO 3 <2.0×10 –21 C32

N 2 (A,v) + O 2 → products 2.5×10 –12 , v=0 1.5 C33

N 2 (A,v) + O 3 → products 4.1×10 –11 , v=0 2.0 C34



### Reactions of Organic Compounds

O + CH 3 → products 1.1×10 –10 0 1.1×10 –10 1.3 250 D 1

O + HCN → products 1.0×10 –11 4000 1.5×10 –17 10 1000 D 2

O + C 2 H 2 → products 3.0×10 –11 1600 1.4×10 –13 1.3 250 D 3

O + H 2 CO → products 3.4×10 –11 1600 1.6×10 –13 1.25 250 D 4

O + CH 3 CHO → CH 3 CO + OH 1.8×10 –11 1100 4.5×10 –13 1.25 200 D 5

O 3 + C 2 H 2 → products 1.0×10 –14 4100 1.0×10 –20 3 500 D 6

O 3 + C 2 H 4 → products 1.2×10 –14 2630 1.7×10 –18 1.25 100 D 7

O 3 + C 3 H 6 → products 6.5×10 –15 1900 1.1×10 –17 1.2 200 D 8

OH + CO → Products 1.5×10 –13 ×(1+0.6P atm ) 0 1.5×10 –13 ×(1+0.6P atm ) 1.3 300 D 9

OH + CH 4 → CH 3 + H 2 O 2.45×10 –12 1775 6.3×10 –15 1.1 100 D10

OH + 13 CH 4 → 13 CH 3 + H 2 O (See Note) D11

### 1-11 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

OH + CH 3 D → products 3.5×10 –12 1950 5.0×10 –15 1.15 200 D12

OH + H 2 CO → H 2 O + HCO 9.0×10 –12 0 9.0×10 –12 1.2 100 D13

OH + CH 3 OH → products 7.3×10 –12 620 9.1×10 –13 1.15 250 D14

OH + CH 3 OOH → products 3.8×10 –12 –200 7.4×10 –12 1.4 150 D15

OH + HC(O)OH → products 4.0×10 –13 0 4.0×10 –13 1.2 100 D16

OH + HCN → products 1.2×10 –13 400 3.1×10 –14 3 150 D17

OH + C 2 H 2 M 

###  →

 products (See Table 2-1)

OH + C 2 H 4 M 

###  →

 products (See Table 2-1)

OH + C 2 H 6 → H 2 O + C 2 H 5 8.7 × 10 –12 1070 2.4×10 –13 1.1 100 D18

OH + C 3 H 8 → H 2 O + C 3 H 7 1.0 × 10 –11 660 1.1×10 –12 1.2 100 D19

OH + CH 3 CHO → CH 3 CO + H 2 O 5.6×10 –12 –270 1.4×10 –11 1.2 200 D20

OH + C 2 H 5 OH → products 6.9×10 –12 230 3.2×10 –12 1.2 100 D21

OH + CH 3 C(O)OH → products 4.0×10 –13 –200 8.0×10 –13 1.25 200 D22

OH + CH 3 C(O)CH 3 → products (See Note) D23

OH + CH 3 CN → products 7.8×10 –13 1050 2.3×10 –14 1.5 200 D24

OH+ CH 3 ONO 2 → products 5.0×10 –13 810 3.3×10 –14 1.5 250 D25

OH + CH 3 C(O)O 2 NO 2 (PAN) → products <4 × 10 –14 D26

OH+ C 2 H 5 ONO 2 → products 6.8×10 –13 320 2.3×10 –13 1.5 200 D27

OH + 1–C 3 H 7 ONO 2 → products 7.1×10 –13 0 7.1×10 –13 1.5 200 D28

OH + 2–C 3 H 7 ONO 2 → products 1.2×10 –12 320 4.1×10 –13 1.5 200 D29

HO 2 + CH 2 O → adduct 6.7×10 –15 –600 5.0×10 –14 5 600 D30

HO 2 + CH 3 O 2 → CH 3 OOH + O 2 4.1×10 –13 –750 5.2×10 –12 1.3 150 D31

HO 2 + C 2 H 5 O 2 → C 2 H 5 OOH + O 2 7.5×10 –13 –700 8.0×10 –12 1.5 250 D32

HO 2 + CH 3 C(O)O 2 → products 4.3×10 –13 –1040 1.4×10 –11 2 500 D33

HO 2 + CH 3 C(O)CH 2 O 2 → products 8.6×10 –13 –700 9.0×10 –12 2 300 D34

### 1-12 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

NO 3 + CO → products <4.0×10 –19 D35

NO 3 + CH 2 O → products 5.8×10 –16 1.3 D36

NO 3 + CH 3 CHO → products 1.4×10 –12 1900 2.4×10 –15 1.3 300 D37

CH 3 + O 2 → products <3.0×10 –16 D38

CH 3 + O 2 M 

###  →

 CH 3 O 2 (See Table 2-1)

CH 3 + O 3 → products 5.4×10 –12 220 2.6×10 –12 2 150 D39

HCO + O 2 → CO + HO 2 5.2×10 –12 0 5.2×10 –12 1.4 100 D40

CH 2 OH + O 2 → CH 2 O + HO 2 9.1×10 –12 0 9.1×10 –12 1.3 200 D41

CH 3 O + O 2 → CH 2 O + HO 2 3.9×10 –14 900 1.9×10 –15 1.5 300 D42

CH 3 O + NO → CH 2 O + HNO (See Note) D43

CH 3 O + NO M 

###  →

 CH 3 ONO (See Table 2-1)

CH 3 O + NO 2 → CH 2 O + HONO 1.1 × 10 –11 1200 2.0 × 10 –13 5 600 D44

CH 3 O + NO 2 M 

###  →

 CH 3 ONO 2 (See Table 2-1)

CH 3 O 2 + O 3 → products 2.9×10 –16 1000 1.0×10 –17 3 500 D45

CH 3 O 2 + CH 3 O 2 → products 9.5×10 –14 –390 3.5×10 –13 1.2 100 D46

CH 3 O 2 + NO → CH 3 O + NO 2 2.8×10 –12 –300 7.7×10 –12 1.15 100 D47

CH 3 O 2 + NO 2 M 

###  →

 CH 3 O 2 NO 2 (See Table 2-1)

CH 3 O 2 + CH 3 C(O)O 2 → products 2.0×10 –12 –500 1.1×10 –11 1.5 250 D48

CH 3 O 2 + CH 3 C(O)CH 2 O 2 → products 7.5×10 –13 –500 4.0×10 –12 2 300 D49

C 2 H 5 + O 2 → C 2 H 4 + HO 2 <2.0×10 –14 D50

C 2 H 5 + O 2 M 

###  →

 C 2 H 5 O 2 (See Table 2-1)

C 2 H 5 O + O 2 → CH 3 CHO + HO 2 6.3 × 10 –14 550 1.0×10 –14 1.5 200 D51

C 2 H 5 O + NO M 

###  →

 products (See Table 2-1)

C 2 H 5 O + NO 2 M 

###  →

 products (See Table 2-1)

C 2 H 5 O 2 + C 2 H 5 O 2 → products 6.8×10 –14 0 6.8×10 –14 2 300 D52

### 1-13 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

C 2 H 5 O 2 + NO → products 2.6×10 –12 –365 8.7×10 –12 1.2 150 D53

CH 3 C(O)O 2 + CH 3 C(O)O 2 → products 2.9×10 –12 –500 1.5×10 –11 1.5 150 D54

CH 3 C(O)O 2 + NO → products 8.1×10 –12 –270 2.0×10 –11 1.5 100 D55

CH 3 C(O)O 2 + NO 2 M 

###  →

 products (See Table 2-1)

CH 3 C(O)CH 2 O 2 + NO → products 2.9×10 –12 –300 8.0×10 –12 1.5 300 D56



### FO × 

### Reactions

O + FO → F + O 2 2.7×10 –11 0 2.7×10 –11 3.0 250 E 1

O + FO 2 → FO + O 2 5.0×10 –11 0 5.0×10 –11 5.0 250 E 2

OH + CH 3 F → CH 2 F + H 2 O (HFC–41) 2.5×10 –12 1430 2.1×10 –14 1.15 150 E 3

OH + CH 2 F 2 → CHF 2 + H 2 O (HFC-32) 1.7×10 –12 1500 1.1×10 –14 1.15 150 E 4

OH + CHF 3 → CF 3 + H 2 O (HFC-23) 6.3×10 –13 2300 2.8×10 –16 1.2 200 E 5

OH + CH 3 CH 2 F → products (HFC-161) 2.5×10 –12 730 2.2×10 –13 1.15 150 E 6

OH + CH 3 CHF 2 → products (HFC-152a) 9.4×10 –13 990 3.4×10 –14 1.1 100 E 7

OH + CH 2 FCH 2 F → CHFCH 2 F + H 2 O (HFC-152) 1.1×10 –12 730 9.7×10 –14 1.1 150 E 8

OH + CH 3 CF 3 → CH 2 CF 3 + H 2 O (HFC-143a) 1.1×10 –12 2010 1.3×10 –15 1.1 100 E 9

OH + CH 2 FCHF 2 → products (HFC-143) 3.9×10 –12 1620 1.7×10 –14 1.2 200 E10

OH + CH 2 FCF 3 → CHFCF 3 + H 2 O (HFC-134a) 1.05×10 –12 1630 4.4×10 –15 1.1 200 E11

OH + CHF 2 CHF 2 → CF 2 CHF 2 + H 2 O (HFC-134) 1.6×10 –12 1660 6.1×10 –15 1.2 200 E12

OH + CHF 2 CF 3 → CF 2 CF 3 + H 2 O (HFC-125) 6.0×10 –13 1700 2.0×10 –15 1.2 150 E13

OH + CH 3 CHFCH 3 → products (HFC-281ea) 3.0×10 –12 490 5.8×10 –13 1.2 100 E14

OH + CF 3 CH 2 CH 3 → products (HFC-263fb) – – 4.2×10 –14 1.5 – E15

OH + CH 2 FCF 2 CHF 2 → products (HFC-245ca) 2.1×10 –12 1620 9.2×10 –15 1.2 150 E16

OH + CHF 2 CHFCHF 2 → products (HFC-245ea) – – 1.6×10 –14 2.0 – E17

OH + CF 3 CHFCH 2 F → products (HFC-245eb) – – 1.5×10 –14 2.0 – E18

OH + CHF 2 CH 2 CF 3 → products (HFC-245fa) 6.1×10 –13 1330 7.0×10 –15 1.2 150 E19

### 1-14 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

OH + CF 3 CF 2 CH 2 F → CF 3 CF 2 CHF + H 2 O ( HF C -2 36cb) 1.3×10 –12 1700 4.4×10 –15 2.0 200 E20

OH + CF 3 CHFCHF 2 → products (HFC-236ea) 9.4×10 –13 1550 5.2×10 –15 1.2 200 E21

OH + CF 3 CH 2 CF 3 → CF 3 CHCF 3 + H 2 O (HFC–236fa) 1.45×10 –12 2500 3.3×10 –16 1.15 150 E22

OH + CF 3 CHFCF 3 → CF 3 CFCF 3 +H 2 O (HFC-227ea) 4.3×10 –13 1650 1.7×10 –15 1.1 150 E23

OH + CF 3 CH 2 CF 2 CH 3 → products (HFC-365mfc) 1.8×10 –12 1660 6.9×10 –15 1.3 150 E24

OH + CF 3 CH 2 CH 2 CF 3 → products (HFC-356mff) 3.4×10 –12 1820 7.6×10 –15 1.2 300 E25

OH + CF 3 CF 2 CH 2 CH 2 F → products (HFC-356mcf) 1.7×10 –12 1100 4.2×10 –14 1.3 150 E26

OH + CHF 2 CF 2 CF 2 CF 2 H → products (HFC-338pcc) 7.7×10 –13 1540 4.4×10 –15 1.2 150 E27

OH + CF 3 CH 2 CF 2 CH 2 CF 3 → products (HFC-458mfcf) 1.1×10 –12 1800 2.6×10 –15 1.5 200 E28

OH + CF 3 CHFCHFCF 2 CF 3 → products (HFC-43-10mee) 5.2×10 –13 1500 3.4×10 –15 1.2 150 E29

OH + CF 3 CF 2 CH 2 CH 2 CF 2 CF 3 → products (HFC–55-10-mcff) 3.5×10 –12 1800 8.3×10 –15 1.5 300 E30

OH + CH 2 =CHF → products 1.5×10 –12 –390 5.5×10 –12 1.3 150 E31

OH + CH 2 =CF 2 → products 6.2×10 –13 –350 2.0×10 –12 1.5 150 E32

OH + CF 2 = CF 2 → products 3.4×10 –12 –320 1.0×10 –11 1.15 100 E33

OH + CF 3 OH → CF 3 O + H 2 O <2×10 –17 E34

OH + CH 2 (OH)CF 3 → products 1.6×10 –12 830 9.8×10 –14 1.15 200 E35

OH + CH 2 (OH)CF 2 CF 3 → products 1.15×10 –12 730 1.0×10 –13 1.2 200 E36

OH + CF 3 CH(OH)CF 3 → products 5.1×10 –13 900 2.5×10 –14 1.3 200 E37

OH + CH 3 OCHF 2 → products (HFOC-152a) 6.0×10 –12 1530 3.5×10 –14 1.3 200 E38

OH + CF 3 OCH 3 → CF 3 OCH 2 + H 2 O (HFOC-143a) 1.5×10 –12 1450 1.2×10 –14 1.1 150 E39

OH + CF 2 HOCF 2 H → CF 2 OCF 2 H +H 2 O (HFOC-134) 1.1×10 –12 1830 2.4×10 –15 1.15 150 E40

OH + CF 3 OCHF 2 → CF 3 OCF 2 + H 2 O (HFOC-125) 4.6×10 –13 2040 4.9×10 –16 1.2 200 E41

OH + CHF 2 OCH 2 CF 3 → products (HFOC-245fa) 3.1×10 –12 1660 1.2×10 –14 1.2 200 E42

OH + CH 3 OCF 2 CHF 2 → products 1.7×10 –12 1300 2.2×10 –14 1.3 200 E43

OH + CH 3 OCF 2 CF 3 → products 1.1×10 –12 1370 1.1×10 –14 1.2 150 E44

### 1-15 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

OH + CH 3 OCF 2 CF 2 CF 3 → products 1.4×10 –12 1440 1.1×10 –14 1.15 150 E45

OH + CH 3 OCF(CF 3 ) 2 → products 1.3×10 –12 1330 1.5×10 –14 1.3 200 E46

OH + CHF 2 OCH 2 CF 2 CHF 2 → products 1.8×10 –12 1410 1.6×10 –14 1.3 200 E47

OH + CHF 2 OCH 2 CF 2 CF 3 → products 1.6×10 –12 1510 1.0×10 –14 1.3 200 E48

F + O 2 M 

###  →

 FO 2 (See Table 2-1)

F + O 3 → FO + O 2 2.2×10 –11 230 1.0×10 –11 1.5 200 E49

F + H 2 → HF + H 1.4×10 –10 500 2.6×10 –11 1.2 200 E50

F + H 2 O → HF + OH 1.4×10 –11 0 1.4×10 –11 1.3 200 E51

F + NO M 

###  →

 FNO (See Table 2-1)

F + NO 2 M 

###  →

 FNO 2 (See Table 2-1)

F + HNO 3 → HF + NO 3 6.0×10 –12 –400 2.3×10 –11 1.3 200 E52

F + CH 4 → HF + CH 3 1.6×10 –10 260 6.7×10 –11 1.4 200 E53

FO + O 3 → products <1 × 10 –14 E54

FO + NO → NO 2 + F 8.2×10 –12 –300 2.2×10 –11 1.5 200 E55

FO + NO 2 M 

###  →

 FONO 2 (See Table 2-1)

FO + FO → 2F + O 2 1.0×10 –11 0 1.0×10 –11 1.5 250 E56

FO 2 + O 3 → products <3.4×10 –16 E57

FO 2 + NO → FNO + O 2 7.5×10 –12 690 7.5×10 –13 2.0 400 E58

FO 2 + NO 2 → products 3.8×10 –11 2040 4.0×10 –14 2.0 500 E59

FO 2 + CO → products <5.1×10 –16 E60

FO 2 + CH 4 → products <2×10 –16 E61

CF 3 + O 2 M 

###  →

 CF 3 O 2 (See Table 2-1)

CF 3 O + M → F + CF 2 O + M (See Table 2-1)

CF 3 O + O 2 → FO 2 + CF 2 O <3 × 10 –11 5000 <1.5 × 10 –18 1.3 – E62

CF 3 O + O 3 → CF 3 O 2 + O 2 2 × 10 –12 1400 1.8 × 10 –14 600 E63

### 1-16 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

CF 3 O + H 2 O → OH + CF 3 OH 3 × 10 –12 >3600 <2 × 10 –17 1.2 – E64

CF 3 O + NO → CF 2 O + FNO 3.7 × 10 –11 –110 5.4 × 10 –11 70 E65

CF 3 O + NO 2 → products (See Note) E66

M 

###  →

 CF 3 ONO 2 (See Table 2-1)

CF 3 O + CO → products <2 × 10 –15 E67

M 

###  →

 CF 3 OCO (See Table 2-1)

CF 3 O + CH 4 → CH 3 + CF 3 OH 2.6 × 10 –12 1420 2.2 × 10 –14 1.1 200 E68

CF 3 O + C 2 H 6 → C 2 H 5 + CF 3 OH 4.9 × 10 –12 400 1.3 × 10 –12 1.2 100 E69

CF 3 O 2 + O 3 → CF 3 O + 2O 2 <3 × 10 –15 E70

CF 3 O 2 + CO → CF 3 O + CO 2 <5 × 10 –16 E71

CF 3 O 2 + NO → CF 3 O + NO 2 5.4 × 10 –12 –320 1.6 × 10 –11 1.1 150 E72

CF 3 O 2 + NO 2 M 

###  →

 CF 3 O 2 NO 2 (See Table 2-1)



### ClO × 

### Reactions

O + ClO → Cl + O 2 3.0×10 –11 –70 3.8×10 –11 1.15 70 F 1

O + OClO → ClO + O 2 2.4×10 –12 960 1.0×10 –13 2.0 300 F 2

O + OClO M 

###  →

 ClO 3 (See Table 2-1)

O + Cl 2 O → ClO + ClO 2.7×10 –11 530 4.5×10 –12 1.3 150 F 3

O + HCl → OH + Cl 1.0×10 –11 3300 1.5×10 –16 2.0 350 F 4

O + HOCl → OH + ClO 1.7×10 –13 0 1.7×10 –13 3.0 300 F 5

O + ClONO 2 → products 2.9×10 –12 800 2.0×10 –13 1.5 200 F 6

O 3 + OClO → products 2.1×10 –12 4700 3.0×10 –19 2.5 1000 F 7

O 3 + Cl 2 O 2 → products – – <1.0×10 –19 – – F 8

OH + Cl 2 → HOCl + Cl 1.4×10 –12 900 6.7×10 –14 1.2 400 F 9

OH + ClO → Cl + HO 2

→ HCl + O 2 7.4×10 –12 6.0×10 –13 –270 –230 1.8×10 –11 1.3×10 –12 1.4 3.0 100 150 F10

OH + OClO → HOCl + O 2 4.5×10 –13 –800 6.8×10 –12 2.0 200 F11

### 1-17 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

OH + HCl → H 2 O + Cl 2.6×10 –12 350 8.0×10 –13 1.1 100 F12

OH + HOCl → H 2 O + ClO 3.0×10 –12 500 5.0×10 –13 3.0 500 F13

OH + ClNO 2 → HOCl + NO 2 2.4×10 –12 1250 3.6×10 –14 2.0 300 F14

OH + ClONO 2 → products 1.2×10 –12 330 3.9×10 –13 1.5 200 F15

OH + CH 3 Cl → CH 2 Cl + H 2 O 2.4×10 –12 1250 3.6×10 –14 1.15 100 F16

OH + CH 2 Cl 2 → CHCl 2 + H 2 O 1.9×10 –12 870 1.0×10 –13 1.15 100 F17

OH + CHCl 3 → CCl 3 + H 2 O 2.2×10 –12 920 1.0×10 –13 1.15 150 F18

OH + CCl 4 → products ~1.0×10 –12

>2300 <5.0×10 –16 – – F19

OH + CH 2 FCl → CHClF + H 2 O (HCFC-31) 2.4×10 –12 1210 4.1×10 –14 1.15 200 F20

OH + CHFCl 2 → CFCl 2 + H 2 O (HCFC-21) 1.2×10 –12 1100 3.0×10 –14 1.2 150 F21

OH + CHF 2 Cl → CF 2 Cl + H 2 O (HCFC-22) 1.05×10 –12 1600 4.8×10 –15 1.1 150 F22

OH + CFCl 3 → products ( CFC-11 ) ~1.0×10 –12 >3700 <5.0×10 –18 – – F23

OH + CF 2 Cl 2 → products (CFC-12) ~1.0×10 –12 >3600 <6.0×10 –18 – – F24

OH + CH 2 ClCH 3 → products 5.4×10 –12 800 3.7×10 –13 1.2 100 F25

OH + CH 3 CCl 3 → CH 2 CCl 3 + H 2 O 1.6×10 –12 1520 1.0×10 –14 1.15 100 F26

OH + CH 3 CFCl 2 → CH 2 CFCl 2 + H 2 O (HCFC-141b) 1.25×10 –12 1600 5.8×10 –15 1.15 150 F27

OH + CH 3 CF 2 Cl → CH 2 CF 2 Cl + H 2 O (HCFC-142b) 1.3×10 –12 1770 3.4×10 –15 1.2 150 F28

OH + CH 2 ClCF 2 Cl → CHClCF 2 Cl +H 2 O (HCFC-132b) 3.6×10 –12 1600 1.7×10 –14 1.5 200 F29

OH + CH 2 ClCF 3 → CHClCF 3 + H 2 O (HCFC-133a) 5.6×10 –13 1100 1.4×10 –14 1.3 200 F30

OH + CHCl 2 CF 2 Cl → CCl 2 CF 2 Cl (HCFC-122) + H 2 O 7.7×10 –13 810 5.1×10 –14 1.2 150 F31

OH + CHFClCFCl 2 → CFClCFCl 2 (HCFC-122a) + H 2 O 7.1×10 –13 1140 1.6×10 –14 1.3 150 F32

OH + CHCl 2 CF 3 → CCl 2 CF 3 + H 2 O (HCFC-123) 6.3×10 –13 850 3.6×10 –14 1.2 100 F33

OH + CHFClCF 2 Cl → CFClCF 2 Cl +H 2 O (HCFC-123a) 8.6×10 –13 1250 1.3×10 –14 1.3 200 F34

OH + CHFClCF 3 → CFClCF 3 + H 2 O (HCFC-124) 7.1×10 –13 1300 9.0×10 –15 1.15 100 F35

OH + CH 3 CF 2 CFCl 2 → products

 (HCFC-243cc) 7.7×10 –13 1720 2.4×10 –15 1.3 200 F36

### 1-18 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

OH + CHCl 2 CF 2 CF 3 → products ( H C F C -22 5ca) 6.3×10 –13 960 2.5×10 –14 1.2 200 F37

OH + CHFClCF 2 CF 2 Cl → products (HCFC-225cb) 5.5×10 –13 1230 8.9×10 –15 1.2 150 F38

OH + CH 2 =CHCl → products 1.3×10 –12 –500 6.9×10 –12 1.2 100 F39

OH + CH 2 =CCl 2 → products 1.9×10 –12 –530 1.1×10 –11 1.15 150 F40

OH + CHCl=CCl 2 → products 8.0×10 –13 –300 2.2×10 –12 1.2 100 F41

OH + CCl 2 =CCl 2 → products 4.7×10 –12 990 1.7×10 –13 1.2 200 F42

OH + CH 3 OCl → products 2.5×10 –12 370 7.1×10 –13 2.0 150 F43

OH + CCl 3 CHO → H 2 O + CCl 3 CO 9.1×10 –12 580 1.3×10 –12 1.3 200 F44

HO 2 + Cl → HCl + O 2 1.8×10 –11 –170 3.2×10 –11 1.5 200 F45

→ OH + ClO 4.1×10 –11 450 9.1×10 –12 2.0 200 F45

HO 2 + ClO → HOCl + O 2 2.7×10 –12 –220 5.6×10 –12 1.3 200 F46

H 2 O + ClONO 2 → products – – <2.0×10 –21 – – F47

NO + OClO → NO 2 + ClO 2.5×10 –12 600 3.4×10 –13 2.0 300 F48

NO + Cl 2 O 2 → products – – <2.0×10 –14 – – F49

NO 3 + OClO M 

###  →

 O 2 ClONO 2 (See Table 2-1)

NO 3 + HCl → HNO 3 + Cl – – <5.0×10 –17 – – F50

HO 2 NO 2 + HCl → products – – <1.0×10 –21 – – F51

Cl + O 2 M 

###  →

 ClOO (See Table 2-1)

Cl + O 3 → ClO + O 2 2.3×10 –11 200 1.2×10 –11 1.15 100 F52

Cl + H 2 → HCl + H 3.7×10 –11 2300 1.6×10 –14 1.25 200 F53

Cl + H 2 O 2 → HCl + HO 2 1.1×10 –11 980 4.1×10 –13 1.3 300 F54

Cl + NO M 

###  →

 NOCl (See Table 2-1)

Cl + NO 2 M 

###  →

 ClONO (ClNO 2 ) (See Table 2-1)

Cl + NO 3 → ClO + NO 2 2.4×10 –11 0 2.4×10 –11 1.5 400 F55

Cl + N 2 O → ClO + N 2 (See Note) F56

### 1-19 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

Cl + HNO 3 → products – – <2.0×10 –16 – – F57

Cl + HO 2 NO 2 → products <1×10 –13 F58

Cl + CO M 

###  →

 ClCO (See Table 2-1)

Cl + CH 4 → HCl + CH 3 9.6×10 –12 1360 1.0×10 –13 1.05 75 F59

Cl + CH 3 D → products – – 7.4×10 –14 2.0 – F60

Cl + H 2 CO → HCl + HCO 8.1×10 –11 30 7.3×10 –11 1.15 100 F61

Cl + HC(O)OH → products 2.0×10 –13 1.5 F62

Cl + CH 3 O 2 → products – – 1.6×10 –10 1.5 – F63

Cl + CH 3 OH → CH 2 OH + HCl 5.5×10 –11 0 5.5×10 –11 1.2 100 F64

Cl + CH 3 OOH → products 5.7×10 –11 2.0 F65

Cl + CH 3 ONO 2 → products 1.3×10 –11 1200 2.3×10 –13 1.5 300 F66

Cl + C 2 H 2 M 

###  →

 ClC 2 H 2 (See Table 2-1)

Cl + C 2 H 4 M 

###  →

 ClC 2 H 4 (See Table 2-1)

Cl + C 2 H 6 → HCl + C 2 H 5 7.7×10 –11 90 5.7×10 –11 1.1 90 F67

Cl + C 2 H 5 O 2 → ClO + C 2 H 5 O – – 7.4×10 –11 2.0 – F68

→ HCl + C 2 H 4 O 2 – 7.7×10 –11 2.0 – F68

Cl + CH 3 CH 2 OH → products 9.6×10 –11 0 9.6×10 –11 1.2 100 F69

Cl + CH 3 C(O)OH → products 2.8×10 –14 2.0 F70

Cl + CH 3 CN → products 1.6×10 –11 2140 1.2×10 –14 2.0 300 F71

Cl + C 2 H 5 ONO 2 → products 1.5×10 –11 400 3.9×10 –12 1.5 200 F72

Cl + CH 3 CO 3 NO 2 → products – – <1×10 –14 – F73

Cl + C 3 H 8 → HCl + C 3 H 7 1.2×10 –10 –40 1.4×10 –10 1.3 250 F74

Cl + CH 3 C(O)CH 3 → CH 3 C(O)CH 2 +HCl 7.7×10 –11 1000 2.7×10 –12 1.3 500 F75

Cl + C 2 H 5 CO 3 NO 2 → products 1.1×10 –12 2.0 F76

Cl + 1-C 3 H 7 ONO 2 → products 4.5×10 –11 200 2.3×10 –11 1.5 200 F77

### 1-20 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

Cl + 2-C 3 H 7 ONO 2 → products 2.3×10 –11 400 6.0×10 –12 2.0 200 F78

Cl + OClO → ClO + ClO 3.4×10 –11 –160 5.8×10 –11 1.25 200 F79

Cl + ClOO → Cl 2 + O 2 2.3×10 –10 0 2.3×10 –10 3.0 250 F80

→ ClO + ClO 1.2×10 –11 0 1.2×10 –11 3.0 250 F80

Cl + Cl 2 O → Cl 2 + ClO 6.2×10 –11 –130 9.6×10 –11 1.2 130 F81

Cl + Cl 2 O 2 → products – – 1.0×10 –10 2.0 – F82

Cl + HOCl → products 2.5×10 –12 130 1.6×10 –12 1.5 250 F83

Cl + ClNO → NO + Cl 2 5.8×10 –11 –100 8.1×10 –11 1.5 200 F84

Cl + ClONO 2 → products 6.5×10 –12 –135 1.0×10 –11 1.2 50 F85

Cl + CH 3 Cl → CH 2 Cl + HCl 3.2×10 –11 1250 4.8×10 –13 1.2 200 F86

Cl + CH 2 Cl 2 → HCl + CHCl 2 3.1×10 –11 1350 3.3×10 –13 1.5 500 F87

Cl + CHCl 3 → HCl + CCl 3 8.2×10 –12 1325 9.6×10 –14 1.3 300 F88

Cl + CH 3 F → HCl + CH 2 F (HFC-41) 2.0×10 –11 1200 3.5×10 –13 1.3 500 F89

Cl + CH 2 F 2 → HCl + CHF 2 (HFC-32) 1.2×10 –11 1630 5.0×10 –14 1.5 500 F90

Cl + CF 3 H → HCl + CF 3 (HFC-23) – – 3.0×10 –18 5.0 – F91

Cl + CH 2 FCl → HCl + CHFCl (HCFC-31) 1.2×10 –11 1390 1.1×10 –13 2.0 500 F92

Cl + CHFCl 2 → HCl + CFCl 2 (HCFC-21) 5.5×10 –12 1675 2.0×10 –14 1.3 200 F93

Cl + CHF 2 Cl → HCl + CF 2 Cl (HCFC-22) 5.9×10 –12 2430 1.7×10 –15 1.3 200 F94

Cl + CH 3 CCl 3 → CH 2 CCl 3 + HCl 2.8×10 –12 1790 7.0×10 –15 2.0 400 F95

Cl + CH 3 CH 2 F → HCl + CH 3 CHF (HFC-161) 1.8×10 –11 290 6.8×10 –12 3.0 500 F96

→ HCl + CH 2 CH 2 F 1.4×10 –11 880 7.3×10 –13 3.0 500 F96

Cl + CH 3 CHF 2 → HCl + CH 3 CF 2 (HFC-152a) 6.4×10 –12 950 2.6×10 –13 1.3 500 F97

→ HCl + CH 2 CHF 2 7.2×10 –12 2390 2.4×10 –15 3.0 500 F97

Cl + CH 2 FCH 2 F → HCl + CHFCH 2 F (HFC-152) 2.6×10 –11 1060 7.5×10 –13 3.0 500 F98

Cl + CH 3 CFCl 2 → HCl + CH 2 CFCl 2 (HCFC-141b) 1.8×10 –12 2000 2.2×10 –15 1.2 300 F99

### 1-21 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

Cl + CH 3 CF 2 Cl → HCl + CH 2 CF 2 Cl ( H C F C -142 b) 1.4×10 –12 2420 4.2×10 –16 1.2 500 F100

Cl + CH 3 CF 3 → HCl + CH 2 CF 3 (HFC-143a) 1.2×10 –11 3880 2.6×10 –17 5.0 500 F101

Cl + CH 2 FCHF 2 → HCl + CH 2 FCF 2 (HFC-143) 5.5×10 –12 1610 2.5×10 –14 3.0 500 F102

→ HCl + CHFCHF 2 7.7×10 –12 1720 2.4×10 –14 3.0 500 F102

Cl + CH 2 ClCF 3 → HCl + CHClCF 3 (HCFC-133a) 1.8×10 –12 1710 5.9×10 –15 3.0 500 F103

Cl + CH 2 FCF 3 → HCl + CHFCF 3 (HFC-134a) – – 1.5×10 –15 1.2 – F104

Cl + CHF 2 CHF 2 → HCl + CF 2 CHF 2 (HCF-134) 7.5×10 –12 2430 2.2×10 –15 1.5 500 F105

Cl + CHCl 2 CF 3 → HCl + CCl 2 CF 3 (HCFC-123) 4.4×10 –12 1750 1.2×10 –14 1.3 500 F106

Cl + CHFClCF 3 → HCl + CFClCF 3 (HCFC-124) 1.1×10 –12 1800 2.7×10 –15 1.3 500 F107

Cl + CHF 2 CF 3 → HCl + CF 2 CF 3 (HFC-125) – – 2.4×10 –16 1.3 – F108

Cl + C 2 Cl 4 M 

###  →

 C 2 Cl 5 (See Table 2-1)

ClO + O 3 → ClOO + O 2 – – <1.4×10 –17 – – F109

→ OClO + O 2 1.0×10 –12

>4000 <1.0×10 –18 – – F109

ClO + H 2 → products ~1.0×10 –12

>4800 <1.0×10 –19 – – F110

ClO + NO → NO 2 + Cl 6.4×10 –12 –290 1.7×10 –11 1.15 100 F111

ClO + NO 2 M 

###  →

 ClONO 2 (See Table 2-1)

ClO + NO 3 → ClOO + NO 2 4.7×10 –13 0 4.7×10 –13 1.5 400 F112

ClO + N 2 O → products ~1.0×10 –12 >4300 <6.0×10 –19 – – F113

ClO + CO → products ~1.0×10 –12 >3700 <4.0×10 –18 – – F114

ClO + CH 4 → products ~1.0×10 –12 >3700 <4.0×10 –18

– – F115

ClO + H 2 CO → products ~1.0×10 –12 >2100 <1.0×10 –15 – – F116

ClO + CH 3 O 2 → products 3.3×10 –12 115 2.2×10 –12 1.5 115 F117

ClO + ClO → Cl 2 + O 2 1.0×10 –12 1590 4.8×10 –15 1.5 300 F118

→ ClOO + Cl 3.0×10 –11 2450 8.0×10 –15 1.5 500 F118

→ OClO + Cl 3.5×10 –13 1370 3.5×10 –15 1.5 300 F118

### 1-22 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

ClO + ClO M 

###  →

 Cl 2 O 2 (See Table 2-1)

ClO + OClO M 

###  →

 Cl 2 O 3 (See Table 2-1)

HCl + ClONO 2 → products – – <1.0×10 –20 – – F119

CH 2 Cl + O 2 M 

###  →

 CH 2 ClO 2 (See Table 2-1)

CHCl 2 + O 2 M 

###  →

 CHCl 2 O 2 (See Table 2-1)

CCl 3 + O 2 M 

###  →

 CCl 3 O 2 (See Table 2-1)

CFCl 2 + O 2 M 

###  →

 CFCl 2 O 2 (See Table 2-1)

CF 2 Cl + O 2 M 

###  →

 CF 2 ClO 2 (See Table 2-1)

CCl 3 O 2 + NO 2 M 

###  →

 CCl 3 O 2 NO 2 (See Table 2-1)

CFCl 2 O 2 + NO 2 M 

###  →

 CFCl 2 O 2 NO 2 (See Table 2-1)

CF 2 ClO 2 + NO 2 M 

###  →

 CF 2 ClO 2 NO 2 (See Table 2-1)

CH 2 ClO + O 2 → CHClO + HO 2 – – 6 × 10 –14 5 – F120

CH 2 ClO 2 + HO 2 → CH 2 ClO 2 H + O 2 3.3 × 10 –13 –820 5.2 × 10 –12 1.5 200 F121

CH 2 ClO 2 + NO → CH 2 ClO + NO 2 7 × 10 –12 –300 1.9 × 10 –11 1.5 200 F122

CCl 3 O 2 + NO → CCl 2 O + NO 2 + Cl 7.3 × 10 –12 –270 1.8 × 10 –11 1.3 200 F123

CCl 2 FO 2 + NO → CClFO + NO 2 + Cl 4.5 × 10 –12 –350 1.5 × 10 –11 1.3 200 F124

CClF 2 O 2 + NO → CF 2 O + NO 2 + Cl 3.8 × 10 –12 –400 1.5 × 10 –11 1.2 200 F125



### BrO × 

### Reactions

O + BrO → Br + O 2 1.9×10 –11 –230 4.1×10 –11 1.5 150 G 1

O + HBr → OH + Br 5.8×10 –12 1500 3.8×10 –14 1.3 200 G 2

O + HOBr → OH + BrO 1.2×10 –10 430 2.8×10 –11 3.0 300 G 3

OH + Br 2 → HOBr + Br 4.2×10 –11 0 4.2×10 –11 1.3 600 G 4

OH + BrO → products – – 7.5×10 –11 3.0 – G 5

OH + HBr → H 2 O + Br 1.1×10 –11 0 1.1×10 –11 1.2 250 G 6

OH + CH 3 Br → CH 2 Br + H 2 O 2.35×10 –12 1300 3.0×10 –14 1.1 100 G 7

### 1-23 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

OH + CH 2 Br 2 → CHBr 2 + H 2 O 2.0×10 –12 840 1.2×10 –13 1.15 150 G 8

OH + CHBr 3 → CBr 3 + H 2 O 1.35×10 –12 600 1.8×10 –13 1.5 100 G 9

OH + CHF 2 Br → CF 2 Br + H 2 O 1.0×10 –12 1380 1.0×10 –14 1.1 100 G10

OH + CH 2 ClBr → CHClBr + H 2 O 2.4×10 –12 920 1.1×10 –13 1.1 100 G11

OH + CF 2 ClBr → products (Halon-1211) ∼ 1×10 –12 >2600 <1.5×10 –16

– – G12

OH + CF 2 Br 2 → products (Halon-1202) ∼ 1×10 –12 >2200 <5.0×10 –16 – – G13

OH + CF 3 Br → products (Halon-1301) ∼ 1×10 –12 >3600 <6.0×10 –18 – – G14

OH + CH 2 BrCH 3 → products 2.9×10 –12 640 3.4×10 –13 1.2 150 G15

OH + CH 2 BrCF 3 → CHBrCF 3 + H 2 O 1.4×10 –12 1340 1.6×10 –14 1.2 150 G16

OH + CHFBrCF 3 → CFBrCF 3 + H 2 O 7.3×10 –13 1120 1.7×10 –14 1.2 100 G17

OH + CHClBrCF 3 → CClBrCF 3 + H 2 O 1.1×10 –12 940 4.7×10 –14 1.2 150 G18

OH + CHFClCF 2 Br → CFClCF 2 Br + H 2 O 8.4×10 –13 1220 1.4×10 –14 1.3 200 G19

OH + CF 2 BrCF 2 Br → products (Halon-2402) ∼ 1×10 –12 >3600 <6×10 –18 – – G20

OH + CH 2 BrCH 2 CH 3 → products 3.0×10 –12 330 1.0×10 –12 1.1 50 G21

OH + CH 3 CHBrCH 3 → products 1.85×10 –12 270 7.5×10 –13 1.15 50 G22

HO 2 + Br → HBr + O 2 1.5×10 –11 600 2.0×10 –12 2.0 600 G23

HO 2 + BrO → products 3.4×10 –12 –540 2.1×10 –11 1.5 200 G24

NO 3 + HBr → HNO 3 + Br – – <1.0×10 –16 – – G25

Cl + CH 2 ClBr → HCl + CHClBr 1.5×10 –11 1070 4.1×10 –13 1.2 300 G26

Cl + CH 3 Br → HCl + CH 2 Br 1.7×10 –11 1080 4.5×10 –13 1.1 100 G27

Cl + CH 2 Br 2 → HCl + CHBr 2 6.7×10 –12 825 4.2×10 –13 1.15 150 G28

Cl + CHBr 3 → CBr 3 + HCl 4.85×10 –12 850 2.8×10 –13 1.5 250 G29

Br + O 3 → BrO + O 2 1.7×10 –11 800 1.2×10 –12 1.2 200 G30

Br + H 2 O 2 → HBr + HO 2 1.0×10 –11 >3000 <5.0×10 –16 – – G31

Br + NO 2 M 

###  →

 BrNO 2 (See Table 2-1)

### 1-24 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

Br + NO 3 → BrO + NO 2 – – 1.6×10 –11 2.0 – G32

Br + H 2 CO → HBr + HCO 1.7×10 –11 800 1.1×10 –12 1.3 200 G33

Br + OClO → BrO + ClO 2.6×10 –11 1300 3.4×10 –13 2.0 300 G34

Br + Cl 2 O → BrCl + ClO 2.1×10 –11 470 4.3×10 –12 1.3 150 G35

Br + Cl 2 O 2 → products – – 3.0×10 –12 2.0 – G36

BrO + O 3 → products ~1.0×10 –12 >3200 <2.0×10 –17 – – G37

BrO + NO → NO 2 + Br 8.8×10 –12 –260 2.1×10 –11 1.15 130 G38

BrO + NO 2 M 

###  →

 BrONO 2 (See Table 2-1)

BrO + NO 3 → products – – 1.0×10 –12 3.0 – G39

BrO + ClO → Br + OClO 9.5×10 –13 –550 6.0×10 –12 1.25 150 G40

→ Br + ClOO 2.3×10 –12 –260 5.5×10 –12 1.25 150 G40

→ BrCl + O 2 4.1×10 –13 –290 1.1×10 –12 1.25 150 G40

BrO + BrO → products 1.5×10 –12 –230 3.2×10 –12 1.15 150 G41

CH 2 BrO 2 + NO → CH 2 O + NO 2 + Br 4×10 –12 –300 1.1 × 10 –11 1.5 200 G42



### IO × 

### Reactions

O + I 2 → IO + I 1.4×10 –10 0 1.4×10 –10 1.4 250 H 1

O + IO → O 2 + I 1.2×10 –10 2.0 H 2

OH + I 2 → HOI + I 1.8×10 –10 2.0 H 3

OH + HI → H 2 O + I 3.0×10 –11 2.0 H 4

OH + CH 3 I → H 2 O + CH 2 I 2.9×10 –12 1100 7.2×10 –14 1.5 300 H 5

OH + CF 3 I → HOI + CF 3 2.5×10 –11 2070 2.4×10 –14 1.3 200 H 6

HO 2 + I → HI + O 2 1.5×10 –11 1090 3.8×10 –13 2.0 500 H 7

HO 2 + IO → HOI + O 2 8.4×10 –11 1.5 H 8

NO 3 + HI → HNO 3 + I (See Note) H 9

Cl + CH 3 I → CH 2 I + HCl 2.9×10 –11 1000 1.0×10 –12 1.5 250 H10

### 1-25 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

I + O 3 → IO + O 2 2.3×10 –11 870 1.2×10 –12 1.2 200 H11

I + NO M 

###  →

 INO (See Table 2-1)

I + NO 2 M 

###  →

 INO 2 (See Table 2-1)

I + BrO → IO + Br – – 1.2×10 –11 2.0 H12

IO + NO → I + NO 2 9.1×10 –12 –240 2.0×10 –11 1.2 150 H13

IO + NO 2 M 

###  →

 IONO 2 (See Table 2-1)

IO + ClO → products 5.1×10 –12 –280 1.3×10 –11 2.0 200 H14

IO + BrO → products – – 6.9×10 –11 1.5 – H15

IO + IO → products 1.5×10 –11 –500 8.0×10 –11 1.5 500 H16

INO + INO → I 2 + 2NO 8.4×10 –11 2620 1.3×10 –14 2.5 600 H17

INO 2 + INO 2 → I 2 + 2NO 2 2.9×10 –11 2600 4.7×10 –15 3.0 1000 H18



### SO × 

### Reactions

O + SH → SO + H – – 1.6×10 –10 5.0 – I 1

O + CS → CO + S 2.7×10 –10 760 2.1×10 –11 1.1 250 I 2

O + H 2 S → OH + SH 9.2×10 –12 1800 2.2×10 –14 1.7 550 I 3

O + OCS → CO + SO 2.1×10 –11 2200 1.3×10 –14 1.2 150 I 4

O + CS 2 → CS + SO 3.2×10 –11 650 3.6×10 –12 1.2 150 I 5

O + SO 2 M 

###  →

 SO 3 (See Table 2-1)

O + CH 3 SCH 3 → CH 3 SO + CH 3 1.3×10 –11 –410 5.0×10 –11 1.1 100 I 6

O + CH 3 SSCH 3 → CH 3 SO + CH 3 S 5.5×10 –11 –250 1.3×10 –10 1.3 100 I 7

O 3 + H 2 S → products – – <2.0×10 –20 – – I 8

O 3 + CH 3 SCH 3 → products – – <1.0×10 –18 – – I 9

O 3 + SO 2 → SO 3 + O 2 3.0×10 –12 >7000 <2.0×10 –22 – – I10

OH + H 2 S → SH + H 2 O 6.0×10 –12 75 4.7×10 –12 1.2 75 I11

OH + OCS → products 1.1×10 –13 1200 1.9×10 –15 2.0 500 I12

### 1-26 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

OH + CS 2 → products (See Note) – – – – I13

OH + CH 3 SH → CH 3 S + H 2 O 9.9×10 –12 –360 3.3×10 –11 1.2 100 I14

OH + CH 3 SCH 3 → H 2 O + CH 2 SCH 3 1.2×10 –11 260 5.0×10 –12 1.15 100 I15

OH + CH 3 SSCH 3 → products 6.0×10 –11 –400 2.3×10 –10 1.2 200 I16

OH + S → H + SO – – 6.6×10 –11 3.0 – I17

OH + SO → H + SO 2 – – 8.6×10 –11 2.0 – I18

OH + SO 2 M 

###  →

 HOSO 2 (See Table 2-1)

HO 2 + H 2 S → products – – <3.0×10 –15 – – I19

HO 2 + CH 3 SH → products – – <4.0×10 –15 – – I19

HO 2 + CH 3 SCH 3 → products – – <5.0×10 –15 – – I19

HO 2 + SO 2 → products – – <1.0×10 –18 – – I20

NO 2 + SO 2 → products – – <2.0×10 –26 – – I21

NO 3 + H 2 S → products – – <8.0×10 –16 – – I22

NO 3 + OCS → products – – <1.0×10 –16 – – I23

NO 3 + CS 2 → products – – <4.0×10 –16 – – I24

NO 3 + CH 3 SH → products 4.4×10 –13 –210 8.9×10 –13 1.25 210 I25

NO 3 + CH 3 SCH 3 → CH 3 SCH 2 + HNO 3 1.9×10 –13 –500 1.0×10 –12 1.2 200 I26

NO 3 + CH 3 SSCH 3 → products 1.3×10 –12 270 5.3×10 –13 1.4 270 I27

NO 3 + SO 2 → products – – <7.0×10 –21 – – I28

N 2 O 5 + CH 3 SCH 3 → products – – <1.0×10 –17 – – I29

CH 3 O 2 + SO 2 → products – – <5.0×10 –17

– – I30

F + CH 3 SCH 3 → products – – 2.4.×10 –10 2.0 – I31

Cl + H 2 S → HCl + SH 3.7×10 –11 –210 7.4×10 –11 1.25 100 I32

Cl + OCS → products – – <1.0×10 –16 – – I33

Cl + CS 2 → products – – <4.0×10 –15 – – I34

### 1-27 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

Cl + CH 3 SH → CH 3 S + HCl 1.2×10 –10 –150 2.0×10 –10 1.25 50 I35

Cl + CH 3 SCH 3 → products (See Note) – – – – I36

ClO + OCS → products – – <2.0×10 –16 – – I37

ClO + CH 3 SCH 3 → products – – 9.5×10 –15 2.0 – I38

ClO + SO → Cl +SO 2 2.8×10 –11 0 2.8×10 –11 1.3 50 I39

ClO + SO 2 → Cl + SO 3 – – <4.0×10 –18 – – I37

Br + H 2 S → HBr + SH 1.4×10 –11 2750 1.4×10 –15 2.0 300 I40

Br + CH 3 SH → CH 3 S + HBr 9.2×10 –12 390 2.5×10 –12 2.0 100 I40

Br + CH 3 SCH 3 → products (See Note) I41

BrO + CH 3 SCH 3 → products 1.5×10 –14 –850 2.6×10 –13 1.3 200 I42

BrO + SO → Br + SO 2 5.7×10 –11 1.4 I43

IO + CH 3 SH → products 6.6×10 –16 2.0 I44

IO + CH 3 SCH 3 → products 1.2×10 –14 1.5 I45

S + O 2 → SO + O 2.3×10 –12 0 2.3×10 –12 1.2 200 I46

S + O 3 → SO + O 2 1.2×10 –11 2.0 I47

SO + O 2 → SO 2 + O 2.6×10 –13 2400 8.4×10 –17 2.0 500 I48

SO + O 3 → SO 2 + O 2 3.6×10 –12 1100 9.0×10 –14 1.2 200 I49

SO + NO 2 → SO 2 + NO 1.4×10 –11 0 1.4×10 –11 1.2 50 I50

SO + OClO → SO 2 + ClO 1.9×10 –12 3.0 I51

SO 3 + H 2 O → products (See Note) – – I52

SO 3 + NH 3 → products (See Table 2-1) – –

SO 3 + NO 2 → products 1.0×10 –19 10.0 I53

SH + O 2 → OH + SO <4.0×10 –19 – I54

SH + O 3 → HSO + O 2 9.0×10 –12 280 3.5×10 –12 1.3 200 I55

SH + H 2 O 2 → products <5.0×10 –15 – I56

### 1-28 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

SH + NO M 

###  →

 HSNO (See Table 2-1)

SH + NO 2 → HSO + NO 2.9×10 –11 –240 6.5×10 –11 1.2 50 I57

SH + Cl 2 → ClSH + Cl 1.7×10 –11 690 1.7×10 –12 2.0 200 I58

SH + BrCl → products 2.3×10 –11 –350 7.4×10 –11 2.0 200 I58

SH + Br 2 → BrSH + Br 6.0×10 –11 –160 1.0×10 –10 2.0 160 I58

SH + F 2 → FSH + F 4.3×10 –11 1390 4.0×10 –13 2.0 200 I58

HSO + O 2 → products <2.0×10 –17 – I59

HSO + O 3 → products 1.0×10 –13 1.3 I60

HSO + NO → products <1.0×10 –15 – I61

HSO + NO 2 → HSO 2 + NO 9.6×10 –12 2.0 I61

HSO 2 + O 2 → HO 2 + SO 2 3.0×10 –13 3.0 I62

HOSO 2 + O 2 → HO 2 + SO 3 1.3×10 –12 330 4.4×10 –13 1.2 200 I63

CS + O 2 → OCS + O 2.9×10 –19 2.0 I64

CS + O 3 → OCS + O 2 3.0×10 –16 3.0 I65

CS + NO 2 → OCS + NO 7.6×10 –17 3.0 I65

CH 3 S + O 2 → products <3.0×10 –18 – I66

CH 3 S + O 3 → products 2.0×10 –12 –290 5.3×10 –12 1.15 100 I67

CH 3 S + NO → products <1.0×10 –13 – I68

CH 3 S + NO M 

###  →

 products (See Table 2-1)

CH 3 S + NO 2 → CH 3 SO + NO 2.1×10 –11 –320 6.1×10 –11 1.15 100 I69

CH 2 SH + O 2 → products 6.5×10 –12 2.0 I70

CH 2 SH + O 3 → products 3.5×10 –11 2.0 I71

CH 2 SH + NO → products 1.9×10 –11 2.0 I72

CH 2 SH + NO 2 → products 5.2×10 –11 2.0 I73

CH 3 SO + O 3 → products 6.0×10 –13 1.5 I74

### 1-29 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

CH 3 SO + NO 2 → CH 3 SO 2 + NO 1.2×10 –11 1.4 I75

CH 3 SOO + O 3 → products <8.0×10 –13 – I76

CH 3 SOO + NO → products 1.1×10 –11 0 1.1×10 –11 2.0 100 I76

CH 3 SO 2 + NO 2 → products 2.2×10 –11 0 2.2×10 –11 2.0 100 I77

CH 3 SCH 2 + O 2 M 

###  →

 CH 3 SCH 2 O 2 (See Table 2-1)

CH 3 SCH 2 + NO 3 → products 3.0 × 10 –10 2.0 I78

CH 3 SCH 2 O 2 + NO → CH 3 SCH 2 O + NO 2 1.9 × 10 –11 2.0 I79

CH 3 SS + O 3 → products 4.6×10 –13 2.0 I80

CH 3 SS + NO 2 → products 1.8×10 –11 2.0 I81

CH 3 SSO + NO 2 → products 4.5×10 –12 2.0 I81



### Metal Reactions

Na + O 2 M 

###  →

 NaO 2 (See Table 2-1)

Na + O 3 → NaO + O 2 1.0×10 –9 95 7.3×10 –10 1.2 50 J 1

→ NaO 2 + O – – <4.0×10 –11 – – J 1

Na + N 2 O → NaO + N 2 2.8×10 –10 1600 1.3×10 –12 1.2 400 J 2

Na + Cl 2 → NaCl + Cl 7.3×10 –10 0 7.3×10 –10 1.3 200 J 3

NaO + O → Na + O 2 3.7×10 –10 0 3.7×10 –10 3.0 400 J 4

NaO + O 2 M 

###  →

 NaO 3 (See Table 2-1)

NaO + O 3 → NaO 2 + O 2 1.1×10 –9 570 1.6×10 –10 1.5 300 J 5

→ Na + 2O 2 6.0×10 –11 0 6.0×10 –11 3.0 800 J 5

NaO + H 2 → NaOH + H 2.6×10 –11 0 2.6×10 –11 2.0 600 J 6

NaO + H 2 O → NaOH + OH 2.2×10 –10 0 2.2×10 –10 2.0 400 J 7

NaO + NO → Na + NO 2 1.5×10 –10 0 1.5×10 –10 4.0 400 J 8

NaO + CO 2 M 

###  →

 NaCO 3 (See Table 2-1)

NaO + HCl → products 2.8×10 –10 0 2.8×10 –10 3.0 400 J 9

### 1-30 Reaction A-Factor a E/R k(298 K) a f(298 K) b g Notes

NaO 2 + O → NaO + O 2 2.2×10 –11 0 2.2×10 –11 5.0 600 J10

NaO 2 + NO → NaO + NO 2 – – <10 –14 – – J11

NaO 2 + HCl → products 2.3×10 –10 0 2.3×10 –10 3.0 400 J12

NaOH + HCl → NaCl + H 2 O 2.8×10 –10 0 2.8×10 –10 3.0 400 J13

NaOH + CO 2 M 

###  →

 NaHCO 3 (See Table 2-1)



### Shaded areas indicate changes or additions since JPL 97-4/JPL 00-3. Italicized entries denote estimates.

a 

### Units are cm 3 

### molecule –1 

### s –1



### . b 

### f(298 K) is the uncertainty factor at 298 K. To calculate the uncertainty at other temperatures, use the expression:

1 1 f(T) = f(298)exp g T 298  

−     

### Note that the exponent is absolute value.

### 1-31 1.3 Notes to Table 1

A1. O + O 3 . The recommended rate expression is from Wine et al . [1316] and is a linear least squares fit of all data (unweighted) from Davis et al. [319], McCrumb and Kaufman [795], West et al. [1294], Arnold and Comes [29], and Wine et al. [1316]. A2. O( 1 D) Reactions. The rate constants are for the disappearance of O( 1 D), which includes physical quenching or deactivation. Where information is available, produc t yields are given. The rate constant recommendations are based on averages of the absolute rate constant measurements reported by Streit et al. [1123], Davidson et al. [312] and Davidson et al. [311] for N 2 O, H 2 O, CH 4, H 2 , N 2 , O 2 , O 3 , CCl 4 , CFCl 3 , CF 2 Cl 2 , NH 3 , and CO 2 ; by Amimoto et al. [18], Amimoto et al. [17], and Force and Wiesenfeld [405,406] for N 2 O, H 2 O, CH 4 , N 2 , H 2 , O 2 , O 3 , CO 2 , CCl 4 , CFCl 3 , CF 2 Cl 2 , and CF 4 ; by Wine and Ravishankara [1317–1319] for N 2 O, H 2 O, N 2 , H 2 , O 3 , CO 2 , and CF 2 O; by Brock and Watson (private communication, 1980) for N 2 , O 2 and CO 2 ; by Lee and Slanger [701,702] for H 2 O and O 2 ; by Gericke and Comes [427] for H 2 O; and by Shi and Barker [1057] for N 2 and CO 2, and Talukdar and Ravishankara [1157] for H 2 . The weight of the evidence from these studies indicates that the results of Heidner and Husain [494], Heidner et al. [493] and Fletcher and Husain [399,400] contain a systematic error. For the cr itical atmospheric reactants, such as N 2 O, H 2 O, and CH 4 , the recommended absolute rate constants are in good agreem ent with the previous relative measurements when compared with N 2 as the reference reactant. A similar comparison with O 2 as the reference reactant gives somewhat poorer agreement.
A3. O( 1 D) + O 2 . The deactivation of O( 1 D) by O 2 leads to the production of O 2 ( 1 ∆ ) with an efficiency of 80±20%: Noxon [901], Biedenkapp and Bair [119], Snelling [1096], and L ee and Slanger [701]. The O 2 ( 1 ∆ ) is produced in the v=0, 1, and 2 vibrational levels in the amounts 60%, 40%, and <3 %, Gauthier and Snelling [424] and Lee and Slanger [701]. A4. O( 1 D) + O 3 . The branching result for reaction of O( 1 D) with O 3 to give O 2 + O 2 or O 2 + O + O is from Davenport et al. [306]. This is supported by measurements of Amimoto et al. [18] who reported that on average one ground state O is produced per O( 1 D) reaction with O 3 . It seems unlikely that this could result from 100% quenching of the O( 1 D) by O 3 . A5. O( 1 D) + H 2 . Wine and Ravishankara [1318] have determined the yield of O( 3 P) is <4.9%. The major products are H + OH. Koppe et al. [649] report a 2.7 times larger rate coefficient at a kinetic energy of 0.12eV. This does not agree with the observations of Davidson et al. [312], who reported that k is independent of temperature (200–350 K) and Matsumi et al. [791] who report no change in k when hot O( 1 D) is moderated with Ar. A6. O( 1 D) + H 2 O. Measurements of the O 2 + H 2 product yield were made by Zellner et al. [1361] (1 +0.5 or –1)% and by Glinski and Birks [445] (0.6 +0.7 or –0.6)%. The yield of O( 3 P) from O( 1 D) + H 2 O is reported to be <(4.9±3.2)% by Wine and Ravishankara [1318] and (2±1)% by Takahashi et al. [1146]. To calculate the rates of OH production via O( 1 D) reactions in the atmosphere, the quantities of interest are the ratios of the rate coeffi cients for the reaction of O( 1 D) with H 2 O to those with N 2 and with O 2 . The ratios of the rate coefficients for O( 1 D) reactions measured using the same method (and often the same apparatus) are more accurate (and precise) than th e individual rate constants that are quoted in Table 1. Ratio data are given in the original references for this reaction. A7. O( 1 D) +N 2 O. The branching ratio for the reaction of O( 1 D) with N 2 O to give N 2 + O 2 or NO + NO is an average of the values reported by Da vidson et al. [309]; Volltrauer et al. [1236]; Marx et al. [790] and Lam et al. [675], with a spread in R=k(NO + NO)/k(Total) = 0.52 – 0.62. Cantrell et al. [198] reported a measurement of R=0.57 and an analysis of all measurements from 1957–1994 leads them to recommend a value of R=0.61±0.06, where the uncertainty indicat es their 95% confidence interval. The recommended branching ratio agrees well with earlier m easurements of the quantum yield from N 2 O photolysis (Calvert and Pitts [189]). The O( 1 D) translational energy and temperature de pendence effects are not clearly resolved. Wine and Ravishankara [1318] have determined that the yield of O( 3 P) from O( 1 D) + N 2 O is <4.0%. The uncertainty for this reaction includes factors for both the overall rate coefficient and the branching ratio. A direct measurement by Greenblatt and Ravishankara [455] of the NO yield from the O( 1 D) + N 2 O reaction in synthetic air agrees very well with the value predicted using the recommended O( 1 D) rate constants for N 2 , O 2 , and N 2 O and the O( 1 D) + N 2 O product branching ratio. These authors suggest that their results support the recommendations and reduce the uncerta inty in the collected rate parameters by over a factor of two. To calculate the rates of NO production via O( 1 D) reactions in the atmosphere, the quantities of interest are the ratios of the rate coeffi cients for the reaction of O( 1 D) with N 2 O to those with N 2 and with O 2 . The ratios of the rate coefficients for O( 1 D) reactions measured using the same method (and often the same apparatus)

### 1-32 are more accurate and precise than the individua l rate constants that are quoted in Table 1. Ratio data are given in the original references for this reaction.
A8. O( 1 D) + NH3. Sanders et al. [1024] have detected the products NH(a1 ∆ ) and OH formed in the reaction. They report that the yield of NH(a1 ∆ ) is in the range 3–15% of the amount of OH detected. A9. O( 1 D) + CH 4 . The reaction products are (a) CH 3 + OH, (b) CH 3 O or CH 2 OH + H and (c) CH 2 O + H 2 . Lin and DeMore [739] analyzed the final products of N 2 O/CH 4 photolysis mixtures and c oncluded that (a) accounted for about 90% and that CH 2 O and H 2 (c) accounted for about 9%. Addison et al. [9] reported an OH yield of 80%. Casavecchia et al. [202] used a molecu lar beam experiment to observe H and CH 3 O (or CH 2 OH) products. They reported that the yield of H 2 was <25% of the yield of H from (b). Satyapal et al. [1029] observed the production of H atoms in a pulsed laser experiment and reported a yield of H of (25±8)%. Matsumi et al. [791] measured the yields of H and O( 3 P) in low pressure gas mixtures and reported the yield of H was (15±3)% and the yield of O( 3 P) was <5%. Wine and Ravishankara [1318] reported that the yield of O( 3 P) was <4.3%. Takahashi et al. [1146] reported that the O( 3 P) yield is <1%. We recommend the following branching ratios: (a) (75±15)%, (b) (20±7)%, (c) (5±5)%. A10. O( 1 D) + HCl. The recommendation is the average of measurements by Davidson et al. [312] and Wine et al. [1325]. Product studies by the latter indicate: O(3P) + HCl (9±5)%; H + ClO (24±5)%; and OH + Cl (67±10)%. Takahashi et al. [1146] report the O(3P) yield is (15±4)%. A11. O( 1 D) + HF. Rate coefficient and product yield measured by Wine et al. (1984, private communication). The O( 3 P) yield is less than 4%. A12. O( 1 D) + HBr. Rate coefficient and products measured by Wine et al. [1325]. Product yields: HBr + O( 3 P) (20±7)%, H + BrO <4.5%, and OH + Br (80±12)%. A13. O( 1 D) + Cl 2 . Rate coefficient and O( 3 P) product were measured by Wine et al. [1314], who reported Cl 2 + O( 3 P) (25±10)%. Takahashi et al. [1146] reported that the ClO yield is (74±15)%, in excellent agreement. An indirect study by Freudenstein and Biedenkapp [409] is in reasonable agreement on the yield of ClO. A14. O( 1 D) + COCl 2 , COClF and COF 2 . For the reactions of O( 1 D) with COCl 2 and COClF the recommended rate constants are derived from data of Fletcher and Husain [401]. For consistency, the recommended values for these rate constants were derived using a scaling fact or (0.5) which corrects for the difference between rate constants from the Husain laboratory and the recommendations for other O( 1 D) rate constants in this table. The recommendation for COF 2 is from the data of Wine and Ravishankara [1319]. Their result is preferred over the value of Fletcher and Husain [401] because it appears to follow the pattern of d ecreased reactivity with increased fluorine substituti on observed for other halocarbons. These reactions have been studied only at 298 K. Based on consideration of similar O( 1 D) reactions, it is assumed that E/R equals zero, and therefore the value shown for the A-factor has been set equal to k(298 K). A15. O( 1 D) + halocarbons. The halocarbon rate constants are for the total disappearance of O( 1 D) and probably include physical quenching. Products of the reactive channels may include CX 3 O + X, CX 2 O + X 2 (or 2X), and CX 3 + XO, where X = H, F, Cl, or Br in various combinations. Bromine, chlorine and hydrogen are more easily displaced than fluorine from halocarbons. Some values have been reported for the fractions of the total rate of disappearance of O( 1 D) proceeding through physical que nching and reactive channels. For CCl 4 : quenching = (14±6)% and reaction = (86±6)% (Force and Wiesenfeld [405]), ClO yield = (90±19)% (Takahashi et al. [1146]; for CFCl 3 : quenching = (25±10)%, ClO formation = (60±15)% (Donovan, private communication, 1980), ClO yield = (88±18)% (Takahashi et al.); for CF 2 Cl 2 : quenching = (14±7)% and reaction = (86±14)% (Force and Wiesenfeld [405]), quenching = (20±10)%, ClO formation = (55±15)% (Donovan), quenching = (19±5)% and ClO formation = (87±18%) (Takahashi et al.). A16. O( 1 D) + CH 3 Br. The recommendation is based on data fro m Thompson and Ravishankara [1165]. They report that the yield of O( 3 P) from physical quenching is 0±7%. A17. O( 1 D) + CH 2 Br 2 . The recommendation is based on data fro m Thompson and Ravishankara [1165]. They report that the yield of O( 3 P) from physical quenching is (5±7)%. A18. O( 1 D) + CHBr 3 . The recommendation is based on data fro m Thompson and Ravishankara [1165]. The rate coefficient is somewhat large compared to analogous compounds. They report that the yield of O( 3 P) from physical quenching is (32±8)%. A19. O( 1 D) + CH 3 F (HFC-41). The recommendation is the average of m easurements of Force and Wiesenfeld [405] and Schmoltner et al. [1039]. The O( 3 P) product yield was reported to be (25±3)% by Force and Wiesenfeld, (11±5)% by Schmoltner et al., and (19±5)% by Takahashi et al. [1146]. Burks and Lin [175] reported observing vibrationally excited HF as a product. Park and Wiesenfeld [929] observed OH.

### 1-33 A20. O( 1 D) + CH 2 F 2 (HFC-32). The recommendation is based upon the measurement of Schmoltner et al. [1039], who reported that the yield of O( 3 P) is (70±11)%. Green and Wayne [453] measured the loss of CH 2 F 2 relative to the loss of N 2 O. Their value when combined with our recommendation for O( 1 D) + N 2 O yields a rate coefficient for reactive loss of CH 2 F 2 that is about three times the result of Schmoltner et al. Burks and Lin [175] reported observing vibrationally excited HF as a product. A21. O( 1 D) + CHF 3 (HFC-23). The recommendation is the average of m easurements of Force and Wiesenfeld [405] and Schmoltner et al. [1039]. The O( 3 P) product yield was reported to be (77±15)% by Force and Wiesenfeld and (102±3)% by Schmoltner et al. Although physical quenching is the dominant process, detectable yields of vibrationally excited HF have been reported by Burks and Lin [175] and Aker et al. [15], which indicate the formation of HF + CF 2 O products. A22. O( 1 D) + CHCl 2 F (HCFC-21). The recommendation is based upon the measurement by Davidson et al. [311] of the total rate coefficient (physical quenching and r eaction). Takahashi et al. [1146] report the yield of ClO is (74±15)%. A23. O( 1 D) + CHClF 2 (HCFC-22). The recommendation is based upon the measurements by Davidson et al. [311] and Warren et al. [1277] of the total rate coefficient. A measurement of the rate of reaction (halocarbon removal) relative to the rate of reaction with N 2 O by Green and Wayne [453] agrees very well with this value when the O( 1 D) + N 2 O recommendation is used to obtain an absolute value. A relative measurement by Atkinson et al. [41] gives a rate coefficient about a factor of two higher. Addison et al. [9] reported the following product yields: ClO (55±10)%, CF 2 (45±10)%, O( 3 P) (28 +10 or –15)%, and OH 5%, where the O( 3 P) comes from a branch yielding CF 2 and HCl. Warren et al. [1277] also report a yield of O( 3 P) of (28±6)%, which they interpret as the product of physical quenching. A24. O( 1 D) + CClF 3 (CFC-13). The recommendation is based on the measurement by Ravishankara et al.[985] who report (31±10)% physical quenching. Takahashi et al. [1146] report the yields of O( 3 P) (16±5)% and ClO (85±18)%. A25. O( 1 D) + CClBrF 2 (Halon 1211). The recommendation is based on data from Thompson and Ravishankara [1165]. They report that the yield of O( 3 P) from physical quenching is (36±4)%. A26. O( 1 D) + CBr 2 F 2 (Halon 1202). The recommendation is based on data from Thompson and Ravishankara [1165]. They report that the yield of O( 3 P) from physical quenching is (54±6)%. A27. O( 1 D) + CBrF 3 (Halon 1301). The recommendation is based on data from Thompson and Ravishankara [1165]. They report that the yield of O( 3 P) from physical quenching is (59±8)%. Lorenzen-Schmidt et al. [753] measured the Halon removal rate relative to the N 2 O removal rate and report that the rate coefficient for the Halon destruction path is (4.0±0.4) × 10 –11

, which is in excellent agreement with Thompson and Ravishankara. A28. O( 1 D) + CF 4 (CFC-14). The recommendation is based upon the measurement by Ravishankara et al. [985], who report (92±8)% physical quenching. Force and Wiesenfeld [405] measured a quenching rate coefficient about 10 times larger. Shi and Barker [1057] report an upper limit that is consistent with the recommendation. The small rate coefficient for this reaction make s it vulnerable to interference from reactant impurities. For this reason the recommendation should probably be considered an upper limit. A29. O( 1 D) + CH 3 CH 2 F (HFC 161). The recommendation is based on data from Schmoltner et al. [1039]. They report that the yield of O( 3 P) from physical quenching is (18±5)%. A30. O( 1 D) + CH 3 CHF 2 (HFC-152a). The recommendation is based on the measurements of Warren et al. [1277], who report (54±7)% physical quenching. A31. O( 1 D) + CH 3 CCl 2 F (HCFC-141b). The recommendation is based upon the measurement of Warren et al. [1277], who report (31±5)% physical quenching. A32. O( 1 D) + CH 3 CClF 2 (HCFC-142b). The recommendation is based upon the measurement of Warren et al. [1277], who report (26±5)% physical quenching. This agrees very well with Green and Wayne [453], who measured the loss of CH 3 CF 2 Cl relative to the loss of N 2 O, when the recommendation for N 2 O is used. A33. O( 1 D) + CH 3 CF 3 (HFC-143a). The recommendation is based upon the relative rate measurement of Green and Wayne [453], who measured the loss of CH 3 CF 3 relative to the loss of N 2 O. The recommendation for N 2 O is used to obtain the value given. It is assumed that there is no physical quenching, although the reported physical quenching by CH 2 FCF 3 and CH 3 CHF 2 suggests some quenching is possible. A34. O( 1 D) + CH 2 ClCClF 2 (HCFC-132b). The recommendation is based upon the relative rate measurement of Green and Wayne [453], who measured the loss of CH 2 ClCF 2 Cl relative to the loss of N 2 O. The recommendation for N 2 O is used to obtain the value given. It is assumed that there is no physical quenching.

### 1-34 A35. O( 1 D) + CH 2 ClCF 3 (HCFC-133a). The recommendation is based upon the measurement of Warren et al. [1277], who report (20±5)% physical quenching. This agrees with Green and Wayne [453] who measured the loss of CH 2 ClCF 3 relative to the loss of N 2 O, when the recommendation for N 2 O is used. A36. O( 1 D) + CH 2 FCF 3 (HFC-134a). The recommendation is based on the measurement of Warren et al. [1277] who report (94+6/–1)% physical quenching. The predominance of physical quenching is surprising, considering the presence of C–H bonds, which are usually reactive toward O( 1 D) . A37. O( 1 D) + CHCl 2 CF 3 (HCFC-123). The recommendation is based upon measurements by Warren et al. [1277]. The relative rate measurement of Green and Wayne [453], who measured the loss of CHCl 2 CF 3 relative to the loss of N 2 O, agrees well with the recommenda tion when the recommendation for N 2 O is used. Warren et al. report (21 ± 8)% physical quenching. A38. O( 1 D) + CHClFCF 3 (HCFC-124). The recommendation is based upon the measurement of Warren et al. [1277], who report (31 ± 10)% physical quenching. A39. O( 1 D) + CHF 2 CF 3 (HFC-125). The recommendation is based upon the measurement of Warren et al. [1277], who report (85+15/–22)% physical quenching. Green and Wayne [453] measured the loss of CHF 2 CF 3 relative to the loss of N 2 O and report a loss corresponding to about 40% of the recommended rate coefficient. This reaction is much faster than one would predict by analogy to similar compounds, such as CH 2 FCF 3 . A40. O( 1 D) + CCl 3 CF 3 (CFC-113a). The recommendation is an estimate based on analogy to similar compounds. A41. O( 1 D) + CCl 2 FCClF 2 (CFC-113). The recommendation is an estimate based on analogy to similar compounds. A42. O( 1 D) + CCl 2 FCF 3 (CFC-114a). The recommendation is an estimate based on analogy to similar compounds. A43. O( 1 D) + CClF 2 CClF 2 (CFC-114). The recommendation is based on the measurement by Ravishankara et al. [985], who report (25 ± 9)% physical quenching. A44. O( 1 D) + CClF 2 CF 3 (CFC-115). The recommendation is based on the measurement by Ravishankara et al.[985], who report (70 ± 7)% physical quenching. A45. O( 1 D) + CBrF 2 CBrF 2 (Halon 2402). The recommendation is based on data from Thompson and Ravishankara [1165]. They report that the yield of O( 3 P) from physical quenching is (25±7)%. Lorenzen-Schmidt et al. [753] measured the Halon removal rate relative to the N 2 O removal rate and report that the rate coefficient for the Halon destruction path is (8.8 ± 1.2) × 10 –11, in fair agreement with the result of Thompson and Ravishankara. A46. O( 1 D) + C 2 F 6 (CFC-116). The recommendation is based on a measurement by Ravishankara et al. [985], who report (85 ± 15)% physical quenching. The small rate coefficient for this reaction makes it vulnerable to interference from reactant impurities. For this reason the recommendation should probably be considered an upper limit. A47. O( 1 D) + CHF 2 CF 2 CF 2 CHF 2 (HFC 338 pcc). The recommendation is based on data from Schmoltner et al. [1039]. They report that the yield of O( 3 P) from physical quenching is (97 ± 9)%. A48. O( 1 D) + c-C 4 F 8 . The recommendation for perfluorocyclobutane is based upon the measurement by Ravishankara et al. [985], who report (100 +0 /–15)% physical quenching. The small rate coefficient for this reaction makes it vulnerable to in terference from reactant impurities. For this reason the recommendation should probably be considered an upper limit. A49. O( 1 D) + CF 3 CHFCHFCF 2 CF 3 (HFC 43-10 mee). The recommendation is based on data from Schmoltner et al. [1039]. The rate coefficients for this compound and CHF 2 CF 3 do not follow the reactivity trend of other HFCs. Schmoltner et al. report that the yield of O( 3 P) from physical quenching is (91±4)%. A50. O( 1 D) + C 5 F 12 (CFC 41-12). The recommendation is based on data from Ravishankara et al. [985]. They report that the yield of O( 3 P) from physical quenching is (79±12)%. A51. O( 1 D) + C 6 F 14 (CFC 51-14). The recommendation is based on data from Ravishankara et al. [985]. They report that the yield of O( 3 P) from physical quenching is (75±9)%. A52. O( 1 D) + 1,2-(CF 3 ) 2 c-C 4 F 6 . The recommendation is based on data from Ravishankara et al. [985]. They report that the yield of O( 3 P) from physical quenching is (84±16)%. A53. O( 1 D) + SF 6 . The recommendation is based upon measurements by Ravishankara et al. [985] who report (32±10)% physical quenching. The small rate coefficient for this reaction makes it vulnerable to interference from reactant impurities. For this reason the recommendation should probably be considered an upper limit.

A54. O 2 ( 1 ∆ ) + O. The recommendation is based on the upper limit reported by Clark and Wayne [232].

### 1-35 A55. O 2 ( 1 ∆ ) + O 2 . The recommendation is the average of eight r oom temperature measurements: Steer et al. [1108], Findlay and Sn elling [392], Borrell et al. [ 140], Leiss et al. [706], T achibana and Phelps [1140], Billington and Borrell [127], Raja et al. [977], and Wildt et al. [1306]. The temperature dependence is derived from the data of Findlay and Snelling and Billington and Borrell. Several other less direct measurements of the rate coefficient agree with the recommendation, including Clark and Wayne [231], Findlay et al. [391], and McLaren et al. [797]. Wildt et al. [1307] report observations of weak emissions in the near IR due to collision-induced radiation. Wildt et al. [1308] give rate coefficients for this process.

A56. O 2 ( 1 ∆ ) + O 3 . The recommendation is the average of the room temperature measurements of Clark et al. [230], Findlay and Snelling [393] , Becker et al. [95], and Collins et al. [266]. Several less direct measurements agree well with the recommendation (McNeal and Cook [798] , Wayne and Pitts [1290], and Arnold and Comes [30]). The temperature dependence is from Findlay and Sn elling and Becker et al ., who agree very well, although both covered a relatively small temperature range. An earlier study by Clark et al. covered a much larger range, and found a much smaller temperature coefficient. The reason for this discrepancy is not clear. The yield of O + 2O 2 products appears to be close to unity, based on many studies of the quantum yield of O 3 destruction near the peak of the Hartley band. For example, measurements of the number of O 3 molecules destroyed per photon absorbed: Von Ellenrieder et al. [1237], Ravishankara et al. [991], Lissi and Heicklen [746], and references cited therein and measurements of O 3 loss and O atom temporal profiles in pulsed experiments Klais et al. [633] and Arnold and Comes [30]. Anderson et al. [26] report that the rate coefficient for atom exchange between O 2 ( 1 ∆ ) and O 3 is < 5×10 –16 at 300 K.

A57. O 2 ( 1 ∆ ) + H 2 O. The recommendation is the average of the measur ements reported by Beck er et al. [94] and Findlay and Snelling [392]. An earlier study by Clark and Wayne [231] reported a value about three times larger.

A58. O 2 ( 1 ∆ ) + N. The recommendation is an upper limit based upon the measurement reported by Westenberg et al. [1301], who used ESR to detect O 2 (X 3 Σ and a 1 ∆ ), O( 3 P) and N( 4 S) with a discharge flow reactor. They used an excess of O 2 ( 1 ∆ ) and measured the decay of N and the appearance of O at 195 and 300 K. They observed that the reaction of N with O 2 ( 1 ∆ ) is somewhat slower than its reaction with O 2 ( 3 Σ ). The recommended rate constant value for the latter provides the basis for the recommendation. Clark and Wayne [232,233] and Schmidt and Schiff [1036] reported observations of an O 2 ( 1 ∆ ) reaction with N that is about 30 times faster than the recommended limit. Schmidt and Schiff attribute the observed loss of O 2 ( 1 ∆ ) in excess N to a rapid energy exchange with some constituent in discharged nitrogen, other than N.

A59. O 2 ( 1 ∆ ) + N 2 . The recommendation is based upon the measurements by Findlay et al. [391] and Becker et al. [94]. Other studies obtained higher values for an upper limit: Clark and Wayne [231] and Steer et al. [1108].

A60. O 2 ( 1 ∆ ) + CO 2 . The recommendation is based on the measurements reported by Findlay and Snelling [392] and Leiss et al. [706]. Upper limit rate coefficients reported by Becker et al. [94], McLaren et al. [797], and Singh et al. [1074] are consistent with the recommendation.

A61. O 2 ( 1 ∆ ) + O. The recommendation is based on the measurement reported by Slanger and Black [1088].

A62. O 2 ( 1 ∆ ) + O 2 . The recommendation is the average of values reported by Martin et al. [788], Lawton et al. [686], and Lawton and Phelps [687], who are in excellent agreement. Measurements by Thomas and Thrush [1164], Chatha et al. [214], and Knickelbein et al. [639] are in reasonable agreement with the recommendation. Knickelbein et al. report an approximate unit yield of O 2 ( 1 ∆ ) product.

A63. O 2 ( 1 ∆ ) + O 3 . The recommendation is based upon the room temperature measurements of Gilpin et al. [439], Slanger and Black [1088], Choo and Leu [229], and Shi and Barker [1057]. Measurements by Snelling [1096], Amimoto and Wiesenfeld [19], Ogren et al. [903], and Turnipseed et al. [1208] are in very good agreement with the recommendation. The temperature dependence is derived from the results of Choo and Leu. The yield of O + 2O 2 products is reported to be (70±20)% by Sl anger and Black and Amimoto and Wiesenfeld.

A64. O 2 ( 1 ∆ ) + H 2 O. The recommendation is the average of room temp erature measurements reported by Stuhl and Niki [1127], Filseth et al. [390], Wildt et al. [1306], and Shi and Barker [1057]. These data cover a range of about a factor of two. Measurements reported by O'Brien and Myers [902], Derwent and Thrush [342], and Thomas and Thrush [1164] are in good agreement with the recommendation. Wildt et al. [1306] report that the yield of O 2 ( 1 ∆ ) ≥ 90%.

A65. O 2 ( 1 ∆ ) + N. The recommendation is based on the limit reported by Slanger and Black [1088].

### 1-36 A66. O 2 ( 1 ∆ ) + N 2 . The recommendation is the average of measurements reported by Izod and Wayne [566], Stuhl and Welge [1130], Filseth et al. [390], Martin et al. [788], Kohse-Höinghaus and Stuhl [646], Choo and Leu [229], Wildt et al. [1306], and Shi and Barker [1057]. Less direct measurements reported by Noxon [901], Myers and O'Brien [843], and Chatha et al. [214] are consistent with the recommendation. Kohse-Höinghaus and Stuhl observed no significant temperature dependence over the range 203–349 K.

A67. O 2 ( 1 ∆ ) +CO 2 . The recommendation is the average of measurements reported by Filseth et al. [390], Davidson et al. [310], Avilés et al. [51], Muller and Houston [840], Choo and Leu [229], Wildt et al. [1306], and Shi and Barker [1057] at room temperature. The temperature dependence is from the work of Choo and Leu. Muller and Houston and Singh and Setser [1075] give evidence that O 2 ( 1 ∆ ) is a product. Wildt et al. report that the yield of O 2 ( 1 ∆ ) ≥ 90%.

B1. O + OH. The rate constant for O + OH is a fit to three temperature dependence studies: Westenberg et al. [1300], Lewis and Watson [727], and Howard and Smith [532]. This recommendation is consistent with earlier work near room temperature as reviewed by Lewis and Watson [727] and with the measurements of Brune et al. [160]. The ratio k(O + HO 2 )/k(O + OH) measured by Keyser [621] agrees with the rate constants recommended here.

B2. O + HO 2 . The recommended values are based on the results of studies over a range of temperatures by Keyser [620] and Nicovich and Wine [871] and the room temperature studies of Sridharan et al. [1099], Ravishankara et al. [991], and Brune et al. [160]. Earlier studies by Hack et al. [467] and Burrows et al. [176,179] are not considered, because the OH + H 2 O 2 reaction was important in these studies and the value used for its rate constant in their analyses has been shown to be in error. Data from Ravishankara et al. [991] at 298 K show no dependence on pressure between 10 and 500 torr N 2 . The ratio k(O + HO 2 )/k(O + OH) measured by Keyser [621] agrees with the rate constants recommended here. Sridharan et al. [1097] showed that the reaction products correspond to abstraction of an oxygen atom from HO 2 by the O reactant. Keyser et al. [625] reported <1% O 2 ( 1 ∆ ) yield.

B3. O + H 2 O 2 . There are two direct studies of the O + H 2 O 2 reaction: Davis et al. [320] and Wine et al. [1316]. The recommended value is a f it to the combined data. Wine et al. suggest that the earlier measurements may be too high because of secondary chemistry. The A-factor for both data sets is quite low compared to similar atom-molecule reactions. An indirect measurement of the E/R by Roscoe [1006] is consistent with the recommendation.

B4. H + O 3 . The recommendation is an average of the results of Lee et al. [693] and Keyser [616], which are in excellent agreement over the 200–400 K range. An earlier study by Clyne and Monkhouse [251] is in very good agreement on the T dependence in the range 300–560 K but lies about 60% below the recommended values. Although we have no reason not to believe the Clyne and Monkhouse values, we prefer the two studies that are in excellent agreemen t, especially since they were carri ed out over the T range of interest. Results by Finlayson-Pitts and Kleindienst [397] agree well w ith the present recommendations. Reports of a channel forming HO 2 + O (Finlayson-Pitts and Kleindienst [397] : ~25%, and Force and Wiesenfeld [406]: ~40%) have been contradict ed by other studies (How ard and Finlayson-Pitts [ 531]: <3%; Washida et al. [1280]: <6%; Finlayson-Pitts et al . [398]: <2%; and Dodonov et al. [357] : <0.3%). Secondary chemistry is believed to be responsible for the observed O-atoms in this system. Washida et al. [1281] measured a low limit (<0.1%) for the production of singlet molecular oxygen in the reaction H + O 3 . B5. H + HO 2 . There are five studies of this reaction: Hack et al. [471], Hack et al. [469], Thrush and Wilkinson [1171], Sridharan et al. [1099] and Keyser [623]. Related early work and combustion studies are referenced in the Sridharan et al. paper. All five studies used discharge flow systems. It is difficult to obtain a direct measurement of the rate constant for this reaction because both reactants are radicals and the products OH and O are very reactive toward the HO 2 reactant. The recommendation is based on the data of Sridharan et al. and Keyser because their measurements were the most direct and required the fewest corrections. The other measurements, (5.0±1.3) × 10 –11 cm 3 molecule –1 s –1 by Thrush and Wilkinson [1171] and (4.65±1) × 10 –11 by Hack et al. [469] are in reasonable agreement with the recommended value. Three of the studies reported the product channels: (a) 2OH, (b) H 2 O + O, and (c) H 2 + O 2 . Hack et al. [471] k a /k = 0.69, k b /k = 0.02, and k c /k = 0.29; Sridharan et al. [1099] k a /k = 0.87±0.04, k b /k = 0.02±0.02, k c /k = 0.09±.045; and Keyser [623] k a /k = 0.90±0.04, k b /k = 0.02±0.02, and k c /k = 0.08±0.04. Hislop and Wayne [511], Keyser et al. [625], and Michelangeli et al. [825] reported on the yield of O 2 (b 1 Σ ) formed in channel (c) as (2.8±1.3) × 10 –4

, <8 × 10 –3 , and <2.1 × 10 –2 respectively of the total reactions. Keyser found the rate coefficient and product yields to be independent of temperature for 245 < T < 300 K.

B6. OH + O 3

. Recommended values are based on the results of st udies over a range of temperatures by Anderson and Kaufman [23], Ravishankara et al. [990], Smith et al. [1091] and Nizkorodov et al. [895] and the room

### 1-37 temperature measurements of Kurylo [660], Zahniser and Howard [1353], and Kulcke et al. [655]. The recommended E/R and k(298 K) values are based on aver ages of the individual E/R and k(298 K) values obtained in the above-mentioned studies. The values reported by Kulcke et al. [655] and Nizkorodov et al. [899] have been corrected for a minor contribution from k(HO 2 + O 3 ).

B7. OH + H 2 . The OH + H 2 reaction has been the subject of numerous studies (see Ravishankara et al. [983] for a review of experimental and theoretical work). The recommendation is fixed to the average of nine studies at 298 K: Greiner [457], Stuhl and Niki [1129], Westenberg and de Haas [1298], Smith and Zellner [1093], Atkinson et al. [43], Overend et al. [923], Tully and Ravishankara [1198], Zellner and Steinert [1360], and Ravishankara et al. [983]. Results reported by Talukdar et al. [1153] are in excellent agreement. B8. OH + HD. The recommendation is based on direct measurements made by Talukdar et al. [1153] using pulsed photolysis-laser induced fluorescence over the temperature range 248–418 K. The recommendation is in excellent agreement with the ratio k(OH + H 2 )/k(OH + HD) = 1.65±0.05 at 298 K reported by Ehhalt et al. [375] when combined with the recommended k(OH + H 2 ).

B9. OH + OH. The recommendation for the OH + OH reaction is the average of six measurements near 298 K: Westenberg and de Haas [1297], McKenzie et al. [ 796], Clyne and Down [240], Trainor and von Rosenberg [1185], Farquharson and Smith [384] , and Wagner and Zellner [1239]. The rate constants for these studies all fall between (1.4 and 2.3) × 10 –12 cm 3 molecule –1 s –1

. The temperature dependence is from Wagner and Zellner, who reported rate constants for the range T = 250–580 K.

B10. OH + HO 2 . A study by Keyser [624] appears to resolve a discrepancy among low-pressure discharge flow experiments that all gave ra te coefficients near 7 × 10 –11 cm 3 molecule –1 s –1 : Keyser [619], Thrush and Wilkinson [1170], Sridharan et al. [1098,1100], Temps and Wagner [1160], and Rozenshtein et al. [1010], and atmospheric pressure studies that gave rate coefficients near 11 × 10 –11 : Lii et al. [735], Hochanadel et al. [517], DeMore [329], Cox et al. [278], Burrows et al. [178], and Kurylo et al. [666]. Laboratory measurements using a discharge flow experiment and a chemical model analysis of the results by Keyser [624] demonstrate that the previous discharge flow m easurements were probably subject to interference from small amounts of O and H. In the presence of excess HO 2 these atoms generate OH and result in a rate coefficient measurement that falls below the true value. The temperature dependence is from Keyser [624], who covered the range 254 to 382 K. A flow tube study by Schwab et al. [1043] reported k = (8.0 +3/–4) × 10 –11

. These workers measured th e concentrations of HO 2 , OH, O, and H and used a computer model of the relevant reactions to test for interference. A flow tube study by Dransfeld and Wagner [365] employing an isotope labelled 18 OH reactant obtained k = (11±2) × 10 –11 in good agreement with the recommendation. They attributed about half of the reactive events to isotope scrambling because control experiments with 16 OH gave k = 6 × 10 –11

. It should be noted that their control experiments were subject to the errors described by Keyser [624] due to the presence of small amounts of H and O, whereas their 18 OH measurements were not. Kurylo et al. [666] found no evidence of significant scrambling in isotope studies of the OH and HO 2 reaction. An additional careful study of the reaction temperature dependence would be useful. Hippler and Troe [509] have anal ysed data for this reaction at temperatures up to 1250 K. In summary, this has historically been a difficult reaction to study. Earlier problems appear to have been resolved, as discusse d above, and results now tend to converge on a central value, but the recommended value is still subject to a large uncertainty.

B11. OH + H 2 O 2

. The recommendation is a fit to the temperature dependence studies of Keyser [618], Sridharan et al. [1101], Wine et al. [1320], Kurylo et al. [670], and Vaghjiani et al. [1224]. The data from these studies have been revised to account for the H 2 O 2 UV absorption cross section recommendations in this evaluation. The first two references contain a discussion of some possible reasons for the discrepancies with earlier work and an assessment of the impact of the new value on other kinetic studies. All of these measurements agree quite well and overlap one another. Measurements by Lamb et al. [676] agree at room temperature but indicate a quite different temperature dependence with k increasing slightly with decreasing temperature. Their data were not incorporated in the fit. Measurements at room temper ature by Marinelli and Johnston [781] and Turnipseed et al. [1208] agree well with the recommendation. Hippler and Troe [509] have analysed data for this reaction at temperatures up to 1250 K.

B12. HO 2 + O 3

. The recommended values are based on results of st udies over a range of temperatures by DeMore [327] at 231 to 334 K, Zahniser and Howard [1353] at 245 to 365 K, Manzanares et al. [772] at 298 K, Sinha et al. [1084] at 243 to 413 K, Wang et al. [1275] at 233 to 400 K and Herndon et al. [501] at 200 to 298 K. The data of Simonaitis and Heickl en [1069] and DeMore and Tschuikow-Roux [338] were not considered. The temperature dependence studies show varying degrees of curvature in the Arrhen ius plots, with the E/R decreasing at lower temperature. This is especially evident in the low temperature data of Herndon et al

### 1-38 where a number of measures were taken to control potential kinetic complications. The recommended E/R and k(298 K) values are based on averages of the individual E/R and k(298 K) values. Furthermore, only data at temperatures less than 298 K were used for the E/ R determination, accordingly the recommendation is not valid for T>298 K. Additional temperature dependence data are needed for this reaction over a larger range to more fully characterize the non-linear behavior of the rate constant. The mechanism of the reaction has been studied using 18 O labelled HO 2 by Sinha et al. [1084], who reported that the reaction occurs 75±10% via H atom transfer at 297 K and by Nelson and Zahniser [851], who reported branching ratios for H transfer vs O transfer over the range 226–355 K. They report that the H atom transfer decreases from 94±5% at 226±11 K to 88±5% at 355±8 K.

B13. HO 2 + HO 2

. Two separate expressions are given for the rate constant for the HO 2 + HO 2 reaction. The effective rate constant is given by the sum of these two equations. This reaction has been shown to have a pressure-independent bimolecular component and a pressure-dependent termolecular component. Both components have negative temperature coefficients. The bimolecular expression is obtained from data of Cox and Burrows [277], Thrush and Tyndall [1167,1168], Kircher and Sander [627] , Takacs and Howard [1144,1145], Sander [1016] and Kurylo et al. [672]. Data of Rozenshtein et al. [1010] are consistent with the low pressure recommendation, but they report no change in k with pressure up to 1 atm. Results of Thrush and Wilkinson [1169] and Dobis and Benson [355] are inconsistent with the recommendation. The termolecular expression is obtained from data of Sander et al. [1021], Simonaitis and Heicklen [1071], and Kurylo et al. [672] at room temperature and Kircher and Sander [627] for the temperature dependence. This equation applies to M = air. On this reaction system there is general agreement among investigators on the following aspects of the reaction at high pressure (P ~1 atm): (a) the HO 2 UV absorption cross section: Paukert and Johnston [934], Cox and Burrows [277], Hochanadel et al. [517], Sander et al. [1021], Kurylo et al. [673], and Crowley et al. [295]; (b) the rate constant at 300K: Paukert and Johnston [934], Hamilton and Lii [476], Cox and Burrows [277], Lii et al. [734], Tsuchiya and Nakamura [1190], Sander et al. [1021], Simonaitis and Heicklen [1071], Kurylo et al. [672], Anderss on et al. [27], and Crow ley et al. [295] (all values fall in the range (2.5 to 4.7) × 10 –12 cm 3 molecule –1 s –1 ); (c) the rate constant temperature dependence: Cox and Burrows [277], Lii et al. [734], and Kircher and Sander [627]; (d) the rate constant water vapor dependence: Hamilton [475], Hochanadel et al. [516], Hamilton and Lii [476], Cox and Burrows [277], DeMore [327], Lii et al. [736], Sander et al. [1021], a nd Andersson et al. [27]; (e) the H/D isotope effect: Hamilton and Lii [476] and Sander et al. [1021]; and (f) the formation H 2 O 2 + O 2 as the major products at 300 K: Su et al. [1133], Niki et al. [887], Sander et al. [1021], and Simonaitis and Heicklen [1071]. Sahetchian et al. [1014,1015] give evidence for the formation of a small amount of H 2 (~10%) at temperatures near 500 K, but Baldwin et al. [58] and Ingold [560] give evidence that the yield must be much less. Glinski and Birks [445] report an upper limit of 1% H 2 yield at a total pressure of about 50 torr and 298 K, but their experiment may have interference from wall reactions. A smaller limit to H 2 production (0.01%) was later determined in the same laboratory (Stephens et al. [1112]). For systems containing water vapor, the multiplicative factor given by Lii et al. [736] and Kircher and Sande r [627] can be used: 1 + 1.4 × 10 –21 [H 2 O] exp(2200/T). Lightfoot et al. [732] reported atmospheric pressure measurements over the temperature range 298–777 K that are in agreement with the recommended value at room temperature but indicate an upward curvature in the Arrhenius pl ot at elevated temperature. A high temperature study by Hippler et al. [510] confirms the strong curvature.

C1. O + NO 2 . The recommended values are based on the results of studies over a range of temperatures by Gierczak et al. [428], Ongstad and Bi rks [909], Slanger et al . [1089] and Geers-Mulle r and Stuhl [425] and the room temperature study of Paulson et al. [935]. In the most recent study of Gierczak et al. [428], special emphasis was placed on accurate measurement of the NO 2 concentration and on measurements at low temperatures. The results of earlier studies by Davis et al. [315] and Bemand et al. [110] were not used in deriving the recommended values either because of possible complications from decomposition of NO 2 at higher temperatures or lack of direct NO 2 detection.

C2. O + NO 3 . Based on the study of Graham and Johnston [451] at 298 K and 329 K. While limited in temperature range, the data indicate no temperature dependence. Furthermore, by analogy with the reaction of O with NO 2 , it is assumed that this rate constant is independent of temperature. Clearly, temperaturedependence studies are needed.

C3. O + N 2 O 5 . Based on Kaiser and Japar [600].

C4. O + HNO 3 . The upper limit reported by Chapman and Wayne [212] is accepted.

C5. O + HO 2 NO 2 . The recommended value is based on the study of Chang et al. [211]. The large uncertainty in E/R and k at 298 K are due to the fact that the recommendation is based on a single study.

### 1-39 C6. H + NO 2 . The recommended value of k 298 is derived from the studies of Wagner et al. [1241], Bemand and Clyne [108], Clyne and Monkhouse [251], Michael et al. [820] and Ko and Fontijn [644]. The temperature dependence is from the studies of Wagner et al. and Ko and Fontijn. The data from Wategaonkar and Setser [1284] and Agrawalla et al. [14] were not considered.

C7. OH + NO 3 . The recommendation is derived from an average of the results of Boodaghians et al. [137], Mellouki et al. [806], Becker et al. [91] and Mellouki et al. [809]. There are no temperature dependence data. The reaction products are probably HO 2 + NO 2 . C8. OH + HONO. The recommended rate expression is derived fro m the work of Jenkin and Cox [577], which supersedes the earlier room temperature study of Cox et al. [284]. Recent results from the Ravishankara group [173] suggest that the r eaction may have a small negative temperature dependence.

C9. OH + HNO 3

. The recent study of Brown et al. [159] furn ishes the most comprehensive set of rate
measurements for N 2 as the bath gas over a significant range of temperature (200–350 K) and pressure (20– 500 torr). They analyzed their results in terms of the mechanism proposed by Smith et al. [1091], involving the formation of a bound, relatively long-lived HO·HNO 3 complex, as well as the direct reaction channel. Studies of the effects of isotopi c substitution on the reactions OD+DNO 3 , OH+DNO 3 , OD+HNO 3 and

18 OH+HNO 3 . by Brown et al. [158] support this mechanism and suggest that the structure of the intermediate consists of a H-bonded six-membered ring. Thus, the P dependence can be represented by combining a low pressure (bimolecular) limit, k 0 , with a Lindemann-Hinshelwood expression for the p-dependence:

3

o 3

2 

### k [M] k([M],T)=k k [M] 1+ k + 14

o

17 2

34 3 

### k 2.4x10 exp(460/T) k 2.7x10 exp(2199 / T) k 6.5x10 exp(1335/T) −

−

− 

###  

=  

=    

=  

The coefficients k 3 and k 2 are the termolecular and high pressure limits for the “association” channel. The value of k at high pressures is the sum k 0 + k 2 . This expression for k([M],T) and the valu es of the Arrhenius parameters for k 0 , k 2 , and k 3 derived by Brown et al. [159] for N 2 as the bath gas constitute the recommended values for this rate coefficient. These recommended values are derived from a fit to the data of Brown et al. [159], Stachnik et al. [1103], Devolder et al. [343] and Margitan and Watson [776]. The reaction yield of NO 3 (per OH removed) is assumed to be unity at all temperatures for either reaction channel. These assumptions are supported by the isotopic studies of Brown et al. [158] and the theoretical calculations of Xia and Lin [1338].

C10. OH + HO 2 NO 2 . The recommendation for both k at 298 K and the Arrhenius expression is based upon the data of Trevor et al. [1186], Barnes et al. [64], C. A. Smith et al. [1091] and Barnes et al. [66]. Trevor et al. studied this reaction over the temperature range 246–324 K and reported a temperature invariant value of 4.0 × 10 –12 cm 3 molecule –1 s –1 , although a weighted least squares fit to their data yields an Arrhenius expression with an E/R value of (193±193) K. In contrast, Smith et al. studied the reaction over the temperature range 240–300 K and observed a negative te mperature dependence with an E/R value of –(650±30) K. The early Barnes et al. study [64] was carried out only at room temperature and 1 torr total pressure while their later study was performed in the pressure range 1–300 torr N 2 and temperature range 268–295 K with no rate constant variation being observed. In addition, k 298 derived in Barnes et al. [64] was revised upward in the later study from 4.1 × 10 –12 to 5.0 × 10 –12 due to a change in the rate constant for the reference reaction. The values of k at 298 K from the four studies are in excellent agreement. An unweighted least squares fit to the data from the above-mentione d studies yields the recommended Arrhenius expression. The less precise value for k at 298 K reported by Littlej ohn and Johnston [747] is in fair agreement with the recommended value. The error limits on the recommended E/R are su fficient to encompass the results of both Trevor et al. and Smith et al. It should be noted that the values of k at 220 K deduced from the two studies differ by a factor of 2. Clearly, additional studies of k as a function of temperature and the identification of the reaction products are needed.

C11. OH + NH 3 . The recommended value at 298 K is the average of the values reported by Stuhl [1125], Smith and Zellner [1094], Perry et al. [943], Silver and Kolb [1061], Stephens [1111] and Diau et al. [346]. The values reported by Pagsberg et al. [925] and Cox et al. [ 283] were not considered because these studies involved the analysis of a complex mechanism and the results are well outside the error limits implied by the above six direct studies. The results of Kurylo [660] and Hack et al. [465] were not considered because of their large discrepancies with the other direct studies (factors of 3.9 and 1.6 at room temperature, respectively). Because the Arrhenius plot disp lays considerable curvature, the temperature dependence is

### 1-40 based only on the data below 300 K, i.e., the studies of Smith and Zellner [1094] and Diau et al. [346], and the A-factor has been sel ected to fit the recommended room temperature value.

C12. HO 2 +NO. The recommendation for HO 2 + NO is based on the average of eight measurements of the rate constant at room temperature and below: Howard and Evenson [530], Leu [713], Howard [527], GlaschickSchimpf et al. [440], Hack et al. [468], Thrush and Wilkinson [1170] and Jemi-Alade Thrush [574], and Seeley et al. [1047]. All of these are in quite good agreement. The results of Imamura and Washida [559] were not considered due to the relatively large uncertainty limits reported in this study. An earlier study, Burrows et al. [176] has been disr egarded because of an error in th e reference rate constant, k(OH + H 2 O 2 ). The room temperature study of Rozenshtein et al. [1010] has also been disregarded due to an inadequate treatment of possible secondary reactions. The recommended Arrhenius paramete rs are obtained from a fit to all the data. The recommended value of k(298 K) is obtained from the Arrhenius line.

C13. HO 2 + NO 2 . Tyndall et al. [1212] obtained an upper limit to the rate coefficient of 5 × 10 –16 cm 3 molecule –1

s –1 based on static photolysis experiments with FTIR analysis at 296 K and 760 torr of N 2 . C14. HO 2 + NO 3 . The recommendation for k 298 is based on a weighted average of the data of Hall et al. [473], Mellouki et al. [806], Becker et al. [91] and Mellouki et al. [809]. There are insufficient data on which to base the temperature dependence of the rate coefficient. The measured branching ratios for the OH + NO 2 + O 2 channel range from 0.57 to 1.0. The most direct measurement is derived from the study of Mellouki et al. [809], which obtained a value of 1.0 +0.0/–0.3 at 298 K

. C15. HO 2 + NH 2 . There is a fairly good agreement on the value of k at 298 K between the direct study of Kurasawa and Lesclaux [659] and the relative studies of Cheskis and Sarkisov [225] and Pagsberg et al. [925]. The recommended value is the average of th e values reported in these three studies. The identity of the products is not known; however, Kura sawa and Lesclaux suggest that th e most probable reaction channels give either NH 3 + O 2 or HNO + H 2 O as products.

C16. N + O 2 . The recommended expression is derived from a least squares fit to the data of Kistiakowsky and Volpi [629], Wilson [1310], Becker et al. [93], Westenberg et al. [1301], Clark and Wayne [233], Winkler et al. [1328] and Barnett et al. [74]. k(298 K) is derived from the Arrhenius expression and is in excellent agreement with the average of all of the room temperature determinations.

C17. N + O 3 . The recommendation is based on the results of Barnett et al. [74]. The value of (1.0±0.2) × 10 –16 cm 3 molecule –1 s –1 reported by Barnett et al. should probably be considered an upper limit rather than a determination. The low values reported by Barnett et al., Stief et al. [1121] and Garvin and Broida [423] cast doubt on the much faster rates reported by Phillip s and Schiff [948], and Ch en and Taylor [221].

C18. N + NO. The recommended temperature dependence is based on the discharge flow-resonance fluorescence studies of Wennberg and Anderson [1293], and the discharge flow-resonance fluorescence and flash photolysis-resonance fluorescence studies of Lee et al. [695]. There is relatively poor agreement between these studies and the results of Clyne and McDerm id [248], Kistiakowsky and Volpi [630], Herron [502], Phillips and Schiff [948], Lin et al. [ 741], Ishikawa et al. [ 563], Sugawara et al. [1134], Cheah and Clyne [215], Husain and Slater [549], Clyne and Ono [255], Brunning and Clyne [161] and Jeoung et al. [587].

C19. N + NO 2 . The recommendation for k 298 is from the discharge flow-resonance fluorescence study of Wennberg and Anderson [1293]. The la tter study had significantly better sensitivity for N( 4 S) than the discharge flowresonance fluorescence study of Clyne and Ono [255], which obtained a value about four times smaller. The results of Husain and Slater [549] and Clyne and McDermid [248] are not considered. The temperature dependence is obtained from the study of Wennberg a nd Anderson. In the latter study, atomic oxygen was shown to be the principal reaction product, in agreement with Clyne and McDermid. A recent study by Iwata et al. [564] suggested an upper limit of 3.3 × 10 –13 cm 3 molecule –1 s –1 for the corresponding reaction involving N( 2 D) and N( 2 P) atoms (sum of all reaction channels).

C20. NO + O 3

. The recommended values are based on the results of studies over a range of temperatures by Birks et al. [129], Lippmann et al. [743], Ray and Watson [997], Michael et al. [814], Borders and Birks [139] and Moonen et al. [833] and the room temperature studies of Stedman and Niki [1105] and Bemand et al. [110]. The six temperature-dependent studies were given e qual weighting in the recommendation by averaging over the E/R’s from each individual data set. Following the Moonen et al

. recommendation, the 200-K data point from their study has been excluded from the fit. All of the temperature dependence studies show some curvature in the Arrhenius plot at temperatures below 298 K. Increasing scatter between the data sets is evident at the lower temperatures. Clough and Thrush [236], Birks et al., Schurath et al. [1042], and Michael et al. have reported individual Arrhenius parameters for the two primary reaction channels producing ground and excited molecular oxygen.

### 1-41 C21. NO + NO 3 . The recommendation is based on the studies of Hammer et al. [477], Sander and Kircher [1020] and Tyndall et al. [1213], which are in excellent agreement.

C22. NO 2 + O 3 . The recommended expression is derived from a least s quares fit to the data of Davis et al. [318], Graham and Johnston [450], Huie and Herron [543], and Cox and Coker [279]. The data of Verhees and Adema [1228] and Stedman and Niki [1105] were not considered because of systematic discrepancies with the other studies.

C23. NO 2 + NO 3 . The existence of the reaction channel forming NO + NO 2 + O 2 has not been firmly established. However, studies of N 2 O 5 thermal decomposition that monitor NO 2 (Daniels and Johnston [304]; Johnston and Tao [591]; Cantrell et al . [196]) and NO (Hjorth et al . [512], and Cantrell et al. [199]) require reaction(s) that decompose NO 3 into NO + O 2 . The rate constant from the first three studies is obtained from the product kK eq , where K eq is the equilibrium constant for NO 2 + NO 3 → N 2 O 5 , while for the latter two studies the rate constant is obtained from the ratio k/k(NO + NO 3 ), where k(NO + NO 3 ) is the rate constant for the reaction NO + NO 3 → 2NO 2 . Using K eq and k(NO + NO 3 ) from this evaluation, the rate expression that best fits the data from all five studies is 4.5 × 10 –14 exp (–1260/T) cm 3 molecule –1 s –1 with an overall uncertainty factor of 2.

C24. NO 3 + NO 3 . . The recommendation for k(298 K) is from the studies of Graham and Johnston [451] and Biggs et al. [123]. The temperature dependence is from Graham and Johnston.

C25. NH 2 + O 2 . This reaction has several product channels which are energetically possible, including NO + H 2 O and HNO + OH. With the exception of the studies of Hack et al. [464] and Jayanty et al. [572] and several studies at high temperature, th ere is no evidence for a reaction. The following upper limits have been measured (cm 3 molecule –1 s –1 ): 3 × 10 –18 (Lesclaux and Demissy [708]), 8 × 10 –15 (Pagsberg et al. [925]), 1.5 × 10 –17 (Cheskis and Sarkisov [225]), 3 × 10 –18 (Lozovsky et al. [760]), 1 × 10 –17 (Patrick and Golden [933]) and 7.7 × 10 –18 (Michael et al. [816]) and 6 × 10 –21 (Tyndall et al. [1215]). The recommendation is based on the study of Tyndall et al ., which was sensitive to reaction paths leading to the products NO, NO 2 and N 2 O. The reaction forming NH 2 O 2 cannot be ruled out, but is apparently not important in the atmosphere.

C26. NH 2 + O 3 . There is poor agreement among the recent studies of Cheskis et al. [224], k(298) = 1.5 × 10 –13 cm 3

s –1

, Patrick and Golden [933], k(298 K) = 3.25 × 10 –13 cm 3 s –1 , Hack et al. [463], 1.84 × 10 –13 cm 3 s –1 , Bulatov et al. [166], 1.2 × 10 –13 cm 3 s –1 , and Kurasawa and Lesclaux [658], 0.63 × 10 –13 cm 3 s –1

. The very low value of Kurasawa and Lesclaux may be due to regeneration of NH 2 from secondary reactions (see Patrick and Golden), and it is disregarded here. The discharge flow value of Hack et al . is nearly a factor of two less than the recent Patrick and Golden flash photolysis value. The large discrepancy between Bulatov et al. and Patrick and Golden eludes explanation. The recommendation is the k(298 K) average of these four studies, and E/R is an average of Patrick and Golden (1151 K) with Hack et al. (710 K).

C27. NH 2 + NO. The recommended value for k at 298 K is the average of the values reported by Lesclaux et al. [710], Hancock et al. [478], Sarkisov et al. [1028], Stief et al. [1119], Andresen et al. [28] Whyte and Phillips [1302], Dreier and Wolfrum [367], Atakan et al. [33], Wolf et al. [1329], Diau et al. [344] and Imamura and Washida [559]. The results of Gordon et al. [447], Gehring et al. [426], Hack et al. [470] and Silver and Kolb [1062] were not considered because th ey lie at least 2 standard deviati ons from the average of the previous
group. The results tend to separate into two groups. The flash photolysis results average 1.8 × 10 –11 cm 3 molecule –1 s –1 (except for the pulse radiolysis study of Gordon et al.), while those obtained using the discharge flow technique average 0.9 × 10 –11 cm 3 molecule –1 s –1

. The apparent discrepancy cannot be due simply to a pressure effect as the pressure range s of the flash photolysis and discharge flow studies overlapped and none of the studies observed a pressure dependence for k. Wh yte and Phillips have suggested that the difference may be due to decomposition of the adduct NH 2 NO, which occurs on the timescale of the flow experiments, but not the flash experiments. There have been many studies of the temperature dependence but most have investigated the regime of interest to combustion and only two have gone below room temperature (Hack et al. from 209–505 K and Stief et al. from 216–480 K. Each study reported k to decrease with increasing temperature The recommended temperature dependence is taken from a fit of to the Stief et al. data at room temperature and below. The reaction proceeds along a complex potential energy surface, which results in product branching ratio s that are strongly dependent on temperature. Ab initio calculations by Walch [1244] show the existence of f our saddle points in the potential surface leading to N 2 + H 2 O without a reaction barrier. Elimination to form OH + HN 2 can occur at any point along the surface. While results from early studies on the branching ratio for OH formation different significantly, the most recent studies (Hall et al., Dolson [359], Silver and Kolb [1065], Atakan et al., Ste phens et al. [1110], Park and Lin [930]) agree on a value around 0.1 at 300 K, with N 2 +H 2 O making up the balance.

C28. NH 2 + NO 2 . There have been four studies of this reaction (Hack et al. [470]; Kurasawa and Lesclaux [657]; Whyte and Phillips [1302]; a nd Xiang et al. [1339]). There is very poor agreement among these studies both

### 1-42 for k at 298 K (factor of 2.3) and for the temperature dependence of k (T –3.0 and T –1.3 ). The recommended values of k at 298 K and the temperature dependence of k are averages of the results reported in these four studies. Hack et al. have shown that the predominant reaction channel (>95%) produces N 2 O + H 2 O. Just as for the NH 2 + NO reaction, the data for this reaction seem to indicate a factor of two discrepancy between flow and flash techniques, although the data base is much smaller.

C29. NH + NO. The recommendation is derived from the room temperature results of Hansen et al. [481], Cox et al. [274] and Harrison et al. [483]. The temperature dependence is from Harrison et al.

C30. NH + NO 2 . The recommendation is derived from the temperature-dependence study of Harrison et al. [483].

C31. O 3 + HNO 2 . Based on Kaiser and Japar [599] and Streit et al. [1124].

C32. N 2 O 5 + H 2 O. The recommended value at 298 K is based on the studies of Tuazon et al. [1193], Atkinson et al. [49] and Hjorth et al. [513]. Sverdrup et al. [1136] obtained an upper limit that is a factor of four smaller than that obtained in the other studies , but the higher upper limit is recomme nded because of the difficulty of distinguishing between homogeneous and hete rogeneous processes in the experiment. See Table 59 for heterogeneous rate data for this reaction.

C33. N 2 (A,v) + O 2 . Rate constants for the overall reaction for th e v=0, 1 and 2 vibrational levels of N 2 (A) have been made by Dreyer et al. [368], Zipf [1374], Piper et al. [951], Iannuzzi and Kaufman [557], Thomas and Kaufman [1163] and De Sousa et al. [324]. The results of these studies are in relatively good agreement. The recommended values are (2.5±0.4), (4.0±0.6) and (4.5±0.6) (× 10 –12 cm 3 molecule –1 s –1 ), from the work of De Sousa et al. The only temperature dependence data are from De Sousa et al., who obtained k(T,v)=k(v,298K)(T/300) 0.55 for v=0,1,2. The observation of high N 2 O production initially reported by Zipf [1374] has not been reproduced by other groups, and the br anching ratio for this channel is probably less than 0.02 (Iannuzzi et al. [556], Black et al. [132], De Sousa et al. [324], Fraser and Piper [407]). The branching ratios for the other channels are poorly established, although there is strong evidence for the formation of both O( 3 P) and O 2 (B 3 Σ u – ).

C34. N 2 (A,v) + O 3 . The only study is that of Bohmer and Hack [136], who obtained 298 K rate constants of 4.1±1.0, 4.1±1.2, 8.0±2.3, and 10±3.0 (×10 –11 cm 3 molecule –1 s –1 ) for the v=0–3 vibrational levels of N 2 (A), respectively. This study determin ed that the NO channel accounts for about 20% of the reaction products.

D1. O + CH 3 . The recommended k(298 K) is the weighted average of three measurements by Washida and Bayes [1282], Washida [1279], and Plumb and Ryan [956]. The E/R value is based on the results of Washida and Bayes [1282], who found k to be independent of temperature between 259 and 341 K.

D2. O + HCN. Because it is a very slow reaction, there are no studies of this reaction below 450 K. Davies and Thrush [313] studied this reacti on between 469 and 574 K while Perry a nd Melius [945] studied it between 540 and 900 K. Results of Perry and Melius are in agreem ent with those of Davies and Thrush. Our recommendation is based on these two studies. The higher-temperature (T>1000 K) combustion-related studies Roth et al. [1007], Szekely et al. [1137], a nd Louge and Hanson [754]] ha ve not been considered. This reaction has two reaction pathways: O + HCN → H + NCO, ∆ H = –2 kcal/mol (k a ); and O + HCN → CO + NH (k b ), ∆ H = –36 kcal/mol. The branching ratio k a /k b for these two channels has been measured to be ~2 at T = 860 K. The branching ratio at lower temperatures, which is likely to vary significantly with temperature, is unknown.

D3. O + C 2 H 2 . The value at 298 K is an average of ten measurements (Arrington et al. [31], Sullivan and Warneck [1135], Brown and Thrush [156], Hoyermann et al. [533,534], Westenberg and deHaas [1295], James and Glass [569], Stuhl and Niki [1128], Westenberg and deHaas [1299], and Aleksandrov et al. [16]). There is reasonably good agreement among these studies. Arrington et al. [31] did not observe a temperature dependence, an observation that was later shown to be erroneous by Westenberg and deHaas [1295]. Westenberg and deHaas [1295], Hoyermann et al. [534] and Aleksandrov et al. [16] are the only authors, who have measured the temperature dependence below 500 K. Westenberg and deHaas observed a curved Arrhenius plot at temperatures higher than 450 K. In the range 194–450 K, Arrhenius behavior provides an adequate description and the E/R obtained by a fit of the data from these three groups in this temperature range is recommended. The A-factor was calculated to reproduce k(298 K). This reaction can have two sets of products, i.e., C 2 HO + H or CH 2 + CO. Under molecular beam conditions C 2 HO has been shown to be the major product. The study by Aleksandrov et al. using a discharge flow-resonance fluorescence method (under undefined pressure conditions ) indicates that the C 2 HO + H channel contributes no more than 7% to the net reaction at 298 K, while a similar study by Vinckier et al. [1234] suggests that both CH 2 and C 2 HO are formed.

### 1-43 D4. O + H 2 CO. The recommended values for A, E/R and k(298 K) are the averages of those determined by Klemm [635] (250 to 498 K) using flash photolysis-resonance fluorescence, by Klemm et al. [636] (298 to 748 K) using discharge flow-resonance fluorescence, and Chang and Barker [208] (296 to 436 K) using discharge flow-mass spectrometry techniques. All three studies are in good agreement. The k(298 K) value is also consistent with the results of Niki et al. [ 884], Herron and Penzhorn [504], and Mack and Thrush [762]. Although the mechanism for O + H 2 CO has been considered to be th e abstraction reaction yielding OH + HCO, Chang and Barker suggest that an additional channel yielding H + HCO 2 may be occurring to the extent of 30% of the total reaction. This conclusion is based on an observation of CO 2 as a product of the reaction under conditions where reactions such as O + HCO → H + CO 2 and O + HCO → OH + CO apparently do not occur. This interesting suggestion needs independent confirmation.

D5. O + CH 3 CHO. The recommended k(298 K) is the average of three measurements by Cadle and Powers [185], Mack and Thrush [763], and Singleton et al. [1078], which are in good agreement. Cadle and Powers and Singleton et al. studied this reaction as a function of temperature between 298 and 475 K and obtained very similar Arrhenius parameters. The recommended E/R value was obtained by considering both sets of data. This reaction is known to proceed via H-at om abstraction (Mack and Thrush [763], Avery and Cvetanovic [50], and Singleton et al. [1078]).

D6. O 3 + C 2 H 2 . The database for this reaction is not well established. Room temperature measurements (Cadle and Schadt [186]; DeMore [325]; DeMore [326]; Stedman a nd Niki [1106]; Pate et al. [932]; and Atkinson and Aschmann [34]) disagree by as much as an order of magnitude. It is probable that secondary reactions involving destruction of ozone by radical products resulte d in erroneously high values for the rate constants in several of the previous measurements. The present recommendation for k(298 K) is based on the room temperature value of Atkinson and Aschmann [34], which is the lowest value obtained and therefore perhaps the most accurate. The temperature dependence is estimated, based on an assumed A-factor of 10 –14 cm 3 s –1 similar to that for the O 3 + C 2 H 4 reaction and corresponding to the expected five-membered ring structure for the transition state (DeMore [325,326]). Further studies, particularly of the temperature dependence, are needed. Major products in the gas phase reaction are CO, CO 2 , and HCOOH, and chemically-activated formic anhydride has been proposed as an intermedia te of the reaction (DeMore [326], and DeMore and Lin [336]). The anhydride intermediates in several alkyne ozonations have been isolated in low temperature solvent experiments (DeMore and Lin [336]).

D7. O 3 + C 2 H 4 . The rate constant of this reaction is well esta blished over a large temperature range, 178 to 360 K. Our recommendation is based on the data of DeMore [325], Stedman et al. [1107], Herron and Huie [503], Japar et al. [570,571], Toby et al. [1176], Su et al. [1132], Adeniji et al. [10], Kan et al. [606], Atkinson et al. [38], and Bahta et al. [55].

D8. O 3 + C 3 H 6 . The rate constant of this reaction is well es tablished over the temperature range 185 to 360 K. The present recommendation is based largely on the data of Herron and Huie [503], in the temperature range 235– 362 K. (Note that a typographical error in Table 2 of that paper improperly lists the lowest temperature as 250 K, rather than the correct value, 235 K.) The recommended Arrhenius expressi on agrees within 25% with the low temperature (185–195 K) data of DeMore [325], and is consistent with, but slightly lower (about 40%) than the data of Adeniji et al. [10] in the temperature range 260–294 K. Room temperature measurements of Cox and Penkett [290], Stedman et al. [1107], Japar et al. [570,571], and Atkinson et al. [38] are in good agreement (10% or better) with the recommendation.

D9. OH + CO. The recommendation allows for an increase in k with pressure. The zero pressure value was derived by averaging direct low pressure determinations (those listed in Baulch et al. [89]) and the values reported by Dreier and Wolfrum [366], Husain et al. [547], Ravishankara and Thompson [986], Paraskevopoulos and Irwin [927], Hofzumahaus and Stuhl [518]. The results of Jonah et al. [593] are too high and were not included. An increase in k with pressure has been observed by a large number of investigators (Overend and Paraske vopoulos [922], Perry et al. [944], Chan et al. [207], Biermann et al. [121], Cox et al. [284], Butler et al. [184], Paraskevopoulos and Irwin [926,927], DeMore [330], Hofzumahaus and Stuhl [518], Hynes et al. [554]). In addition, Niki et al. [892] have measured k relative to OH + C 2 H 4 in one atmosphere of air by following CO 2 production using FTIR. The recommended 298 K value was obtained by using a weighted nonlinear least s quares analysis of all pressure-dependent data in N 2 (Paraskevopoulos and Irwin [927], DeMore [330], Hofzum ahaus and Stuhl [518], and Hynes et al. [554]) as well as those in air (Niki et al. [894], Hynes et al. [554]), to the form k = (A+BP)/(C+DP), where P is pressure in atmospheres. The data were best fit with D = 0 a nd therefore a linear form is recommended. Previous controversy regarding the effect of small amounts of O 2 (Biermann et al. [121]) has been resolved and is attributed to secondary reactions (DeMore [330], Hofzumah aus and Stuhl [518]). The results of Butler et al. [184] have to be re-evaluated in the light of refinements in the rate coefficient for the OH + H 2 O 2 reaction. The corrected rate coefficient is in appr oximate agreement with the recommended value. Currently,

### 1-44 there are no indications to suggest that the presence of O 2 has any effect on the rate coefficient other than as a third body. The E/R value in the pressure range 50–760 torr ha s been shown to be essentially zero between 220 and 298 K by Hynes et al. [554]. Further substantiation of the temperature independence of k at 1 atm. may be worthwhile. Beno et al. [111] observe an enhancement of k with water vapor, which is in conflict with the flash photolysis studies; e.g., Ravishankara and Thompson [986], Parask evopoulos and Irwin [927], and Hynes et al. [554]. The uncertainty factor is for 1 atm. of air. The bimolecular channel yields H + CO 2 while the addition leads to HOCO. In the presence of O 2 , the HOCO intermediate is converted to HO 2 + CO 2 (DeMore [330], Miyoshi et al. [827]). Miyoshi et al. report a rate constant for the reaction of HOCO with O 2 of ~1.5 × 10 –12 cm 3 molecule –1 s –1 at 298 K). Therefore, for atmospheric purposes, the products can be taken to be HO 2 and CO 2 . D10. OH + CH 4 . This reaction has been extensively studied. The most recent data are from Vaghjiani and Ravishankara [1223], Saunders et al. [1030], Finlayson-Pitts et al. [396], Dunlop and Tully [370] , Mellouki et al. [812], and Gierczak et al . [434], who measured the absolute rate coefficients for this reaction using discharge flow and pulsed photolysis techniques. Sharkey and Smith [1056] have reported a high value (7.7 × 10 –15 cm 3 molecule –1 s –1 ) for k(298 K), and this value has not been considered here. The current recommendation for k(298 K) was derived from the resu lts of Vaghjiani and Ravishankara, Dunlop and Tully, Saunders et al., Mellouki et al., Finlayson-Pitts et al., and Gierczak et al. The temperature dependence of this rate coefficient has been measured by Vaghjiani and Ravishankara (223–420 K), Dunlop and Tully (above 298 K), Finlayson-P itts et al. (278–378 K), and Mellouki et al. (233–343 K). Gierczak et al have extended the measurements of k to 195 K, and it appears that the rate coefficient does not strictly follow an Arrhenius expression. The recommended E/R was obtained from these results using data below 300 K. A more accurate representation of the rate constant as a function of temperature is obtained by using the threeparameter expression: k = 2.80×10 –14 T 0.667 exp(–1575/T). This three-parameter fit may be preferred for lower stratosphere and upper troposphere calculations.

D11. OH + 13 CH 4 . This reaction has been studied relative to the OH + CH 4 reaction, since the ratio of the rate coefficients is the quantity needed for quantifying methane sources. Rust and Stevens [1011], Davidson et al. [308], and Cantrell et al. [200] have measured k 12 /k 13 at 298 K to be 1.003, 1.010, and 1.0055, respectively. Cantrell et al.'s data supersede the results of Davidson et al. The recommended value of 1.005 ± 0.002 is based on the results of Rust and Stevens and Cantrell et al. Cantrell et al. find k 12 /k 13 to be independent of temperature between 273 and 353 K.

D12. OH + CH 3 D. The rate coefficient for this reaction has been measured between 249 and 422 K using a pulsed laser photolysis-laser induced fluorescen ce system by Gierczak et al. [433]. The recommended values of k (298 K) and E/R are from this study. The recommendation agrees within about 10% at 298 K with the rate constant measured by DeMore [334] in a relativ e rate study over the temperature range 298 – 360 K. The difference, while small in an absolute sense, is nevertheless significant for the isotopic fractionation of atmospheric CH 3 D and CH 4 by OH. An earlier result of Gordon and Mulac at 416 K [448] is in good agreement with the extrapol ated data of both of these determinations. However, that measurement has not been explicitly included in this recommendation because the experime nts were carried out at higher temperatures and therefore are le ss applicable to the atmosphere. The rate coefficients for the reactions of OH with other deuterated methanes have also been measured. (Dunlop and Tully [370], Gierczak et al. [1153], Gordon and Mulac [448]).

D13. OH + H 2 CO. The value for k(298 K) is the average of those determined by Niki et al. [893], Atkinson and Pitts [46], Stief et al. [1120], Yetter et al. [1345], and Temps and Wagner [1161]. The value reported by Morris and Niki [836] agrees within the stated uncertainty. There are two relative va lues that are not in agreement with the recommendations. The value of Niki et al. [886] relative to OH + C 2 H 4 is higher, while the value of Smith [1095] relative to OH + OH is lower. The latter data are also at variance with the negligible temperature dependence observed in the two flash photolysis studies. The later report of Niki et al. [893] is assumed to supersede the earlier rate constant. The rate coefficient repor ted by Zabarnick et al. [1348] at and above 298 K are consistently higher th an the average value recommended here, but overlap within the combined uncertainty. The combined data set suggests E/R = 0, although a slight negative temperature dependence cannot be rule d out The abstraction reaction shown in the table is the major channel (Temps and Wagner [1161], Niki et al. [892]); other channels may contribute to a small extent (Horowitz et al. [525]).

D14. OH + CH 3 OH. The recommended value for k(298 K) is the average of seven direct studies (Overend and Paraskevopoulos [921], Ravish ankara and Davis [979], Ha gele et al. [472], Meier et al. [800], Greenhill and O'Grady [456], Wallington and Kurylo [1264], and Hess and Tully [506]). When these measurements were not at exactly 298 K, their values have been recal culated for 298 K by using the E/R recommended here.

### 1-45 Indirect measurements by Campbell et al. [190], Barnes et al. [65], Tuazon et al. [1194] and Klopffer et al. [638] are in good agreement with the recommended value. The temperature dependence of k has been measured by Hagele et al., Meier et al., Greenhill and O'Grady, Wallington and Kurylo, and Hess and Tully. The recommended value of E/R was calculated using the results obtained in the temperature range of 240 to 400 K by Greenhill and O'Grady [456] , Wallington and Kurylo [1264], He ss and Tully, Meier et al., and Haegle et al. Hess and Tully report a curved Arrhenius plot over the temperature range 298 – 1000 K, while Meier et al. do not observe such a curvature. This reaction has two pathways: abstraction of the H-atom from the methyl group to give CH 2 OH + H 2 O or from the OH group to give CH 3 O + H 2 O. The results of Hagele et al., Meier et al., and Hess and Tully suggest that H abstraction from the methyl group to give CH 2 OH + H 2 O is the dominant channel below room temperature. At 298 K, for example, the branching ratio for the formation of CH 2 OH is about 0.85 and increases as the temperature decreases. In the Earth's atmosphere, the eventual products of OH + CH 3 OH reaction are the same: CH 2 O and HO 2 . D15. OH + CH 3 OOH. The recommended value for k(298 K) is the average of the rate coefficients measured by Niki et al. [891] and Vaghjiani and Ravishankara [1222], which differ by nearly a factor of two. Niki et al. measured the rate coefficient relative to that for OH with C 2 H 4 (= 8.0 × 10 –12 cm 3 molecule –1 s –1 ) by monitoring CH 3 OOH disappearance using an FTIR system. Vaghjiani and Ravishankara monitored the disappearance of OH, OD, and 18 OH in excess CH 3 OOH in a pulsed photolysis-LIF system. They measured k between 203 and 423 K and report a negative activation energy with E/R = –190 K; the recommended E/R is based on their results. The reaction of OH with CH 3 OOH occurs via abstraction of H from the oxygen end to produce the CH 3 OO radical and from the CH 3 group to produce the CH 2 OOH radical, as originally proposed by Niki et al. and confirmed by Vaghjiani and Ravishankara. CH 2 OOH is unstable and falls apart to CH 2 O and OH within a few microseconds. The possible reaction of CH 2 OOH with O 2 is unimportant under atmospheric conditions (Vaghjiani and Ravishankara). The recommended branching ratios are,

OH + CH 3 OOH → CH 3 O 2 + H 2 O (a) 70%

OH + CH 3 OOH → CH 2 OOH + H 2 O (b) 30%, (from Vaghjiani and Ravisha nkara) and are nearly inde pendent of temperature. D16. OH + HC(O)OH. The recommended value of k(298 K) is the average of those measured by Zetzsch and Stuhl [1363], Wine et al. [1311], Jolly et al. [592], Dagaut et al. [303], and Singleton et al. [1083]. The temperature dependence of k has been studied by Wine et al. and by Singleton et al., who observed k to be essentially independent of T.

Wine et al. found the rate coefficient for the OH + HC(O)OH reaction to be the same as that for OH + DC(O)OH reaction. Jolly et al. found the formic acid dimer to be unreactive toward OH, i.e., abstraction of the H atom attached to C was not the major pathway for the reaction. A comprehensive study of Singleton et al. showed that reactivity of HC(O)OH is essentially the same as that of DC(O)OH, but DC(O)OD reacts much slower than HC(O)OH and DC(O)OH. These observations show that the reaction proceeds via abstraction of the acidic H atom. Wine et al. and Jolly et al. also found that H atoms are produced in the reaction, which is consistent with the formation of HC(O)O, which would rapidly fall apart to CO 2 and H. End product studies are also consistent with the formation of CO 2 and H 2 O in this reaction (Singleton et al. [1083]). The products of this reaction w ould be mostly HC(O)O and H 2 O. The fate of HC(O)O in the atmosphere will be to give HO 2 either directly via reaction with O 2 or via thermal decomposition to H atom, which adds to O 2 . Wine et al. have suggested that, in the atmosphere , the formic acid could be hydrogen bonded to a water molecule and its reactivity with OH could be lowered b ecause the hydrogen bonded water would obstruct the abstraction of the H atom. This suggestion needs to be checked.

D17. OH + HCN. This reaction is pressure dependent. The recommended value is the high pressure limit measured by Fritz et al. [414] using a laser photolysis-resonance fluorescence apparatus. Phillips [947] studied this reaction using a discharge fl ow apparatus at low pressures and found th e rate coefficient to have reached the high pressure limit at ~10 torr at 298 K. Fritz et al.’s results contradict this finding. They agree with Phillip’s measured value, within a factor of two, at 7 torr, but they find k to increase further with pressure. The products of the reaction are unknown.

D18. OH + C 2 H 6 . There are nineteen studies of this reaction at 298 K (Greiner [458], Howard and Evenson [529], Overend et al. [923], Lee and Tang [697], Leu [713], Tully et al. [1199], Jeong et al. [584], Tully et al. [1197], Nielsen et al. [879], Zabarnick et al. [1348] , Wallington et al. [1266], Smith et al. [1091], Baulch et al. [88], Bourmada et al. [144], Abbatt et al. [2], Schiffman et al. [1033], Talukdar et al. [1155], Sharkey and Smith [1056] and Anderson and Stephens [24]). The recommended value is obtained by averaging the results of the recent investigations by Tully et al., Wallington et al., Abbatt et al ., Schiffman et al ., Talukdar et al.

### 1-46 and Anderson and Stephens. The results of Sharkey and Smith are approximately 20% higher than those recommended here. When the measurements were not carried out at exactly 298 K, we have recalculated k using an E/R of 1070 K. The temperature dependence of the rate coefficient below 298 K has been measured only by Jeong et al., Wallingt on et al., Talukdar et al. and Anderson and Stephens. The last three studies are in good agreement. The recommended E/R is obtained from an analys is of the data of these three studies. The ratio of the rate coefficients for OH reactions with C 2 H 6 and C 3 H 8 has been measured by Finlayson-Pitts [396]. Our recommendations are in reasona ble agreement with this ratio. Crowley et al. [294] have measured k at 247, 294, and 303 K, and the results are in agreement with the recommendations.

D19. OH + C 3 H 8 . There are many measurements of the rate coefficients at 298 K. In this evaluation we have considered only the direct measurements (Greiner [458], Tully et al. [1199], Droege and Tully [369], Schmidt et al. [1037], Baulch et al. [88], Bradley et al. [147], Abbatt et al. [2], Schiffman et al. [1033], Talukdar et al. [1155], Anderson and Stephens [24] and Mellouki et al. [812]). The 298 K value is the average of these ten studies. Greiner, Tully et al. [1196], Droege and Tully, Talukdar et al. and Mellouki et al. have measured the temperature dependence of this reaction. The recommended E/R was obtained from a linear least squares analysis of the data of Droege and Tully below 400 K and the data of Talukdar et al., Anderson and Stephens, and Mellouki et al. The A-factor was adjusted to reproduce k(298 K). This reaction has two possible channels, i.e., abstraction of the primary and the secondary H-atom. Therefore, non-Arrhenius behavior is exhibited over a wide temperature range, as s hown by Tully et al. and Droege and Tully. The branching ratios were estimated from the latter study:

k primary = 6.3 × 10 –12 exp(–1050/T) cm 3 molecule –1 s –1

k secondary = 6.3 × 10 –12 exp(–580/T) cm 3 molecule –1 s –1
These numbers are in reasonable agreemen t with the older data of Greiner. The ratio of the rate coefficients for OH reactions with C 2 H 6 and C 3 H 8 has been measured by Fi nlayson-Pitts et al. [396]. Our recommendations are in reasonabl e agreement with this ratio.

D20. OH + CH 3 CHO. There are six measurements of this rate coefficient at 298 K (Morris et al. [838], Niki et al. [886], Atkinson and Pitts [ 46], Kerr and Sheppard [613] , Semmes et al. [1054], a nd Michael et al. [815]). The recommended value of k(298 K) is the average of these measurements. Atkinson and Pitts, Semmes et al., and Michael et al. measured the temperature dependence of this rate coefficient and found it to exhibit a negative temperature dependence. The recommended E/R is the aver age value of these studies. The A-factor has been adjusted to yield the recommended value of k(298 K).

D21. OH + C 2 H 5 OH. The recommended value for k(298 K) is the average of those reported by Campbell et al. [190], Overend and Paraskevopoulos [921], Ravishanka ra and Davis [979], Cox and Goldstone [288], Kerr and Stocker [614], Walli ngton and Kurylo [1264], and Hess and Tully [505]. The value reported by Meier et al. is nearly a factor of two lower than that recommended here. The recommended value of E/R was obtained by using the data of Wallington and Kurylo, Hess and Tully, and Meier et al. The temperature dependent rate coefficient values of Meier et al. we re assumed to have the same systematic error that , hence, would not be reflected in the derivation of the E/R value. The A-factor has been adjusted to yield the recommended value of k(298 K). This reaction has three possible product channels: (a) CH 3 CH 2 O + H 2 O, (b) CH 3 CHOH + H 2 O, and (c) CH 2 CH 2 OH+H 2 O. At atmospheric temperatures, channel (b) is the major pathway (Meier et al. [801], Hess and Tully [505]), accounting for more than 75% of the reaction. The branching ration for channel (b) is expected to increase with decreasing temperature, based on the work of Hess and Tully [505]. The CH 3 CHOH radical that is produced in channel (b) and CH 3 CH 2 O radical formed in channel (a) will both rapidly react with O 2 leading to CH 3 CHO and HO 2 . However, the CH 2 CH 2 OH radical produced in channel (c) will lead to a different set of products in the atmosphere. The exact values for these reaction pathways under atmospheric temperatures have not been quantified. Extrapolations of the higher temperature data to atmospheric temperatures may not be valid.

D22. OH + CH 3 C(O)OH. The recommended k(298K) is the average of the values obtained by Dagaut et al. [303] and Singleton et al. [1082]. The earlier results of Zetzsch and Stuhl [1363] are lower than these values, but within the uncertainty of the recommended value. The temperature dependence has been studied by Dagaut et al., who observe a very slight increase in k with temperature between 298 and 440 K and by Singleton et al., who observe a significant decrease with increase in temperature between 298 and 446 K. Further, Singleton et al. observe that the A rrhenius plot is curved. While Dagaut et al. observed th at the acetic acid dimer reacts twice as fast as the monomer, Si ngleton et al. found the dimer to be essentially unreactive toward OH! The latter observations are consistent with the mechanism for the OH + HC(O)OH reaction, which is discussed in the note for that reaction. It is also consistent with the decr ease in reactivity upon D substitution on the carboxylic site and no change upon substitution on the methyl group (Si ngleton et al. [1082]). Thus, there is some uncertainty as to the T de pendence and the reaction mechanism. Here we recommend a slightly

### 1-47 negative T dependence, based on an average of both temp erature dependence studies but with an uncertainty that encompasses both the studies. The A factor and E/R suggest that this reaction may not be a simple metathesis reaction. Based on the analogy with OH + HC(O)OH reac tion and the evidence of Singleton et al., the products are expected to be mostly CH 3 C(O)O + H 2 O. In the atmosphere, CH 3 C(O)O is expected to give CH 3 + CO 2 . D23. OH + CH 3 C(O)CH 3. The rate coefficient for this reaction has been measured at temperatures close to 298 K by Cox et al. [286], Zetzsch [1362], Chiorboli et al. [227], Kerr a nd Stocker [614], Wa llington and Kurylo [1265], LeCalve et al. [690], Wollenha upt et al. [1330], and Gi erczak et al. [429]. C ox reported only an upper limit of <5 × 10 –13 cm 3 molecule –1 s –1 , which is consistent with this recommendation. The primary aim of Chiorboli et al. was to examin e the atmospheric degradation of styrene, which produces acetone. They employed a relative rate measurement and reported a value of k(298 K) that is almost three times faster than the recommended value. Because of possible complications in their system, we have not included their results in arriving at the recommended value. Wallington and Kurylo, LeCalve et al., Wollenhaupt et al. and Gierczak et al. have reported k as a function of temperature; all these st udies directly measured the rate constant using the pulsed photolysis method where the temporal profile of OH was measured using resonance fluorescence or laser induced fluorescence. The extensive data of Wollenhaupt et al. and Gierczak et al. seem to show that this rate coefficient does not follow an Arrhenius expression. The results of LeCalve et al. and Wallington et al. are in general ag reement with the results of Wolle nhaupt et al. and Gierczak et al. The nonArrhenius behavior was not evident in the results of Wallington et al. and LeCalve et al. because they measured the rate constant at a few temperatures and did not explore temperature below 240 K, where the curvature becomes in creasingly evident. The following recommendation reproduces all reported data, except that of Chiorboli et al. within the recommended uncertainty of 25% at all temperatures: k(T) = 1.33 × 10 –13 + 3.82 × 10 –11 exp(–2000/T) This reaction can proceed via the abst raction of an H atom or via the form ation of a complex that decomposes to give many different products, which include CH 3 + CH 3 C(O)OH, CH 3 OH + CH 3 C(O), CH 4 + CH 3 CO 2 , H 2 O + CH 3 C(O)CH 2 . The branching ratios for the formation of diffe rent sets of products will, most likely, vary with temperature. Wollenhaupt and Crowley (2000) have deduced that CH 3 radicals are produced with a yield of ~50% at 298 K and ~30% at 233 K. A similar branching ratio has also been reported by Vasvari et al. [1227]. The results of Gierczak et al. on OH + CD 3 C(O)CD 3 reaction, whose rate coefficient nearly obeys anArrhenius expression between 240 and 400 K and is nearly an order of magnitude smaller than the nondeuterated analog at 250 K, suggests that H abstraction may be the dominant channel. Because of this conflicting evidence, we have not reco mmended the products of this reaction.

D24. OH + CH 3 CN. This rate coefficient has been measured as a function of temperature by Harris et al. [482] between 298 and 424 K, Kurylo and Knable [667] between 250 and 363 K, Rhasa [1002] between 295 and 520 K, and Hynes and Wine [552] between 256 and 388 K. In addition, the 298 K value has been measured by Poulet et al. [961]. The 298 K results of Harris et al. are in disagreement with all other measurements and therefore have not been included. The recommended 298 K value is a weighted average of all other studies. The temperature dependence was computed using the results of Kurylo and Knable, the lower temperature values (i.e., 295–391 K) of Rhasa, and the data of Hynes and Wine. Three points are worth noting: (a) Rhasa observed a curved Arrhenius plot even in the temperature range of 295 to 520 K, and therefore extrapolation of the recommended expression could lead to large errors; (b) Hynes and Wine observed a pressure dependent increase of k(298 K) that levels off at about 1 atmosphere, and this observation is contradictory to the results of other investigations; (c) Hynes and Wine have carried out extensive pressure, temperature, O 2 concentration, and isotope variations in this reaction. Hynes and Wine postulate that the reaction proceeds via addition as well as abstraction pathways. They observe OH regeneration in the presence of O 2 . The recommended k(298 K) and E/R are applicab le for only lower tropospheric conditions. Because of the unresolved questions of pressure dependence and reaction mechanism, the recommended value may not be applicable under upper tropospheric and stratospheric conditions.

D25. OH + CH 3 ONO 2 . The rate coefficient for this reaction at 298 K has been measured by Kerr and Stocker [614], Nielsen et al. [881], Gaffney et al. [417], Talukdar et al. [417], Kakesu et al. [604] and Shallcross et al. [1055]. The results of Kerr and Stocker and of Nielsen et al . are a factor of ten higher than those reported by the other groups There are no obvious reasons for the reported diffe rences but the lower values are preferred for a number of reasons. Firstly, Talukdar et al. have carried out a large number of checks which ruled out possible effects in their system due to the regeneration of OH via secondary reactions, to bath gas pressure, and to formation of an adduct that could undergo further reac tion in the presence of oxygen. Secondly, the lower values are more consistent with reactivity pr edictions of Atkinson and Aschmann [36], who assumed that the series of nitrate reactions pr oceed by H-atom abstraction pathways. Kinetic measurements of Talukdar et al. performed with isotopi cally substituted hydroxyl radical (OH, 18 OH, and OD) and methyl

### 1-48 nitrate (CH 3 ONO 2 and CD 3 ONO 2 ) are all consistent with this reacti on proceeding via an H-atom abstraction pathway.. Accordingly, the recommended value of k(298 K) is based on an average of the values given by Gaffney et al, Talukdar et al., Kakesu et al. and Shallcross et al. Further verification of the reaction mechanism by identification of the products of the reaction is needed. The temperature dependence of the rate coefficient has been measured by Nielsen et al, Talukdar et al and Shallcross et al. While Nielsen et al. report a negative activation energy, Ta lukdar et al. and Shallcross et al. report positive values. For the reasons given above, the temperature dependence recommended here is based on an average of Talukdar et al. and Shallcross et al.

D26. OH + CH 3 C(O)O 2 NO 2 (PAN). This reaction has been studied by f our groups, Winer et al. [1326], Wallington et al. [1248], Tsalkani et al. [1187], and Talukdar et al. [1152]. Winer et al. obtained only an upper limit for the rate coefficient. Tsalkani et al. noted that their system was very ill-behave d and obtained a value of k(298 K) that is a factor of ~2 lower than that obtained by Wallington et al. The pulsed photolysis study of Wallington et al. yielded consistent results, but PAN was not directly measured and photodissociation of H 2 O in the vacuum UV, where PAN absorbs strongly, was used as the OH source. The recent study of Talukdar et al. [1152] yielded much lower rate coefficients. These investigators measured th e PAN concentration directly in their system, minimized seconda ry reactions due to the photodissoci ation of PAN, and carried out extensive tests for decomposition of P AN, impurities, and secondary reactions. The recommended upper limit is a factor two higher than the highest value measured by Talukdar et al. at 298 K and at 272 K. The quoted upper limit is expected to be valid at all atmospheric temperatures. The products of the reaction are not known. Further measurements of the rate coefficients a nd information on the reaction pathways are needed.

D27. OH + C 2 H 5 ONO 2 . The rate constant for this reaction at 298 K has been measured by Kerr and Stocker [614], Nielsen et al. [881], Talukdar et al. [1154], Kakesu et al. [604], and Shallcross et al. [1055]. As in the case of the reaction of OH with CH 3 ONO 2 , the results of Kerr and Stocker and of Nielsen et al. are larger (by a factor of 3) than those of the more recent studies . The reasons for the differences are not clear. Because of the exhaustive tests carried out (see the note for the OH + CH 3 ONO 2 reaction), the values of Talukdar et al., Kakesu et al., and Shallcross et al. ar e recommended, with a large uncertainty. Nielsen et al., Talukdar et al., and Shallcross et al. have measured the rate constant as a function of temperature. As with the OH + CH 3 ONO 2 reaction, Nielsen et al. report a negative activation energy while Talukdar et al. and Shallcross et al. have observed a small positive activation energy. Talukdar et al. note that the rate coefficient for this reaction does not strictly follow Arrhenius behavior, consistent with the abstraction of both the primary and the secondary H atoms. Above 298 K, E/R values measured by Shallcross et al and Talukdar et al. are in excellent agreement. Only Talukdar et al have kinetics data below 298 K and the recommended E/R value was obtained by fitting the rate coeffi cients measured by Talukdar et al. at ≤ 298 K. The large uncertainty encompasses the results of Kerr and Stocker and Nielsen et al.

D28. OH + 1-C 3 H 7 ONO 2 . The reaction has been studied by Kerr a nd Stocker [614] and Atkinson and Aschmann [36] at room temperature and by Nielsen et al. [881] between 298 and 368 K. The results of the three studies are in good agreement at room temperature. Nielsen et al. find that the reaction is temperature independent within the measurement uncertainty over the range studied. However as discussed above, the Nielson et al. results for the analogous reactions of OH with CH 3 ONO 2 and C 2 H 5 ONO 2 , yield negative activation energies that disagree with the positive activation energies obtained by others. Judging from the E/R’s for the analogous reactions, one might expect the E/R for th is reaction to be on the order of 300 kcal/mole. Accordingly, we place a large uncertainty on the recommended temperature dependence. A thorough investigation of the temperature dependence of this reaction is needed.

D29. OH + 2-C 3 H 7 ONO 2 . The reaction has been studied by Atkinson and Aschman [36], Atkinson et al [37] and Becker and Wirtz [98] at room temperature and by Talukdar et al. [1117] over the range 233 and 395 K. The results of Atkinson and Aschmann supersede those of Atkinson et al. There is fair agr eement between the results of the three studies at room temperature, with roughly a factor of two spread in the values. The recommendation is based on an average of the room temperature values and the E/R measured by Talukdar et al.

D30. HO 2 + CH 2 O. There is sufficient evidence to suggest that HO 2 adds to CH 2 O (Su et al. [1131,1133], Veyret et al. [1231], Zabel et al. [1349], Barnes et al. [70], and Veyret et al. [1230]). The recommended k(298 K) is the average of values obtained by Su et al. [1131], Veyret et al. [1231], and Veyret et al. [1230]. The temperature dependence observed by Veyret et al. [1230] is recommended. The value reported by Barnes et al. at 273 K is consistent with this recommendation. The adduct HO 2 •CH 2 O seems to isomerize to HOCH 2 OO reasonably rapidly and reversibly. There is a great deal of discrepancy between measured values of the equilibrium constants for this reaction.

D31. HO 2 + CH 3 O 2 . This recommendation is from Tyndall et al. [1210]. The kinetics of this reaction has been studied by using UV absorption following pulsed photolytic production of the radicals. These authors first

### 1-49 analyzed the available data for the products of th e reaction and concluded th at the major products are CH 3 OOH and O 2 . They used this product yield information with their evaluated UV absorption cross sections for HO 2 and CH 3 O 2 to reanalyze the UV absorption profiles measured in kinetics experiments by Dagaut et al. [301] and by Lightfoot et al. [733], the two groups that carried out the most extensive studies. They found that rate coefficients reported by these two groups need to be increased by ~20%. The recommended value is based on the average of the corrected data from these two groups. The temperature dependence was evaluated by Tyndall et al. by assuming that the absorption cross sections of CH 3 O 2 and HO 2 are independent of temperature at the wavelengths used for the kinetics studies.

D32. HO 2 + C 2 H 5 O 2 . The recommended value is the weighted average of those measured by Cattell et al. [205], Dagaut et al. [302], Fenter et al. [389], and Maricq and Szente [778]. In all experiments the rate coefficient was obtained by modeling the reaction system. Also, the calculated rate co efficients depended on the UV absorption cross sections of both C 2 H 5 O 2 and HO 2 . The absorption cross section of C 2 H 5 O 2 is not welldefined. The value reported by Dagaut et al. would be ~30% higher if the cross sections used by Maricq and Szente were used. The recommended E/R is that measured by Daga ut et al., Fenter et al., and Maricq and Szente. Wallington and Japar [1263] have shown that C 2 H 5 O 2 H and O 2 are the only products of this reaction.

D33. HO 2 + CH 3 C(O)O 2 . This recommendation is from Tyndall et al. [1210]. This reaction has two sets of products:

CH 3 C(O)O 2 + HO 2 a k



###  → CH 3 C(O)O 2 H + O 2 (a)

CH 3 C(O)O 2 + HO 2 b k



###  → CH 3 C(O)OH + O 3 (b) The majority of the reaction pr oceeds via channel (a), but there is clear evidence for channel (b). Tyndall et al. reevaluated the available data on e nd products of this reaction, particular ly those of Crawford et al. [293], Moortgat et al. [834], and Horie and Moortgat [522], a nd concluded that channel (a ) contributes ~80% while channel (b) contributes ~20% at 298 K. They also concluded that k a /k b = 37 × exp(–660/T) with a large uncertainty in this value. They derived the overall rate coefficient fo r this reaction, which has been measured only by following the radical concentrations via UV absorption. They based their recommendation mostly on the results of Moortgat et al [834] and Tomas et al. [1180].

D34. HO 2 + CH 3 C(O)CH 2 O 2 . This recommendation is from Tyndall et al. [1210]. This reaction has been studied by only Bridier et al. [152] and Tyndall et al. based their recommendation on this one study.

D35. NO 3 + CO. The upper limit is based on the results of Hjorth et al. [514], who monitored isotopically labeled CO loss in the presence of NO 3 by FTIR. Burrows et al. [180] obtained an upper limit of 4 × 10 –16 cm 3 molecule –1 s –1 , which is consistent with the Hjorth et al. study. Products are expected to be NO 2 + CO 2 , if the reaction occurs.

D36. NO 3 + CH 2 O. There are three measurements of this rate coefficient at 298 K: Atkinson et al. [48], Cantrell et al. [201], and Hjorth et al. [515]. The value reported by Atkinson et al. [48], k = (3.23 ± 0.26) × 10 –16 cm 3 molecule –1 s –1 , is corrected to 5.8 × 10 –16 cm 3 molecule –1 s –1 to account for the different value of the equilibrium constant for the NO 3 + NO 2 → N 2 O 5 reaction that was measured subsequent to this study by the same group using the same apparatus. This correction is in accordance with their suggestion (Tuazon et al. [1195]). The values reported by Cantrell et al. and Hjorth et al., k = 6.3 × 10 –16 cm 3 molecule –1 s –1 and (5.4±1.1) × 10 –16 cm 3 molecule –1 s –1 , respectively, are in good agreement with the corrected value of Atkinson et al. The recommended value is the av erage of these three studies. Cantrell et al. have good evidence to suggest that HNO 3 and CHO are the products of this reaction. The temperature dependence of this rate coefficient is unknown, but comparison with the analogous NO 3 + CH 3 CHO reaction suggests a large E/R.

D37. NO 3 + CH 3 CHO. There are four measurements of this rate constant: Morris and Niki [837], Atkinson et al. [48], Cantrell et al. [195], and Dlugokencky and Howard [349]. The value reported by Atkinson et al. [48], k = (1.34±0.28) × 10 –15 cm 3 molecule –1 s –1 , is corrected to 2.4 × 10 –15 cm 3 molecule –1 s –1 as discussed for the NO 3 + H 2 CO reaction above and as suggested by Tuazon et al. [1195]. The recommended value is the average of the values obtained by Atkinson et al., Cantrell et al., and Dlugokencky and Howard. The results of Morris and Niki agree with the recommended value when their original data is re-analyzed using a more recent value for the equilibrium constant for the reaction NO 2 + NO 3 ↔ N 2 O 5 as shown by Dlugokencky and Howard. Dlugokencky and Howard have studied the temperatur e dependence of this reaction. Their measured value of E/R is recommended. The A-factor has been calculated to yield the k(298K) recommended here. Morris and Niki, and Cantrell et al. observed the formation of HNO 3 and PAN in their studies, which strongly suggests that HNO 3 and CH 3 CO are the products of this reaction.

### 1-50 D38. CH 3 + O 2 . This bimolecular reaction is not expected to be important, based on the results of Baldwin and Golden [57], who found k < 5 × 10 –17 cm 3 molecule –1 s –1 for temperatures up to 1200 K. Klais et al. [632] failed to detect OH (via CH 3 + O 2 → CH 2 O + OH) at 368 K and placed an upper limit of 3 × 10 –16 cm 3 molecule –1 s –1 for this rate coefficient. Bhaskaran et al. [116] measured k = 1×10 –11 exp (–12,900/T) cm 3 molecule –1 s –1 for 1800 < T < 2200 K. The latter two studies thus support the results of Baldwin and Golden. Studies by Selzer and Bayes [1053] and Plumb and Ryan [956] confirm the low value for this rate coefficient. Previous studies of Washida and Bayes [1282] are superseded by those of Selzer and Bayes. Plumb and Ryan have placed an upper limit of 3 × 10 –16 cm 3 molecule –1 s –1 based on their inability to find HCHO in their experiments. A study by Zellner and Ewig [ 1359] suggests that this reacti on is important at combustion temperature but is unimportant for the atmosphere.

D39. CH 3 + O 3 . The recommended A-factor and E/R are those obtained from the results of Ogryzlo et al. [904]. The results of Simonaitis and Heickl en [1070], based on an analysis of a complex system, are not used. Washida et al. [1281] used O + C 2 H 4 as the source of CH 3 . Studies on the O + C 2 H 4 reaction (Schmoltner et al. [1038], Kleinermanns and Luntz [634], Hunziker et al. [544], and Inoue and Akimoto [561]) have shown this reaction to be a poor source of CH 3 . Therefore, the results of Wash ida et al. are also not used.

D40. HCO + O 2 . The value of k(298 K) is the average of the determinations by Washida et al. [1283], Shibuya et al. [1059], Veyret and Lesc laux [1229], Langford and Moor e [680], Nesbitt et al. [ 859], Temps et al. [1161] and Ninomiya et al. [896]. There are three measurements of k wher e HCO was monitored via the intracavity dye laser absorption techni que (Reilly et al. [998] , Nadtochenko et al. [844] , and Gill et al. [435]). Even though these studies agree with the recent measurements of Nesbitt et al., the only recent measurement to obtain a low value, they have not been included in deriving the recommended value of k(298 K). However, the uncertainty has been increased to overlap w ith those measurements. The main reason for not including them in the average is th e possible depletion of O 2 in those static systems (as suggested by Veyret and Lesclaux). Also, these experiments were designed more for the study of photochemistry than kinetics. The temperature dependence of this rate coefficient has b een measured by Veyret and Lesclaux, Timonen et al. [1175] and Nesbitt et al. While Timonen et al. obtain a slightly positive activation energy, Veyret and Lesclaux, and Nesbitt et al. measure slightly negative activation energy. It is very likely that the Arrhenius expression is curved. We recommend an E/R value of zero, with an uncertainty of 100 K. Veyret and Lesclaux preferred a T n form (k = 5.5 × 10 –11 T –(0.4±0.3) cm 3 molecule –1 s –1 ). Hsu et al.[535] suggest that this reaction proceeds via addition at low temperat ure and abstraction at higher temperatures.

D41. CH 2 OH + O 2 . The rate coefficient was first measured directly by Radford [973] by detecting the HO 2 product in a laser magnetic resonance spectrometer. The wall loss of CH 2 OH could have introduced a large error in this measurement. Radford also showed that the previous measurement of Avramenko and Kolesnikova [52] was in error. Wang et al. [1273] measured a value of 1.4 × 10 –12 cm 3 molecule –1 s –1 by detecting the HO 2 product. Recently, Dobe et al. [352] , Grotheer et al. [460], Payne et al . [937], Grotheer et al. [461] and Nesbitt et al. [862] have measured k(298 K) to be close to 1.0 × 10 –11 cm 3 molecule –1 s –1 under conditions where wall losses are small. This reaction appears to exhibit a very complex temperature dependence. Based on the recent data of Grotheer et al. [461] and Ne sbitt et al. [862], k appears to increase from 200 K to approximately 250 K in an Arrhenius fashion, levels off at approximately 300 K, decreases from 300 to 500 K, and finally increases as temperature is increased. This complex temperature dependence is believed to be due to the formation of a CH 2 (OH)•O 2 adduct which can isomerize to CH 2 O•HO 2 or decompose to reactants. The CH 2 O•HO 2 isomer can also decompose to CH 2 O and HO 2 or reform the original adduct. At temperatures less than 250 K, the data of Nesbitt et al. suggests an E/R value of ~1700 K. For atmospheric purposes, the value E/R = 0 is appropriate.

D42. CH 3 O + O 2 . The recommended value for k(298 K) is the average of those reported by Lorenz et al. [752] and Wantuck et al. [1276]. The recommended E/R was obtained using the results of Gutman et al. [462] (413 to 608 K), Lorenz et al. [752] (298 to 450 K), and Wantuck et al. [1276] (298 to 498 K). These investigators have measured k directly under pseudo–f irst order conditions by following CH 3 O via laser induced fluorescence. Wantuck et al. measured k up to 973 K and found the Arrhenius plot to be curved; only their lower temperature data are us ed in the fit to obtain E/R. The A factor has been ad justed to reproduce the recommended k(298 K). The previous high temperature measuremen ts (Barker et al. [61] and Batt and Robinson [85]) are in reasonable agreement with the derived expression. This value is consistent with the 298 K results of Cox et al. [285]

, obtained from an end product analysis study, and with the upper limit measured by Sanders et al. [1025]. The A-factor appears low for a hydrogen atom transfer reaction. The reaction may be more complicated than a simple abstraction. At 298 K, the products of this reaction are HO 2 and CH 2 O, as shown by Niki et al. [889].

D43. CH 3 O + NO. The reaction of CH 3 O with NO proceeds mainly via addition to form CH 3 ONO (Batt et al. [84], Wiebe and Heicklen [1305], Frost and Smith [415], and Ohmori et al. [905]). However, a fraction of the

### 1-51 energized CH 3 ONO adducts decompose to CH 2 O + HNO, and appear to be a bimolecular channel. This reaction has been investigated r ecently by direct detection of CH 3 O via laser-induced fluorescence (Zellner [1357]; Frost and Smith [415]; Ohmori et al. [905]). The previous end-product studies (Batt et al. [84], Wiebe and Heicklen [1305]) are generally consistent with this conclusion. Since the fraction of the CH 3 ONO adduct that falls apart to CH 2 O + HNO decreases with increases in pressure and decreases in temperature, it is not possible to derive a “bimol ecular” rate coefficient. A value of k < 8×10 –12 cm 3 molecule –1 s –1 can be deduced from the work of Frost and Smith [415] and Ohmo ri et al.[905] for lowe r atmospheric conditions.

D44. CH 3 O + NO 2 . The reaction of CH 3 O with NO 2 proceeds mainly via the formation of CH 3 ONO 2 . However, a fraction of the energized adducts fall apart to yield CH 2 O + HNO 2 . The bimolecular rate coefficient reported here is for the fraction of the reaction that yields CH 2 O and HNO 2 . It is not meant to represent a bimolecular metathesis reaction. The recommended value was derived from the study of McCaulley et al.[794] and is discussed in the section on association reactions.

D45. CH 3 O 2 + O 3 . This recommendation is from Tyndall et al. [1210]. Their recommendation is based mostly on the recent study by Tyndall et al. [1220]. The temperature dependence is based on the assumption that the only possible reaction which can occur is the O atom transfer from the CH 3 O 2 radical and that the activation energy of ~2 kcal mol –1 for this O-atom transfer is similar to that in the HO 2 + O 3 reaction.

D46. CH 3 O 2 + CH 3 O 2 . This recommendation is from Tyndall et al. [1210]. There are two confirmed sets of products for this reaction.

CH 3 O 2 + CH 3 O 2 a k



###  → CH 3 O + CH 3 O + O 2 (a)

CH 3 O 2 + CH 3 O 2 b k



###  → CH 3 OH + HCHO + O 2 (b)
The relative product yield, k a /k b, was evaluated by Tyndall et al. to be (26.2 ± 6.6) × exp ((–1130 ± 240)/T). They concluded that there was no ev idence for the formation of the CH 3 OOCH 3 . The kinetics of this reaction has been studied by using UV absorption following pulsed photolytic production of the radicals. Tyndall et al. used the values of k/ σ measured by a large number of groups along with the σ values from their evaluation to calculate k. ( σ is the absorption cross section of the radical at the wavelength at which it was monitored.) They only used the kinetics data obtained at wavelengths larger than 240 nm, since the absorption by HO 2 radicals that are unavoidably produced in th ese measurements can significantly contribute to the measure UV profiles at shorter wavelengths. They noted that the values of k/ σ measured by various groups were much more accurate than the values of σ measured by the same groups. The value of k obtained by this method was then corrected using the above branching ratio for the production of CH 3 O that leads to the unavoidable occurrence of the CH 3 O 2 + HO 2 side reaction; this side reaction consumes another CH 3 O 2 radical.

D47. CH 3 O 2 + NO. This recommendation is from Tyndall et al. [1210]. They evaluated the available information to deduce that the main set of products under atmospheric conditions is CH 3 O + NO 2 . They noted, however, that a very small yield, <0.5%, of CH 3 ONO 2 is also possible. The rate coefficient for the reaction at 298 K and its temperature dependence is based on numerous direct st udies of this reaction that have been reported.

D48. CH 3 O 2 + CH 3 C(O)O 2 . This recommendation is from Tyndall et al. [1210]. This reaction has two sets of products:

CH 3 C(O)O 2 + CH 3 O 2 a k



###  → CH 3 + CO 2 + CH 3 O + O 2 (a)

CH 3 C(O)O 2 + CH 3 O 2 b k



###  → CH 3 C(O)OH + HCHO + O 2 (b) Tyndall et al. reanalyzed the previously available data on the branching ratios for this reaction and concluded that the branching ratio for channel (a) was k a /k = 0.9 ± 0.1 and k b /k = 0.1 ± 0.1 at 298 K. They also concluded that branching ratios could not be derived for other te mperatures from the existing data and therefore did not make a recommendation for the temperature dependence. The recommendation from Tyndall et al. is based on the work of Roehl et al. [ 1005] and Villenave et al. [1232]. Their recommended temperature dependence for the overall rate coefficient is based on analogy with other RO 2 reactions.

D49. CH 3 O 2 + CH 3 C(O)CH 2 O 2 . This recommendation is from Tyndall et al. [1210]. This reaction has three possible sets of products:

CH 3 C(O)CH 2 O 2 + CH 3 O 2 a k



###  → CH 3 C(O) + HCHO + CH 3 O + O 2 (a)

CH 3 C(O)CH 2 O 2 + CH 3 O 2 b k



###  → CH 3 C(O)CH 2 OH + HCHO + O 2 (b)

### 1-52 CH 3 C(O)CH 2 O 2 + CH 3 O 2 c k



###  → CH 3 C(O)CHO + CH 3 OH + O 2 (c)
The branching ratios for these channels, k a /k = 0.3 ± 0.1, k b /k = 0.2 ± 0.1, and k c /k = 0.5 ± 0.1, are based on the work of Bridier et al. [152] and Jenkin et al. [578]. The overall rate coefficient for this reaction has been studied only at 298 K by Bridier et al. and the recommendation is based on this value. The recommended values of E/R and g are based on analogy with other RO 2 reactions.

D50. C 2 H 5 + O 2 . This is a complex reaction that involves the formation of an C 2 H 5 O 2 adduct, which can either be stabilized by collisions or fall apart to HO 2 and C 2 H 4 (Wagner et al. [1238], Bo zzelli and Dean [146], and Kaiser et al. [601]). The fraction of the energized adducts that fall apart to give HO 2 and C 2 H 4 will decrease with increasing pressure and decreas ing temperature, i.e., as the C 2 H 5 O 2 formation increases. The C 2 H 4 - formation channel cannot be sepa rated from the addition reaction. We recommend a conservative upper limit as a guide to the extent of this reaction. This upper limit is applicable only for lower atmospheric pressure and temperature conditions.

D51. C 2 H 5 O + O 2 . The recommendation is based on the pulsed laser photolysis studies of Gutman et al. [462] and Hartmann et al. [484]. In both these studies, removal of C 2 H 5 O in an excess of O 2 was directly monitored via laser induced fluorescence. Gutman et al. measured k at only tw o temperatures, while Hartmann et al. measured k at 5 temperatures between 295 and 411 K. The E/R is from Hartmann et al. The 298 K value deduced from an indirect study by Zabarnick and Heicklen [1347] is in reasonable agreement with the recommended value.

D52. C 2 H 5 O 2 + C 2 H 5 O 2 . k(298 K) has been studied by Adachi et al. [7], Anastasi et al. [22], Munk et al. [841], Cattell et al. [205], Anastasi et al. [21], Wallington et al. [1254] , Bauer et al. [87], a nd Fenter et al. [389]. All the above determinations used only UV absorption to monitor C 2 H 5 O 2 and hence measured k/ σ , where σ is the absorption cross section of C 2 H 5 O 2 at the monitoring wavelength. These investigators also measured the σ that was used in evaluating the rate coefficient. There are large discrepancies in the measured values of σ

. For this evaluation, we have used the cross sections recommended here and recalculated the values of k from each investigation. The recommended k is based on the results of Cattell et al., Wallington et al., Bauer et al., and Fenter et al. In all these experiments the observed rate coeffi cient is higher than the true rate coefficient because of secondary reactions involving HO 2 . HO 2 is formed by the reaction of CH 3 CH 2 O with O 2 and it reacts with C 2 H 5 O 2 to enhance the observed rate coefficient (see Wallington et al. [1256] or Lightfoot et al. [731] for further discussion). Based on product branching ratios discussed below, which determine the magnitude of the necessary correction, the recommended rate coefficient is 0.6 times the average observed rate coefficient. The recommended value of E/R was obtained from the results of Anastasi et al., Wallington et al., Anastasi et al., Ca ttell et al., Bauer et al. and Fenter et al. The observed products (Niki et al. [890]), suggest that at 298 K the channel to yield 2 C 2 H 5 O + O 2 accounts for about 60% of the reaction; the channel to yield CH 3 CHO + C 2 H 5 OH + O 2 accounts for about 40% of the reac tion; and the channel to yield C 2 H 5 O 2 C 2 H 5 + O 2 accounts for less than 5% of the reaction. These branching ratios were used above to obtain the true rate coefficient fro m the observed rate coefficient.

D53. C 2 H 5 O 2 + NO. The recommended k(298 K) is obtained from the results of Plumb et al. [958], Sehested et al. [1051], Daele et al. [300], Eberhard and Howard [371], and Maricq and Szente [779]. The value reported by Adachi and Basco [6], which is a factor of three lower than the recommended value, was not used. The rate coefficient for the CH 3 O 2 + NO reaction measured by Basco and co-workers (Adachi et al. [7]), using the same apparatus, is also much lower than the value recommended here. The recommended temperature dependence is derived from Eberhardt and Howard a nd Maricq and Szente, which are in good agreement.

D54. CH 3 C(O)O 2 + CH 3 C(O)O 2 . This reaction has been studied by Addison et al. [8], Basco and Parmar [83], Moortgat et al. [834] Maricq and Szente [779], and Roehl et al. [1005], using UV absorption techniques. The recommended value is obtained from the data of Moortg at et al., Maricq and Szente, and Roehl et al. As pointed out by Moortgat et al., the six times lower value of k obtained by Addison et al. is likely due to the use of incorrect UV absorption cross sections for the peroxyradical. The k obtained by Basco and Parmar is ~2 times lower than the recommended value. This discrepancy is possibly due to neglecting the UV absorption of CH 3 O 2 and other stable products in their data analysis (Moortgat et al., Maricq and Szente). The recommended temperature dependence was calculated from the data of Moortgat et al. and Maricq and Szente. Addison et al. reported the formation of O 3 , which was attributed to the reaction channel which produces CH 3 C(O)OCH 3 C(O) + O 3 . Moortgat et al. place an upper limit of 2% for this channel. The main products of this reaction appear to be CH 3 C(O)O + O 2 . The CH 3 C(O)O radicals rapidly decompose to give CH 3 and CO 2 . D55. CH 3 C(O)O 2 + NO. This recommendation is from Tyndall et al. [1210]. These authors have argued that the only set of products of importance in the atmosphere is the production of CH 3 + CO 2 + NO 2 . This is because

### 1-53 the alkoxy radical produced upon O ab straction from the peroxy radical by NO will be unstable towards decomposition to give CH 3 and CO 2 . The rate coefficient for the reacti on was deduced primarily from direct studies, but was found to be consistent with the relative rate studies. In the relative rate studies, this rate coefficient was measured relative to the rate coefficient for the reaction of CH 3 C(O)O 2 with NO 2 . The temperature dependence of this rate coefficient were derived from a set of direct measurement and kept consistent with the observed temperature de pendence of the rate coefficient for the CH 3 C(O)O 2 + NO 2 reaction.

D56. CH 3 C(O)CH 2 O 2 + NO. This recommendation is from Tyndall et al. [1210]. They deduced, based on the results of Sehested et al. [1048], Jenkin et al. [ 578] and Orlando et al. [918], that the products of this reaction are CH 3 C(O)CH 2 O + NO 2 . The CH 3 C(O)CH 2 O radical decomposes rapidly to give CH 3 C(O) + CH 2 O. The only kinetics study of this reaction by Sehested et al. forms the basis for the rate coefficient at 298 K. This value is uncertain because of the corrections that had to be made in th e study of Sehested et al. to account for the production of NO 2 , the monitored species, via the reaction of peroxy radicals (such as CH 3 C(O)O 2 and CH 3 O 2 ) with NO. The temperature dependence of the reaction is derived based on analogy with other peroxy radical reactions.

E1. O + FO. The recommended value is based on results of the room temperature study of Bedzhanyan et al. [106] The temperature dependence of the rate constant is expected to be small, as it is for the analogous ClO reaction.

E2. O + FO 2 . No experimental data. The rate constant for such a radical-ato m process is expected to approach the gas collision frequency, and is not expected to exhibit a strong temperature dependence.

E3. OH + CH 3 F (HFC-41). The recommended values for k(298 K) and E/R are averages of these parameters derived from fits to the data of Schmoltner et al. [1039], Nip et al [898], Hsu and DeMore [538], and DeMore [335] (with the relative rate constants from the la st two studies recalcula ted based on the current recommendations for the rate constants for the OH + CH 3 CHF 2 and OH + CH 3 Cl reference reactions respectively.) The A factor was then calculated. The re normalization procedure for relative rate measurements referenced to the OH + CH 3 CHF 2 reaction is discussed in the note for that reaction. The results of Howard and Evenson [528], Jeong and Kaufman [586], and Wallington a nd Hurley [1260] appear to be systematically lower than those of the other studies ove r the temperature region of interest and were not used to derive the recommended parameters.

E4. OH + CH 2 F 2 (HFC-32). The recommended value of k(298 K) is an average from the studies of Nip et al. [898], Jeong and Kaufman [586], Tal ukdar et al. [1150], Hsu and DeMore [538] (recalculated based on the current recommendation for the rate constant for the OH + CH 3 CHF 2 reference reaction, as described in the note for that reaction), and Szilagyi et al. [1138]. The recommended value for E/R is derived from an Arrhenius fit to the data from these same five studies below 400 K. The results of Howard and Evenson [528], Clyne and Holt [244], and Bera and Hanrahan [113] were not used in deriving the recommended parameters.

E5. OH + CHF 3 (HFC-23). The recommended values for k(298 K) and E/R are averages of the values Schmoltner et al. [1039], and Hsu and DeMore [538] (recalculated based on th e current recommendation for the rate constant for the OH + CHF 2 CF 3 reference reaction). The results of Jeong and Kaufman [586], and Medhurst et al. [799], being predominantly above room temperature, were not used in deriving the recommended parameters. The results from Clyne and Holt [244] and Bera and Hanrahan [113] were also not used due to their inconsistency with the other studies. The room temperature values of Howard and Evenson [528] and Nip et al [898] are encompassed within the 2 σ confidence limits.

E6. OH + CH 3 CH 2 F (HFC-161). The recommended value for k(298 K) is an average of the values from Nip et al. [898], Schmoltner et al. [1039], and Kozlov et al. [651]. The value of E/R is based on a fit to the data from these three studies from room temperature and below. The relative rate study by Hsu and DeMore [538] reports a temperature dependence that is markedly different from those of Schmoltner et al. [1039] and Kozlov et al. [651], which are in excellent agreement. This difference is due to significantly lower rate constant values being obtained in the Hsu and De More study in the region near room temperature. Given the most recent results for the reaction of OH + CH 3 CHF 2 (HFC-152a), it seems likely that the HFC-161 reaction also has two channels with different activation ener gies and that the temperature dependence below room temperature should be less than that recommended for HFC-152a, consistent with the present recommendation. Curvature in the Arrhenius plot is evident from the study by Kozlov et al. [651], which was conducted over an extended temperature ra nge above and below room temperature. Singleton et al. [1080] determined that 85 ± 3% of the ab straction by OH is from the fluorin e substituted methyl group at room temperature. Hence this curvature is quite possibly due to the increasing importance of hydrogen abstraction

### 1-54 from the unsubstituted methyl group with increasing temperature. Due to such occurrence, the recommended parameters should not be used for calculati ng rate constants above room temperature.

E7. OH + CH 3 CHF 2 (HFC-152a). The recommended value for k(298 K) is an average of the values from Howard and Evenson [529], Handwerk and Zelln er [480], Nip et al. [898], Gierczak et al. [431] (two different absolute determinations), Hsu and De More [538] (two relative rate dete rminations which have been recalculated based on the current recommendations for the rate constants of the OH + CH 4 and OH + CH 3 CCl 3 reference reactions), and Kozlov et al [651]. There are systematic differences in the temperature dependencies determined in the absolute studies (particularly below room temperature) and relative studies (conducted at room temperature and above). Curvature in the Arrhenius plot (as sugge sted by the data of Gierczak et al. [431]) has been more clearly demonstrated by the study of Kozlov et al. [651] and seems to explain the earlier cited differences between the relative and absolute rate data. This curvature is likely due to the presence of two hydrogen-abstraction reaction channels. Hence, care must be taken in deriving a recommended rate expression suitable for atmospheric modeling (in the temperature region below room temperature). In spite of the noticeable Arrhen ius curvature over the temperature range from 480 K to 210 K, the data below 300 K can be well represented by a two-parameter Arrhenius expression. Thus, the recommended value for E/R is derived from a fit to the data (T ≤ 300 K) of Gierczak et al. and Kozlov et al. The results from Clyne and Holt [244], Brown et al. [154], Nielsen [875], and Liu et al. [749] (superceded by the study of Kozlov et al.) were not used in deriving the recommended parameters. Clearly, in light of the observed Arrhenius curvature, the above procedure for deriving our recommendation for E/R below 300 K does not yield a pa rameter suitable for use in recalcu lating rate constants from relative rate studies in which the OH + CH 3 CHF 2 reaction was the reference and which were conducted at temperatures above 300 K. Use of the below-room-temperature value fo r E/R for such purposes results in rate constant values that are systemati cally different from those determined relative to other reactions or determined by absolute techniques. For such renormalization purposes, one should use an Arrhenius expression derived from data over the appropriate temperature range. A fit to the absolute rate data of Gierczak et al. [431] and Kozlov et al. [651] between room temperature and 400 K yields the Arrhenius expression

k abs = 2.36 × 10 –12 exp{–1255/T} This is in good agreement with the expression derived from the relative rate data of Hsu and DeMore [538]

k rel = 2.1 × 10 –12 exp{–1265/T} The small difference in the pre-exponential factors results from a slight systematic difference in the actual rate constants determined in these three studies that is probably within the combined uncertainties of the determinations. Thus, the following expression derived from the above room temperature E/R value and the recommended k(298 K) has been used for renormalization purposes in this evaluation.

k T ≥ 300K = 2.33 × 10 –12 exp{–1260/T} However, this expression should not be used below 298 K, as erroneous values for OH + CH 3 CHF 2 reaction rate constants would be obtained.

E8. OH + CH 2 FCH 2 F (HFC-152). The recommended value for k(298 K) is an average of the values from Martin and Paraskevopoulos [787], Kozlov et al. [651], and DeMore et al. [341] (three relative rate studies using HFC-152a, cyclopropane, and etha ne as reference reactants). The value for E/R is from a fit to the data of Kozlov et al. [651] at room temperature and below. The A factor was then calcu lated to yield the recommended value for k(298 K). The data above room temperature from Kozlov et al [651] are in excellent agreement with the three relative rate data sets of DeMore et al. [341]. Together, they show a pronounced curvature in the Arrhenius plot, wh ich may indicate the existence of di fferent conformers for HFC-152, each with differing temperature populations and reactivities.

E9. OH + CH 3 CF 3 (HFC-143a). The recommended value for k(298 K) is an average of the values from Martin and Paraskevopoulos [787], Orkin et al. [910], Talukdar et al. [1150] (two different determinations), and Hsu and DeMore [538] (two relative rate determinations which have been recalculated based on the current recom-mendations for the rate constants of the OH + CH 4 and OH + CHF 2 CF 3 reference reactions). The value for E/R is an average of the E/R valu es from the last three of these studi es which are in excellent agreement (Martin and Paraskevopoulos having made measurements only at room temperature). The data of Clyne and Holt [244] were not used due to their inconsistency with the other studies.

E10. OH + CH 2 FCHF 2 (HFC-143). The recommended temperature dependence is based on results of the relative rate study of Barry et al. [79] normalized to the value of the rate constant for the reference reaction (OH + CH 3 CCl 3 ) recommended in this evaluation. The value for k(298 K) is an average of the room temperature

### 1-55 values of Martin and Paraskevopoulos [787] and Barry et al. The significantly higher values reported by Clyne and Holt [244] were not used in th e derivation of the recommended parameters.

E11. OH + CH 2 FCF 3 (HFC-134a). The recommended value for k(298 K) is an average of the values from Martin and Paraskevopoulos [787], Bednarek et al. [101], Orkin and Khamaganov [912], Leu and Lee [711], Gierczak et al. [431] (two different determinations), Liu et al . [749], and DeMore [333] (three determinations which have been recalculated based on the current reco mmendations for the rate constants for the reference reactions OH + CH 4 , OH + CH 3 CCl 3 , and OH + CHF 2 CF 3 ). The value for E/R is an av erage of the E/R values from the last five of these investigations (the studies by Martin and Paraskevopoulos and by Bednarek et al. being conducted only at room temperature). The 270 K result of Zhang et al. [1365] is in excellent agreement with the recommendation. The data of Jeong et al. [584], Brown et al. [154], and Clyne and Holt [244] were not used in deriving the recommended parameters.

E12. OH + CHF 2 CHF 2 (HFC-134). The preferred rate expression is based on results of the three relative rate measurements by DeMore [333] (which have been recalculated based on the current rate constant recommendations for the OH + CH 3 CCl 3 , OH + CH 2 FCF 3 , and OH + CHF 2 CF 3 reference reactions). The room temperature value of Clyne and Holt [244] agrees within the 2 σ confidence limits.

E13. OH + CHF 2 CF 3 (HFC-125). The recommended rate expression is derived from a combined fit to the temperature dependence data of Talukdar et al. [1150] and DeMore [333] and the room temperature data of Martin and Paraskevopoulos [787]. The data of Brown et al. [154] and Clyne and Holt [244] were not used in deriving the recommended parameters.

E14. OH + CH 3 CHFCH 3 (HFC-281ea). The recommended parameters were derived from a fit to the data of DeMore and Wilson [340] who conducted five independent relative rate determinations. Using infrared detection, these investigators based their determ inations on the reference reactions of OH with C 2 H 6 , C 3 H 8 , and C 2 H 5 Cl. Using gas chromatographic detection, they based their determinations on the reference reactions of OH with C 2 H 6 and C 3 H 8 . All of the data were recalculated base d on the current recommendations for the reference rate constants.

E15. OH + CH 3 CH 2 CF 3 (HFC-263fb). Based on room temperature measurement of Nelson et al. [853].

E16. OH + CH 2 FCF 2 CHF 2 (HFC-245ca). The absolute rate constant results of Zhang et al. [1368] differ from the relative rate data (Hsu and DeMore [538]) by appr oximately 30 to 40% over the temperature region of measurement overlap. Both studies, however, derive nearly identical T-dependencies. The recommended rate expression, hence, averages both the k(298 K) and E/R va lues from these studies (with the results of Hsu and DeMore [538] recalculated using the current recommendation for the rate constant of the OH + CH 4 reference reaction).

E17. OH + CHF 2 CHFCHF 2 (HFC-245ea). Based on room temperature measurement of Nelson et al. [853].

E18. OH + CH 2 FCHFCF 3 (HFC-245eb). Based on room temperature measurement of Nelson et al. [853].

E19. OH + CHF 2 CH 2 CF 3 (HFC-245fa). The recommended room temperature va lue is the mean of the values reported by Orkin et al. [910] and Nelson et al. [853], which are in good agreement. The temperature dependence is from Orkin et al. The A-factor has been calculated to fit the recommended room temperature value.

E20. OH + CH 2 FCF 2 CF 3 (HFC-236cb). The recommended rate expression is estim ated as being the same as that for the reaction of OH with CH 2 FCF 3 (HFC-134a), since these reactions ar e expected to have very similar Arrhenius parameters. This estimate is preferred over the results reported by Garland et al. [420], the only published experimental study. The A-factor reported in that study is much lower than expected and the value reported for E/R (1107 K) in lower than that reported for any similar halocarbon reaction.

E21. OH + CHF 2 CHFCF 3 (HFC-236ea). The recommended value for k(298 K) averages the values reported by Hsu and DeMore [538] by a relativ e rate method (recalculated based on the current recommendation for the rate constant of the OH + CH 4 reference reaction) and by Nelson et al. [853] by an absolute technique. The temperature dependence is from Hsu and DeMore [538], with the A-factor adjusted to fit the recommended room temperature value. The higher and somewhat more s cattered values of Garland et al. [420] and Zhang et al. [1368] were not used in deriving the recommended expression.

E22. OH + CF 3 CH 2 CF 3 (HFC-236fa). The recommended rate expression is derived from a combined fit to the data from the relative rate study of Hsu and DeMore [538] (recalculated based on the current recommendation for the rate constant for the reference reaction OH + CHF 2 CF 3 ) and the absolute rate study of Gierczak et al. [432]. The higher results of Nelson et al. [853] and of Garland and Nelson [421], which superseded the earlier results of Garland et al. [421], were not used. A relative rate determination at room temperature by Barry et al. [77] yields a rate constant in excellent agreement w ith the recommended value. However, the

### 1-56 extremely small rate constant ratio measured (relative to OH + CH 3 CF 2 CH 2 CF 3 ) resulted in fairly large uncertainties. Hence this determination was not directly used in the evaluation.

E23. OH + CF 3 CHFCF 3 (HFC-227ea). The recommended rate expression is derived from a combined fit to the data (below 400 K) from the absolute studies of Nelson et al. [849], Zellner et al. [1358], and Zhang et al. [1368] and the relative rate studies of Hsu and DeMo re [538] (two determinations which have been recalculated based on the current recommendations for th e rate constants for the reference reactions OH + CH 4 and OH + CHF 2 CF 3 ).

E24. OH + CH 3 CF 2 CH 2 CF 3 (HFC-365mfc). The recommended value of k(298 K) is an average of the values obtained from the individual rate expressions by Mellouki et al. [813] and Barry et al. [77] (renormalized to the current recommendation for the rate c onstant for the reference reaction OH + CH 3 CCl 3 ). The value for E/R is an average of the values for th is parameter from the same two studies.

E25. OH + CF 3 CH 2 CH 2 CF 3 (HFC-356mff). The recommended value of k(298 K) is an average of the values from Nelson et al.[853] and Zhang et al. [1368]. The temperature dependence is from a fit to the data of Zhang et al. excluding the lowest temperature points (at 260 K), which are somewhat higher than an extrapolation from their other data would indicate. The A-factor has been calculate d to fit the recommended room temperature value.

E26. OH + CH 2 FCH 2 CF 2 CF 3 (HFC-356mcf). The recommended parameters are based on a fit to the data of Nelson et al. [853].

E27. OH + CHF 2 CF 2 CF 2 CHF 2 (HFC-338pcc). The recommended values for both k(298 K) and E/R are averages of these values taken from the individual fits to the data of Schmoltner et al. [1039] and Zhang et al. [1370].

E28. OH + CF 3 CH 2 CF 2 CH 2 CF 3 (HFC-458mfcf). The recommended values for both k(298 K) and E/R are from a fit to the data of Nelson et al. [853].

E29. OH + CF 3 CHFCHFCF 2 CF 3 . (HFC-43-10mee). The recommended rate expression is derived from a combined fit to the data from Schmoltner et al. [1039] and Zhang et al. [1370].

E30. OH + CF 3 CF 2 CH 2 CH 2 CF 2 CF 3 (HFC-55-10mcff). The recommended value for k(298 K) is based on Nelson et al. [853]. As expected, the rate constant is similar to that for CF 3 CH 2 CH 2 CF 3 . Hence the recommendation for E/R is estimated as being approximately the same as for this reaction, with the A-factor calculated to yield k(298 K).

E31. OH + CH 2 =CHF. The recommended parameters were derived from a fit to the data of Perry et al. [941].

E32. OH + CH 2 =CF 2 . The recommended value for k(298 K) is from Howard [526]. The value of E/R was estimated as being similar to that for the reactions of OH with CH 2 =CHF and with CF 2 =CF 2 , and the value for A was then calculated.

E33. OH + CF 2 =CF 2 . The recommended value for k(298 K) is an average of the values determined in the studies of Acerboni et al. [5] (two relative rate determinations referenced to the ra te constants for the reactions of OH with propene and cyclohexane) and the absolute rate st udies of Orkin et al. [911], and Orkin et al. [916]. The value for E/R is from a fit to the data of Orkin et al [916], with the value for A calculated to yield the recommended value for k(298 K).

E34. OH + CF 3 OH. There are no measurements of the ra te coefficient of this reaction. The recommendation is based on the recommended limit for the reverse reaction rate coefficient and an estimated equilibrium
constant. The thermochemistry of CF 3 O and CF 3 OH are taken from ab initio calculations (Montgomery et al. [832] and Schneider and Walli ngton [1040]) and laboratory m easurements (Huey et al. [542]) to estimate ∆ G° 298 (OH + CF 3 OH →

 CF 3 O + H 2 O) to be about (2±4) kcal mol –1

. In considering the large uncertainty in the free energy change, the estimated rate coefficient limit is based on the assumption that the reaction is approximately thermoneutral.

E35. OH + CH 2 (OH)CF 3 . The recommended value for k(298 K) is an av erage of the values reported by Wallington et al. [1255], Inoue et al. [562], and Tokuhashi et al. [1177] (two independent studies). The recommended value for E/R is derived from the data of and Tokuhashi et al. [1177]. The A factor was calculated to agree with the recommended value for k(298 K).

E36. OH + CH 2 (OH)CF 2 CF 3 . The recommended parameters were derived from a combined fit to the data of Tokuhashi et al. [1177] (two independent absolute measurement studies) and the relative rate study of Chen et al. [220] (recalculated based on the current recommendation for the rate constant for the OH + CH 2 Cl 2 reference reaction).

### 1-57 E37. OH + CF 3 CH(OH)CF 3 . The recommended parameters were derived from a fit to the data (below 400 K) of Tokuhashi et al. [1177] (two independent absolute measurement studies).

E38. OH + CH 3 OCHF 2 (HFOC-152a). The recommended rate expression is derived from a fit to the data of Orkin et al. [914] below 400 K.

E39. OH + CH 3 OCF 3 (HFOC-143a). The preferred rate expression is derived from a combined fit to the data of Orkin et al. [914] and Hsu and DeMore [539] (two relative rate dete rminations which have been recalculated based on the current recommendations for the rate constants of the OH + CH 3 CHF 2 and OH + CH 2 F 2 reference reactions). The renormalization procedure for relative rate measurements referenced to the OH + CH 3 CHF 2 reaction is discussed in the note for that reaction. The room temperature result of Zhang et al. [1371] was not used in the derivation since it is significantly higher than the values of the other studies and may be influenced by the presence of reactive impurities.

E40. OH + CHF 2 OCHF 2 (HFOC-134). The recommended values of k(298 K) and E/R were derived from a combined fit to the data of Hsu and DeMore [539] (a relative rate study whose results have been recalculated using the current recommendation for the rate constant of the OH + CH 3 CCl 3 reference reaction), Orkin et al. [917], and Wilson et al. [1309]. The more scattered measurements of Garland et al. [420] were not used in derivation of the preferred value.

E41. OH + CHF 2 OCF 3 (HFOC-125). The recommended rate expression is based on results of the relative rate study of Hsu and DeMore [ 539] (recalculated using the ra te constant for the CHF 3 reference reaction given in this evaluation). Additional measurements by Hsu and DeMore [539] relative to CHF 2 CF 3 and CH 4 are encompassed well within the 2 σ limits, but were not used for assigning the recommended rate expression due to the large differences in reactivity between these two species and the target molecule. The room temperature result of Zhang et al. [1371] lies significantly higher than the recommended value, possibly due to the presence of reactive impurities in the sample.

E42. OH + CHF 2 OCH 2 CF 3 (HFOC-245fa). The recommended rate expression is derived from a fit to the data of Orkin et al. [914] below 400 K.

E43. OH + CH 3 OCF 2 CHF 2 . The recommended parameters were derived from a fit to the data (below 400 K) of Tokuhashi et al. [1179] (two independent absolute measurement studies). A room temperature measurement by Heathfield et al. [490] is nearly an order of magnitude higher than recommended and may be affected by reactive impurities.

E44. OH + CH 3 OCF 2 CF 3 . The recommended parameters were derived from a fit to the data (below 400 K) of Tokuhashi et al. [1178] (two independent absolute measurement studies). The expression, as expected, is similar to those for the OH + CH 3 OCF 3 and OH + CH 3 OCF 2 CF 2 CF 3 reactions.

E45. OH + CH 3 OCF 2 CF 2 CF 3 . The recommended value for k(298 K) is an average of the values reported by Tokuhashi et al. [1178] (two independent absolute measurement studies) and Nonomiya et al. [896] (two relative rate determinations which have been recalcu lated based on the current recommendations for the rate constants of the OH + CH 4 and OH + CH 3 Cl reference reactions). The value for E/R was determined from a fit to the data (below 400 K) of Tokuhashi et al. and the A factor calculated to agree with the value for k(298 K). The expression, as expected, is similar to those for the OH + CH 3 OCF 3 and OH + CH 3 OCF 2 CF 3 reactions.

E46. OH + CH 3 OCF(CF 3 ) 2 . The recommended parameters were derived from a fit to the data (below 400 K) of Tokuhashi et al. [1178] (two independent absolute measurement studies).The rate constants from this study are surprisingly somewhat larger than those for the similar OH + CH 3 OCF 3 and OH + CH 3 OCF 2 CF 3 reactions.

E47. OH + CHF 2 OCH 2 CF 2 CHF 2 . The recommended parameters were derived from a fit to the data (below 400 K) of Tokuhashi et al. [1179] (two independent absolute measurement studies).

E48. OH + CHF 2 OCH 2 CF 2 CF 3 . The recommended parameters were derived from a fit to the data (below 400 K) of Tokuhashi et al. [1179] (two independent absolute measurement studies).

E49. F + O 3 . The recommended value is based on results of the room temperature study of Bedzhanyan et al. [103] and the temperature-dependent study of Wagner et al. [1242]. The value appears to be quite reasonable in view of the well-known reactivity of atomic chlorine with O 3 . E50. F + H 2 . The value of k at 298 K seems to be well established with the results reported by Zhitneva and Pshezhetskii [1373], Heidner et al. [491,492], Wurzberg and Houston [1337], Dodonov et al. [356], Clyne et al. [249], Bozzelli [145], Igoshin et al. [558], Clyne and Hodgson [242] a nd Stevens et al. [1115] being in excellent agreement (range of k being 2.3–3.0 × 10 –11 cm 3 molecule –1 s –1 ). The preferred value at 298 K is taken to be the mean of the values reported in these references. Values of E/R range from 433–595 K

### 1-58 (Heidner et al.; Wurzberg and Houston; Igoshin et al.; and Stevens et al.). The preferred value of E/R is derived from a fit to the data in these studies. The A-factor was chosen to fit the recommended room temperature value.

E51. F + H 2 O. The recommended temperature-independent value is based on results reported in the study by Stevens et al. [1115] over the temperature range 240–373 K using a discharge flow system with chemical conversion of fluorine atoms to de uterium atoms and detection of th e latter by resonanace fluorescence. This value is in excellent agreement with the room temperature results of Frost et al. [416] and Walther and Wagner [1268]. The latter authors in a limited temperature-dependent study reported an E/R value of 400 K. Although these data have not been included in the deriva tion of the preferred value, with the exception of the one low temperature data point, they are encompassed within the indicated uncertainty limits.

E52. F + HNO 3 . The recommendation is based on results of the temperature-dependent study of Wine et al. [1324] and the room temperature results of Mellouki et al. [805], Rahman et al. [975] and Becker et al. [90]. The values at room temperature are in good agreement. The study of Wine et al. [1324] was over the temperature range 260–373 K. Below 320 K the data were fitted with th e Arrhenius expression recommended here, whereas at higher temperatures a temperature-independent value was found, suggesting the occurrence of different mechanisms in the two temperature regimes.

E53. F + CH 4 . The recommended room temperature value is the mean of the results of Wagner et al. [1240], Clyne et al. [249], Kompa and Wanner [648], Foon and Reid [404], Fasano and Nogar [386], and Persky et al. [946]. The temperature dependence is that reported by Pers ky et al. in a competitiv e study using the reaction F + D 2 as the reference reaction. These results are preferred over the te mperature dependences reported in the earlier studies of Wagner et al. and Foon and Reid.

E54. FO + O 3 . Recommended upper limit is based on the results of Li et al. [729] in a study using a discharge flow-mass spectrometric technique. FO was produced in the reacti on of F atoms with excess O 3 . No appreciable decay of FO, and only a small increase in FO 2 , was detected, allowing an upper limit to the rate constant of 10 –14 cm 3 molecule –1 s –1 to be derived. A two orders of magnitude higher upper limit was derived by Sehested et al. [1052]. A lower value of the upper limit was derived by Colussi and Grela [268] from a reanalysis of data on the quantum yields for ozone destruction in F 2 /O 3 mixtures reported by Starrico et al. [1104]. The results of the recent, more direct, study of Li et al. [729] are preferred over the earlier results of Starrico et al. There are two possible pathways which are exothermic, resulting in the production of F + 2O 2 or FO 2 + O 2 . E55. FO + NO. The recommended value is based on results of the temperature-dependent study of Bedzhanyan et al. [105] and the value reported by Ray and Watson [996] for k at 298 K using the discharge flow-mass spectrometric technique.

E56. FO + FO. The recommended value is based on the results of Bedzhanyan et al. [104] and Clyne and Watson [260]. Wagner et al. [1242], in a less direct study, report a higher value. The results of Bedzhanyan et al. indicate the predominant reaction ch annel is that to produce 2F + O 2 . E57. FO 2 + O 3 . Recommended value is based on results of Sehested et al. [1052]. A higher upper limit has been reported by Li et al. [729].

E58. FO 2 + NO. Recommended values are based on results of Li et al. [729], the only temperature-dependent study. The room temperature value is nearly a factor of 2 less than the previous recommendation, which was based on the results of Sehested et al. [1052].

E59. FO 2 + NO 2 . Recommended values are based on results of Li et al. [729], the only temperature-dependent study. The room temperature value is a factor of 2.5 less than the previous recommendation, which was based on the results of Sehested et al. [1052]. This discrepancy might be attributable to a small NO impurity in the NO 2 sample used in the Sehested et al. study.

E60. FO 2 + CO. Recommended value is based on results of Sehested et al. [1052], the only published study of this reaction.

E61. FO 2 + CH 4 . Recommended value is based on results of Li et al. [729]. This upper limit is a factor of 20 less than the previously recommended upper limit, which was based on the results of Sehested et al. [1052].

E62. CF 3 O + O 2 . The recommendation is based upon the results of Turnipseed et al. [1202] who reported k(373 K) 

### ≤ 4 × 10 –17

. Assuming an E/R of 5000 K, which is equal to the reaction endothermicity, yields the recommended A and k(298 K) limits. By comparison to other reactions involving abstraction by O 2 the Afactor is likely to be much smaller.

### 1-59 E63. CF 3 O + O 3 . The recommendation is based on the average of room temperature measurements reported by Turnipseed et al. [1202], Wallington and Ball [1251] , and Bourbon et al. [141]. Turnipseed et al. and Bourbon et al. made direct measurements using LIF detection of CF 3 O with pulsed photolysis and flow tube reactors, respectively. Wallington and Ball used a competetive reaction scheme with IR absorption detection and CF 3 O + CH 4 as the reference reaction. The recommended A factor is estimated by comparison to other CF 3 O reactions, and the E/R is calculated to give the recommended k(298 K). Upper limits reported by Maricq and Szente [777], Nielsen a nd Sehested [880], and Wa llington et al. [1261] are consistent with the k(298 K) recommendation. Measurements reported by Fockenberg et al. [402] and Meller and Moortgat [802] gave rate coefficients about an order of magnitude less than the recommended value. Although the reason for this discrepancy is not known, bot h studies appear to have the possibility of significant secondary chemistry. The reaction products have not been observed.

E64. CF 3 O + H 2 O. The recommendation is based upon the measurement k(381) 

### ≤ 2 × 10 –16 reported by Turnipseed et al. [1200]. The A factor is estimated and the E/R is calculated to fit k(381). The limits k = (0.2–40) × 10 –17 at 296 ± 2 K given by Wallingt on et al. [1262] are consiste nt with the recommendation.

E65. CF 3 O + NO. The recommendation is based upon the room temperature rate coefficients reported by Sehested and Nielsen [1050], Turnipseed et al. [1202], and Jensen et al. [581] which are in very good agreement. An earlier low value given by Bevilacqua et al. [115] is superseded by Jensen et al. The temperature-dependence is derived from measurements by Turnipseed (233–360 K) and Jensen et al. (231–393 K). Room temperature results from Bourbon et al. [142] and Bhatnagar and Carr [117] and a temperature dependence study by Dibble et al. [347] are in good agreement with th e recommendation. The reaction products have been reported by Chen et al. [218] Bevilacqua et al. [115], Bhatnagar and Carr and Dibble et al.

E66. CF 3 O + NO 2 . There are no published measurements of th e rate coefficient for this reaction. The reaction products have been reported by Chen et al. [217] who used photolysis of CF 3 NO to prepare CF 3 O 2 and subsequently CF 3 O in 700 torr of air at 297±2 K. They considered two product channels: (a) CF 3 ONO 2 obtained via three-body recombination and (b) CF 2 O + FNO 2 obtained via fluorine transfer. Products from both channels were observed and found to be thermally stable in their reactor. They report k a /(k a + k b ) ≥ 90%
and k b /(k a + k b ) 

### ≤ 10%, thus the formation of CF 3 ONO 2 is the dominant channel at 700 torr and 297 K.

E67. CF 3 O + CO. The kinetics of this reaction were studied by Turnipseed et al. [1200], who used pulsed laser photolysis with pulsed laser-induced fl uorescence detection and a flow tube reactor with chemical ionization detection to obtain data at temperatures from 233 to 332 K and at pressures from 0.8 to about 300 torr in He and at about 300 torr in SF 6 . The reaction was found to be predominantly a three-body recombination, presumably producing CF 3 OCO as described in Table 2. The bimolecular reaction has at least two product channels: (a) CF 2 O + CFO and (b) CF 3 + CO 2 . The recommended bimolecular rate coefficient limit is derived from the low pressure results of Turnipseed et al., where the r eaction was in the fall-off region. Their low pressure data indicate that k b < 4 × 10 –16 cm 3 molecule –1 s –1 at 298 K. The fate of the CF 3 OCO adduct is uncertain, and it may lead to the regeneration of CF 3 or CF 3 O radicals in the atmosphere. Wallington and Ball [1252] report a yield of 96±8% CO 2 at one atmosphere and 296±2 K.

E68. CF 3 O + CH 4 . The absolute rate coefficients reported by Saathoff and Zellner [1013], Barone et al. [75], Jensen et al. [581], Bourbon et al. [143], and Bednarek et al. [102] at room temperature are in excellent agreement. Kelly et al. [611] used a relative method with FTIR detection to determine the ratio k(CF 3 O + CH 4 )/k(CF 3 O + C 2 H 6 ) = R = 0.01±0.001 at 298±2 K. This does not agree with the ratio of our recommended values, which is 0.017. A relative rate measurement reported by Chen et al. [219] using FTIR methods also gives a low result for the rate coefficient. A relative rate measurement reported by Wallington and Ball [1252], R = 0.0152±0.0023 at 296 K, is in good agreement with the recommended rate coefficients. The temperature dependence is from the data of Barone et al. (247–360 K), Jensen et al. (231–385 K), and Bednarek et al. (235–401 K), who agree very well. Measurements at higher temperatures by Bourbon et al. (296–573 K) gave a higher E/R (1606 K). The k(298 K) is the average of the three absolute studies. The CF 3 OH product was observed by Jensen et al. and Bevilacqua et al. [115].

E69. CF 3 O + C 2 H 6 . The room temperature recommendation is based on results reported by Saathoff and Zellner [1013], Barone et al. [75], and Bourbon et al. [143]. These workers are in excellent agr eement. Chen et al. [219] measured the rate coefficient relative to that for the CF 3 O + NO reaction in 700 torr of air at 297 K. Their ratio is in good agreement with the values recommended in this evaluation. Kelly et al. [611] used a relative method with FTIR detection to determine the ratio k(CF 3 O + CH 4 )/k(CF 3 O + C 2 H 6 ) = 0.01±0.001 at 298±2 K. This does not agree with the ratio of our recommended values, which is 0.017. A relative rate measurement reported by Wallington and Ball [1252], R = 0.0152±0.0023 at 296 K is in good agreement with the recommended rate coefficients. The temperature dependence is from the work of Barone et al., who studied the reaction over the temperature range from 233 to 360 K. Measurements by Bourbon et al. (295–

### 1-60 573 K) gave a higher E/R (642 K). The products are inferred by analogy to other reactions of CF 3 O with organic compounds.

E70. CF 3 O 2 + O 3 . The recommended upper limit is given by the measurements reported by Ravishankara et al. [987] who used chemical ionization detection of CF 3 O 2 with a flow tube reactor. No measurable reaction was observed in their study. The less direct studies of Nielsen and Sehested [880], Maricq and Szente [777] and Turnipseed et al. [1202] all report somewhat larger upper limits to the rate coefficient. An observable reaction was reported in an indirect measurement by Meller and Moortgat [802]. Their result for the CF 3 O + O 3 reaction is not consistent with the value recomme nded above. Their study may have interference from unknown reactions. The products are assumed to be CF 3 O + 2O 2 . E71. CF 3 O 2 + CO. The recommended upper limit is reported by Turnipseed et al. [1200] who used chemical ionization mass spectrometric detection of CF 3 OO with a flow tube reactor at 296 K. This result is at odds with an earlier study by Czarnowski and Schumacher [298], who deduced a "fast reaction" when they observed the thermal decomposition of CF 3 OOOCF 3 to accelerate in the presence of CO at 315–343K. It is possible that the reaction of CF 3 O with CO could account for their observations.

E72. CF 3 O 2 + NO. The recommendation is an average of the room te mperature rate coeffici ents reported by Plumb and Ryan [957], Dognon et al. [358], Peeters et al. [939], Bevilacqua et al. [115], Sehested and Nielsen [1050], Turnipseed et al. [1202], Bourbon et al. [142], and Bhatnagar and Carr [117], all of whom are in excellent agreement. The temperature dependence is derived from the results of Dognon et al. Several studies have confirmed the identity of the products.

F1. O + ClO. There have been five studies of this rate c onstant over an extended temperature range using a variety of techniques: Leu [716]; Margitan [775]; Schwab et al. [1044]; Ongstad and Birks [909]; and Nicovich et al. [873]. The recommended value is based on a least squares fit to the data reported in these studies and in the earlier studies of Zahniser and Kaufman [1354] and Ongstad and Birks [908]. Values reported in the early studies of Bemand et al. [109] and Clyne and Nip [254] are significantly higher and were not used in deriving the recommended value. Leu and Yung [725] were unable to detect O 2 ( 1 ∆ ) or O 2 ( 1 Σ ) and set upper limits to the branching ratios for their production of 4.4 × 10 –4 and 2.5 × 10 –2 respectively.

F2. O + OClO. The recommended value is based on results of the DF-RF study of Gleason et al. [443]. Over the temperature range from 400 K down to 240 K their data ar e well fitted by this Arrhenius expression, but at lower temperatures down to 200 K their data show an abrupt change to a negative temperature dependence. At 200 K the value measured is a factor of 3 higher than that calculated from the Arrhenius expression. Similar results were obtained in a recent study (Toohey, Avallone, a nd Anderson, private communication). Over the temperature range 413 – 273 K their data showed a temperature dependence very similar to that reported by Gleason et al. over the same temperature range. Moreover, as the temperature was lowered further their rate constant values also levelled off and then increased at the lowest temperature. Their rate constant values were nearly 50% lower than the va lues of Gleason et al. from 400 K down to 273 K and 30% lower at 253 K. Colussi [267], using a laser-flash photolysis–resonance fluorescence technique over an extended pressure range, reported a value of the bimolecu lar rate coefficient at r oom temperature 50% higher than the recommended value. Colussi et al. [269] extended these measurements down to 248 K; in contrast to the positive temperature dependence over this temperature range reported by Gleason et al., these authors report a negative temperature dependence. The bimolecular rate constants reported by Colussi et al. are not directly measured but are derived quantities which are consistent with fall-off curves fitted to the experimental data over the pressure range 20–600 torr. It appears that the experiments of Bemand et al. [109], were complicated by secondary chemistry. The results of Colussi and Colussi et al. over an extended pressure range demonstrate the importance of the termolecular reaction O + OClO + M → ClO 3 + M (see entry for this reaction in Table 2). It should be noted that the termolecular rate constants derived by Gleason et al. on the basis of their low temperature data are not consistent with the termolecular rate constant expression recommended in this evaluation (factor of 3 differen ce). The recommended expression is based on the results of Colussi [267] and Colussi et al. [269].

F3. O + Cl 2 O. Recommended value is based on the results of Stevens and Anderson [1114] and Miziolek and Molina [828], which are in good agreement. The significantly lower values of Wecker et al. [1291] are not included, nor are earlier results by Basco and Dogra [82] and Freeman and Phillips [408] due to data analysis difficulties in both studies.

F4. O + HCl. Fair agreement exists between the results of Brown and Smith [157], Wong and Belles [1331], Ravishankara et al. [984], Hack et al. [466] and Singleton and Cvetanovic [1077] at 300 K (some of the values for k(300 K) were obtained by extrapolation of the experimentally determined Arrhenius expressions), but these are a factor of ~7 lower than that of Balakhnin et al. [56]. Unfortunately, the values reported for E/R

### 1-61 are in complete disagreement, ranging from 2260–3755 K. The preferred value was based on the results reported by Brown and Smith, Wong and Belles, Ravishankara et al., Hack et al. and Singleton and Cvetanovic, but not on those reported by Balakhnin et al.

F5. O + HOCl. Recommended value is based on results of Schindler et al. [1035]. In this study the rate constant was found to be practically independent of temperature in the range 213–298 K. Product analysis indicated that Cl atom abstraction is the pr edominant primary reaction channel.

F6. O + ClONO 2 . The results reported by Molina et al. [830] and Kurylo [661] are in good agreement, and these data have been used to derive the preferred Arrhenius expression. The value reported by Ravishankara et al. [980] at 245 K is a factor of 2 greater than those from the other studies, and this may possibly be attributed to (a) secondary kinetic complications, (b) the presence of NO 2 as a reactive impurity in the ClONO 2 , or (c) formation of reactive photolytic products. None of the studies reported identification of the reaction products. The room temperature result of Adler-Golden and Wiesenfeld [11] is in good agreement with the recommended value.

F7. O 3 + OClO. The recommended value is based on results ove r the temperature range 262–296 K reported by Wongdontri-Stuper et al. [1332]. Within the indicated uncertainty limits it also encompasses the somewhat lower room temperature result of Birks et al. [128].

F8. O 3 + Cl 2 O 2 . The recommended upper limit is that determined by DeMore and Tschuikow-Roux [339]. It refers to a temperature of 195 K, and while the reacti on possibly could be faster at higher temperatures, the value of the rate at the higher temperatures would be of no significance because of the thermal decomposition of the dimer.

F9. OH + Cl 2 . The recommended room temperature value is the average of the results reported by Boodaghians et al. [138], Loewenstein and Anderson [750], Ravish ankara et al. [981], and Leu and Lin [721]. The temperature dependence is from Boodaghians et al. Loewenstein and Anderson dete rmined that the exclusive products are Cl + HOCl.

F10. OH + ClO. The reaction has two known product channels under atmospheric conditions: OH + ClO → Cl + HO 2 and OH + ClO → HCl + O 2 . Most studies measure the rate coe fficients for the overall reaction (OH + ClO → products) that is presumably the sum of the two channels. The recommendation for the Cl + HO 2 channel is obtained from the difference between a criti cal assessment of the measurements of the overall reaction and the recommendation for the HCl + O 2 channel as discussed below. The assessment of the overall reaction (OH + ClO → products) is based on a fit to the 219–373 K data of Hills and Howard [508], the 208– 298 K data of Lipson et al. [745], the 234–356 K data of Kegley-Owen et al. [610] and the 298 K data of Poulet et al. [965]. Data reported in the studies of Burrows et al. [181], Ravishankara et al. [981], and Leu and Lin [721] were not used in deriving the recommended value because ClO was not measured directly in these studies and the concentration of ClO was determined by an indirect method. Recent measurements of the overall rate constant by Wang and Keyser ( 218–298 K) [1269], Bedjanian et al. (230–360 K) [100] and Tyndall et al. (298 K) [1211] are consistent with the recommendation. The minor reaction channel forming HCl poses significant experimental difficulties due to the complications associated with the measurement of the HCl reaction product. Early studies inferred the HCl branching ratio without measuring HCl. These included the 298 K measurements of Leu and Lin [721] (>0.65); Burrows et al. [181] (0.85±0.2) and Hills and Howard [508] (0.86±0.14). Poulet et al. [965] measured the HCl product yield to be 0.98±0.12 using mass spectroscopy but their HCl sensitivity was marginal. These studies were not considered in the evaluation. Later studies using mass spectroscopy [744] and diode laser spectroscopy [1270] improved the precision of the HCl product channel measurements. Lipson et al. measured rate constants for the HCl channel over the temper ature range 207–298 K while Wang and Keyser [1270] measured the HCl yield between 218–298 K. obtaining (9.0 ± 4.8) %, independent of temperature. The recommendation for the HCl channel is based on an average of the results of Lipson et al. and the rate expression obtained from the product of the HCl yield of Wang and Keyser and the evaluated overall rate constant as discussed above. Recent measurements by Tyndall et al. [1211] and Bedjanian et al. [100] are noted but are not considered in this evaluation.

F11. OH + OClO. The recommended value is that reported by Poulet et al. [969], the only reported study of this rate constant, using a discharge fl ow system in which OH decay was measured by LIF or EPR over the temperature range 293–473 K. Product HOCl was detected by modulated molecular beam mass spectrometry. The branching ratio for the channel to produce HOCl + O 2 was determined to be close to unity, but experimental uncertainty would allow it to be as low as 0.80.

F12. OH + HCl. The recommended value is based on a least squares fit to the data over the temperature range 240–300 K reported in the studies by Molin a et al. [831], Keyser [622], Ravi shankara et al. [993] and Battin-

### 1-62 Leclerc et al. [86]. In these studies particular attention was paid to the determination of the absolute concentration of HCl by UV and IR spectrophotometry. Earlier studies by Takacs and Glass [1143], Zahniser et al. [1355], Smith and Zellner [1093], Ravishankara et al. [984], Hack et al. [466], Husain et al. [547], Cannon et al. [191], Husain et al. [548], and Smith and Williams [1092] had reported somewhat lower room temperature values. The data of Sharkey and Smith [1056] over the temperature range 138–216 K and BattinLeclerc et al. [86] below 240 K depart from normal Arrhenius behavior. It is unknown whether this is due to an effect such as tunneling at low temperature or a sy stematic experimental erro r. Additional work at low temperature is needed.

F13. OH + HOCl. In the only reported study of this system Ennis and Birks [379] reported the value of this rate constant at room temperature to lie in the range (1.7 – 9.5) × 10 –13 cm 3 molecule –1 s –1

. A temperature-dependent expression has been estimated by choosing a pre-exponential factor by analogy with the OH + H 2 O 2 reaction and selecting the midpoint of the experiment al range for the room temperature rate constant. The large uncertainty factor is need ed to encompass the entire range.

F14. OH + ClNO 2 . The recommended value is based on results of the direct study of Ganske et al. [418,419] using the discharge flow-resonance fluorescence technique. Mass spectrometric studies showed HOCl to be the major chlorine-containing product, with no evidence for a channel to produce HONO 2 + Cl.

F15. OH + ClONO 2 . The results reported by Zahniser et al. [1352] and Ravishankara et al. [980] are in good agreement at ~245 K (within 25%), considering the difficulties associated with handling ClONO 2 . The preferred value is that of Zahniser et al. Neither study reported any data on the reaction products.

F16. OH + CH 3 Cl. The recommended rate expression is derived from a combined fit (for T ≤ 400 K) of the data from the relative rate study by Hs u and DeMore [537] (recalculated ba sed on the current recommendation for the rate constant for the OH + CH 3 CHF 2 reference reaction, as described in the note for that reaction) and the absolute rate studies of Orkin et al. [914] and Herndon et al. [500]. Data from the earlier studies of Howard and Evenson [528], Perry et al. [942], Davis et al. [317], Paraskevopoulos et al. [928], Taylor et al. [1158], and Jeong and Kaufman [586] are reasonably well encompassed within the 2 σ limits. The room temperature value from Taylor et al. [1158] is inconsistent with the higher temperature results in the same study and with the other investigations and lies outside of the 2 σ band, as do the higher room temperature values of Cox et al. [281] and Brown et al. [155].

F17. OH + CH 2 Cl 2 . The recommended values for k(298 K) and E/R are averages of the values from the absolute rate studies of Villenave et al. [ 1233] and Herndon et al. [500] and the relative rate study of Hsu and DeMore [537] (two determinations which ha ve been recalculated based on the cu rrent recommendations for the rate constants of the OH + CH 3 CHF 2 and OH + CH 3 CH 2 F reference reactions). The renormalization procedure for relative rate measurements referenced to the OH + CH 3 CHF 2 reaction is discussed in the note for that reaction. The rate constant determined relative to the rate constant of the OH + CH 3 CH 2 F was renormalized using a rate constant of the reference reaction calcu lated from the data of Schmoltner et al. [1039] and Kozlov et al. [650] above room temperature. The results of Cox et al. [281] and Davis et al. [317] support this recommendation. The results from Taylor et al. [1159], Jeong and Kaufman [586], Perry et al. [942] and Howard and Evenson [528] lie considerably highe r and were not used in deriving the recommended parameters.

F18. OH + CHCl 3 . The recommended value for k(298 K) is an average of the values from the relative rate study of Hsu and DeMore [537] (which has been recalculate d based on the current recommendation for the rate constant of the OH + CH 3 CHF 2 reference reaction, as described in the note for that reaction) and the absolute rate studies of Taylor et al. [1159] (which supersed ed Taylor et al. [1158]), Jeong and Kaufman [586], Davis et al. [317], and Howard and Evenson [528]. The recommended value of E/R is an average of values for this parameter derived in the first four of the above studies.

F19. OH + CCl 4 . The recommended upper limit at 298 K is based on the upper limit reported in the competitive study by Cox et al. [281]. The value given there has been increased by a factor of four to allow for uncertainties in the number of NO molecules oxidized. The recommendation is compatible with the less sensitive upper limits reported by Howard a nd Evenson [528] and Clyne and Holt [243]. None of these investigators reported any evidence for reaction between these species. The A-factor was estimated and a lower limit for E/R was derived.

F20. OH + CH 2 FCl (HCFC-31). The recommended value for k(298 K) is an average of the values from the relative rate study of DeMore [335] (which has been recalculated based on the current recommendation for the rate constant of the OH + CH 2 Cl 2 reference reaction) and the absolute ra te studies of Howard and Evenson [528], Paraskevopoulos et al. [928], Watson et al. [1286], Handwerk and Zellner [480] and Jeong and Kaufman

### 1-63 [586]. The recommended value for E/R is an average of the values for this parameter determined by DeMore and by Watson et al., Handwerk and Zelln er, and Jeong and Kaufman below 400 K.

F21. OH + CHFCl 2 (HCFC-21). The recommended rate expression is derived from a combined fit to the data of Howard and Evenson [528], Perry et al. [942], Watson et al. [1286], Chang and Kaufman [209], Paraskevopoulos et al. [928], Jeong and Kaufman [586], and Fang et al. [382]. The rate constants reported by Clyne and Holt [244] are significantly higher than those from the other seven studies and were not used in deriving the recommended parameters.

F22. OH + CHF 2 Cl (HCFC-22). Results for this compound show very good agreement among both absolute and relative rate constant measurements. The recommended rate expression is derived from a combined fit to the relative rate data of Hsu and DeMo re [538] (which has been recalcu lated based on the current recommendation for the rate constant of the OH + CH 4 reference reaction), and the absolute rate studies of Orkin and Khamaganov [912], Fang et al. [382], Atkinson et al. [43], Watson et al. [1286], Chang and Kaufman [209], Paraskevopoulos et al. [928] and Jeong and Kaufman [586]. The more scattered results of Handwerk and Zellner [480] are in general agreement. The results from the studies of Howard and Evenson [528] and Clyne and Holt [244] are significantly different from those of th e other studies and were not used in the derivation.

F23. OH + CFCl 3 (CFC-11). The A-factor was estimated, and a lower limit for E/R was derived by using the upper limit for the rate constant reported by Chang and Kaufman [210] at about 480 K. This expression is compatible with the upper limits reported by Atkinson et al. [43], Howard and Evenson [528], Cox et al. [281] and Clyne and Holt [243]. None of the investigators reported any evidence for reaction.

F24. OH + CF 2 Cl 2 (CFC-12). The A-factor was estimated, and a lower limit for E/R was derived by using the upper limit for the rate constant reported by Chang and Kaufman [210] at about 480 K. This expression is compatible with the upper limits reported by Atkinson et al. [43], Howard and Evenson [528], Cox et al. [281] and Clyne and Holt [243]. None of the investigators reported any evidence for reaction.

F25. OH + CH 2 ClCH 3 . The recommended value for k(298 K) is an average of the values reported by Howard and Evenson [529], Paraskevopoulos et al. [928], Kasner et al. [608], and Herndon et al. [500]. The recommended value for E/R is an average of the values for this parameter determined by Kasner et al. and Herndon et al. with the value for A calculated to yield the recommended value for k(298 K). Data from the study by Markert and Nielsen [782] were not used to derive the r ecommended parameters, as they are somewhat more scattered.

F26. OH + CH 3 CCl 3 . The recommended value for k(298 K) is an aver age of the values from the absolute rate studies of Talukdar et al. [1156] and Finlayson-Pitts et al. [395], and a relative ra te study of DeMore [332] (recalculated based on the current recommendati on for the rate constant of the OH + CH 4 reference reaction). The temperature dependence is a fit to the data between 243 K and 379 K of Talukdar et al. [1156]. These studies indicate both a lower k(298 K) and E/R than was reported in earlier studies: Nelson et al. [856], Jeong and Kaufman [585], and Kurylo et al. [664]. More recent measurements by Jiang et al. [588] and Lancar et al. [678] yield rate constants that are slightly higher at 298 K than this recommendation.

F27. OH + CH 3 CFCl 2 (HCFC-141b). Both absolute and relative rate measur ements are in exce llent agreement for this compound, and the data are linear over a wide temperature range. The recommended rate expression is derived from a combined fit to the data of Huder and DeMore [541] (two relative rate determinations which have been recalculated based on the current recomme ndations for the rate constants for the reference reactions OH + CH 4 and OH + CH 3 CCl 3 ), Lancar et al. [678], Zhang et al. [1365] (together with the data at 330 K and above from Liu et al. [749], Talukdar et al . [1150] above 253 K (two studies), and Mors et al.[839]. The temperature-dependence data of Brown et al. [154] were not considered because the relatively large rate constants and Arrhenius curvat ure are suggestive of sample impurities.

F28. OH + CH 3 CF 2 Cl (HCFC-142b). The recommended value for k(298 K) is an average of the values from Howard and Evenson [529], Cox et al. [281], Paraskevopoulos et al. [928], Mors et al. [839], Watson et al. [1286], Handwerk and Zellner [480], Liu et al. [749], Gierczak et al . [431], and Fang et al. [383]. The recommended value of E/R is an average of values for this parameter derived in the last five of these studies. The data from Brown et al. [154] and Clyne and Holt [244] were not used to derive the recommended parameters. The 270 K data of Zhang et al. [1365] are in reasonable agreement with the recommendation.

F29. OH + CH 2 ClCF 2 Cl (HCFC-132b). The recommended rate expression was derived from the data of Watson et al. [1288], which were corrected by these au thors for the presence of alkene impurities. The data of Jeong et al. [584], indicating fast er rate constants, may have been affected by such impurities; hence they were not included in deriving the recommendation.

F30. OH + CH 2 ClCF 3 (HCFC-133a). The recommended value of k 298 is the average of the values of Howard and Evenson [529] and Handwerk and Zellner [480] adjusted to 298 K. The recommended temperature

### 1-64 dependence was derived from the data of Handwerk and Zellner [480]. The data of Clyne and Holt [244] were not used in deriving the recommended parameters but (below 400 K) are encompassed within the 2 σ limits.

F31. OH + CHCl 2 CF 2 Cl (HCFC-122). The recommended rate expression is derived from a combined fit to the data of Orkin and Khamaganov [912] (below 400 K) and DeMo re [335] (two determinations which have been recalculated based on the current recommendati ons for the rate constants of the OH + CH 2 Cl 2 and OH + CHCl 2 CF 3 reference reactions).

F32. OH + CHFClCFCl 2 (HCFC-122a). The recommended rate expression was derived from the relative rate data of Hsu and DeMore [538] (recalcula ted based on the current recommendati on for the rate constant for the OH + CH 3 CHF 2 reference reaction, as discusse d in the note for that reaction).

F33. OH + CHCl 2 CF 3 (HCFC-123). The recommended value of k 298 is the average of the values from the absolute studies of Gierczak et al. [431] (two determinations) Liu et al. [749], and Yamada et al. [1342], and from the relative rate study by Hsu and DeMo re [538] (recalculated based on the current recommendation for the rate constant for the OH + CH 3 CHF 2 reference reaction, as discusse d in the note for that reaction). The recommen-dation for the temperature dependence is derived from a fit to the data of these same five investigations. The temperature dependence data of Nielsen [875], Watson et al. [1288], Clyne and Holt [244], and Brown et al. [154] and the room temperature data of Howard and Evenson [529] were not used in the derivations.

F34. OH + CHFClCF 2 Cl (HCFC-123a). The recommended rate expression is based on the data of Orkin and Khamaganov [912].

F35. OH + CHFClCF 3 (HCFC-124). The recommended value for k(298 K) is an average of the values from the studies of Watson et al. [ 1288], Gierczak et al. [431] (2 studies), Yamada et al. [1342], and Hsu and DeMore [538] (two relative rate determina tions which have been recalculated based on the current recommendations for the rate constants of the OH + CH 4 and OH + CHF 2 CHF 2 reference reactions). The room temperature rate constant of Howard and Evenson [529] is considerably higher than these other values and was not included in the average. The recommended temperature dependence is an average of the dependencies derived from these same studies (but using only data below 400 K from Gierczak et al. [431] and Yamada et al. [1342].

F36. OH + CH 3 CF 2 CFCl 2 (HCFC-243cc). The recommended rate expression is derived from the temperaturedependence data of Nelson et al. [852]. Although there is only a single study of this reaction, the uncertainties have been assigned to reflect our belief that the rate constant for this reaction should be less than that for OH + CH 3 CF 2 Cl.

F37. OH + CHCl 2 CF 3 CF 2 (HCFC-225ca). The recommended value for k(298 K) is an average of the values from Nelson et al. [852] and Zhang et al. [1366]. The recommendation for E/R is taken from Nelson et al. [852]. The temperature-dependence data of Br own et al. [153] were not considered because th e relatively large rate constants at and below room temperature and the A rrhenius curvature are sugge stive of sample impurities. The temperature dependence results of Zhang et al. [ 1366] are in reasonable agreement with those of Nelson et al. [852] over the temperature range of measurement overlap. However, the complete Zhang et al. [1366] data set yields a value for E/R much larger than currently recommended for the OH + CHCl 2 CF 3 (HFC-123) reaction, for which the activation energy should be similar.

F38. OH + CF 2 ClCF 2 CHFCl (HCFC-225cb). The recommended rate expression is derived from a combined fit to the temperature-dependence data of Nelson et al. [852] and Zhang et al. [1366], which are in excellent agreement.

F39. OH + CH 2 =CHCl. The recommended value for k(298 K) is an average of the values reported by Howard [526], Perry et al. [941], Liu et al. [748] and [1343]. The recommended value for E/ R is an average of the values for this parameter derived from fits to the data of Perry et al., Liu et al. and Yamada et al. at temperatures below about 400 K. In the 400–500 K region the rate constant levels off before increasing at higher temperatures, suggesting the stronger importance of an abstraction mechanism at the higher temperatures.

F40. OH + CH 2 =CCl 2 . The recommended value for k(298 K) is an average of the values reported by Edney et al. [373], Tuazon et al. [1191], Abbatt and Anderson [1], Zhang et al. [1367], Canosa-Mas et al. [193] and [1341]. The recommended value for E/R comes from a combined fit to the data of Abbatt and Anderson, Zhang et al. and Yamada et al. The data of Kirchner et al. [628] were not used in deriving the recommended parameters since they were obtained at very low pr essure and the much stronger temperature dependence obtained may be indicative of a pressure dependence above room temperature.

### 1-65 F41. OH + CHCl=CCl 2 . The recommended value for k(298 K) is the mean of the values reported by Howard [526], Chang and Kaufman [209], Kirchner et al. [628], Kl opffer et al. [638], Edney et al. [373] and Tichenor et al. [1172]. The recommended value of E/R is an average of va lues for this parameter derived by Chang and Kaufman [209], Kirchner et al. [628] and Tichenor et al. [1172]. The value for k(298 K) derived from a relative rate study by Winer et al. [1327] is a factor of ~2 greater than the other values and is not considered in deriving the preferred value. An absolute study by Jiang et al. [589] yielding a significantly higher value for k(298 K) as well as a considerably stronger temp erature dependence (E/R = –970 K) is assumed to be superseded by Tichenor et al. [1172].

F42. OH + CCl 2 =CCl 2 . The recommended value for k(298 K) is the mean of the values reported by Howard [526], Chang and Kaufman [209], and Kirchner et al. [628]. The room temperature value reported by Winer et al. [1327] is more than a factor of 10 greater and was not used in deriving the recommendation. The recommended value for E/R is an average of values fo r this parameter derived by Chang and Kaufman [209] and Kirchner et al. [628]. A study by Tichenor et al. [1173] yields a value for k(298 K) slightly lower than these other studies, but a temperature dependence less than half of that recommended. While these latest results were not used in deriving the recommendations, they are encompassed within the 95% confidence limits.

F43. OH + CH 3 OCl. The recommended rate expression is derived from a fit to the data of Crowley et al. [294], the only reported study of this reaction.

F44. OH + CCl 3 CHO. The recommended value for k(298 K) is an average of the values reported by Barry et al. [78] (using three independent techniques), Dobe et al. [350], Nelson et al. [856], Ballestra-Garcia et al. [59], and Scollard et al. [1045]. The temperature dependence is derived from a fit to the data of Dobe et al. [350]. The A factor was then calculated to agree with the recommended value for k(298 K).

F45. HO 2 + Cl. The recommendations for the two reaction channels are based upon the results by Lee and Howard [703] using a discharge flow system with laser magnetic resonance detection of HO 2 , OH, and ClO. The total rate constant is temperature independent with a value of (4.2±0.7) × 10 –11 cm 3 molecule –1 s –1 over the temperature range 250–420 K. This value for the total rate constant is in agreement with the results of indirect studies relative to Cl + H 2 O 2 (Leu and DeMore [717], Poulet et al. [967], Burrows et al. [176]] or to Cl + H 2 (Cox [275]). The contribution of the reaction channel producing OH + ClO (21% at room temperature) is much higher than the upper limit reported by Burrows et al. (1% of total reaction). Cattell and Cox [206], using a molecular modulation-UV absorption technique over the pressure range 50–760 torr, report results in good agreement with those of Lee and Howard both fo r the overall rate constant and for the relative contribution of the two reaction channels. A study by Dobis and Benson [355] reports a total rate constant in good agreement with this recommendation but a much lower contribution (5±3%) of the channel producing OH + ClO. The rate constant for the channel producing ClO + OH can be combined with that for the reaction ClO + OH > Cl + HO 2 to give an equilibrium constant from which a value of the heat of formation of HO 2 at 298 K of 3.0 kcal/mol can be derived.

F46. HO 2 + ClO. Three new studies by Nickolaisen et al [865], Knight et al. [640], and Laszlo et al. [682] have been added to the previous five studies of this rate constant (Reimann and Kaufman, [999]; Stimpfle et al. [1122]; Leck et al. [691]; Burrows and Cox [177]; Cattell and Cox [206]). The studies span a wide variety of pressure conditions and detection techniques. The studies of Cattell and Cox and Nickolaisen et al. were performed over extended pressure ranges and indicat e that the reaction is pressure independent. However, the room temperature rate constant obtai ned by averaging the five low pressu re (< 10 torr) studies is slightly lower (5.1 ± 1.5 vs. 6.5 ± 1.2 in units of 10 –12 cm 3 molecule –1 s –1 ) than that obtained by averaging the higher pressure measurements (> 50 torr). Although within the combined uncertainty, this offset may suggest possible systematic experimental complications (e.g. unknown secondary reactions) in the low or high pressure experiments. The recommended value for k(298 K) is the mean of the eight studies. Temperaturedependence data has been obtained by Stimpfle et al., Nickolaisen et al., Knight et al., and Laszlo et al. The earliest study (Stimpfle et al.) observed nonlinear Arrhenius behavior. The data were best described by a four parameter equation of the form n k=Aexp(-B/T) CT + , possibly suggesting that two different mechanisms may be occurring. The more recent studies find the T-dependence to display linear Arrhenius behavior over the entire temperature range. Moreover, they derive much smaller E/R values (17 to 312) than that obtained by Stimpfle (E/R ≈ 700 for T<300 K). The recommended value for E/R is ba sed on an average of the four studies over their entire temperature ranges. The two most probable pairs of reaction products are, (1) HOCl + O 2 and (2) HCl + O 3 . Leu [715], Leck et al., Knight et al., and Laszlo et al. used mass spectrometric detection of ozone to place upper limits on channel 2 of 1.5%, 2%, 1%, and 2%, respectively at 298 K. In addition, Leck et al. and Laszlo set upper limits of 3.0% (248 K); and 5.0% (243 K), respectively, on k 2 /k. Burrows and Cox report an upper limit of 0.3% for k 2 /k at 300 K. Finkbeiner et al. [394], using matrixisolation/FTIR spectroscopy, studied product formation between 210 and 300 K at 700 torr. HOCl was

### 1-66 observed as the dominant product (> 95% at all temperatures). The branching ratio values for k 2 /k were determined to be <1% at 300 K and 270 K, 2±1% at 240 K, and 5±2% at 210 K. No evidence for any other product channel was found. Theoretical calculations by Ni ckolaisen et al. suggest th at the reaction to channel (1) proceeds mainly through the ClO-HO 2 complex on the triplet potential surface. However, these calculations also suggest that collisionally stabili zed HOOOCl formed on the singl et surface will possess an appreciable lifetime. Further studies on po ssible formation of HOOOCl are warranted.

F47. H 2 O + ClONO 2 . This recommendation is based on the upper limits to the homogeneous bimolecular rate constant reported by Atkinson et al. [ 49], and by Hatakeyama and Leu [487,488]. Atkinson et al. observed by FTIR analysis the decay of ClONO 2 in the presence of H 2 O in large-volume (2500 and 5800 liters) Teflon or Teflon-coated chambers. Their observed decay rate gives an upper limit to the homogeneous gas phase rate constant, and they conclude that the decay observed is due to heterogeneous processes. Hatakeyama and Leu, using a static photolysis system with FTIR analysis, derive a similar upper limit. Rowland et al. [1008] concluded that the decay they observed re sulted from rapid heterogeneous processes. The homogeneous reaction is too slow to have any significant effect on atmospheric chemistry.

F48. NO + OClO. The Arrhenius expression was estimated based on 298 K data reported by Bemand, Clyne and Watson [109].

F49. NO + Cl 2 O 2 . The recommended upper limit is that determined by Friedl (private communication) in a study using a DF-MS technique.

F50. NO 3 + HCl. The recommended upper limit is that reported by Mellouki et al. [807] in a study using DF-EPR techniques. This upper limit shows that this reaction is of ne gligible importance in stratospheric chemistry. Somewhat lower upper limits have been reported by Cantrell et al. [197] and Canosa-Mas et al. [194]; the latter study also reports Arrhenius parameters at higher temperatures (333–473 K).

F51. HO 2 NO 2 + HCl. This upper limit is based on results of static photolysis-FTIR experiments reported by Leu et al. [720].

F52. Cl + O 3 . The results reported for k(298 K) by Watson et al. [1287], Zahniser et al. [1356], Kurylo and Braun [665], Clyne and Nip [253], Nicovich et al. [868] and Seeley et al. [1046] are in good agreement, and have been used to determine the pref erred value at this temperature. The values reported by Leu and DeMore [717] (due to the wide error limits) and Clyne and Watson [259] (the value is inexplicably high) are not considered. The six Arrhenius expressions are in fair agreement within the temperature range 205–300 K. In this temperature range, the rate constants at any particular temperature agree to within 30–40%. Although the values of the activation energy obtained by Watson et al. and Kury lo and Braun are in excelle nt agreement, the value of k in the study of Kurylo and Braun is consistently (~17%) lower than that of Watson et al. This may suggest a systematic underestimate of the rate constant, as the values from the other three agree so well at 298 K. The two most recent studies (Nicovi ch et al. and Seeley et al.) obtai ned significantly smaller temperature dependences than those observed in the earlier studies. There is no reason to prefer any one set of data to any other; therefore, the preferred Arrhenius expression s hown above was obtained by computing the mean of the six results between 205 and 298 K. DeMore [331] directly determined the ratio k(Cl + O 3 )/k(Cl + CH 4 ) at 197–217 K to be within 15% of that calculated from the absolute rate constant values recommended here. Vanderzanden and Birks [1226] have interpreted thei r observation of oxygen atoms in this system as evidence for some production (0.1–0.5%) of O 2 ( 1

g + 

### Σ ) in this reaction. The possible production of singlet molecular oxygen in this reaction has also been discussed by DeMore [328], in connection with the Cl 2 photosensitized decomposition of ozone. However Choo and Leu [228] were unable to detect O 2 ( 1 Σ ) or O 2 ( 1 ∆ ) in the Cl + O 3 system and set upper limits to the branching ratios for their production of 5 × 10 –4 and 2.5 × 10 –2 , respectively. They suggested two possible mechanisms for the observed production of oxygen atoms, involving reactions of vibrationally exc ited ClO radicals with O 3 or with Cl atoms, respectively. Burkholder et al. [172], in a study of infrared line intensities of th e ClO radical, present evidence in support of the second mechanism. In their experiments with excess Cl atoms, the vibrationally excited ClO radicals produced in the Cl + O 3 reaction can react with Cl atoms to give Cl 2 and oxygen atoms, which can then remove additional ClO radicals. These authors point out the possibility for systematic error from assuming a 1:1 stoichiometry for [Cl]:[O 3 ] o when using the Cl + O 3 reaction as a quantitative source of ClO radicals for kinetic and spectroscopic studies.

F53. Cl + H 2 . This Arrhenius expression is based on the data below 300 K reported by Watson et al. [1285], Lee et al. [694], Miller and Gordon [826] , and Kita and Stedman [631]. The results of these studies are in excellent agreement below 300 K; the data at higher temperatures are in somewhat poorer agreement. The results of Watson et al., Miller and Gordon, and K ita and Stedman agree well (after ex trapolation) with the results of Benson et al. [112] and Steiner and Rideal [1109] at higher temperatures. For a discussion of the large body

### 1-67 of rate data at high temperatures, see the review by Baulch et al. [89][86]. The room temperature value ofKumaran et al. [656], in a study primarily at high temperatures, is in excellent agreement with this recommendation. Miller and Gordon and Kita and Stedman also meas ured the rate of the reverse reaction, and found the ratio to be in good agreemen t with equilibrium constant data.

F54. Cl + H 2 O 2 . The absolute rate coefficients determined at ~298 K by Watson et al. [1287], Leu and DeMore [717], Michael et al. [824], Poulet et al. [967] and Keyser [617] range in value from (3.6–6.2) × 10 –13

. The studies of Michael et al., Keyser, and Poulet et al. are presently c onsidered to be the most reliable. The preferred value for the Arrhenius expression is taken to be that reported by Keyser. The A-factor reported by Michael et al. is considerably lowe r than that expected from theoretical considerations and may possibly be attributed to decomposition of H 2 O 2 at temperatures above 300 K. The data of Michael et al. at and below 300 K are in good agreement with the Arrhenius expression reported by Keyser. More data are required before the Arrhenius parameters can be considered to be well-established. Heneghan and Benson [498], using mass spectrometry, confirmed that this reaction pro ceeds only by the abstracti on mechanism giving HCl and HO 2 as products.

F55. Cl + NO 3 . The recommended value at room temperature is based on the discharge flow-EPR study of Mellouki et al. [805] and the discharge flow-mass spectrometric study of Becker et al. [92]. The results of these direct absolute rate studies ar e preferred over results of the earlier relative rate studies of Cox et al. [276], Burrows et al. [180], and Cox et al. [287], in all of which NO 3 was monitored in the photolysis of Cl 2 - ClONO 2 -N 2 mixtures. Complications in the chemistry of the earlier systems probably contributed to the spread in reported values. This radical-radical reaction is expect ed to have negligible temperature dependence, which is consistent with the results from the study of Cox et al. [287] in which the complications must have been temperature independent.

F56. Cl + N 2 O. This rate coefficient has been determined in a study of the halogen-catalyzed decomposition of nitrous oxide at about 1000 K by Kaufman et al. [609]. The largest value reported was 10 –17 cm 3 molecule –1

s –1 , with an activation energy of 34 kcal/mol. Extrapolation of these results to low temperature shows that this reaction cannot be of any significance in atmospheric chemistry.

F57. Cl + HNO 3 . The recommended upper limit at room temperature is that reported in the study of Wine et al. [1324], in which long-path laser absorption spectroscopy was used to look for the appearance of NO 3 following the pulsed laser photolysis of Cl 2 -HNO 3 mixtures with no evidence for NO 3 production was observed. In the same study a less sensitive upper limit wa s derived from monitori ng Cl atom decay by resonance fluorescence. A less sensitive upper limit was also found in the discharge flow-EPR study of Zagogianni et al. [1350]. Higher values obtained in earlier studies (Leu and DeMore [717], Kurylo et al. [671], and Clark et al. [234]) as well as the higher temperature results of Poulet et al. [967] are not used.

F58. Cl + HO 2 NO 2 . The only study of this reaction is by Simonaitis and Leu [1072] using the low pressure discharge flow technique coupled with resonance fluores cence detection of Cl and mass spectrometric detection of HO 2 NO 2 ion fragments. Consistent results were obtained monitoring either Cl or HO 2 NO 2 decays and retrieved rate constants were less than 1 × 10 –13 cm 3 molecule –1 s –1 for all conditions. Impurities in the HO 2 NO 2 sample (especially H 2 O 2 ) complicated the measurements. A limited temperature study over the 298– 399 K range suggests that E/R is in the range of 500 – 1500. Given the experimental difficulties, only an upper limit is recommended for the reaction rate.

F59. Cl + CH 4 . The values of k at 298 K reported from thirteen absolute rate constant studies (Manning and Kurylo [770], Whytock et al. [1303], Michael and Lee [817], Lin et al. [740], Zahniser et al. [1351], Keyser [615], Ravishankara and Wine [988], Heneghan et al . [499], Dobis and Benson [353], Sawerysyn et al. [1031], Beichert et al. [107], Seeley et al. [1046], and Pilgrim et al. [950]) fall in the range (0.92 – 1.13) × 10

–
13 , with a mean value of 0.99 × 10 –13

. An earlier absolute study by Watson et al. [1287] gives rate constant values slightly higher than those of the aforementioned studies, which may be due to uncertainties in correcting the data for OH loss via r eaction with trace levels of ethane and propane in the methane samples used. The values derived for k at 298 K from the competitiv e chlorination studies of Pritchard et al. [970], Pritchard et al. [971], Knox [641], Knox and Nelson [643], Lee and Rowland [692], and Lin et al. [740] range from (0.8–1.6) × l0 –13 when the original data are referenced to the presently recommended rate constant values for the reactions of Cl with H 2 and C 2 H 6 . Of these relative rate studies, that of Lin et al. [740], yields a room temperature rate constant (1.07 × 10 –13 ) that is most consistent with the absolute measured values. Thus, the recommended value for k at 298 K (1.0 × 10 –13 ) is derived from an unweighted average of the rate constants from the thirteen preferred absolute studies and the relative rate study of Lin et al. [740].

There have been nine absolute studi es of the temperature dependence of k in which the measurements extend below 300 K (Watson et al. [1287], Manning and Kurylo [770], Whytock et al. [1303], Lin et al. [740],

### 1-68 Zahniser et al. [1351], Keyser [615], Ravishankara and Wine [988], Heneghan et al. [499], and Seeley et al. [1046]). In general, the agreement among most of these studies is quite good. However, systematic differences in activation energies are apparent when calculated using data obtained below 300 K versus data from above 300 K. Three resonance fluorescence studies have b een performed over the temperature region between 200 and 500 K (Whytock et al . [1303], Zahniser et al. [1351] and Keyser [615]), and in each case a strong non-linear Arrhenius behavior was observed. Ravishankara and Wine [988] also noted nonlinear Arrhenius behavior over a more limited temperature range. This behavior tends to partially explain the variance in the values of E/R reported between those investigators who mainly studied this reaction below 300 K (Watson et al. [1287], Manning and Kurylo [770], and Seeley et al. [1046])] and those who only studied it above 300 K (Clyne and Walker [258], Poulet et al. [966], and Lin et al. [740]). The agreement between all studies below 300 K is reasonably good, with values of E/R ranging from (1063–1320) K, and k(230 K) in the range (2.6–3.2) × 10 –14

. There have not been any absolu te studies at stratospheric temperatures other than those which utilized the resonance fluorescence technique. Ravishankara and Wine [988] have suggested that the re sults obtained using the discharge flow and competitive chlorination techniques may be in error at the lower temper atures (<240 K) due to a non-equilibration of the 2 P 1/2 and 2 P 3/2 states of atomic chlorine. Ravishankara and Wine observed that at temperatures below 240 K the apparent bimolecular rate constant was depe ndent upon the chemical composition of the reaction mixture; i.e., if the mixture did not contain an efficient spin equilibrator, e.g., Ar or CCl 4 , the bimolecular rate constant decreased at high CH 4 concentrations. The chemical composition in each of the flash photolysis studies contained an efficient spin equilibrator, whereas this was not the case in the discharge flow studies. However, the reactor walls in the discharge flow studies could have been expected to have acted as an efficient spin equilibrator. Consequently, until the hypothesis of Ravishankara and Wine is proven it is assumed that the discharge flow and competitive chlorination results are reliable. A composite unweighted Arrhenius fit to all of the temperature dependent absolute studies with data in the temperature region ≤ 300 K (with the exception of the data of Watson et al. [1287], which appear to be systematically high due to reactive impurities) yields E/R = 1253 K and k(298 K) = 1.0 × 10 –13

. The competitive chlorination results differ from those obtained in the absolute studies in that linear Arrhenius behavior is observed. The values of E/R are consistently larger than those obtained from the absolute studies, with an average value of approximately 1500 K. Until the hypothesis of Ravisha nkara and Wine [988] is reexamined, the preferred Arrhenius expression attempts to best fit the results obtained between 200 and 300 K from all sources. Thus, using the relative rate results of Lin et al. [740] (referenced to the current recommendation for the Cl + C 2 H 6 reaction) as representative of the relative rate studies below 300 K, together with the composite fit to the absolute studies given above, we obtain a recommended E/R value of 1360 K. Taken with the recommended value for k(298 K) = 1.0 × 10 –13 , we compute an Arrhenius A factor of 9.6 × 10 –12

. However, the A-factor thus derived seems somewhat low (on a per hydrogen atom basis) when compared with the A-factors for some similar reactions.

F60. Cl + CH 3 D. Recommended value is based on results of Wallington and Hurley [1259].

F61. Cl + H 2 CO. The results from five of the six published studies (Michael et al. [821], Anderson and Kurylo [25], Niki et al. [885], Fasano and Nogar [385] and Poulet et al. [962]) are in good agreement at ~298 K, but are ~50% greater than the value reported by Foon et al. [403]. The preferred value at 298 K was obtained by combining the absolute values repor ted by Michael et al., Anderson and Kurylo, and Fasano and Nogar, with the values obtained by combining the ratio of k(Cl + H 2 CO)/k(Cl + C 2 H 6 ) reported by Niki et al. (1.3±0.1) and by Poulet et al. (1.16±0.12) with the preferred value of 5.7 × 10 –11 for k(Cl + C 2 H 6 ) at 298 K. The preferred value of E/R was obtained from a least squares f it to all the data reported in Michael et al. and in Anderson and Kurylo. The A-factor was adjusted to yield the preferred value at 298 K. F62. Cl + HC(O)OH. The room temperature kinetics of this reaction have been studied by Wallington et al. [1245] and Li et al. [728]. Wallington et al. used a relative rate technique at atmospheric pressu re while Li et al. employed flash photolysis and operated at 10 torr. The results of the two studies are in excellent agreement and have been averaged together to derive the recommended value. Reaction products have been investigated by Tyndall et al. [1221] at room temperature and 700 torr pressure. They measured the CO 2 yield to be 96 ± 5% and suggested that the HOCO complex reacted with either O 2 or Cl 2 in their experiment to give the observed product.

F63. Cl + CH 3 O 2 . Recommended value is based on results of Maricq et al. [780], Jungkamp et al. [598], and Daele and Poulet [299]. All three studies agree that this overall reaction is very fast. However, there is a discrepancy in the reported values of the branching ratios for the two pathways producing ClO + CH 3 O (a) and HCl + CH 2 O 2 (b). The branching ratio for the reaction channels producing HCl + CH 2 O 2 (b) has been reported to be 50% by both Maricq et al. [780] and Jungkamp et al., but has been reported to be 90% by Daele and Poulet. Because of this large discrepancy no branching ratios are recommended.

### 1-69 F64. Cl + CH 3 OH. This recommendation at 298 K) is based on results of the absolute rate studies of Michael et al. [822], Payne et al. [937], Dobe et al. [351], Pagsberg et al. [924] and Tyndall et al. [1214], and results obtained in the competitive chlorination studies of Walli ngton et al. [1267], Lightfoot et al. [733], Nelson et al. [855] and Tyndall et al. The temperature independence of the rate constant was reported by Michael et al. in a direct study. This is consistent with the indirect results of Lightfoot et al. who deduced the rate coefficient for this reaction relative to that for methane as a function of temperature. This reaction can have two sets of products: CH 2 OH + HCl, channel (a) and CH 3 O + HCl, channel (b). Product analysis and isotopic substitution have established that the reaction pro ceeds via channel (a) rather than via channel (b). See Radford [973], Radford et al. [974], Meier et al. [800], and Payne et al. [937]. This reaction has been used in the laboratory as a source of CH 2 OH and as a source of HO 2 by the reaction of CH 2 OH with O 2 . F65. Cl + CH 3 OOH. The only study of this reaction was by Wallington et al [1245], who measured the rate relative to Cl + C 2 H 6 at 295 K and atmospheric pressure.

F66. Cl + CH 3 ONO 2 . This reaction has been studied at 298 K by Nielsen et al [881] using a relative rate technique. The reference compound was ethane. The recommended value is adjusted fro m that given by Nielsen et al. using the currently recommended value for k (Cl + C 2 H 6 ). The temperature dependence is estimated by assuming an A-factor equal to approximately 20 times that of OH + CH 3 ONO 2 . This is consistent with observed OH/Cl A-factor ratios for primary H-abstraction from alkanes.

F67. Cl + C 2 H 6 . The absolute rate coefficients reported in all four studies (Davis et al. [314], Manning and Kurylo [770], Lewis et al. [726], and Ray et al. [995]) are in good agreement at 298 K. The value reported by Davis et al. was probably overestimated by ~10% (the authors assumed that I f was proportional to [Cl] 0.9 , whereas a linear relationship between I f and [Cl] probably held under their experimental conditions). The preferred value at 298 K was taken to be a simple mean of the four values (the value reported by Davis et al. was reduced by 10%), i.e., 5.7 × 10 –11

. The two values reported for E/R are in good agreement; E/R = 61 K (Manning and Kurylo) and E/R = 130 K (Lewis et al.). A simple least squares fit to all the data would unfairly weight the data of Lewis et al. due to the larger temperature range covered. Therefore, the preferred value of 7.7 × 10 –11 exp(–90/T) is an expression which best fits the data of Lewis et al. and Manning and Kurylo between 220 and 350 K. The recent temperature-dependent resu lts of Dobis and Benson [354] and room temperature results of Kaiser et al. [602], Hooshiyar and Niki [521] and Beichert et al. [107] are in good agreement with the recommendation.

F68. Cl + C 2 H 5 O 2 . Recommended value is based on results of Maricq et al. [780].

F69. Cl + CH 3 CH 2 OH. The rate coefficient for this reaction has been studied at 298 K by four groups using a relative rate technique: Nelson et al. [855] (relative to Cl + cyclohexane), Wallington et al. [1267] (relative to Cl + C 2 H 6 ), Edelbuttel-Einhaus et al. [372] (relative to Cl + C 2 H 6 ), and Taatjes et al. [1139]. Nelson et al measured this rate constant relative to the Cl + cyclohexane while the others used the Cl + C 2 H 6 reaction. Taatjes et al. also measured this rate coefficient by measuring the temporal profile of the HCl product. The agreement between these five measurements is quite good, yielding an average value that is recommended. The temperature dependence of this rate coefficient is based on the results of Taatjes et al., who studied this reaction above 298 K and found it to be e ssentially independent of temperature. We recommend the same independence of temperature at atmospheric temperatures. This reaction can have three sets of products: CH 2 CH 2 OH + HCl, channel (a); CH 3 CHOH, channel (b); and CH 3 CH 2 O channel (c). Taatjes et al. have deduced that channel (c) is negligible and that channel (a) is about 8% at 298 K. Therefore, the majority of reaction is expected to occur via channel (b). It is very unlikely that these branching ratios will change significantly at lower atmospheric temperatures.

F70. Cl + CH 3 C(O)OH. Koch and Moortgat [645] have studied this reaction at room temperature using the relative rate technique. Deuterium substitution of the methyl hydrogens decreased the observed rate by a factor of 3.75. In addition, CO and CO 2 reaction products were observed in a stoichiometric ratio of 1:1. These observations were interpreted in terms of methyl hydrogen abstraction from acetic acid to form the CH 2 C(O)OH radical followed by reaction with O 2 to form a peroxy radical. Thermal decomposition of the peroxy radical produces HCHO, CO 2 , and atomic H. In the laboratory system, the HCHO reacts with atomic chlorine to yield CO.

F71. Cl + CH 3 CN. The recommendation is based on results of the study of Tyndall et al. [1216]. The results of this study, using both relative and absolute methods and measured over a wide range of experime ntal conditions are preferred over the results of earlier studies of Kurylo and Knable [667], Poulet et al. [961], and Olbregts et al. [906]. Product studies reported by Tyndall et al. show that reaction proceeds predominantly by hydrogen atom abstraction.

### 1-70 F72. Cl + C 2 H 5 ONO 2 . Wallington et al. [1258] a nd Nielsen et al [881] have measured the rate of this reaction at room temperature relative to atomic chlorine reac tions with ethyl chloride and ethane, respectively. The two studies are in excellent agreem ent and the recommended value is based on an average of the two. The values given in Wallington et al a nd Nielsen et al. were ad justed based on the currently accepted values of the reference rate constants. The temperature dependence is estimated by assuming an A-factor equal to approximately 20 times that of OH + CH 3 ONO 2 . This is consistent with observed OH/Cl A-factor ratios for primary H-abstraction from alkanes.

F73. Cl + CH 3 CO 3 NO 2 (PAN). The recommended value is based on results of the relative rate study of Wallington et al. [1245]. In this study no reaction of PAN was observed in the presence of Cl atoms. These results are preferred over the results of the direct study of Tsalkani et al. [1187] using a discharge flow system with EPR detection of Cl atom d ecay (in which study the authors reporte d a rate constant of (3.7±1.7) × 10 –13 cm 3 molecule –1 s –1 ). In both studies the major impurity in the PAN samples would be the alkane solvent. The presence of 0.1% tridecane in the PAN sample used by Tsalkani et al. could account for the observed Cl atom decay; however, solvent impurities in the PAN sample would be of no consequence in the relative rate study of Wallington et al.

F74. Cl + C 3 H 8 . The recommended room temperature value is the mean of results of the competitive chlorination studies of Pritchard et al. [971] , Knox and Nelson [643], Atkinson and Aschmann [ 35], Wallington et al. [1267], and Hooshiyar and Niki [521], and the absolute rate studies of Lewis et al. [726] and Beichert et al. [107]. The temperature dependence is from Lewis et al. The A-factor from that st udy has been adjusted slightly to fit the recommended room temperature value.

F75. Cl + CH 3 C(O)CH 3 . The rate coefficient for this reaction has only been reported at 298 K. Wallington et al. [1267] and Olsson et al. [907] report values of 2.37 × 10 –12 and 1.69 ×10 –12 cm 3 molecule –1 s –1 at 298 K measured via relative rate methods. The only direct measurement of this rate constant is by Notario et al. [900] who report a value of (3.06 ± 0.38) × 10 –12 cm 3 molecule –1 s –1 at 298 K. Because of the reasons noted by Wallington et al. [1267], the value reported by Olsson et al. is suspect and is not considered here. The average of the results from Wallington et al. and Notario et al. is recommended for k(298 K). In the absence of temper-ature dependent measurements, based on anal ogy with other Cl atom reactions with halogenated hydrocarbons whose rate coefficients at 298 K are close to that for Cl + CH 3 C(O)CH 3 , we recommend an E/R value of 1000 K with a g value of 500 K. Such a temper ature dependence is consistent with this reaction proceeding via H atom abstraction. This E/R and k(298 K) lead to an A factor of 7.7 × 10 –11 cm 3 molecule –1

s –1

. This A factor is the same as that for the reaction of Cl atom with ethane, which also contains six primary C–H bonds. End product studies clearly show th at the products of this reaction are CH 3 C(O)CH 2 and HCl.

F76. Cl + C 2 H 5 CO 3 NO 2 . Wallington et al. [1245] have measured this rate constant relative to Cl + CH 3 Cl. The recommended value is adjusted from that given by Wallington et al. using the currently recommended value for the reference reaction rate constant.

F77. Cl + 1-C 3 H 7 ONO 2 . Wallington et al. [1258] a nd Nielsen et al [881] have measured the rate of this reaction at room temperature relative to atomic chlorine reac tions with ethyl chloride and ethane, respectively. The two studies are in excellent agreem ent and the recommended value is based on an average of the two. The values given in Wallington et al a nd Nielsen et al. were ad justed based on the currently accepted values of the reference rates. The temperature dependence is estimated by assuming an A-factor equal to approximately 20 times that of OH + CH 3 ONO 2 . This is consistent with observed OH/Cl A-factor ratios for primary Habstraction from alkanes.

F78. Cl + 2-C 3 H 7 ONO 2 . This reaction has been measured by Wallington et al [1258] at 295 K relative to Cl + C 2 H 5 Cl. The reported ratio of 0.46 ± 0.03 has been converted to an absolute rate using the currently recommended value for the ethyl chloride reaction rate. The temperature dependence is estimated by assuming an A-factor equal to approximately 20 times that of OH + CH 3 ONO 2 . This is consistent with observed OH/Cl A-factor ratios for primary H-abstraction from alkanes.

F79. Cl + OClO. The data of Toohey [1181] are in good agreement with the results of Bemand et al. [109] at room temperature, and the recommended value at room temperat ure is the mean of the values reported in these two studies. The slight negative temperature dependence repor ted by Toohey [1181] is accepted but with error limits that encompass the temperature i ndependence reported in the earlier study.

F80. Cl + ClOO. The recommended value is based on the results of studies by Mauldin et al. [792] and Baer et al. [54], in which ClOO was formed by the pulsed photolysis of Cl 2 /O 2 mixtures and its overall loss rate was monitored by UV absorption. In both studies k was found to be independent of temperature. These results are preferred over the results of the earlier, indirect studies of Johnston et al. [590], Cox et al. [282], and Ashford et al. [32]. The earlier studies did show that the predominant reaction pathway is that yielding Cl 2 + O 2 as

### 1-71 products. From the branching ratio data of Cox et al., Ashford et al., and Nicholas and Norrish [863], it can be estimated that this reaction channel constitutes 95% of the overall reaction with ClO + ClO the products of the minor (5%) reaction channel.

F81. Cl + Cl 2 O. The preferred value was determined from results of the temperature-dependent study of Stevens and Anderson [1114] and the results of two independent ab solute rate coefficient studies reported by Ray et al. [995], which used the discharge flow-resonance fluorescence and discharge flow-mass spectrometric techniques. This value has been confirmed by Burrows and Cox [177], who determined the ratio k(Cl + Cl 2 O)/k(Cl + H 2 ) = 6900 in modulated photolysis experiments. The earlier value reported by Basco and Dogra [80] has been rejected.

F82. Cl + Cl 2 O 2 . The recommended value is that determined by Friedl (private communication) in a study using a DF-MS technique. It is in agreement with the value reported by Cox and Hayman [289] in a study using a static photolysis technique with photodiode array UV spectroscopy.

F83. Cl + HOCl. This recommendation is based on results over the temperature range 243–365 K reported by Cook et al. [270] and the room temperature result of Vogt and Schindler [1235]. There is a significant discrepancy in the reported values of the product branching ratios. Ennis and Birks [378] reported that the major reaction channel is that to give the products Cl 2 + OH with a yield of 91±6%, whereas Vogt and Schindler report this yield to be 24±11%, with the major reaction channel giving HCl + ClO as products.

F84. Cl + ClNO. The discharge flow-resonance fluorescence study of Abbatt et al. [4] provides the first reliable data on the temperature dependence. The laser photolysis-LMR study of Chasovnikov et al. [213] provides rate data for each Cl atom spin st ate, and they attribute the low valu e reported by Nelson and Johnston [854] in a laser flash photolysis-resonance fl uorescence study to reaction of the Cl 2 P 1/2 state. Adsorption and decomposition of ClNO on the walls of their static system may account for the very low value of Grimley and Houston [459]. The results of Clyne and Cruse [239] in a discharge flow-resonance fluorescence study are significantly lower th an all recent results. The recommended value at room te mperature is the mean of the values reported by Abbatt et al. [4 ], Chasovnikov et al. [213], Nesbitt et al. [861], and Kita and Stedman [631]. The recommended temperature dependence is from the study of Abbatt et al. [4].

F85. Cl + ClONO 2 . Recommended value is based on the results of Yokelson et al. [1346] and those of Margitan [773]. These results are in excellent agreement; the slightly higher values of Kurylo et al. [668] are encompassed within th e stated uncertainties. Yokelson et al. report that at 298 K, more than 95% of this reaction proceeds by the reaction channel giving Cl 2 + NO 3 as products.

F86. Cl + CH 3 Cl. The recommended room temperature value is the mean of results of the absolute rate studies of Manning and Kurylo [770] and Beichert et al. [107] and the relative rate study of Walli ngton et al. [1245]. The temperature dependence is from Manning and Kurylo. The A-factor from that st udy has been adjusted slightly to fit the recommended room temperature value. The results reported by Clyne and Walker [258] and Manning and Kurylo [770] are in good agreement at 298 K. However, the value of the activation energy measured by Manning and Kurylo is significantly lower than that measured by Clyne and Walker. Both groups of workers measured the rate constant for the Cl + CH 4 and, similarly, the activation energy measured by Manning and Kurylo was significantly lower than that measured by Clyne and Walker. It is suggested that the discharge flow-mass spectrometric technique used by Clyne and Walker was in this case subject to a systematic error, and that the flash photolysis results of Manning and Kurylo provide the basis for the recommended rate constant.

F87. Cl + CH 2 Cl 2 . The recommended value is based on results of the relative rate study of Tschuikow-Roux et al. [1188] normalized to the value of the rate constant for the reference reaction (Cl + CH 4 ) recommended in this evaluation. The room temperature value is in good agreement with results of the relative rate study of Niki et al. [888] and the absolute rate study of Beichert et al. [107]. The higher results of Clyne and Walker [258] were not used.

F88. Cl + CHCl 3 . There have been three recen t studies of this reaction. In the studies of Beichert et al. [107] by an absolute technique and Brahan et al. [148] by a re lative technique, room temperature values about 50% greater than the previous recommendation, which was based on the relative study of Knox [642], were reported. Talhaoui et al. [1148] in a temperature-dependent absolute rate study by the discharge flow-mass spectrometric technique reported a room temperature value in excellent agreem ent with the previous recommendation. The recommended room temperature value is the mean of the values reported in the studies of Knox , Beichert et al., Brahan et al., and Talhaoui et al. The temperature dependence is from Talhaoui et al. and Knox. The A-factor has been fitted to the recommended room temperature value.

F89. Cl + CH 3 F (HFC-41). The recommended value is based on results of the temperature-dependent relative rate study of Tschuikow-Roux et al. [1188] and the relative rate studies of Tuazon et al. [ 1192] and Wallington et

### 1-72 al. [1253] at room temperature. The results of the absolute rate study of Manning and Kurylo [770] are in good agreement at room temperature but show a weak er temperature dependence, which is encompassed within the error limits.

F90. Cl + CH 2 F 2 (HFC-32). The recommended room temperature value is th e mean of results of the relative rate studies of Tschuikow-Roux et al. [1189] and of Nielsen et al. [876], both normalized to the value of the rate constant for the reference reaction (Cl + CH 4 ) recommended in this evaluation. The temperature dependence is from Tschuikow-Roux et al. The A-factor from that study has been adjusted to fit the recommended room temperature value.

F91. Cl + CF 3 H (HFC-23). Recommended value is based on resu lts of Coomber and Whittle [271].

F92. Cl + CH 2 FCl (HCFC-31). The recommended value is based on the room temperature results of Tuazon et al. [1192] and the temperature dependence reported by Tschuikow-Roux et al. [1188], normalized to the value of the rate constant for the reference reaction (Cl + CH 4 ) recommended in this evaluation.

F93. Cl + CHFCl 2 (HCFC-21). The recommended room temperature value is the mean of results of the relative rate study of Tuazon et al. [1192] and the absolute rate study of Talhaoui et al. [1148]. The temperature dependence is from Talhaoui et al. The A-factor from that study has b een adjusted to fit the recommended room temperature value. These results are preferred over the earlier results of Glavas and Heicklen [441].

F94. Cl + CHF 2 Cl (HCFC-22). The recommended room temperature value is the mean of results of the relative rate studies of Tuazon et al. [1192] and the absolute ra te studies of Sawerysyn et al. [1032] and Talhaoui et al. [1148]. The temperature dependence is from Talhaoui et al. The A-factor from that study has been adjusted to fit the recommende d room temperature value.

F95. Cl + CH 3 CCl 3 . Recommended value is based on results of the absolute rate study of Talhaoui et al. [1149]. It is consistent with the previous recommendation, which was a much higher upper limit reported by Wine et al. [1321] in a study in which it was c oncluded that a reactive impurity account ed for a significant fraction of the Cl atom removal. The value reported by Platz et al. [955] is in agreement with the recommendation.

F96. Cl + CH 3 CH 2 F (HFC-161). The recommended values for the two reaction channels are based on results of the relative rate study of Tschuikow-Roux et al. [1189], normalized to the value of the rate constant for the reference reaction (Cl + CH 4 ) recommended in this evaluation.

F97. Cl + CH 3 CHF 2 (HFC-152a). The recommended values for the two reaction channels are based on results of the relative rate study of Yano and Tschuikow-Roux [1344], normalized to the value of the rate constant for the reference reaction (Cl + C 2 H 6 ) recommended in this evaluation. The overall rate constant value is in good agreement with results of the room temperature relative rate studies of Wallington and Hurley [1259], and Tuazon et al. [1192].

F98. Cl + CH 2 FCH 2 F (HFC-152). The recommended value is based on results of the relative rate study of Yano and Tschuikow-Roux [1344] , normalized to the value of the rate constant for the reference reaction (Cl + C 2 H 6 ) recommended in this evaluation.

F99. Cl + CH 3 CFCl 2 (HCFC-141b). The recommended value is based on results of absolute rate studies of Talhaoui et al. [1149] by the discharge flow - mass spectrometric technique and Warren and Ravishankara [1278] by the pulsed photolys is-resonance fluorescence technique and th e relative rate studies of Wallington and Hurley [1259] and Tuazon et al. [1192].

F100.Cl + CH 3 CF 2 Cl (HCFC-142b). The recommended room temperature value is based on results of the relative rate studies of Wallington and Hurley [1259], and Tuazon et al. [1192], and the absolute rate study of Talhaoui et al. [1149]. The temperature dependence is from Talhaoui et al. The A-factor from that study has been adjusted to f it the recommended room temperature value.

F101. Cl + CH 3 CF 3 (HFC-143a). The recommended value is based on results of the relative rate study of Tschuikow-Roux et al. [1189], normalized to the value of the ra te constant for the reference reaction (Cl + CH 4 ) recommended in this evaluation.

F102. Cl + CH 2 FCHF 2 (HFC-143). The recommended values for the two reaction channels are based on results of the relative rate study of Tschuikow-Roux et al. [1189] normalized to the value of the rate constant for the reference reaction (Cl + CH 4 ) recommended in this evaluation.

F103. Cl + CH 2 ClCF 3 (HCFC-133a). The recommended value is based on results of the direct study of Jourdain et al. [595] using the discharg e flow-mass spectrometric technique to monitor the decay of the HCFC in the presence of a large excess of Cl atoms. The A-factor is lower than expected.

### 1-73 F104. Cl + CH 2 FCF 3 (HFC-134a). The recommended value is based on results of the relative rate studies of Wallington and Hurley [1259], and Tuazon et al. [1192], and the absolute rate study of Sawerysyn et al. [1032].

F105. Cl + CHF 2 CHF 2 (HFC-134). The recommended value is based on results of the relative rate study of Nielsen et al. [877] and that of Yano and Tschuikow-Roux [1344], normalized to the value of the rate constant for the reference reaction (Cl + C 2 H 6 ) recommended in this evaluation.

F106. Cl + CHCl 2 CF 3 (HCFC-123). The recommended value is based on results of the temperature-dependent study of Warren and Ravishankara [1278] using the pulse d photolysis-resonance fluorescence technique, and the relative rate studies of Wallington and Hurley [1259] and Tuazon et al. [1192] at room temperature.

F107. Cl + CHFClCF 3 (HCFC-124). The recommended value is based on results of the temperature-dependent study of Warren and Ravishankara [1278] using the pulsed photolysis-resonance fluorescence technique and the relative rate study of Tuazon et al. [1192] at room temperature. The A-factor is lower than expected.

F108. Cl + CHF 2 CF 3 (HFC-125). Recommended value is based on results of the relative rate studies of Tuazon et al. [1192] and Sehested et al. [1049].

F109. ClO + O 3 . There are two possible channels for this reaction: ClO + O 3 → ClOO + O 2 (k 1 ); and ClO + O 3
→ OClO + O 2 (k 2 ). The recommended upper limit for k 1 at 298 K is based on results of the recent study by Stevens and Anderson [1113]. These authors also report that k 1 = (4±2) × 10 –16 cm 3 molecule –1 s –1 at 413 K. These data can be combined to derive the Arrhenius parameters A = 2 × 10 –12 cm 3 molecule –1 s –1 and E/R > 3600 K. The upper limit for k 2 is based on results reported by DeMore et al. [337] and WongdontriStuper et al. [1332]; the Arrhenius parameters for k 2 were estimated.

F110. ClO + H 2 . The Arrhenius expression was estimated based on the ~600 K data of Walker (reported in Clyne and Watson [259]).

F111. ClO + NO. The absolute rate coefficients determined in th e four discharge flow-mass spectrometric studies (Clyne and Watson [259], Leu and DeMore [719], Ra y and Watson [996] and Clyne and MacRobert [245]) and the discharge flow laser magnetic resonance study of Lee et al. [704] are in excellent agreement at 298 K, and are averaged to yield the preferred value. The value reported by Zahniser and Kaufman [1354] from a competitive study is not used in the derivation of the preferred value as it is about 33% higher. The magnitudes of the temperature dependences reported by Le u and DeMore [719] and Lee et al. are in excellent agreement. Although the E/R value reported by Zahniser and Kaufman [1354] is in fair agreement with the other values, it is not considered as it is dependent upon the E/R value assumed for the Cl + O 3 reaction. The Arrhenius expression was derived from a least squares f it to the data reported by Clyne and Watson, Leu and DeMore, Ray and Watson, Clyne and MacRobert, and Lee et al.

F112. ClO + NO 3. The recommended value is based on results reported by Cox et al. [276], Cox et al. [287] Biggs et al. [124], and Kukui et al. [652]. Biggs et al. report the rate constant to be independent of temperature, consistent with the results of Cox et al. [287]. This recent study of Kukui et al. supersedes the earlier study of Becker et al. [92] from the same laboratory, which had indicated the major products to be OClO + NO 2 . There is now agreement among all studies that the major reaction channel forms ClOO + NO 2 (see Biggs et al. [124] Cox et al. [287], and Kukui et al. From a study of the OClO/NO 3 system Friedl et al. [413] conclude that at 220 K the formation of ClOO + NO 2 is favored.

F113. ClO + N 2 O. The Arrhenius expression was estimated based on the ~600 K data of Walker (reported in Clyne and Watson [259]).

F114. ClO + CO. The Arrhenius expression was estimated based on the ~600 K data of Walker (reported in Clyne and Watson [259]).

F115. ClO + CH 4 . The Arrhenius expression was estimated based on the ~600 K data of Walker (reported in Clyne and Watson [259]).

F116. ClO + H 2 CO. Poulet et al. [968] have reported an upper limit of 10 –15 cm 3 molecule –1 s –1 for k at 298 K using the discharge flow-EPR technique.

F117. ClO + CH 3 O 2 . The recommended expressions for the overall rate c onstant is based on the results of Helleis et al. [495]. It is consistent with the room temperature measurements of Simon et al. [1067] and Kenner et al. [612]. The results of Kukui et al. [654] for the overall r eaction are in agreement w ith the recommendation at room temperature, but these values show a slight nega tive temperature dependence in contrast with the slight positive temperature dependence recommended here. There is general agreemen t that the only important reaction channels are the two channels resulting in the production of ClOO + CH 3 O (a) and CH 3 OCl + O 2 (b). However, there is severe disagreement on their relative importance; at room temperature reaction channel (a)

### 1-74 is reported to be the major channel by Helleis et al. [495], Simon et al. [1067], Kukui et al. and Helleis et al. [496] but it is reported to be the minor channel by Biggs et al. [122] and Daele and Poulet [299]. Because of this large discrepancy, no branching ratios are recommended. The branching ratio studies that go down to low temperatures (Helleis et al. [495], K ukui et al. , and Helleis et al. [496]) report that reaction channels (a) and (b) are both significant down to lower polar stratospheric temperatures.

F118. ClO + ClO. There are three bimolecular channels for this reaction: ClO + ClO → Cl 2 + O 2 (k 1 ); ClO + ClO

→ ClOO + Cl (k 2 ); and ClO + ClO → OClO + Cl (k 3 ). The recommended values for the individual reaction channels are from the study of Nickolaisen et al. [864]. This study, using a flash photolysis/long path ultraviolet absorption technique, is the most comprehens ive study of this system, covering a wide range of temperature and pressure. These results are preferred over the re sults of earlier studies of the total bimolecular rate coefficient at low pressures by Clyne and Coxon [237], Clyne and White [263], and Clyne et al. [250], and those of other studies reported by Hayman et al. [489], Cox and Derwent [280], Simon et al. [1068], Horowitz et al. [523], and Horowitz et al. [524]. The room temperature branching ratio are k 1 :k 2 :k 3 = 0.29:0.50:0.21. The reaction exhibits both bimolecular and termolecular reaction channels (see entry in Table 2). The termolecular reaction dominates at pressures higher than about 10 torr. The equilibrium constant for formation of the Cl 2 O 2 dimer is given in Table 3.

F119. HCl + ClONO 2 . Results of four studies of the kinetics of this system have been published, in which the following upper limits to the homogeneous bimo lecular rate constant were reported: 10 –19 cm 3 molecule –1 s –1 by a static wall-less long-path UV absorption technique and a steady-state flow FTIR technique (Molina et al. [829]); 5 × 10 –18 using a flow reactor with FTIR analys is (Friedl et al. [411]); and 8.4 × 10 –21 using a static photolysis system with FTIR analysis (Hatakeyama and Leu [487] and Leu et al. [720]), and 1.5 × 10 –19 by FTIR analysis of the decay of ClONO 2 in the presence of HCl in large-volume (2500 and 5800 liters) Teflon or Teflon-coated chambers (Atkinson et al. [40]). Earlier, Birks et al. [128] had reported a higher upper limit. All studies found this reaction to be catalyzed by surfaces. The differences in the reported upper limits can be accounted for in terms of the very different reactor characteristics and detection sensitivities of the various studies. The homogeneous reaction is too slow to have any significant effect on atmospheric chemistry.

F120. CH 2 ClO + O 2 . The CH 2 ClO radical is reported to be resistant to unimolecular dissociation into Cl + CH 2 O products, according to chain reaction/ product analysis studies by Sanhueza and Heicklen [1026] and Niki et al. [888] and kinetics studies by Catoire et al. [204]. The recommendation is based on the work of Kaiser and Wallington [603] who studied the co mpetition between reaction with O 2 and HCl elimination in a complex photochemical reaction syst em using FTIR detecti on of stable products. The recommendation is a factor of 5 higher than estimated using the empirical relationship given by Atkinson and Carter [42]. The fate of CH 2 ClO in the atmosphere is this reaction with O 2 . F121. CH 2 ClO 2 + HO 2 . The recommendation is based on the measurement reported by Catoire et al. [204], who used pulsed photolysis with UV absorption detection at 1 atm pressure and 251–588 K.

F122. CH 2 ClO 2 + NO. The recommendation is based on the value reported by Sehested et al. [1051], who used pulsed radiolysis and UV absorption detection of NO 2 to measure the rate coefficient. The temperature dependence is estimated by analogy to similar RO 2 + NO reactions.

F123. CCl 3 O 2 + NO. The recommendation is based upon the measurements of Ryan and Plumb [1012] and Dognon et al. [358], who agree well at room temperature. The temperature dependence is derived from the data of Dognon et al., who covered the temperature range 228–413 K. The CCl 3 O primary product of the reaction of CCl 3 O 2 with NO decomposes rapidly to eliminat e Cl, according to Le sclaux et al. [709].

F124. CCl 2 FO 2 + NO. The recommendation is based on the measurements made by Dognon et al. [358] using pulsed photolysis with mass spectrometry detection at 1–10 torr and 228–413 K. These results supersede the earlier study of Lesclaux and Caralp [707]. The CCl 2 FO radical primary product of the CCl 2 FO 2 + NO reaction is reported by Lesclaux et al.[709] and Wu and Carr [1336] to rapidly decompose to eliminate Cl and to give the products indicated.

F125. CClF 2 O 2 + NO. The recommendation is based on the measurements made by Dognon et al. [358], who used pulsed photolysis with mass spectrometry detection at 1–10 torr and 228–413 K, and Sehested et al. [1051], who used pulsed radiolysis with UV absorption detection of the NO 2 product at one atm and 298 K. Wu and Carr [1336] observed the CClF 2 O radical primary product to rapidly dissociate to CF 2 O and Cl.

G1. O + BrO. The preferred value is based on the value reported by Thorn et al. [1166] using a dual laser flash photolysis/long path absorption/resonance fluorescence technique. Clyne et al. [252] reported a value approximately 40% lower.

G2. O + HBr. Results of the flash photolysis-resonance fluorescence study of Nava et al. [846] for 221–455 K and the laser flash photolysis-resonance fluorescence study of Nicovich and Wine [872] for 250–402 K provide

### 1-75 the only data at stratospheric temperatures. Results reported include those of Singleton and Cvetanovic [1076] for 298–554 K by a phase-shift technique, and disc harge flow results of Brown and Smith [157] for 267–430 K and Takacs and Glass [1142] at 298 K. The preferred value is based on the results of Nava et al., as well as those of Nicovich and Wine and those of Singleton and Cvetanovic over the same temperature range, since these results are less subject to complications due to secondary chemistry than are the results using discharge flow techniques. The uncertainty at 298 K has been set to encompass these latter results.

G3. O + HOBr. Recommended room temperature value is the mean of results of Monks et al. [1166] and Kukui et al. [653]. The temperature dependence is from Nesbitt et al. [860]. The A-factor from that study has been adjusted to fit the recomme nded room temperature value. Kukui et al. determined that the Br atom abstraction channel is the only pathway at room temperature.

G4. OH + Br 2 . The recommended room temperature value is the average of the values reported by Boodaghians et al. [138], Loewenstein and Anderson [750], and Poulet et al. [963]. The temperature independence is from Boodaghians et al. Loewenstein and Anderson determined that the exclusive products are Br + HOBr.

G5. OH + BrO. Recommended room temperature value is that reported by Bogan et al. [135]. This study, using discharge flow reactor techniques and beam sampling mass spect rometry, is the only experimental measurement of this rate constant. Because of the difficulty of anal yzing the data, we assign a large uncertainty factor. The authors suggest that the reaction proceed s by recombination to form vibrationally excited HOOBr that dissociates to Br + HO 2 . G6. OH + HBr. The preferred value at room temperature is the av erage of the values reported by Ravishankara et al. [989] using FP-RF, by Jourdain et al. [597] using DF-DPR, by Cannon et al. [191] using FP-LIF, and by Ravishankara et al. [992] using LFP-RF and LFP-LIF techniques. In this latest study the HBr concentration was directly measured in-situ in the slow flow system by UV absorption. The rate constant determined in this re-investigation is identical to the value recommended here. The data of Ravishankara et al. [989] show no dependence on temperature over the range 249–416 K. Values reported by Takacs and Glass [1141] and by Husain et al. [547] are a factor of 2 lower and were not included in the derivation of the preferred value. Data by Sims et al. [1073] are in good agreement with the reommendation at 298 K but show a negative temperature dependence at lower temperatures.

G7. OH + CH 3 Br. The recommended rate expression is derived from a combined fit to the data from the relative rate study of Hsu and DeMore [537] (recalcu lated based on the current recomme ndation for the rate constant for the OH + CH 3 CHF 2 reference reaction, as discussed in the note for that reaction) and the absolute determinations by Chichinin et al. [226], Mellouki et al. [811] and Zhang et al. [1369]. The results of these extensive studies are in excellent agreement and are preferred over the higher values reported in the earlier studies of Davis et al. [317] and Howard and Evenson [528].

G8. OH + CH 2 Br 2 . The recommended value for k(298 K) is an average of the values from the absolute studies of Mellouki et al. [811] and Zhang et al. [1364] and from the relative rate measurements of DeMore [335] (recalculated based on the current recommendati on for the rate constant for the OH + CH 2 Cl 2 reference reaction) and Orlando et al. [920] (recalculated based on the current r ecommendation for the rate constant for the OH + CH 3 (CO)CH 3 reference reaction). The recommended value of E/R is from the study of Mellouki et al. [811].

G9. OH + CHBr 3 . The recommended rate expression is derived from a fit to the data from the relative rate study of DeMore [335] (recalculated base d on the current recommendation for the rate constant for the OH + CH 2 Cl 2 reference reaction). The results of Orkin et al. [914] are higher by a factor of 2 but have the same temperature dependence. They are encompassed within the 2 σ confidence limits.

G10. OH + CHF 2 Br. The recommended values for k(298 K) and E/R are derived from a fit to the data of Talukdar et al. [1151] (two studies), Orkin and Khamaganov [913], and Hsu and DeMore [538] (a relative rate measurement recalculated using the current reco mmendation for the rate constant for the OH + CH 4 reference reaction). These data are preferred over the consiste ntly higher results reported by Brown et al. [153].

G11. OH + CH 2 ClBr. The recommended value for k(298 K) is an average of the values from two relative rate studies by DeMore [335] (recalcula ted based on the current recommendati on for the rate constant for the OH + CH 2 Cl 2 reference reaction) and Bilde et al. [126] (recalculated usi ng the current recommendation for the rate constant for the OH + CH 2 Br 2 reference reaction) and two absolute determinations by Orkin et al. [915], all of which are in good agreement. The recommended E/R is obtained from a fit to the data of DeMore and Orkin et al.. The A factor was then calculated.

### 1-76 G12. OH + CF 2 ClBr. The A-factor was estimated, and a lower limit for E/R was derived using the upper limit for the rate constant at 298 K reported by Burkholder et al . [174] in a study using pulsed photolysis-LIF and DFLMR techniques. A less sensitive upper limit was reported by Clyne and Holt [243].

G13. OH + CF 2 Br 2 . The A-factor was estimated, and a lower limit for E/R was derived by using the upper limit for the rate constant at 298 K reported by Burkholder et al . [174] in a study using pulsed photolysis-LIF and DFLMR techniques.

G14. OH + CF 3 Br. The A-factor was estimated and a lower limit for E/R was derived by using the upper limit for the rate constant at 460 K reported by Orkin and Khamaganov [913]. These parameters were then used to calculate an upper limit for k(298 K). The upper limit for k(298 K) determined by Burkholder et al. [174] in a study using pulsed photolysis-LIF and DF-LMR techni ques at room temperature is understandably higher. A less sensitive upper limit was also reporte d by Le Bras and Combourieu [688].

G15. OH + CH 2 BrCH 3 . The recommended values for k(298 K) and E/R are derived from a fit to the data (T ≤ 300 K) of Herndon et al. [500]. These data suggest a curvature of the Arrhenius plot similar to that found for the OH reaction with CH 3 CH 2 F. The data of Qiu et al. [972] (which include earlier data reported by the same research group in Xing et al. [1340]) were not used because th ey were obtained mainly at above room temperature and exhibit a very steep temperature dependence resulting in a value for E/R that is larger than the E/R value obtained from data at T > 298 K for the OH reaction with CH 3 CH 2 F. The k(300 K) value reported by Donaghy et al . [363] seems too low for this reaction when compared with the recommendation for presumably slower (and better studied) OH reaction with CH 3 CH 2 F.

G16. OH + CH 2 BrCF 3 . The recommended values for k(298 K) and E/R are from a combined fit to the data of Nelson et al. [849] and Orkin and Khamaganov [913].

G17. OH + CHFBrCF 3 . The recommended rate expression is derived from a combined fit to the data (below 400 K) of Orkin and Khamaganov [913] and Brown et al. [153].

G18. OH + CHClBrCF 3 . The recommended rate expression is derived from a fit to the data of Orkin and Khamaganov [913] (for T ≤ 400 K). The room temperature value measured by Brown et al. [154] lies somewhat higher than this recommendation but is encompassed within the 2 σ confidence limits.

G19. OH + CHFClCF 2 Br. The recommended rate expression is derived from a fit to the data from the relative rate study of DeMore [335] (recalculated based on the current recommendation fo r the rate constant for the OH + CH 3 CCl 3 reference reaction).

G20. OH + CF 2 BrCF 2 Br. The A-factor was estimated and a lower limit for E/R was derived by using the upper limit for the rate constant at 460 K reported by Orkin and Khamaganov [913]. These parameters were then used to calculate an upper limit for k(298 K). The upper limit for k(298 K) determined by Burkholder et al. [174] in a study using pulsed photolysis-LIF and DF-L MR techniques at room temperature is understandably higher.

G21. OH + CH 2 BrCH 2 CH 3 . The recommended values for k(298 K) and E/R are derived from a fit to the data (T ≤ 300 K) from Donaghy et al. [363], Te ton et al. [1162], Nelson et al. [850], Herndon et al. [500], Gilles et al. [436], and Kozlov et al. [650]. Significant curvature in the Arrhenius plot has been observed over the 480 to 210 K temperature range, due to the three different hydrogen-abstraction reac tion channels that occur. These channels have been quantified in the study of Gilles et al. In spite of the noticeable Arrhenius curvature, the data below 300 K can be well represented by a two-parameter Arrhenius fit.

G22. OH + CH 3 CHBrCH 3 . The recommended values for k(298 K) and E/R are averages of the parameters derived from a fit to the data (T ≤ 300 K) of Herndon et al. [500] and Kozlov et al. [650] which are in excellent agreement. The A factor was then calculated. The room temp erature relative rate determination by Donaghy et al. [363] and the absolute temperature dependent data of Teton et al. [1162] lie systematically higher than those from these two more recent studies. Significant curvature in the Arrhenius plot has been observed overthe 480 K to 210 K temperature range by Kozlov et al., presumably due to the two different hydrogenabstraction reaction channels that occur. In spite of the noticeab le Arrhenius curvature, the data below 300 K can be well represented by a two-parameter Arrhenius fit.

G23. HO 2 + Br. This recommendation is based on results obtained over the 260–390 K temperature range in the study by Toohey et al. [1183], using a discharge flow system with LMR detection of HO 2 decay in excess Br. The room temperature value reported in this study is a factor of 3 higher than that reported by Poulet et al. [964] using LIF and MS techniques and is an order of magnitude larger than the value of Posey et al. [959]. The uncertainty in E/R is set to encompass the value E/R = O, as it is for othe r radical-radical reactions. The value determined by Laverdet et al. [685] using DF-EPR techniques is in good agreement with this

### 1-77 recommendation. The reactions of Br atoms with H 2 O 2 , HCHO, and HO 2 are all slower than the corresponding reactions of Cl atoms by one to two orders of magnitude.

G24. HO 2 + BrO. The recommendation is based on results of the temperature-dependent studies of Larichev et al. [681], Elrod et al. ([377], and Li et al. [730]. The studies of Larichev et al. and Elrod et al. were done under pseudo–first-order conditions with excess HO 2 ; the study of Li et al. was done under pseudo–first-order conditions with either HO 2 or BrO in excess. The recommended room temperatur e value is the mean of the values reported in these studies, with the valu es of Li et al. under both conditions included. These studies all report a similar negative temperature dependence. The room temperature value of Bridier et al. [151], which was not obtained under pse udo–first-order decay conditions, was not included in derivation of the recommendation. Larichev et al. have determined an upper limit of 1.5% for production of HBr and O 3 . From a study of the reverse reaction above room temperature, Mellouki et al. [810] determined by extrapolation that the yield of HBr + O 3 is an insignificant fraction (<0.01%) of the total reaction down to 200 K.

G25. NO 3 + HBr. The recommended upper limit is the upper limit reported by Mellouki et al. [807] in a study using DF-EPR techniques. This upper limit shows that this reacti on is of negligible importance in stratospheric chemistry. Canosa-Mas et al. [194] reported a value that is consistent, within experimental error, with the upper limit of Mellouki et al.

G26. Cl + CH 2 ClBr. Recommended value is based on results of Tschuikow-Roux et al. [1188] (normalized to the value of the rate constant for the reference reaction (Cl + CH 4 ) recommended in this evaluation ) and Bilde et al. [126] (normalized to most recent va lues for the rate coefficients for th e reference reactions, i.e., the rate coefficients for the Cl + CH4 reaction given in JPL 00-3 [1019] and for Cl + CH 2 Br 2 given in the current recommendation, respectively.) The products of this reaction are e xpected to be CHClBr and HCl.

G27. Cl + CH 3 Br. Recommended value is based on results of the abso lute rate studies of Gierczak et al. [430], Orlando et al. [920], Kambanis et al. [605] and Piety et al. [949]. Results of these studies are in excellent agreement. Results of the relative rate study Tschuikow-Roux et al. [1188] were not used in derivation of the recommended value. The product of this reaction is expected to be mostly CH 2 Br and HCl. The possible production of CH 3 Cl + Br is very small in the atmosphere [446].

G28. Cl + CH 2 Br 2 . Recommended value is based on results of the abso lute rate studies of Gierczak et al. [430], Orlando et al. [920], and Kambanis et al. [605]. Results of these studies ar e in excellent agreement. Results of the relative rate study of Tschuikow-Roux et al. [1188] were not used in derivation of the recommended value. The products of this reacti on are expected to be CHBr 2 and HCl.

G29. Cl + CHBr 3 . The recommendation is based on the only reported study of this reaction by Kambanis et al. [605], who employed a very low pressure reactor and monitored reactants and products using mass spectrometry. The products of this reaction are CBr 3 and HCl.

G30. Br + O 3 . The results reported for k(298 K) by Clyne and Watson [261], Leu and DeMore [718], Michael et al. [818], Michael and Payne [823], and Toohey et al. [1184] are in excellent agreement. The preferred value at 298 K is derived by taking a simple mean of these five values. The temperature dependences reported for k by Leu and DeMore and by Toohey et al. are in good agreem ent, but they can only be considered to be in fair agreement with those reported by Mi chael et al. and Michael and Payne. The preferred value was synthesized to best fit all the data reported from these five studies. The results of Nicovich et al. [868] are in excellent agreement with this recommendation.

G31. Br + H 2 O 2 . The recommended upper limit to the value of the rate constant at room temperature is based on results reported in the study by Toohey et al. [1183] using a discharge flow-resonance fluorescence/laser magnetic resonance technique. Their upper limit determined over the temperature range 298–378 K is consistent with less sensitive upper limits determined by Leu [714] and Posey et al. [959] using the discharge flow-mass spectrometric technique. The much higher value reported by Heneghan and Benson [498] may result from the presence of excited Br at oms in the very low pressure reactor. The pre-exponential factor was chosen to be consistent with that for the Cl + H 2 O 2 rate constant, and the E/R value was fitted to the upper limit at 298 K. Mellouki et al. [810] have measured the rate of the reverse reaction.

G32. Br + NO 3 . The recommended value is that reported by Mellouki et al. [807] in a study using DF-DPR techniques.

G33. Br + H 2 CO. There have been two studies of this rate constant as a function of temperature: Nava et al. [848], using the flash photolysis–resonance fluorescence technique, and Poulet et al. [962], using the discharge flow-mass spectrometric technique. These results are in reasonably good agreement. The Arrhenius expression was derived from a least squares fit to the data reported in these two studies. The higher room temperature value of Le Bras et al. [689], using the di scharge flow–EPR technique, has been shown to be in error due to secondary chemistry (Poulet et al.).

### 1-78 G34. Br + OClO. The recommended value at room temperature is th e mean of the values reported by Clyne and Watson [262] and Toohey [1181]. In the study of Clyne and Watson, correction for the effect of the rapid reverse reaction was required. The temperature dependence reported by Toohey [1181] is accepted but with increased error limits.

G35. Br + Cl 2 O. The recommended value is based on results repor ted by Stevens and Anderson [1114] and by Sander and Friedl [1018], which are in good agreement.

G36. Br + Cl 2 O 2 . The recommended value is that determined by Friedl (private communication) in a study using a DF-MS technique.

G37. BrO + O 3 . There have been two recent studies of this reaction. Rattigan et al. [978] report an overall rate constant of ~10 –17 cm 3 molecule –1 s –1 over the temperature range 318–343 K. Rowley et al. [1009] report a room temperature upper limit of 2 × 10 –17 cm 3 molecule –1 s –1

. Both papers report a value of ~2 × 10 –18 cm 3 molecule –1 s –1 for the channel to produce OBrO + O 2 . The recommended upper limit of 2 × 10 –17 cm 3 molecule –1 s –1 is a factor of 2.5 less than the previously recommended upper limit of 5 × 10 –17 , which was based on Mauldin et al. [793]. The pre-exponential factor was estimated, and E/R was calculated.

G38. BrO + NO. The results of the three low pressure mass spectrometric studies (Clyne and Watson [261]; Ray and Watson [996]; Leu [712]) and the high pressure UV absorption study (Watson et al. [1289]), which all used pseudo–first-order conditions, are in excellent agreement at 298 K and are thought to be much more reliable than the earlier low pressure UV absorption study (Clyne and Cruse [238]). The results of the two temperature-dependence studies are in good agreement and both show a small negative temperature dependence. The preferred Arrhenius expression was derived fro m a least squares fit to all the data reported in the four recent studies. By combining the data reported by Watson et al. with those from the three mass spectrometric studies, it can be shown that this reac tion does not exhibit any observable pressure dependence between 1 and 700 torr total pressure. The temperature dependences of k for the analogous ClO and HO 2 reactions are also negative and are similar in magnitude.

G39. BrO + NO 3 . The recommended value is the geometric mean of the lower and upper limits reported by Mellouki et al. [807] in a study using DF-DPR techniques. These reported limits are encompassed within the indicated uncertainty limits.

G40. BrO + ClO. Friedl and Sander [412], using DF/MS techniques, measured the overall rate constant over the temperature range 220–400 K and also over this temperature range determined directly branching ratios for the reaction channels producing BrCl and OClO. The same authors in a separate study using flash photolysis– ultraviolet absorption techniques (Sander and Friedl [1018]) determined the overall rate constant over the temperature range 220–400 K and pressure range 50–750 to rr and also determined at 220 K and 298 K the branching ratio for OClO production. The results by these two independent techniques are in excellent agreement, with the overall rate constant showing a negative temperature dependence. Toohey and Anderson [1182], using DF/RF/LMR techniques, reported room temper ature values of the overall rate constant and the branching ratio for OClO production. They also found evidence for the direct production of BrCl in a vibrationally excited Π state. Poulet et al. [960], using DF/MS techniques, reported room temperature values of the overall rate constant and branch ing ratios for OClO and BrCl production. Overall room temperature rate constant values reported also include those fro m the DF/MS study of Clyne and Watson [262] and the very low value derived in the flash photolysis study of Basco and Dogra [81] using a different interpretation of the reaction mechanism. The recommended Arrhenius expressions for the individual reaction channels are taken from the study of Friedl and Sander [412] and Turnipseed et al

. [1205] . These studies contain the most comprehensive sets of rate cons tant and branching ratio data. The overall rate constants reported in these two studies are in good agreement (20%) at room temperature and in excellent agreement at stratospheric temperatures. Both studies report that OClO production by channel (1) accounts for 60% of the overall reaction at 200 K. Both studies report a BrCl yield by channel (3) of about 8%, relatively independent of temperature. The recommended expressions are consistent with the body of data from all studies except those of Hills et al. [507] a nd Basco and Dogra [81].

G41. BrO + BrO. Measurements of the overall rate constant can be divided into categories—those in which BrO was monitored by UV absorption and those in which BrO was monitored by mass spectrometer. Gilles et al. [438] have re-analyzed the results of the UV absorption studies and scaled the reported values of the rate constant to the UV absorption cross sections reported in their paper. When scaled in this manner, the room temperature rate constant values reported in the UV absorption studies (Sander and Watson [1023], Mauldin et al. [793], Bridier et al. [151], Rowley et al. [1009], Laszlo et al. [683], and Gilles et al.) come into very good agreement among themselves and also with results of the mass spectrometric studies of Clyne and Watson [261] and Lancar et al. [677]. This provides the basis for the reommended room temperature value.

### 1-79 The temperature dependence is based on results of Sande r and Watson, Turnipseed et al. [1204] and Gilles et al.
There are two possible bimolecula r channels for this reaction: BrO + BrO → 2Br + O 2 (k 1 ) and BrO + BrO → Br 2 + O 2 (k 2 ). The partitioning of the total rate c onstant into its two components, k 1 and k 2 , has been measured at room temperature by Sander and Watson [1023], Turnipseed et al. [1204] and Lancar et al. [677], by Jaffe and Mainquist [568] from 258 to 333 K, by Cox et al. [292] from 278 to 348 K and by Mauldin et al. [793] from 220 to 298 K. All are in agreement that k 1 /k = 0.85±0.03 at 298 K. From the values of k 1 /k = 0.85 at298 K (all studies) and 0.68 at 220 K (Mauldin et al. and Cox et al. extrapolated), one can derive the temperature-dependent expression k 1 /k = 1.60 exp(–190/T). From the recommended Arrhenius expression for the overall rate constant k = k 1 + k 2 and the expression for the branching ratio k 1 /k, one can derive the following Arrhenius expressions for the individual reaction channels: k 1 = 2.4 × 10 –12 exp(40/T) cm 3 molecule –1 s –1 and k 2 = 2.8 × 10 –14 exp(860/T) cm 3 molecule –1 s –1

. G42. CH 2 BrO 2 + NO. The recommendation is based on the 298 K measurement of Sehested et al. [1051], who used pulsed radiolysis with UV absorption detection of the NO 2 product formation rate. The temperature dependence is estimated based on analogy to similar RO 2 + NO reactions. The CH 2 BrO product has been shown to undergo rapid unimolecular decomposition to yield CH 2 O + Br by Chen et al. [216] and Orlando et al. [919] The domination of this channel over the reaction of CH 2 BrO with O 2 is consistent with the fate of other alkoxy radicals (Chen et al. and Orlando et al.), but contradicts the earlier result of Nielson et al. [878].

H1. O + I 2 . Based on the room temperature data of Ray and Watson [996] and Laszlo et al. [684]. The molecular beam study of Parrish and Herschbach [931] suggests a zero activation energy, consistent with the near gas kinetic value of k at 298 K.

H2. O + IO. Based on results of Laszlo et al. [684], the only reported study of this rate constant. This value was derived from modeling a system in which the concentrations of I 2 and IO were monitored simultaneously. This rate constant is a factor of 4 greater than th e values for the corresponding reactions of O with ClO and BrO.

H3. OH + I 2 . Based on the data of Loewenstein and Anderson [751] and Jenkin et al. [575].

H4. OH + HI. Based on the data of Lancar et al. [679] and MacLeod et al. [765].

H5. OH + CH 3 I. The recommended rate expression is derived from a fit to the data of Brown et al. [155], the only reported study of this reaction.

H6. OH + CF 3 I. The recommended rate expression is derived from a fit to the data of Gilles et al. [437]. The results from the studies by Garraway and Donovan [422] a nd Berry et al. [114] were not used in deriving the recommendation as the results were possi bly influenced by reactant photolysis. The room temperature value from the discharge flow/resonance fluorescence study of Brown et al. [155]agrees within the 2 σ limits.

H7. HO 2 + I. Based on the data of Jenkin et al. [580], the only reporte d study of this reaction.

H8. HO 2 + IO. The recommended value is the average of the values reported by Jenkin et al. [579] and Maguin et al. [768].

H9. NO 3 + HI. No recommendation is given, based on the poten tial for severe complications resulting from secondary chemistry in the only reported study of the reaction (Lancar et al. [679]).

H10. Cl + CH 3 I. This reaction, thought to be a simp le H abstraction reaction, has been shown by Ayhens et al. [53] to be quite complex. At low temperatures, Cl atom reversibly adds to CH 3 I to form CH 3 ICl. Thus, there are at least two channels for this reaction,

Cl + CH 3 I → CH 2 I + HCl (a)

Cl + CH 3 I ↔ CH 3 ICl (b) The rate coefficient for channel (a) has been measured by Ayhens et al. above 364 K, Kambanis et al. [605] between 273 and 363 K, Bilde and Wa llington [125] at 298 K, and Cotte r et al. [273] at 298 K. The recommendation is based on these studies. Under atmospheric conditions reaction (b) to form the a dduct is about two orders of magnitude faster than reaction (a). However, the fate of the CH 3 ICl adduct in the atmosphere is unclear. Its lifetime, based on the studies of Ayhens et al., can be as long as a few seconds at 200 K and a few hundred Torr pressure. Therefore, it is possible th at it could react with O 2 or be photolyzed. At 298 K, in one atmosphere of O 2 , it appears that the overall fate of the CH 3 ClI is to decompose back to the r eactants, based on the work of Bilde and Wallington [125]. Therefore, if O 2 were to react with CH 3 ICl, this rate coefficient has to be less than about

### 1-80 10 –17 cm 3 molecule –1 s –1 , using the rate coefficient for its d ecomposition measured by Ayhens et al. If the rate coefficient for CH 3 ICl + O 2 were to remain approximately the same, i.e., 10 –17 cm 3 molecule –1 s –1 , at lower temperatures, the possible loss of CH 3 ICl via reaction with O 2 cannot be ignored. Further, the possible atmospheric photolysis of CH 3 ICl may be important if it has a J-value greater than 0.1 s –1

. There is a third possible product cha nnel for this reaction to yield CH 3 Cl + I (Goliff and Rowland [446]). Based on the results of Bilde and Wallington and Goliff and Rowland, we recommend that the rate coefficient for the Cl + CH 3 I → CH 3 Cl + I reaction to be less than 0.2k a at 298 K. Since such a reaction is likely to have a significant barrier in the gas phase, even though it is exothermic by ~14 kcal mol –1 at 298 K, the branching ratio for the production of CH 3 Cl and I in the atmosphere will be likely less than that at 298 K.

H11. I + O 3 . Based on the room temperature data of Jenkin and Cox [576] and Sander [1017], and the temperature dependent data of Buben et al. [164] and Turnipseed et al. [1207].

H12. I + BrO. Based on results of Laszlo et al. [683], the only reported study of this rate constant. This value was derived from modeling the simultaneous decay of BrO and IO in a Br 2 /I 2 /N 2 O system.

H13. IO + NO. Based on the data of Ray and Watson [996], Dayk in and Wine [322], Buben et al. [165], and Turnipseed et al. [1207].

H14. IO + ClO. Based on results of Turnipseed et al. [1206] , the only reported study of this reaction. These authors also reported the product yield for channel(s) yielding an I atom to be 0.8 ± 0.2.

H15. IO + BrO. Based primarily on results of Laszlo et al. [683]. Gilles et al. [438] reported the following Arrhenius expression for non-iodine atom producing channels: 2.5 × 10 –11 exp (260/T) cm 3 molecule –1 s –1

. They also reported a branching ratio of <0.35 for channels producing I atoms. From their data they could constrain the value of the overall rate constant to be: 6 × 10 –11 < k < 10 × 10 –11 cm 3 molecule –1 s –1 , the range of which is consistent with the results of Laszlo et al.

H16. IO + IO. Changed from the previous recommendation, which was based on the results of Sander [1017]. In that study, over the temperature range 250–373 K, a negative temperature dependence was reported for the overall rate constant and for the absorption cross section at 427.2 nm. In the recent study of Harwood et al. [485], the overall rate constant and the absorption cross section were found to be independent of temperature from 253 to 320 K. The recommended room temperature value is the average of the values reported by Sander, Harwood et al., and Laszlo et al. [684]. The recommended temperaure de pendence is the average of the values reported by Sander and by Harwood et al., with an uncertainty sufficient to encompass the two reported values. The A-factor has been fitted to the recommended room temperature rate constant and the recom-mended temperature dependence. The overall rate constant for the decay of IO in the absence of ozone has been found to be independent of pressure by Sander, Laszlo et al., and Harwood et al. A comparison of the overall rate observed in excess ozone to that in th e absence of ozone was interpreted by Sander and by Harwood et al. to imply that formation of the dimer I 2 O 2 is the dominant reaction channel in the IO selfreaction.

H17. INO + INO. Based on the data of Van den Bergh and Troe [1225].

H18. INO 2 + INO 2 . Based on the data of Van den Bergh and Troe [1225].

I1. O + SH. This recommendation accepts the resu lts of Cupitt and Glass [296]. The large uncertainty reflects the absence of any confirming investigation.

I2. O + CS. The room temperature recommendation is an average of the rate constants determined by Slagle et al. [1087], Bida et al. [118], Lilenfeld and Richardson [737], and Hancock and Smith [479]. The temperature dependence is that of Lilenfeld and Richardson, with the A-factor adjusted to yield the recommended value of k(298 K).

I3. O + H 2 S. This recommendation is derived from an unweighted least squares fit of the data of Singleton et al. [1079] and Whytock et al. [1304]. The results of Slagle et al. [1085] show very good agreement for E/R in the temperature region of overlap (300 – 500 K) but lie systematically higher at every temperature. The uncertainty factor at 298 K has been chosen to encompass the room temperature rate constant values of Slagle et al. [1085] a nd Hollinden et al. [519]. Other than the 263 K data point of Whytock et al. and the 281 K point of Slagle et al., the main body of rate constant data below 298 K comes from the study of Hollinden et al., which indicates a dramatic cha nge in E/R in this temperature region. Thus, ∆ E/R was set to account for these observations. Such a nonlinearity in the Arrhenius plot might indicate a change in the reaction mechanism from abstraction (as written) to addition. An addition channel (resulting in H atom displacement) has been proposed by Slagle et al. [1085], Singleton et al. [1079], and Singleton et al. [1081]. In the latter two studies, an upper limit of 20% was placed on the displacement channel. Direct observations of product HSO was made in the reactive scattering experiments of Clemo et al. [235] and Davidson et al. [307]. A threshold

### 1-81 energy of 3.3 kcal/mole was observed (similar to th e activation energy measured in earlier studies), suggesting the importance of this direct displacement channel. Addition products from this reaction have been seen in a matrix by Smardzewski and Lin [1090]. Further kinetic studies in the 200–300-K temperature range, as well as quantitative direct mechanistic information, could clarify these issues. However, this reaction is thought to be of limited importance in stratospheric chemistry.

I4. O + OCS. The value of k(298 K) is the average of the determinations by Westenberg and de Haas [1296], Klemm and Stief [637], Wei and Ti mmons [1292], Manning et al. [771], and Breckenri dge and Miller [150]. The recommended value of E/R is the average va lue taken from the first three listed studies. Hsu et al. [536] report that this reaction proceeds ex clusively by a stripping mechanism. The vibrational and rotational state distributions in the SO and CO products have been reported by Chen et al. [222] and Nickolaisen et al. [866] respectively.

I5. O + CS 2 . The value of k(298 K) is an average of the rate constants determined by Wei and Timmons [1292], Westenberg and de Haas [1296], Slagle et al. [1086], Callear and Smith [188], Callear and Hedges [187], Homann et al. [520], and Graham and Gutman [449]. The E/R value is an average of the determinations by Wei and Timmons and Graham and Gutman. The g value has been set to en compass the limited temperature data of Westenberg and de Haas. The principal reaction products are thought to be CS + SO. However, Hsu et al. [536] report that 1.4% of the reaction at 298 K proceeds through a channel yielding CO + S 2 and calculate a rate constant for the overall proce ss in agreement with that recommended. Graham and Gutman [449] have found that 9.6% of the reaction proceeds to yield OCS + S at room temperature. Using time-resolved diode laser spectroscopy, Cooper and Hershberger [272] dete rmined the branching ratios for the CO and OCS producing channels to be (3.0±1.0 )% and (8.5±1.0)% respectively.

I6. O + CH 3 SCH 3 . This recommendation is based on a fit of the data from Nip et al. [897], Lee et al. [700], and Lee et al. [699]. Product studies by Cvetanovic et al. [297] indicate that the r eaction proceeds almost entirely by addition followed by rapid fragmentation to the products as written. Pavanaja et al. [936] examined the pressure and reactant ratio dependencies of OH(A 2 Σ + ) and SO 2 ( 3 B, 1 B) emissions in this reaction system. Their observations are consistent with initial product fo rmation as written, followe d by secondary generation of both OH and SO 2 . I7. O + CH 3 SSCH 3 . This recommendation averages the 298 K rate constants of Nip et al. [897] and Lee et al. [696], which differ by nearly a factor of 2. The temperature dependence is that of Nip et al.; Lee et al. having reported no temperature dependence over the limited range of 270–329 K. The A-factor has been adjusted to yield the recommended (averaged) value of k(298 K). Product studies by Cvetanovic et al. [297] indicate that the reaction proceeds mainly by addition followed by rapid fragmen tation to the products as written. Pavanaja et al. [936] examined the pressure and reactant ratio dependencies of OH(A 2 Σ + ) and SO 2 ( 3 B, 1 B) emissions in this reaction system. Their observations are consistent with initia l product formation as written, followed by secondary generation of both OH and SO 2 . I8. O 3 + H 2 S. This upper limit was determined by Becker et al. [96] from measurements of the rates of SO 2 production and O 3 consumption. The heterogeneous reaction between H 2 S and O 3 is far more efficient in most laboratory systems.

I9. O 3 + CH 3 SCH 3 . This rate constant upper limit is based on the measurements of Martinez and Herron [789], which represent the only reported study of this reaction.

I10. SO 2 + O 3 . This recommendation is based on the limited data of Davis et al. [318] at 300 K and 360 K in a stopped flow investigation using mass spectrometric and UV spectroscopic detection.

I11. OH + H 2 S. The values of k(298 K) and E/R are derived from a composite unweighted least squares fit to the individual data points of Perry et al. [943], Cox and Sh eppard [291], Wine et al. [1313], Leu and Smith [723], Michael et al. [819], Lin [738], Lin et al. [742], Barnes et al. [63], and Lafage et al. [674]. The studies of Leu and Smith [723], Lin et al. [742], Lin [738], and Lafage et al. [674] show a slight parabolic temperature dependence of k with a minimum occurring near room temperature. However, with the error limits stated in this evaluation, all data are fit reasonably well by an Arrhenius expression. Lafage et al. and Michael et al. discuss the results in terms of a two-channel reaction scheme involving direct H atom abstraction and complex (adduct) formation. Lafage et al. analyzed their results above room temperature to yield an apparent E/R = 400 K for the abstraction channel, in good agreement with the E/R value determined above room temperature by Westenberg and de Haas [1297]. The results of these latter workers lie systematically higher (by about 70%), presumably due to secondary reactions. The room temperature value measured by Stuhl [1126] lies just outside the 2 σ error limit set for k(298 K).

I12. OH + OCS. The value of k(298 K) is an average of the determinations by Wahner and Ravishankara [1243] and Cheng and Lee [223]. The room temperature rate constants from these studies are a factor of 3 higher

### 1-82 than the earlier determination by Leu and Smith [722]. As discussed in the later studies, this difference may be due to an overcorrection of the Leu and Smith data to account for OH reaction with H 2 S impurities and also to possible regeneration of OH. Nevertheless, the uncertainty factor at 298 K has been set to encompass the earlier study within 2 σ

. The work by Wahner and Ravishankara [1243] supersedes the study of Ravishankara et al. [982], which minimized complications due to s econdary and/or exc ited state reactions that presumably were interfering with the experiments of Atkinson et al. [45] and of Kurylo [663]. The upper limit for k(298 K) reported by Cox a nd Sheppard [291] is too insensitive to permit comparison with the more recent studies. The room temperature measurements of Wahner and Ra vishankara demonstrate the lack of an effect of total pressure (or O 2 partial pressure) on the rate constant a nd are supported by the more limited pressure and O 2 studies of Cheng and Lee. The recommendation for E/R is based on the study of Cheng and Lee who determined a value considerably lower than reported by Leu and Smith, although this difference may be due in part to the earlier mentioned overcorrection of the data by the latter authors. Product observations by Leu and Smith indicate that SH is a primary produc t of this reaction and tentatively confirm the suggestion of Kurylo a nd Laufer [669] that the predomin ant reaction pathway is to produce SH + CO 2 through a complex (adduct) mechanism similar to that observed for the OH + CS 2 reaction. However, the absence of an O 2 /pressure effect for OH + OCS is in marked contrast with the strong dependence seen in studies of OH + CS 2 (see note for the latter reaction). Experiments by Greenblatt and Howard [454] have s hown that oxygen atom exch ange in the reaction of

18 OH with OCS is relatively unimportant, leading to an upper limit of 10 –15 being set on the rate constant of the exchange reaction.

I13. OH + CS 2 . There is a consensus of experiment al evidence that this reaction pr oceeds very slowly as a direct bimolecular process. Wine et al. [1322] set an upper limit on k(298 K) of 1.5 × 10 –15 cm 3 molecule –1 s –1

. A consistent upper limit is also reported by Iyer and Ro wland [565] for the rate of direct product of OCS, suggesting that OCS and SH are primary products of the bimolecular process. This mechanistic interpretation is further supported by the studies of Leu and Smith [724] and of Biermann et al. [120], which set somewhat higher upper limits on k(298 K). The more rapid reaction rates measured by Atkinson et al. [45], Kurylo [663], and Cox and Sheppard [291] may be attributable to severe complications arising from excited state and secondary chemistry in their photolytic systems. The Cox and Sheppard study in particular may have been affected by the reaction of electronically excited CS 2 (produced via the 350 nm photolysis) with O 2 (in the 1- atm synthetic air mixture) as well as by the accelerating effect of O 2 on the OH + CS 2 reaction itself, which has been observed by other workers as summarized below. The possible importance of electronically excited CS 2 reactions in the tropospheric oxidation of CS 2 to OCS has been discussed by Wine et al. [1312]. An accelerating effect of O 2 on the OH + CS 2 reaction rate has been observed by Jones et al. [594], Barnes et al. [69], and Hynes et al. [553], along with a near unity product yield for SO 2 and OCS. In the latter two studies the effective bimolecular rate constant was found to be a function of total pressure (O 2 + N 2 ), and exhibited an appreciably negative temperature dependence. These observations are consistent with the formation of a long-lived adduct as postulated by Kurylo [663] and Kurylo and Laufer [669] followed by its reaction with O 2 :

OH + CS 2 + M a

b k

k 

###  → ←



 HOCS 2 + M

HOCS 2 + O 2 c k



###  → Products Hynes et al. [553], Murrells et al. [842], Becker et al. [97], and Bulatov et al. [167] directly observed the approach to equilibrium in th is reversible adduct formation. In the Hynes et al. study, the equilibrium constant was measured as a function of temperature, and the heat of formation of HOCS 2 was calculated (–27.4 kcal/mole). A rearrangement of this adduct followed by dissociation into OCS and SH corresponds to the bimolecular (low k) channel referred to earlier. Hynes et al. [553] measured the rate constant for this process in the absence of O 2 (at approximately one atmosphere of N 2 ) to be < 8 × 10 –16 cm 3 molecule –1 s –1

. Hynes et al. [553], Murrells et al. [842], and Diau and Lee [345] agree quite well on the value of k c, with an average value of 2.9 × 10 –14 being reported independent of temperature and pressure. Diau and Lee also report the rate constants for the reactions of the adduct (CS 2 OH) with NO and NO 2 to be 7.3 × 10 –13 and 4.2 × 10 –11 respectively.

The effective second order rate constant for CS 2 or OH removal in the above reaction scheme can be expressed as

1/k eff = (k b /k a k c )(1/P O2 ) + (1/k a )(1/P M )

### 1-83 where P O 2 is the partial pressure of O 2 and P M equals P O 2 + P N 2 . The validity of this expression requires that k a and k b are invariant with the P O 2 /P N 2 ratio. A 1/k vs 1/P O 2 plot of the data of Jones et al. [594] taken at atmospheric pressure exhibits marked curvature, suggesting a more complex mechanistic involvement of O 2 , whereas the data of Barnes et al. [69] and Hynes et al. [553] are more satisfactorily represented by this analytical expression. Nevertheless, while the qualitative features of the data from all three laboratories agree, there are some quantitative inconsistencies. First, under similar conditions of O 2 and N 2 pressures, the Barnes et al. rate constants lie approximately 60% higher than those of Jones et al. and up to a factor of 2 higher than those derived by Hynes et al. Secondly, two fits each of both the Barnes et al. and Hynes et al. data can be made: one at fixed P M and varying P O 2 , and the other at fixed P O 2 and varying P M (i.e., varying added N 2 ). Within each data set, rate constants calculated from bot h fits agree reasonably well for mole fractions of O 2 near 0.2 (equivalent to air) but disagree by more than a factor of 2 for measurements in a pure O 2 system. Finally, the temperature dependence (from 264–293 K) of the k eff values from Barnes et al. varies systematiccally from an E/R of –1300 K for experiments in pure O 2 (at 700 torr total pressure) to –2900 K for experiments in a 50 torr O 2 plus 650 torr N 2 mixture. An Arrhenius fit of the Hynes et al. data (from 251–348 K) recorded in synthetic air at 690 torr yields an E/R = –3300 K, although the data show marked curvature over the temperature range of study. These observations suggest that k a and k b may not be independent of the identity of M. For this reason, we limit our recommendation to air mixtures (i.e., P O 2 /P N 2 = 0.25) at atmospheric pressure. Since most CS 2 is oxidized within the atmospheric boundary layer, such restriction does not limit the applicability of this recommendation in atmospheric modeling. The present recommendation accepts the m easurements of Hynes et al. [553] , which appear to be the most sensitive of the three investigations. Thus, k(298 K) is derived from the Arrhenius fit of the data near room temperature. k(298 K) = 1.2 × 10 –12 cm 3 molecule –1 s –1

The uncertainty factor, f(298 K) = 1.5, encompasse s the results of Barnes et al. [69] within 2 σ

. To compute values of k below 298 K, we have accep ted the analysis of Hynes et al. k(T) = {1.25 × 10 –16 exp(4550/T)}/{T + 1.81 × 10 –3 exp(3400/T)} This recommendation is only valid for one atmosphere pressure of air. It is interesting to note that measurements by Hynes et al. [553] at approximately 250 K and 700 torr total pressure result in k eff values that are independent of the amount of O 2 for partial pressures between 145–680 torr. This suggests that the adduct is quite stable with respect to dissociation into the reactants (OH + CS 2 ) at this low temperature and the that effective rate constant for reactant removal approaches the elementary rate constant for adduct formation. From a mechanistic viewpoint, the primary produc ts of reaction c determine the products of CS 2 oxidation in air. Lovejoy et al. [757] have shown that the yields of both HO 2 and SO 2 are equal and near unity. Together with the earlier mentioned unity yield of OCS, these observations suggest that the oxidation equation

OH + CS 2 + 2O 2 → OCS + HO 2 + SO 2 describes this atmospheric system. Further insight is provided by the mechanistic study of Stickel et al. [1116], who observe OCS and CO product yields of (0.83±0.08) and (0.16±0.03) respectively. The results from this study are interpreted to imply that OCS and CO are formed either as primary products of the CS 2 OH + O 2 reaction or as products of a secondary reaction between a primary product and O 2 . These same authors report an SO 2 yield of (1.15±0.10), with the results suggesting that only about 75% of the SO 2 formed as a prompt product, with the remainder generate d via a slow reaction of SO (generated as a prompt product of the CS 2 OH + O 2 reaction) with O 2 . Insight into the specific reacti on pathways can be gleaned from the study of Lovejoy et al. [756] in which k c for the reaction of DOCS 2 + O 2 was found to be the same as that for HOCS 2 , indicating that simple H atom abstraction is not the likely process. Rather, HO 2 production most likely involves complex formation followed by HO 2 elimination. Lovejoy et al. [758] found that the 18 O atom in the 18 OH reactant is transferred pre dominantly (90 ± 20)% to the SO 2 product. These findings are consistent with an S–O-bonded CS 2 –OH adduct and preservation of the S–O bond in the steps leading to SO 2 formation. Additional work involving direct intermediate observations would be helpful in elucidating this reaction mechanism.

I14. OH + CH 3 SH. This recommendation is based on a composite fit to the data of Atkinson et al. [44], Wine et al. [1313], Wine et al. [1323], and Hynes and Wine [551], which are in excellent agreement. The results from the relative rate study of Barnes et al . [63] are in agreemen t with this recommendation and indicate that the higher value of Cox and Sheppard [291] is due to complications resulting from the presence of O 2 and NO in their reaction system. MacLeod et al. [766,767] and Lee and Tang [698] obtained rate constants at 298 K approximately 50% lower than recommended here. These authors also obtained lower values for the

### 1-84 ethanethiol reaction in comparison with results from studies upon which the methanethiol recommendation is made. Wine et al. [1323] present evidence that this reaction proceeds via adduct formation to produce a species that is thermally stable over the temperatur e range and time scales of the kinetic measurements. Tyndall and Ravishankara [1218] have determined the yield of CH 3 S (via laser–induced fluorescence) to be unity, indicating that any adduct must be short lived (less than 100 μs). Longer lifetimes would have led to anomalies in the OH decay kinetics used for the rate constant determinations. Hynes and Wine [551] failed to observe any effect of O 2 on the rate constant.

I15. OH + CH 3 SCH 3 . This recommendation is based on the results of Hynes et al. [555], Wine et al. [1313], Hsu et al. [540], Abbatt et al. [3], and Barone et al.[76]. The earlier higher rate constant values of Atkinson et al. [45] and Kurylo [662] are presumably due to reactive impurities, while t hose of MacLeod et al. [767] were most likely overestimated because of heterogeneous reactions. Absolute determinations lower than those recommended were obtained by Martin et al. [785], Wallingt on et al. [1247], and Ni elsen et al. [883]. While the reasons for these differences are not readily a pparent, these results are encompassed within the 2 σ error limits of the 298 K recommendation. Hynes et al. have demonstrated the importance of a second reaction channel involving addition of OH to dimethyl sulfide (approximately 30% in 1 atmosphere of air at 298 K). More recently, Hynes et al. and Bar one et al. have examined the reac tion mechanism in more detail using fully deuterated DMS. Both groups report similar rate constants for the bimolecular (non–adduct–forming) rate constant and adduct bond strengt hs (13.0 and 10.1 kcal/mole—Hynes et al.; 10.2 and 10.7 kcal/mole— Barone et al.) from second and third law calculations, respectively. Values of the rate constant for the reaction of the adduct with O 2 were also nearly identical (8 × 10 –13 cm 3 molecule –1 s –1 from Hynes et al., and 10 –12 cm 3 molecule –1 s –1 from Barone et al for both DMS and d 6 –DMS) independent of pressure and temperature. The recommendation given here is for the abstraction reaction only. Confirmation of the products as written is obtained from the study of Stickel et al. [1118] who determined an HDO product yield of (0.84±0.15) for the OD + CH 3 SCH 3 . Further mechanistic insight comes from the studies of Barnes et al. [72,73] and Turnipseed et al. [1203] who find that the abstraction product, CH 3 SCH 2 , leads predominantly to CH 3 S under atmospheric conditions. Barnes et al. measure a 0.7% yield of OCS under low NO
x conditions, which they attribute to further oxidation of CH 3 S. Both Barnes et al. and Turnipseed et al. find a significant (20–30%) yield of dimethyl sulfoxide, apparently produced via the reaction of the DMS–OH adduct with O 2 . Zhao et al. [1372] determined an upper yield of 0.07 for CH 3 elimination in the OD + CH 3 SCH 3 reaction system. Due to the rapid decomposition of a DMS–OH adduct, only the direct abstraction channel is measured in the absence of O 2 . The reaction of the adduct with O 2 , as quantified most r ecently by Hynes et al. and Barone et al., is responsible for the majority of the products formed in the atmospheric oxidation of DMS. An increase in the observed rate constant (k obs ) with increasing O 2 concentration has clearly been observed by Hynes et al. [555], Wallington et al. [ 1247], Barnes et al. [62], Niel sen et al. [883], Barone et al. [76], and Hynes et al. [550]. This O 2 effect has been suggested as an explanation fo r the higher rate constants obtained in many of the earlier relative rate studies. Hynes et al. give the following expression for the observed rate constant in one atmosphere of air:

10 10

obs 11 

### T exp( 234 / T) 8.46x10 exp(7230 / T) 2.68x10 exp(7810 / T) k 1.04x10 T 88.1exp(7460 / T) − − 

### −+ +

= + This expression was derived empirically from the analysis of a complex data set, which also yielded a value of the rate constant for reaction of the adduct with O 2 that was a factor of 4 larger than the values derived by Hynes et al. [550] and Barone et al. [76] and app eared to be both pressure and temperature dependent. The effect of these revisions in the adduct + O 2 rate constant on the k obs expression is not easily ascertained.

I16. OH + CH 3 SSCH 3 . This recommendation is based on the temperature–dependent studies of Wine et al. [1313] and Abbatt et al. [3] and the room temperature relative rate study of Cox and Sheppard [291]. Domine and Ravishankara [361] have observed both CH 3 S (via laser–induced fluorescence) and CH 3 SOH (via photoionization mass spectrometry) as products of this reaction. At 298 K, the yield of CH 3 S alone was quantified at approximately 30%. An FTIR product study of the photooxidation of dimethyl disulfide by Barnes et al. [71] presents evidence that oxidation of the CH 3 SOH product is the principal source of the methane sulfonic acid observed.

I17. OH + S. This recommendation is based on the study by Jourdain et al. [596]. Their measured value for k(298 K) compares favorably with the r ecommended value of k(O + OH) when one considers the slightly greater exothermicity of the present reaction.

I18. OH + SO. The value recommended for k(298 K) is an average of the determinations by Fair and Thrush [380] and Jourdain et al. [596]. Both sets of data have been corrected using the present recommendation for the O + OH reaction.

### 1-85 I19. HO 2 + H 2 S, HO 2 + CH 3 SH, HO 2 + CH 3 SCH 3 . These upper limits are taken from the discharge flow laser magnetic resonance study of Mellouki and Ravishankara [808]. The H 2 S value disagrees with the rate constant reported by Bulatov et al. [171] by approximately three orders of magnitude. The reason for this difference is not readily apparent. However, the recommended upper limit is consistent with the values for CH 3 SH and CH 3 SCH 3 , which respectively agree with upper limits from the work of Barnes et al. [63] and Niki (reported as a private communication in the Mellouki and Ravishankara paper).

I20. HO 2 + SO 2 . This upper limit is based on the atmospheric pressure study of Graham et al. [452]. A low pressure laser magnetic resonance study by Burrows et al. [176] places a some what higher upper limit on k(298 K) of 4 × 10 –17 (determined relative to OH + H 2 O 2 ). Their limit is based on the assumption that the products are OH and SO 3 . The weight of evidence from both studies suggests an error in the earlier determination by Payne et al. [938].

I21. NO 2 + SO 2 . This recommendation is based on the study of Penzhorn and Canosa [940] using second derivative UV spectroscopy. While these authors actually report a measured value for k(298 K), their observations of strong heterogene ous and water vapor catalyzed e ffects prompt us to accept their measurement as an upper limit. This value is approximately two orders of magnitude lower than that for a dark reaction observed by Jaffe and Klein [567], much of which may have been due to heterogeneous
processes. Penzhorn and Canosa suggest that the products of this reaction are NO + SO 3 . I22. NO 3 + H 2 S. This recommendation accepts the upper limit set by Dlugokencky and Ho ward [348] based on experiments in which NO 3 loss was followed in the presence of large concentrations of H 2 S. Less sensitive upper limits for the rate constant have been reported by Wallington et al . [1249] and Cantre ll et al. [197].

I23. NO 3 + OCS. This upper limit is based on the relative rate data of MacLeod et al. [764].

I24. NO 3 + CS 2 . This upper limit is based on the study of Burrows et al. [180]. A somewhat higher upper limit was derived in the relative rate data of MacLeod et al. [764].

I25. NO 3 + CH 3 SH. The recommended values are derived from a composite fit to the data of Wallington et al. [1249], Rahman et al. [975], and Dlugokencky and Howard [348]. The room temperature rate constant derived in the relative rate experiments of MacLeod et al. [764] is in good agreement with the recommended value. The suite of investigations shows the rate cons tant to be pressure independent over the range 1–700 torr. Dlugokencky and Howard place an upper limit of 5% on the production of NO 2 via this reaction at low pressure. Based on the product distribution observed in their investigation, Jensen et al. [583] propose a reaction mechanism initiated by abstraction of th e hydrogen atom from the SH group, possibly after formation of an initial adduct as suggested by Wallington et al. and Dlugokencky and Howard.

I26. NO 3 + CH 3 SCH 3 . The recommended values are derived from a composite fit to the data of Wallington et al. [1249], Tyndall et al. [1209], and Dlugokencky and Howard [348]. The relative rate study of Atkinson et al. [47] yields a rate constant at room temperature in good agreement with that recommended. The experimental data from all investigations demonstrate the pressure independence of the rate constant over the range 1–740 torr. Room temperature investigations by Daykin and Wine [323] and Wallington et al. [1250] are also in agreement with the recommended value. Jensen et al. [582] propose a mechanism that involves hydrogen abstraction as the first step to explain their observed product distribution. In a later study, Jensen et al. [583] measured a kinetic isotope effect for the rate constant for CH 3 SCH 3 vs. that for CD 3 SCD 3 of k H /k D = (3.8±0.6), providing further confirmation of such abstraction. Butkovskaya and Le Bras [182] utilized chemical titration of th e primary radical produced from NO 3 + CH 3 SCH 3 in a discharge flow mass spectrometer system to show that the reaction produces predominantly CH 3 SCH 2 + HNO 3 . An upper limit of 2% was placed on the reaction channel yielding CH 3 + CH 3 SONO 2 . I27. NO 3 + CH 3 SSCH 3 . The recommended values were derived from a composite fit to the data of Wallington et al. [1249] and Dlugokencky and Howard [348]. The investigation by Atkinson et al. [39] indicates that the relative rate technique cannot be cons idered as yielding reliable rate data for this reaction due to chemical complexities. Thus, the much lower room temperature results from the study of MacLeod et al. [764] can be considered to be erroneous. Based on their observations of intermediate and end products, Jensen et al. [583] proposed a reaction mechanism in which the initial addition of NO 3 to one of the sulfur atoms results in formation of CH 3 S + CH 3 SO + NO 2 . I28. NO 3 + SO 2 . This recommended upper limit for k(298 K) is based on the study by Daubendiek and Calvert [305]. Considerably higher upper limits have been derived by Burrows et al. [180], Wallingt on et al. [1249], Canosa–Mas et al. [192], and Dlugokencky and Howard [348].

I29. N 2 O 5 + CH 3 SCH 3 . This recommendation is based on the value es timated by Tyndall and Ravishankara [1219] from the study by Atkinson et al. [47].

### 1-86 I30. CH 3 O 2 + SO 2 . This recommendation accepts the results from th e study of Sander a nd Watson [1022], which is believed to be the most appropriate for stratospheric modeling purposes. These authors conducted experiments using much lower CH 3 O 2 concentrations than employed in the earlier investigations of Sanhueza et al. [1027] and Kan et al. [607], both of which resulted in k(298 K) values approximately 100 times greater. A later report by Kan et al . [606] postulates that these differences are due to the reactive removal of the CH 3 O 2 SO 2 adduct at high CH 3 O 2 concentrations prior to its reversible decomposition into CH 3 O 2 and SO 2 . They suggest that such behavior of CH 3 O 2 SO 2 or its equilibrated adduct with O 2 (CH 3 O 2 SO 2 O 2 ) would be expected in the studies yielding high k values, while decomposition of CH 3 O 2 SO 2 into reactants would dominate in the Sander and Watson experiments. It does not appear likely that such secondary reactions involving CH 3 O 2 , NO, or other radical species would be rapid enough, if they occur under normal stratospheric conditions to comp ete with the adduct decomposition. This interpretation, unfortunately, does not explain the high rate consta nt derived by Cocks et al. [ 265] under conditions of low [CH 3 O 2 ].

I31. F + CH 3 SCH 3 . This recommendation is based on the discharge flow mass spectrometric study by Butkovskaya et al. [183]. The uncertainty placed on this recomme ndation has been increased over that estimated by the authors to reflect the lack of any confirming investigations. Titration of the primary organic radical products indicated that the reaction proceeds via two channels to produce HF + CH 3 SCH 2 and CH 3 + CH 3 SF with a branching ratio of approximately 0.8/0.2 respectively.

I32. Cl + H 2 S. This recommendation is based on the study by Nicovich et al. [870], who conducted an elaborate study with attention to sources of possible systematic error. The rate constant at 298 K is in good agreement with that determined by Nesbitt and Leone [857], who refined the data of Braithwaite and Leone [149], but is significantly greater than the values reported by Clyne and Ono [256], Clyne et al. [247], and Nava et al. [847]. The small, but clearly observed, negative activation energy determined by Ni covich et al. contrasts with the lack of a temperature dependence observed by Nava et al.. In fact, at the lowest temperature of overlap, the results from these two studies differ by 50%. Nevertheless, the Nicovich et al. study yields consistent results for both H 2 S and CH 3 SH as well as for D 2 S and CD 3 SD. While the reason for these differences remains to be determined, the full range of reported values is encompassed within the 2 σ error limits recommended. Lu et al. [761] also measured a temperature–independent rate constant but report a value at 298 K, about 40% greater than that of Nicovich et al. However, the presence of 4000 torr of CF 3 Cl bath gas in the Lu et al. may suggest a slight pressure dependence of th e reaction, although Nicovi ch et al. observed no pressure dependence for pressures ranging up to 600 torr with N 2 . I33. Cl + OCS. This upper limit is based on the minimum detectable decrease in atomic chlorine measured by Eibling and Kaufman [376]. Based on the observation of product SCl, these authors set a lower limit on k(298 K) of 10 –18 for this reaction channel. Considerably higher upper limits on k(298 K) were determined in the studies of Clyne et al. [247] and Nava et al. [847].

I34. Cl + CS 2 . This upper limit for the overall reaction is based on determinations by Nic ovich et al. [869] and Wallington et al. [1246]. The first authors confirm that the reacti on proceeds via reversible adduct formation as suggested by Martin et al. [783]. The much larger rate constant values determined by Martin et al. may possibly be attributed to reactive impurities in the CS 2 sample. Nicovich et al. set an upper limit on the rate constant for the adduct (CS 2 Cl) reacting with O 2 of 2.5 × 10 –16 at room temperature.

I35. Cl + CH 3 SH. This recommendation is based on the results of Nicovich et al. [870], who used laser photolysis with resonance fluorescence detection to study the reactions of Cl with H 2 S, D 2 S, CH 3 SH, and CD 3 SD. The room temperature determination by Nesbitt and Le one [857] is in good agreement with the value recommended. The k(298 K) value from the study by Mellouki et al. [804] is nearly a factor of 2 lower. However, the low sensitivity of EPR detection of Cl atoms did not permit these latter authors to conduct a precise determination of k under pse udo–first–order conditions, and a more complex analysis of experiments conducted under second–order conditions was required. Nesbitt and Leone [858] report that less than 2% of the reaction occurs via abstrac tion of an H atom from the CH 3 group.
I36. Cl + CH 3 SCH 3 . Stickel et al. [1117] have used laser photolysis resonance fluorescence to measure that rate constant between 240–421 K, over the pressure range of 3–700 torr. The rate constant is near collisional but increases with increasing pressure from a low pressure limit of 1.8×10 –10 to a value of 3.3×10 –10 at 700 torr. The yield of HCl at 297 K, measured by diode laser spectroscopy, decreased from near unity at low pressure to a value of approximately 0.5 at 203 to rr, suggesting that st abilization of a (CH 3 ) 2 SCl adduct becomes competitive with hydrogen atom abstraction with increasing pressure. These investigators also observed a negative temperature dependence for the reaction. Butkovskaya et al. [183] conducted a discharge flow mass spectrometric study at 298 K, in which they determined that the reaction proceeds to form HCl + CH 3 SCH 2 almost exclusively at 1 torr total pressure. The sum of all other possible cha nnels was estimated at less than 3%. Zhao et al. [1372] used laser photolysis coupled with CH 3 detection by time–resolved tunable diode laser

### 1-87 absorption spectroscopy to determine an upper limit for CH 3 elimination at 298 K and pressures between 10–30 torr. Room temperature measurements by Nielsen et al. [882] at 740 torr and Kinnison et al. [626] at 760 torr agree quite well with the results of Stickel et al. Kinnison et al. also observed the rate constant to increase from 3.6 × 10 –10 to 4.2 × 10 –10 cm 3 molec –1 s –1 when the bath gas was changed from pure N 2 to synthetic air, suggesting that the (CH 3 ) 2 SCl adduct reacts with O 2 . I37. ClO + OCS; ClO + SO 2 . These recommendations are based on the discharge flow mass spectrometric data of Eibling and Kaufman [376]. The upper limit on k(298 K) for ClO + OCS was set from the minimum detectable decrease in ClO. No products were observed. The upper limit on k(298 K) for ClO + SO 2 is based on the authors’ estimate of their SO 3 detection limit. The upper limit for this same reaction based on the minimum detectable decrease in ClO was not used due to the potential problem of ClO reformation from the Cl + O 3 source reaction.

I38. ClO + CH 3 SCH 3 . This recommendation is based on the study by Barnes et al. [67] using discharge flow mass spectrometry. The authors prefer the present value of the rate constant to one a factor of 4 higher, which they determined in an earlier version of their apparatus. The uncertainty factor re flects the absence of any confirming investigations.

I39. ClO + SO. The value of k(298 K) is an average of the determinations by Clyne and MacRobert [246] and Brunning and Stief [162]. The temperature independence is taken from the latter study with the A–factor recalculated to fit the k(298 K) recommendation.

I40. Br + H 2 S, Br + CH 3 SH. These recommendations are based on the study by Nicovich et al. [867] who measured both the forward and reverse reactions by time–resolved resonance fluorescence detection of Br
atoms. The uncertainties placed on these recommendations have been increased over those estimated by the authors to reflect the absence of any confirming investigations.

I41. Br + CH 3 SCH 3 . Wine et al. [1315] used laser photolysis res onance fluorescence to study reversible adduct formation in the Br + CH 3 SCH 3 reaction system over the temperature range 260 – 310 K from which they derive a (CH 3 ) 2 S–Br bond strength of 14.5 ± 1.2 kcal mole –1

. Above 375 K, adduct decomposition is so rapid that the addition channel is effectively negligible. Extrapolation of these data to conditions typical of the springtime Arctic boundary layer (760 torr, 230 – 270 K) leads these authors to suggest that under such conditions, the addition of Br to CH 3 SCH 3 proceeds with a rate constant of approximately 1.3 × 10 –10 cm 3 molecule –1 s –1

. Researchers from the same laboratory (Jefferson et al. [573]) studied th e abstraction reaction over the temperature range 386 – 604 K. These authors observed the reactants to be in equilibrium with the products HBr + CH 3 SCH 2 and determined Arrhenius expressions for the forward and reverse reactions respectively of 9.0 × 10 –11 exp(–2386/T) cm 3 molecule –1 s –1 and 8.6 × 10 –13 exp(836/T) cm 3 molecule –1 s –1

. Analysis of the equilibrium data also permitted determination of the heat of formation of CH 3 SCH 2 (see Appendix 1).

I42. BrO + CH 3 SCH 3 . This recommendation is based on the discharge flow mass spectrometric study by Bedjanian et al. [99], performed at 1 torr over the temperature range 233–320 K. The rate constant at 298 K is nearly identical to that derived by Barnes et al. [67], using a similar experimental system. Bedjanian et al. also determined a near unity yield for the production of di methylsulfoxide and suggest that the reaction proceeds via production of an adduct that decomposes into the sulfoxide and bromine atoms.

I43. BrO + SO. This recommendation is based on the measurements of Brunning and Stief [163] performed under both excess BrO and excess SO conditions. The rate constant is supported by the lower limit assigned by Clyne and MacRobert [246] from measurements of SO 2 production.

I44. IO + CH 3 SH. The value of k(298 K) comes from the study by Maguin et al. [769] using discharge flow mass spectrometry. The investigators establish a branching ratio near unity for the production of HOI. The uncertainty factor reflects the absen ce of any confirming investigations.

I45. IO + CH 3 SCH 3 . This recommendation comes from the studies by Daykin and Wine [321] using laser photolysis absorption spectroscopy and by Maguin et al. [769] and Barnes et al. [67] using discharge flow mass spectroscopy. These groups obtained rate constants of 

### ≤ 3.5 × 10 –14 , 1.5 × 10 –14 , and 8.8×10 –15 respectively. The last two studies supersede earlier, less direct measurements by the same groups, which resulted in rate constants of 1.5 × 10 –11 (Martin et al. [784]) and 3.0 × 10 –11 (Barnes et al. [68]).

I46. S + O 2 . This recommendation is based primarily on the study of Davis et al. [316]. Modest agreement at 298 K is found in the studies of Fair and Thrush [380], Fa ir et al. [381], Donovan and Little [364], and Clyne and Townsend [257]. The study by Clyne and Whitefield [264], which indicates a slightly negative E/R between 300 and 400 K, is encompassed by the assigned uncertainty limits.

### 1-88 I47. S + O 3 . This recommendation accepts the only available expe rimental data of Cl yne and Townsend [257]. In this study the authors measure a value of the rate constant for S + O 2 in reasonable agreement with that recommended above.

I48. SO + O 2 . This recommendation is based on the low temperature measurements of Black et al. [133,134]. The room temperature value accepts the results of the more recent pape r as recommended by the authors. The uncertainties cited reflect the need for further confirmation and the fact that these results lie significantly higher than an extrapolation of the higher temperature data of Homann et al. [520]. A room temperature upper limit on k set by Breckenridge and Miller [150] is consistent with the Black et al. data.

I49. SO + O 3 . The value of k(298 K) is an average of the determinations by Halstead and Thrush [474], Robertshaw and Smith [1004], and Black et al . [133,134] using widely different techniques. The value of E/R is an average of the values reported by Halstead a nd Thrush and Black et al. [134], with the A-factor recalculated to fit the recommendation for k(298 K).

I50. SO + NO 2 . The value of k(298 K) is an average of the determinations by Clyne and MacRobert [245], Black et al. [133], and Brunning and Stief [162], which agree quite well with the rate constant calculated from the relative rate measurements of Clyne et al. [241]. The Arrhenius parameters are taken from Brunning and Stief.

I51. SO + OClO. This recommendation is based on the room temperature study by Clyne and MacRobert [246]. The uncertainty reflects the absence of any confirming investigation.

I52. SO 3 + H 2 O. Several research groups have attempted to quantif y the rate of sulfuric acid formation via this reaction in the gas phase. Reiner and Arnold [1000] placed an upper limit of 2.4 × 10 –15 cm 3 molec –1 s –1 on the rate constant, slightly lower than that determined by Wang et al. [1274]. The inability to cite the results as other than an upper limit is due to the difficulty in excluding all heterogeneous effects from the experiments. The higher rate constant reported earlier by Castleman et al. [203] may have resulted from an underestimation of the effects of such heterogeneous reactions. Subsequently, Reiner and Arnold [1001] sought to improve their rate constant determinati on by more detailed quantification of heterogeneous contributions. They derived a value of 1.2 × 10 –15 cm 3 molec –1 s –1 , independent of pressure (from 31–260 mbar of synthetic air). Evidence was also obtained that H 2 SO 4 was, indeed, the product of the reaction. Kolb et al. [647] attempted to measure the gas phase reaction using a turbulent flow reactor designed to minimize wall effects. Their results, when analyzed as representing a bimolecular reaction, support a rate constant between (1 – 7) × 10 –15 cm 3 molec –1 s –1

. However, a more considered analysis of the data indicated that the gas phase reaction was second order in water vapor. The reaction rate was also observed to increase as the temperature was lowered from 333 K to 243 K. These observations, together with calculations by Morokuma and Mugurama [835], led the latter authors to suggest that SO 3 consumption likely involved its reaction with the water dimer or the reaction of SO 3 . H 2 O + H 2 O, leading to the formation of sulfuric acid.

A laminar flow reactor st udy by Lovejoy et al. [ 755] over the temperature ra nge 256–360 K also revealed SO 3 loss to be second order in water concentration a nd independent of pressure (from 20 to 80 torr of N 2 at 300 K). These latter authors measured a strong negative temperature dependence for the rate constant and a significant kinetic isotope effect (k H2O ≈ 2k D2O ), leading them to describe th e reaction as proceeding via the rapid association between SO 3 and H 2 O followed by a slower reaction between the adduct and water to form sulfuric acid. Lovejoy at al.’s measurement of a –13 kcal mol –1 “activation” energy was viewed as energetically inconsistent with the SO 3 + water dimer reaction mechanis m since it would require a large negative activation energy for the SO 3 + (H 2 O) 2 step. The first order expression for SO 3 loss derived by these authors is 2.26 × 10 –43 T exp(6544/T) [H 2 O] 2 and is recommended here.

I53. SO 3 + NO 2 . This recommendation is based on the study of Penzhorn and Canosa [940] using second derivative UV spectroscopy. These authors observe the production of a white aerosol, which they interpret to be the adduct NSO 5 . This claim is supported by ESCA spectra.

I54. SH + O 2 . This upper limit for k(298 K) is based on the study by Stac hnik and Molina [1102] utilizing experiments sensitive to the production of OH. Somewhat higher upper limits of 1.0 × 10 –17 and 1.5 × 10 –17 were assigned by Friedl et al. [410] and Wang et al . [1272] respectively from the detection sensitivities for OH detection and SH decay respectively. An even higher upper limit by Black [130], based on the lack of SH decay, may have been compli cated by SH regeneration. Much less sensitive upper limits have been calculated by Tiee et al. [1174], Nielsen [874], and C upitt and Glass [296]. Stachnik and Molina [1102] also report a somewhat higher upper limit (< 1.0 × 10 –18 ) for the rate constant for the sum of the two SH + O 2 reaction channels (producing OH + SO and H + SO 2 ).

I55. SH + O 3 . The value for k(298 K) is an average of the determinations by Friedl et al. [410] (laser–induced fluorescence detection of SH), Schonle et al. [1041] (mass spectrometric de tection of reactant SH and product

### 1-89 HSO) as revised by Schindler and Benter [1034], a nd Wang and Howard [1271] (laser magnetic resonance detection of SH). The temperature dependence is from Wang and Howard with the A–factor calculated to agree with the recommended value for k(298 K). ∆ E/R reflects the fact that the temperature dependence comes from measurements above room temperature and, thus, extrapolation to lower temperatures may be subject to additional uncertainties. Wang and Howard report observing a minor reaction channel that produces H + SO + O 2 . I56. SH + H 2 O 2 . This recommended upper limit for k(298 K) is based on the study of Friedl et al. [410]. Their value is calculated from the lack of SH decay (measur ed by laser–induced fluores cence) and the lack of OH production (measured by resonance fluorescence). The three possible product channels yield: H 2 S + HO 2 , HSOH + OH, and HSO + H 2 O.

I57. SH + NO 2 . This recommendation is based on the measurements of Wang et al. [1272]. These authors suggest that the lower values of k(298 K) reported by Black [130], Friedl et al. [410], and Bulatov et al. [168] are due to SH regeneration from the H 2 S source compound. In the study by Stachnik and Molina [1102], attempts were made at minimizing such regenerati on, and the reported value of k(298 K) was significantly higher than that from the earlier studies, but still 30% lower than that measured by Wang et al., who used two independent SH source reactions. A slightly higher rate constant measured by Schonle et al. [1041], as revised by Schindler and Benter [1034], has not been recommended due to the somewhat more limited database for their determination. The reaction as written represents the most exothermic channel. In fact, HSO has been detected as a product by Leu and Smith [723], Bulatov et al. [168], Schonle et al. [1041], and Wang et al. [1272]. The absence of a primary deuterium isotope effect, as observed by Wang et al. [1272], coupled with the large magnitude of the rate constant suggests that the (four–center intermediate) channels producing SO + HNO and OH + SNO are of minor importance. No evidence for a three–body combination reaction was found by either Black [130] or Friedl et al. [410]. Based on a pressure independence of the rate constant between 30–300 torr, Black set an upper limit of 7.0 × 10 –31 for the termolecular rate constant. Similarly, Stachnik and Molina [1102] saw no change in decay rate between 100 and 730 torr with O 2 (although these O 2 experiments were designed prim arily to limit SH regeneration). The recommendation given here is supported by the recent discharge flow lase r–induced fluorescence study of the SD + NO 2 reaction by Fenter and Anderson [388]. These investigators report a rate constant at 298 K of 6.8 × 10 –11 cm 3 molec –1 s –1 , which compares favorably with the value of 7.1 × 10 –11 cm 3 molecule –1 s –1 determined in the Wang et al. of the same reaction. Fenter and Anderson also obtained an E/R value of –210 K, very similar to the –237 K value derived by Wang et al. for the SH reaction.

I58. SH + Cl 2 ; SH + BrCl; SH + Br 2 ; SH + F 2 . The recommendations for these reactions are derived from the data of Fenter and Anderson [387] for the SD radical. The uncertainties have been in creased over those estimated by the investigators to reflect the absence of any conf irming investigations and the influence of the secondary isotope effect. For the BrCl reaction, the channel producing ClSD + Br was found to be described by the rate expression k = 2.3 × 10 –11 exp(100/T).

I59. HSO + O 2 . This recommendation is based on the study by Lovejoy et al. [759], who employed laser magnetic resonance monitoring of HSO in a discharge flow system. The upper limit thus derived for k(298 K) is nearly two orders of magnitude lower than measured by Bulatov et al. [170].

I60. HSO + O 3 . This recommendation is based on the determinations by Friedl et al. [410] and Wang and Howard [1271]. In the first study, performed at higher O 3 concentrations, greater quantities of HSO were produced in the flow tube and SH approached a steady state due to its generation via HSO + O 3 . The rate constant for this reaction was thus determined relative to SH + O 3 from measurements of the stead y state SH concentration as a function of the initial SH concentration. In the second study, the rate constant and its branching ratio were measured at two temperatures. At room temperature, the overall rate constant is in excellent agreement with that of Friedl et al. More recently, Lee et al. [705] determined a room temperature rate constant of 4.7 × 10 –14 for the sum of all reaction channels not producing HS. This value is approximately 30% greater than that measured by Wang and Howard for the same channels. Lee et al. derive an Arrh enius activation energy of 1120 K for these channels from data between 273–423 K, in agreement with the more limited temperature data of Wang and Howard. The lack of an isotope effect when SD was employed in the Friedl et al. study suggests that the products of the HSO + O 3 reaction are SH + 2O 2 (analogous to those for HO 2 + O 3 ). However, Wang and Howard found that only 70% of the reaction leads to HS formation. In addition, their observations of HO 2 production in the presence of O 2 suggests the existence of a reaction channel producing HSO 2 + O 2 followed by HSO 2 + O 2 → HO 2 + SO 2 . At the present time, no recommendation is given for the product channels. Further mechanistic work is suggested, since it is important to understand wh ether this reaction in the atmosphere leads to HS regeneration or to oxidation of the sulfur.

### 1-90 I61. HSO + NO; HSO + NO 2 . The recommendations for these reactions are based on the study by Lovejoy et al. [759] in which laser magnetic resonance was used to monitor HSO in a discharge flow system. Their upper limit for the NO reaction is a factor of 25 lower than the rate constant measured by Bulatov et al. [169] using intracavity laser absorption at pressures between 10 and 100 torr. Since it is unlikely that this reaction rate undergoes a factor of 25 increase between 1 torr (the pressure of the Lovejoy et al. work) and 10 torr, the higher rate constant may be due to secondary ch emistry associated with the HSO production methods employed.

The recommendation for the NO 2 reaction is a factor of 2 higher than the rate constant reported by Bulatov et al. [168]. Lovejoy et al. have attributed this differe nce to HSO regeneration under the experimental conditions used by Bulatov et al. [168]. The product assignment for this reac tion is discussed in the note for the HSO 2 + O 2 reaction.

I62. HSO 2 + O 2 . This recommendation is based on the rate of HO 2 formation measured by Lovejoy et al. [759] upon addition of O 2 to the HSO + NO 2 reaction system. While HSO 2 was not observed directly, a consideration of the mechanistic possibilities for HSO + NO 2 , coupled with measurements of the HO 2 production rate at various O 2 pressures, led these authors to suggest that HSO 2 is both a major product of the HSO + NO 2 reaction and a precursor for HO 2 via reaction with O 2 . I63. HOSO 2 + O 2 . This recommendation is based on the studies of Gleason et al. [444] and Gleason and Howard [442] in which the HOSO 2 reactant was monitored using a chemical ionization mass spect rometric technique. Gleason and Howard conducted their measurements over the 297–423 K temperature range in the only temperature dependence investigation. Thus, ∆ E/R has been increased from th eir quoted limits to account for the potential uncertainties in extrapolating their data to sub–ambient temperatures. The value of k(298 K) derives further support from the studies of Margitan [774] and Martin et al. [786], both of whom used modeling fits of OH radical decays in the OH + SO 2 + M reaction system in the presence of O 2 and NO. In this latter analysis, the HOSO 2 reacts with O 2, yielding HO 2 , which subsequently regenerates OH through its reaction with NO. The infrared spectrum of HOSO 2 has been recorded in low temperature matrix isolation experiments by Hashimoto et al. [486] and Nagase et al. [845]. Mass spectrometric detection of HOSO 2 in the gas phase has also been reported by Egsgaard et al. [374].

I64. CS + O 2 . The recommendation given for k(298 K) is based on the work of Black et al. [132] using laser– induced fluorescence to monitor CS. This value agrees with the somewhat less precise determination by Richardson [1003] using OCS formation rates. The latter author presents evid ence that this reaction channel dominates over the one producing SO + CO by more than a factor of 10. Measurements by Richardson at 293 K and 495 K yield an E/R of 1860 K. However, use of this activation energy with the recommended value of k(298 K) results in an unusually low Arrhenius A-factor of 1.5 × 10 –16

. In view of this, no recommendation is given for the temperature dependence.

I65. CS + O 3 ; CS + NO 2 . The k(298 K) recommendations for both reacti ons accept the results of Black et al. [132], who used laser–induced fluorescence to monitor the CS reactant in a room temperature experiment. The uncertainty factors reflect the ab sence of any confirming measurements.

I66. CH 3 S + O 2 . This upper limit is based on the study by Tyndall and Ravishankara [1217]. Somewhat higher upper limits were derived in the earlier studies of Balla et al. [60] and Black and Jusinski [131].

I67. CH 3 S + O 3 . This recommendation is based on the temperature–dependent study of Turnipseed et al. [1201] and the room temperature determinations of Tyndall and Ravishankara [1218] and Domine et al. [362]. Domine et al. measured the yield of CH 3 SO to be 15% at low pressure and used this value to revise the corrections applied in the Tyndall and Ravi shankara investigation to account for CH 3 S regeneration by CH 3 SO + O 3 . A failure to observe significant reaction in the study by Black and Jusinski [131] is interpreted as due to rapid regeneration of CH 3 S in their system. The value of g has been set larger than that derived by Turnipseed et al. to reflect the existence of only one temperature dependence investigation.

I68. CH 3 S + NO. The upper limit for the bimolecular reaction between CH 3 S and NO is based on estimates by Balla et al. [60], who conducted a temperature dependence study of the termolecular reaction.

I69. CH 3 S + NO 2 . This recommendation is based on the temperature dependent data of Turnipseed et al. [1201] and the room temperature results of Tyndall and Ravishankara [1217]. The room temperature value of Domine et al. [360] is encompassed by the recommended uncertainty factor. The value of ∆ E/R has been set larger than that derived by Turnip seed et al. to reflect the existen ce of only one temperature dependence investigation. An earlier study by Balla et al. [60] yielded a room temperature rate constant nearly a factor of two higher than the present recommendation, which may be attributed to seconda ry reactions at higher radical concentrations. Tyndall and Ravishankara determined the NO yield to be (80 ± 20)%. Together with

### 1-91 the unity yield of CH 3 SO obtained by Domine et al., this implies that the primary reaction channel is as written.

I70. CH 2 SH + O 2 . This recommendis the ation average of the rate constant obtained by Rahman et al. [976] in a fast flow mass spectrometer system and that from Anastasi et al. [20] using a pulse radiolysis kinetic absorption apparatus. The value of Anastasi et al. is n early twice that of Rahman et al. It is difficult at present to indicate a preference for the results of one study over the other, and the value of f(298 K) has been chosen to reflect this uncertainty. Since this is a fast bimolecular reaction, one would expect the products to be HO 2 + CH 2 S, by analogy with the reaction between CH 2 OH and O 2 . I71. CH 2 SH + O 3 . The value of k(298 K) comes from the study by Rahman et al. [976] using fast flow mass spectrometry. The uncertainty factor re flects the absence of any confirming investigations.

I72. CH 2 SH + NO. The value of k(298 K) comes from the study by Anastasi et al. [20] using a pulse radiolysis kinetic absorption apparatus. The uncertainty factor re flects the absence of any confirming investigations.

I73. CH 2 SH + NO 2 . This recommendation averages the rate constant obtained by Rahman et al. [976] in a fast flow mass spectrometer system with that from Anastasi et al. [20], using a pulse radiolysis kinetic absorption apparatus. The value of Rahman et al. is near ly twice that of Anastasi et al. It is difficult at present to indicate a preference for the results of one study over the other, and the value of f(298 K) has been chosen to reflect this uncertainty.

I74. CH 3 SO + O 3 . This recommendation is based on the study by Domine et al. [362]. It is supported by the study of Tyndall and Ravishankara [1218], in which the rate constant was derived from a complex analysis of the CH 3 S + O 3 reaction system. Domine et al. place the direct yield of CH 2 SO at approximately 10% and that of CH 3 S at 13% at low pressure.

I75. CH 3 SO + NO 2 . This recommendation is based on the direct measurements of Domine et al. [360]. The results are supported by somewhat less direct measurements of Tyndall and Ravishankara [1217] and Mellouki et al. [803].

I76. CH 3 SOO + O 3 , CH 3 SOO + NO, CH 3 SOO + NO 2 . These recommendations are based on the experiments of Turnipseed et al. [1201] in which CH 3 S was monitored by LIF in equilibrium with CH 3 SOO. The upper limit for the O 3 reaction was determined from experiments at 227 K. The results for the NO and NO 2 reactions were independent of temperature over the ranges 227–256 K and 227–246 K, respectively. The uncertainties placed on these recommendations have been increased ove r those estimated by the authors to reflect the absence of any confirming investigations.

I77. CH 3 SO 2 + NO 2 . This recommendation is based on the study by Ray et al. [994] using a di scharge flow reactor equipped with laser–induced fluorescence and mass spectrometric detection. The CH 3 SO 2 was produced by the sequential oxidation of CH 3 S and CH 3 SO by NO 2 and is to be differentiated from the weakly bound adduct, CH 3 SOO, formed by the reaction of CH 3 S with O 2 at low temperature (Turnipseed et al [1201]). The uncertainty limit on the rate constant has been increased over that given by the aut hors to reflect the absence of any confirming investigation. However, some additional support for this recommendation does come from the study of the CH 3 S + NO 2 reaction by Tyndall and Ravishankara [1217]. These authors observed fluorescence from a product species tentatively identified as CH 3 SO 2 , produced by the reaction of CH 3 SO with NO 2 . Computer simulation of the rise and fall of the fluorescence signal yielded an approximate rate constant value for the reaction CH 3 SO 2 + NO 2 of 7.0 × 10 –12 cm 3 molec –1 s –1

. However, an unambiguous differentiation between the production and disapp earance rate constants was not possible.

I78. CH 3 SCH 2 + NO 3 . This recommendation is based on the experime nts of Butkovskaya and Le Bras [182]. The uncertainty factor reflects the absen ce of any confirming investigation.

I79. CH 3 SCH 2 O 2 + NO. This recommendation is based on the experiments of Wallington et al. [1257]. The uncertainty factor reflects the absen ce of any confirming investigation.

I80. CH 3 SS + O 3 . This recommendation is based on the discharge flow photoionization mass spectroscopy study by Domine et al. [362]. The uncertainty factor re flects the absence of any confirming investigations. The rate constant ratio for the reactions of CH 3 SS with O 3 and NO 2 is consistent with the rate constant ration for the corresponding CH 3 S reactions.

I81. CH 3 SS + NO 2 ; CH 3 SSO + NO 2 . These recommendations are based on the discharge flow photoionization mass spectroscopy study by Domine et al. [360]. The rate constant ratio for these two reactions agrees with that observed for other RS/RSO radicals with NO 2 . The assigned uncertainties re flect this agreement but acknowledge the absence of any confirming investigation. In the Domine et al. study, CH 3 SSO was produced by reacting away all CH 3 SS with high NO 2 concentrations. Thus, as expected, O atom transfer may be the primary channel in the CH 3 SS reaction.

### 1-92 J1. Na + O 3 . The recommendation is based on the measurements of Ager et al. [13], Worsnop et al. [1333] as corrected in Worsnop et al. [1334], and Plane et al. [953]. The data of Worsnop et al. supersede earlier work from that laboratory (Silver and Kolb [1063]). Measurements made by Husain et al. [546] at 500 K are somewhat lower, probably because they did not recognize that secondary chemistry, NaO + O 3 → Na + 2O 2 , interferes with the rate coefficient measurement. The temperature dependence is from results of Worsnop et al. [1334] (214–294 K) and Plane et al. [953] (208–377K). Ager et al. [13] estimate that the NaO 2 + O product channel is 

### ≤ 5%. Evidence that the NaO product is in the 2 Σ + excited electronic state was reported by Shi et al. [1058] and Wright et al. [1335].

J2. Na + N 2 O. The recommendation incorporates the data of Husain and Marshall [545], Ager et al. [13], Plane and Rajasekhar [954], and Worsnop et al. [1334]. Silver and Kolb [1063] measured a rate coefficient at 295 K that is lower and is superseded by Worsnop et al. [1334]. Helmer and Plane [497] report a measurement at 300 K in excellent agreement with the recommendation. Earlier, less direct studies are discussed by Ager et al. [13]. The NaO product does not r eact significantly with N 2 O at room temperature [k (for Na + N 2 + O 2 products) 

### ≤ 10 –16 and k (for NaO 2 + N 2 products) 

### ≤ 2 × 10 –15 (Ager et al.)]. Wright et al. [1335] used UV photoelectron spectroscopy to determine the product NaO is formed predominantly in the excited 2 Σ + state.

J3. Na + Cl 2 . Two measurements of the rate coefficient fo r this reaction are in excellent agreement: Silver [1060] and Talcott et al. [1147]. The recommended value is the average of these room temperature results.

J4. NaO + O. The recommendation is based on a measurement at 573 K by Plane and Husain [952]. They reported that 

### ≤ 1% of the Na product is in the 3 2 P excited state.

J5. NaO + O 3 . This reaction was studied by Silver and Kolb [1063], Ager et al. [13], and Plane et al. [953], who agree on the rate coefficient and branching ratio. This agreement may be fortuit ous because Silver and Kolb used an indirect method and an analysis based on their rate coefficient for the Na + O 3 reaction, which is about 1/2 of the recommended value. Ager et al. employed a somewhat more direct measurement, but the study is complicated by a chai n reaction mechanism in the Na/O 3 system. Plane et al. reported rate coefficient measurements for the NaO 2 + O 2 product channel over the temperature range 207–377 K using pulsed photolysis LIF methods. The recommendation for that channel is based on all three studies, and the recommendation for the Na + 2O 2 channel is based upon the results of Silver and Kolb and Ager et al. The latter reaction channel may also have a significant temperature dependence.

J6. NaO + H 2 . The recommendation is based on a measurement by Ager and Howard [12]. They also reported a significant Na + H 2 O product channel and that a small fraction of the Na from this channel is in the 3 2 P excited state.

J7. NaO + H 2 O. The recommendation is based on a measurement by Ager and Howard [12].

J8. NaO + NO. The recommendation is based on an indirect measurement reported by Ager et al. [13].

J9. NaO + HCl. There is only one indirect measurement of the ra te coefficient for this reaction, that from the study by Silver et al. [1066]. They indicate that the products are NaCl and OH, although some NaOH and Cl production is not ruled out.

J10. NaO 2 + O. The recommendation is based on a flow tube study at 300 K by Helmer and Plane [497].

J11. NaO 2 + NO. This reaction is endothermic. The upper limit recommended is from an experimental study by Ager et al. [13].

J12. NaO 2 + HCl. The recommendation is based on a measurement reported by Silver and Kolb [1064]. They indicated that the products are NaCl + HO 2 , but NaOOH + Cl may be possible products.

J13. NaOH + HCl. The recommendation is based on the study by Silver et al. [1066], which is the only published study of this reaction.

### 1-93 1.4 References

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### 2-1 

## SECTION 2. TERMOLECULAR REACTIONS

Table of Contents

section 2. Termol ecular Reactions .............................................................................................. ..................................2-1 2.1 Introduction .................................................................................................................. ..........................2-1 2.2 Low–Pressure-Limiting Rate Constant, 

## ( ) x

o 

### k T .........................................................................................2-1 2.3 Temperature Dependence of Low–Pressure Limiting Rate Constants: T n ...................................................2-2 2.4 High-Pressure-Limit Rate Constants, k
∞ (T) ................................................................................................2-2 2.5 Temperature Dependence of High-Pressure-Limiting Rate Constants: T m ..................................................2-3 2.6 Uncertainty Estimat es.......................................................................................................... ........................2-3 2.7 Notes to Table 2............................................................................................................... ............................2-8 2.8 References .................................................................................................................... ......................2-16



### Tables Table 2–1. Rate Constants for Termolecular Reactions ........................................................................... .....................2-4



### 2.1 Introduction

Rate constants for association reactions (Table 2–1) of the type A + B ↔ [AB]* M 

### → AB can be pressure dependent. The low-pressure-limiting rate constants are given in the form:



## ( ) -n 300

o o T kT k 300  

=     cm 6 molecule –2 s –1

,

(where 300

o k has been adjusted for air as the third body), together with a recommended value of n. The limiting highpressure rate constant is given in a similar form:


## ( ) -m 300 

### T kT k 300

∞ ∞ 

###  

=     cm 3 molecule –1 s –1

.

To obtain the effective second-orde r rate constant for a given cond ition of temperature and pressure (altitude), the following formula is used:



## ( ) 

## [ ] ( ) 

## [ ]

( ) ( ) -1 2

o 10 T

o f

o k (T) M 1+ log k 

### kTM k ([M],T)= 0.6 kTM 1 k T                        

∞  

         

∞ 

###        

+    

The fixed value 0.6 that appears in this formula fits the data for all listed reactions adequately, although in principle this quantity may be different for each r eaction, and also temperature dependent. Thus, a compilation of rate constants of this type requires the stipulation of the four parameters, k o (300), n, k
∞ (300), and m. These can be found in Table 2–1. The discussion that follows outlines the general methods we have used in establishing this table, and the notes to the table discuss specific data sources. Recent advances in theory have allowed direct calculation of rate constants for some reactions using RRKM/Master Equation methods.


### 2.2 Low-Pressure-Limiting Rate Constant, 

## ( ) x

o 

### k T

Troe [259] has described a si mple method for obtaining low-pr essure-limiting rate constants. In essence this method depends on the definition: 

## ( ) x x
o x o,sc 

### kT k β ≡

### 2-2 Here sc signifies “strong” collisi ons, x denotes the bath gas, and β
x is an efficiency parameter (0 < β
x <1), which provides a measure of energy transfer.

The coefficient β
x is related to the average energy transferred in a collision with gas x, 〈∆ E 〉
x , via: 

# ( ) x x

E x 

### E

F kT 1- β β ∆

=

Notice that 〈∆ E 〉 is quite sensitive to β

. F E is the correction factor of the energy dependence of the density of states (a quantity of the order of 1.1 fo r most species of stratospheric interest).For some of the reactions of possible stratospheric interest reviewed here, there exist data in the lowpressure limit (or very close thereto), and we have c hosen to evaluate and unify this data by calculating 

### ( ) x

o k T for the appropriate bath gas x and computing the value of

x 

### β corresponding to the experimental value (Troe [259]). A compilation (Patrick and Golden [ 211]) gives details for many of the reactions considered here.

From the

x 

### β values (most of which are for N 2 , i.e.,

2 N 

### β ), we compute 〈∆ E 〉 X according to the above equation. Values of

2 N 

### E 〈∆ 〉 of approximately 0.3–1 kcal mole –1 are generally expected. If multiple data exist, we average the values of

2 N 

### E 〈∆ 〉 and recommend a rate constant corresponding to the

2 N 

### β computed in the equation

above. Where no data exist we have sometimes estimated the low-pressure rate constant by taking

2 N 

### β = 0.3 at T = 300 K, a value based on those cases where data exist.


### 2.3 Temperature Dependence of Low–P ressure Limiting Rate Constants: T n

The value of n recommended here comes from meas urements or, in some cases, a calculation of

2 N 

### E 〈 ∆ 〉 from the data at 300 K, and a computation of

2 N 

### β (200 K) assuming that

2 N 

### E 〈 ∆ 〉 is independent of temperature in this

range. This

2 N 

### β (200 K) value is combined with the computed value of k o sc (200 K) to give the expected value of the

actual rate constant at 200 K. This latter, in combination with the value at 300 K, yields the value of n. This procedure can be directly comp ared with measured values of k o (200 K) when those exist. Unfortunately, very few values at 200 K are available. There are often temperature-dependent studies, but some ambiguity exists when one attempts to extrapolate these down to 200 K. If data are to be extrapolated beyond the measured temperature range, a choice must be made as to the functional form of the temperature dependence. There are two general ways of expressing th e temperature dependence of rate constants. Either the Arrhenius expression

k o (T) = A exp(–E/RT)

or the form

k o (T) = A ′ T –n is employed. Since neither of these extrapolation techniques is s oundly based, and since they often yield values that differ substantially, we have used the method expl ained earlier as the basis of our recommendations.



### 2.4 High-Pressure-Limit Rate Constants, k ∞ 

### (T)

High-pressure rate constants can often be obtained expe rimentally, but those for the relatively small species of atmospheric importance usually reach the hi gh-pressure limit at inaccessibly high pressures. This leaves two sources of these numbers, the first being guesses based upon some model, and the second being extrapolation of falloff data up to higher pressures. Stratospheric conditions generally re nder reactions of interest much closer to the low-pressure limit and thus are fairly insensitive to the high-pressure value. This means that while the extrapolation is long, and the value of k
∞ (T) not very accurate, a “reasonable guess” of k
∞ (T) will then suffice. In some cases we have declined to guess since the low-pressure limit is effective over the entire range of stratospheric conditions.

### 2-3 2.5 Temperature Dependence of High- Pressure-Limiting Rate Constants: T m

There are very few data upon which to base a recommendation for values of m. Values in Table 2–1 are often estimated, based on models for the transition state of bond-association reactions and wh atever data are available.


### 2.6 Uncertainty Estimates

For three-body reactions (Table 2–1) uncertainties are assigned using a pro cedure that is analogous to that employed for bimolecular reactions. Values of f(298 K) are given for these rate constants at room temperature and assumed to be valid at all pressures. The additional uncertainty arising from the temperature extrapolation has in previous evaluations been expressed as an uncertainty in the temperature coefficients n and m. In this evaluation, those reactions that have been re-evaluated or added have uncertainties expressed with a g-factor as in Table 1–1. In future evaluations we will con tinue to update this format.

### 2-4 Table 2–1. Rate Constants for Termolecular Reactions

Low-Pressure Limit a k o (T) = k o 300 (T/300) –n High-Pressure Limit b k

∞ (T) = k

∞ 300 (T/300) –m Reaction
k o 300 n k

∞ 300 m f g Notes



### O x 

### Reactions

O + O 2 M 

### → O3 (6.0) (–34) 2.4 – – 1.1 50 A1



### O( 1 

### D) Reactions

O( 1 D) + N 2 M 

### → N 2 O (3.5±3.0) (–37) 0.6± 2.0 0.6 – – A2



### HO x 

### Reactions

H + O 2 M 

### → HO 2 (5.7±0.5) (–32) 1.6±0.5 (7.5±4.0) (–11) 0±1.0 B1

OH + OH M 

### → H 2 O 2 (6.9) (–31) 1.0 (2.6) (–11) 0 1.5 100 B2



### NO x 

### Reactions

O + NO M 

### → NO 2 (9.0±2.0) (–31) 1.5±0.3 (3.0±1.0) (–11) 0±1.0 C1

O + NO 2 M 

### → NO 3 (2.5) (–31) 1.8 (2.2) (–11) 0.7 1.3 100 C2

OH + NO M 

### → HONO (7.0±1.0) (–31) 2.6±0.3 (3.6±1.0) (–11) 0.1±0.5 C3

OH + NO 2 M 

### → HONO 2 (See Note) (2.0) (–30) 3.0 (2.5) (–11) 0 1.3 100 C4

HO 2 + NO 2 M 

### → HO 2 NO 2 (1.8±0.3) (–31) 3.2±0.4 (4.7±1.0) (–12) 1.4±1.4 C5

NO 2 + NO 3 M 

### → N 2 O 5 (2.0) (–30) 4.4 (1.4) (–12) 0.7 1.2 100 C6

NO 3 M 

### → NO + O 2 See Note C7



### Hydrocarbon Reactions

CH 3 + O 2 M 

### → CH 3 O 2 (4.5±1.5) (–31) 3.0±1.0 (1.8±0.2) (–12) 1.7±1.7 D1

C 2 H 5 + O 2 M 

### → C 2 H 5 O 2 (1.5±1.0) (–28) 3.0±1.0 (8.0±1.0) (–12) 0±1.0 D2

OH + C 2 H 2 M 

### → HOCHCH (5.5±2.0) (–30) 0.0±0.2 (8.3±1.0) (–13) –2± 2 1 D3

OH + C 2 H 4 M 

### → HOCH 2 CH 2 (1.0±0.6) (–28) 0.8±2.0 (8.8±0.9) (–12) 0± 0 2 D4

CH 3 O + NO M 

### → CH 3 ONO (1.4±0.5) (–29) 3.8±1.0 (3.6±1.6) (–11) 0.6±1.0 D5

CH 3 O + NO 2 M 

### → CH 3 ONO 2 (5.3) (–29) 4.4 (1.9) (–11) 1.8 1.1 0 D6

C 2 H 5 O + NO M 

### → C 2 H 5 ONO (2.8±1.0) (–27) 4.0±2.0 (5.0±1.0) (–11) 1.0±1.0 D7

### 2-5 Low-Pressure Limit a k o (T) = k o 300 (T/300) –n High-Pressure Limit b k

∞ (T) = k

∞ 300 (T/300) –m Reaction
k o 300 n k

∞ 300 m f g Notes

C 2 H 5 O + NO 2 M 

### → C 2 H 5 ONO 2 (2.0±1.0) (–27) 4.0±2.0 (2.8±0.4) (–11) 1.0±1.0 D8

CH 3 O 2 + NO 2 M 

### → CH 3 O 2 NO 2 (1.5±0.8) (–30) 4.0±2.0 (6.5±3.2) (–12) 2.0±2.0 D9

C 2 H 5 O 2 + NO 2 M 

### → C 2 H 5 O 2 NO 2 (1.2)(–29) 4.0 (9.0)(–12) 0.0 1.3 50 D10

CH 3 C(O)O 2 + NO 2 M 

### → CH 3 C(O)O 2 NO 2 (9.7±3.8) (–29) 5.6±2.8 (9.3±0.4)(–12) 1.5±0.3 D11

CH 3 CH 2 C(O)O 2 + NO 2

. M 

### → CH 3 CH 2 C(O)O 2 NO 2 (9.0) (–28) 8.9 (7.7) (–12) 0.2 2.0 100 D12

CH 3 C(O)CH 2 + O 2 M 

### → CH 3 C(O)CH 2 O 2 See Note D13



### FO x 

### Reactions

F + O 2 M 

### → FO 2 (4.4±0.4) (–33) 1.2±0.5 – – E1

F + NO M 

### → FNO (1.8±0.3) (–31) 1.0±10 (2.8±1.4) (–10) 0.0±1.0 E2

F + NO 2 M 

### → FNO 2 (6.3±3.0) (–32) 2.0±2.0 (2.6±1.3) (–10) 0.0±1.0 E3

FO + NO 2 M 

### → FONO 2 (2.6±2.0) (–31) 1.3±1.3 (2.0±1.0) (–11) 1.5±1.5 E4

CF 3 + O 2 M 

### → CF 3 O 2 (3.0±0.3) (–29) 4.0±2.0 (4.0±1.0) (–12) 1.0±1.0 E5

CF 3 O + NO 2 M 

### → CF 3 ONO 2 3.1(–28) 2.0 1.5(–11) 2.8 1.1 50 E6

CF 3 O 2 + NO 2 M 

### → CF 3 O 2 NO 2 (2.2±0.5) (–29) 5.0±1.0 (6.0±1.0) (–12) 2.5±1.0 E7

CF 3 O + CO M 

### → CF 3 OCO (2.5±0.2) (–31) – (6.8±0.4) (–14) –1.2 E8

CF 3 O M 

### → CF 2 O + F See Note E9



### ClO x 

### Reactions

Cl + O 2 M 

### → ClOO (2.7±1.0) (–33) 1.5±0.5 – – F1

Cl + NO M 

### → ClNO (9.0±2.0) (–32) 1.6±0.5 – – F2

Cl + NO 2 M 

### → ClONO (1.3±0.2) (–30) 2.0±1.0 (1.0±0.5) (–10) 1.0±1.0 F3

M 

### → ClNO 2 (1.8±0.3) (–31) 2.0±1.0 (1.0±0.5) (–10) 1.0±1.0

Cl + CO M 

### → ClCO (1.3±0.5) (–33) 3.8±0.5 – – F4

Cl + C 2 H 2 M 

### → ClC 2 H 2 ((5.9±1.0) (–30) 2.1±1.0 (2.1±0.4) (–10) 1.0±0.5 F5

Cl + C 2 H 4 M 

### → ClC 2 H 4 (1.6) (–29) 3.3 (3.1) (–10) 1.0 1.5 50 F6

Cl + C 2 Cl 4 M 

### → C 2 Cl 5 (1.4) (–28) 8.5 (4.0) (–11) 1.2 1.2 50 F7

### 2-6 Low-Pressure Limit a k o (T) = k o 300 (T/300) –n High-Pressure Limit b k

∞ (T) = k

∞ 300 (T/300) –m Reaction
k o 300 n k

∞ 300 m f g Notes

ClO + NO 2 M 

### → ClONO 2 (1.8±0.3) (–31) 3.4±0.2 (1.5±0.4) (–11) 1.9±0.5 F8

OClO + NO 3 M 

### → O 2 ClONO 2 See Note F9

ClO + ClO M 

### → Cl 2 O 2 (1.6) (–32) 4.5 (2.0) (–12) 2.4 1.1 25 F10

ClO + OClO M 

### → Cl 2 O 3 (6.2±1.0) (–32) 4.7±0.6 (2.4±1.2) (–11) 0±1.0 F11

OClO + O M 

### → ClO 3 (1.9±0.5) (–31) 1.1±1.0 (3.1±0.8) (–11) 0±1.0 F12

CH 2 Cl + O 2 M 

### → CH 2 ClO 2 (1.9±0.1) (–30) 3.2±0.2 (2.9±0.2) (–12) 1.2±0.6 F13

CHCl 2 + O 2 M 

### → CHCl 2 O 2 (1.3±0.1) (–30) 4.0±0.2 (2.8±0.2) (–12) 1.4±0.6 F14

CCl 3 + O 2 M 

### → CCl 3 O 2 (6.9±0.2) (–31) 6.4±0.3 (2.4±0.2) (–12) 2.1±0.6 F15

CFCl 2 + O 2 M 

### → CFCl 2 O 2 (5.0±0.8) (–30) 4.0±2.0 (6.0±1.0) (–12) 1.0±1.0 F16

CF 2 Cl + O 2 M 

### → CF 2 ClO 2 (3.0±1.5) (–30) 4.0±2.0 (3±2) (–12) 1.0±1.0 F17

CCl 3 O 2 + NO 2 M 

### → CCl 3 O 2 NO 2 (5.0±1.0) (–29) 5.0±1.0 (6.0±1.0) (–12) 2.5±1.0 F18

CFCl 2 O 2 + NO 2 M 

### → CFCl 2 O 2 NO 2 (3.5±0.5) (–29) 5.0±1.0 (6.0±1.0) (–12) 2.5±1.0 F19

CF 2 ClO 2 + NO 2 M 

### → CF 2 ClO 2 NO 2 (3.3±0.7) (–29) 6.7±1.3 (4.1±1.9) (–12) 2.8±0.7 F20



### BrO x 

### Reactions

Br + NO 2 M 

### → BrNO 2 (4.2±0.8) (–31) 2.4±0.5 (2.7±0.5) (–11) 0±1.0 G1

BrO + NO 2 M 

### → BrONO 2 (5.2±0.4) (–31) 3.2±0.8 (6.9±0.4) (–12) 2.9±0.1 G2



### IO x 

### Reactions

I + NO M 

### → INO (1.8±0.5) (–32) 1.0±0.5 (1.7±1.0) (–11) 0±1.0 H1

I + NO 2 M 

### → INO 2 (3.0±1.5) (–31) 1.0±1.0 (6.6±5.0) (–11) 0±1.0 H2

IO + NO 2 M 

### → IONO 2 (5.9±2.0) (–31) 3.5±1.0 (9.0±1.0) (–12) 1.5±1.0 H3



### SO x 

### Reactions

HS + NO M 

### → HSNO (2.4±0.4) (–31) 3.0±1.0 (2.7±0.5) (–11) 0± 0 2 I1

CH 3 S +NO M 

### → CH 3 SNO (3.2±0.4) (–29) 4.0±1.0 (3.9±0.6) (–11) 2.7±1.0 I2

O + SO 2 M 

### → SO 3 (1.3± 1.3 0.7 )(–33) –3.6±0.7 I3

OH + SO 2 M 

### → HOSO 2 (3.0±1.0) (–31) 3.3±1.5 (1.5±0.5) (–12) 0± 0 2 I4

### 2-7 Low-Pressure Limit a k o (T) = k o 300 (T/300) –n High-Pressure Limit b k

∞ (T) = k

∞ 300 (T/300) –m Reaction
k o 300 n k

∞ 300 m f g Notes

CH 3 SCH 2 + O 2 M 

### → CH 3 SCH 2 O 2 See Note I5

SO 3 + NH 3 M 

### → H 3 NSO 3 (3.9±0.8) (–30) 3.0±3.0 (4.7±1.3) (–11) 0±1.0 I6



### Metal Reactions

Na + O 2 M 

### → NaO 2 (3.2±0.3) (–30) 1.4±0.3 (6.0±2.0) (–10) 0±1.0 J1

NaO + O 2 M 

### → NaO 3 (3.5±0.7) (–30) 2.0±2.0 (5.7±3.0) (–10) 0±1.0 J2

NaO + CO 2 M 

### → NaCO 3 (8.7±2.6) (–28) 2.0±2.0 (6.5±3.0) (–10) 0±1.0 J3

NaOH + CO 2 M 

### → NaHCO 3 (1.3±0.3) (–28) 2.0±2.0 (6.8±4.0) (–10) 0±1.0 J4

Shaded areas indicate changes or additions since JPL 97–4 and/or JPL 00–03. The values quoted are suitable for air as the third body, M. a Units are cm 6 /molecule 2 -s. b Units are cm 3 /molecule-s. f(298 K) is the uncertainty factor at 298 K. To calculate the uncertainty at othe r temperatures, use the expression:


### 1 1 f(T) = f(298)exp g T 298  

−     Note that the exponent is absolute value

### 2-8 2.7 Notes to Table 2

A1. O + O2. Low pressure limit and T dependence are an averag e of Klais et al. [145], Huie et al. [127] and Lin and Leu [167]. These studies in N 2 and Ar are in the temperature range (200<T/K<268). The result is in agreement with the study of Hippler et al. [119] and the extrapolated recommendation fits their lower pressure N 2 data down to 100 K. High pressure studies by Croce de Cobos and Troe [72] are in agreement with this recommendation. Rawlins et al. [224] estimate values in Ar between 80 and 150 K from nascent vibrational distributions that are a factor of two higher than th e recommendation extrapolated to 80 K. The temperature dependence of the rate constant determined from the experimental data is in excellent agreement with the value of n=2.36 determined from the calculations of Patrick and Golden [211]. Kaye [139] has calculated isotope eff ects for this reaction, using methods similar to those discussed in the Introduction of this document (see Troe [259] and Patrick and Golden [211].) Isotope effects have been reported by Anderson et al. [8 ] and Gross and Billing [111]. Measurements of isotopic fractionation by Mauersberger and colleagues [288] and Thiemens and co–workers [236] reveal distinctly non–statistical effects. Various attempts at theoretical explanations exist [115], but the detailed knowledge of the potential energy surface required is unavailable. A2. O( 1 D) + N 2 . Low pressure limit from Kajimoto and Cvetanovic [138]. The T dependence is obtained by assuming a constant β

. The rate constant is extremely low in th is special system due to electronic curve crossing. Maric and Burrows [174] extract (8.8±3.3)×10 –37 cm 6 s –1 from a study of the photolysis of synthetic air, in agreement with the recommended value within mutual error limits.

B1. H + O 2 . Kurylo [151], Wong and Davis [290] and Hsu et al. [126] are averaged to obtain the low pressure limiting value at 300 K. The first two studies include T dependence, as does a study by Hsu et al. [125]. The recommended value is chosen with constant 〈∆ E 〉 N2 ~0.05 kcal mol –1

. This very low number reflects rotational effects. The high pressure limit is from Cobos et al. [59]. The temperature dependence is estimated. Cobos et al. [59] estimate m = –0.6, which is within our uncertainty. High temperature measurements in Ar by Pirraglia et al. [216] are in good agreement. Measurements in the range 298<T/K<750 by Carleton et al. [51] agree within error limits. High temperature theoretical and expe rimental studies examining wide ranges of pressure and temperature [260], [24] are in good agreement with the recommendation.

B2. OH + OH. Recommended values are from fits of measurements by Zellner et al. [297] in N 2 , by Forster et al. [99] and Fulle et al. [105] in 1–150 bar He scaled to N 2 . A study by Fagerstrom et al. [94] in 85–1000 mbar SF 6 gives slightly different values. A pressure independent bimolecular channel to H 2 O + O with a rate 4.2×10 –12 exp(–240/T) is observed (see Table 1–1). Zellner et al . used somewhat different values for this rate constant to make substantial corrections to their measured values. Changing to the accepted value will make large changes in the Zellner et al. values and it is unclear how to evaluate this. Trainor and von Rosenberg [258] report a value at 300 K that is lower than recommended by a factor of 2.7.

C1. O + NO. Low pressure limit and n from direct measurements of Schieferstein et al. [237] and their re–analysis of the data of Whytock et al. [284]. Error limits encompass other studies. High pressure limit and m from Baulch et al. [26] and Baulch et al. [25], slightly modified. Hippler et al. [120] report higher values for the high pressure limiting rate constant. Atkinson et al. [14] use F c =exp(–T/1850). This yields rate constants 10–20% higher than obtained from Table 2–1. Shock tube measurements by Yarwood et al. [293] in argon from 300– 1300 K are consistent with the values in Table 2–1.

C2. O + NO 2 . Values of rate constants and temperature dependen ces from a combination of the study by Burkholder and Ravishankara [44] and that of Hahn et al. [112]. At 300K these studies almost overlap at the highest pressure of Burkholder and Ravishankara and the lowest pressure studied by Hahn et al.. The former values are larger by a factor of 2.2 under these conditions. This recommendation is in r easonable agreement with the evaluation of Baulch et al. [26], which fits the Hahn et al. values very well.

C3. OH + NO. The low pressure limit rate constant has been repor ted by Anderson and Kaufman [6], Stuhl and Niki [254], Morley and Smith [185], Westenberg and de H aas [283], Anderson et al. [7], Howard and Evenson [124], Harris and Wayne [114], Atkinson et al. [16], Overend et al. [201], Anastasi and Smith [5], Burrows et al. [46] and Atkinson and Smith [11]. The general agreement is good, and the recommended values of both the rate constant and the temperature dependence are wei ghted averages. Studies by Sharkey et al. [242] and Donahue et al. [88] in the transition regime between low and high pressure limits are in agreement and serve to reduce the uncertainty. These latter studies yield a value for the high pressure limiting rate constant in

### 2-9 agreement with the results of Fo rster et al. [99], whose study r eached pressures of 100 bar in He. The temperature dependence of the high pressure limiting rate constant is from the data of Anastasi and Smith [5] and Sharkey et al. (Both cis- and trans-HONO are expected to be formed.) Fulle et al. [106] report a high pressure limit in agreement with Forster et al. [99]. Pagsberg et al. [202] report low pressure values in SF 6 that are compatible (i.e. the ratio of co llision efficiencies is about a fact or of two.) with the recommendation. A study by Zabarnick [294] is noted.

C4. OH + NO 2 . This reaction has been the subject of detailed study. Golden and Smith [108] concluded that there were two pathways, one to HONO 2 (nitric acid) and the other to HOONO (pernitrous acid). They offered parameters in the format of this recommendation that were given in the note in JPL 00-3.[232] Donahue et al. [87] support the finding of two pathways in an analysis of isotopic effects. The low pressure limit and the high pressure limiting rate constants and their temperature dependences in JPL 00-3 are from a fit to the data of Anastasi and Smith [4] Wine et al. [286], Donahue et al. [88], Dransfield et al. [90], Brown et al. [39] and D’Ottone et al.[89]. (Brown et al. report that O 2 is about 30% less efficient than N 2 as a collider and suggest that air might therefore have a total efficiency of 0.94 relative to N 2 ) Data from Anderson et al. [7] Howard and Evenson [89], Burrows et al. [46], and Erler et al. [93] are in essential agreement. Data of Forster et al [99] and Fulle et al. [106] appear to be about 30% too high [118]. Experiments up to about 100 bar at 300 K and the finding of a double exponential decay of OH at 430 K and 100 bar imp licate a second pathway [118]. Burkholder et al. [42] and Dransfield et al. [90] have searched for the isomer HOONO and have been unable to identify it. Nizkorodov and Wennberg [193] report 5% HOONO at 253K and 20 Torr of an N 2 /He buffer gas . The presence of the HOONO isomer at 300 and 430 K can be accounted for with model transition states and RRKM calculations. However, this description of the reaction between HO and NO 2 , requires that the data obtained at lower than 300 K represent the sum of the two pathways. Thus the fate of HOONO might have to be included in models. If this fate involves rapid loss due to reac tion or photolysis, the effect of the second pathway is the diminution of the HONO 2 forming rate constant. However, evaluation of data, taking into account both pathways, indicates that the contribution of the HOONO form ing reaction is quite small under atmospheric conditions. Thus, the r ecommendation is to use only the HONO 2 forming reaction. The following parameters relating to HOONO are provided for the purposes of model evaluation only and are not part of the Panel’s recommendation for reaction C4. Extrapolation of the model transition states used to fit the higher temperature results allows the formulation below. Fits to individual product species in Table 2–1 format:

HONO 2 : k o (300) = 2.0 × 10 –30 ; n = 3.0; k
∞ (300) =2.5 × 10 –11 ; m = 0

HOONO: k o (300) = 1.0 × 10 –31 ; n = 4.0; k
∞ (300) = 1.0 × 10 –10 ; m = 0 For the HOONO case, the reverse reaction must be taken into account through the equilibrium constant. In the format of Table 3-1:

A = 4.66 × 10 –27 ; B = 10028; K(298 K) = 1.92 × 10 –12 and f(298 K) = 10

C5. HO 2 + NO 2 . Kurylo and Ouellette [152] have remeasured the 300-K rate constants. Kurylo and Ouellette [153] have also remeasured the temperature dependence. The recommended values are taken from this latter reference wherein their data were combined with that of Sander and Peterson [233]. The recommended k o (300 K) is consistent with Howard [123]. Other studies by Simonaitis and Heicklen [245] and Cox and Patrick [70] are in reasonable agreement with the r ecommendation, as is the value of Christensen et al. [56].

C6. NO 2 + NO 3 . Data with N 2 as the bath gas from Kircher et al. [143], Smith et al. [248], Burrows et al. [45], Wallington et al. [272] and Orlando et al. [199] ranging from 236 to 358 K were used to obtain k o , k
∞ , n and m. Values from Croce de Cobos et al. [71] are excluded due to arguments given by Orlando et al. [199], who point out that a reanalysis of these data using better values for the rate constant for NO 3 + NO → 2NO 2 yields a negative value for NO 2 + NO 3 + M. The study of Fowles et al. [100] is noted, but not used. Johnston et al. [130] have reviewed this reaction. Hahn et al. [112] have st udied this reaction between 300 and 400 K at pressures from 30 to 900 bar. Their suggested parameterization yields values indistinguishable from those in this recommendation under most atmospheric conditions. (There are deviations of 30 to 50% at pressures less than a mbar and greater than 5 bar.) A study of the reverse reaction has been carried out by Cantrell et al. [47]. These data are in excellent agreement with those obtained by Connell and Johnston [62] and Viggiano et al. [267]. The equilibrium

### 2-10 constant recommended in Table 3-1 is the one given in Cantrell et al. [47], who computed it from the ratio of the rate constant of Orlando et al. [199] and their rate consta nts for the reverse reaction.

C7. O 2 + NO

. Johnston et al. [130] and Davidson et al. [78] ha ve suggested significant thermal decomposition of NO 3 . This has been disputed by Russell et al. [227]. Davis et al. [80] claim th at the barrier to thermal dissociation is 47.3 kcal mol –1

. This would seem to rule out such a process in the atmosphere.

D1. CH 3 + O 2 . Low pressure limit from Selzer and Bayes [240]. (These workers determined the rate constants as a function of pressure in N 2 , Ar, O 2 , and He. Only the N 2 points were used directly in the evaluation, but the others are consistent.) Plumb and Ryan [218] report a value in He which is consistent within error limits with the work of Selzer and Bayes. Pilling and Smith [215] have measured this process in Ar (32–490 Torr). Their low pressure limiting rate constant is consistent with this evaluation, but their high pressure value is a little low. Cobos et al. [58] have made measurements in Ar and N 2 from 0.25 to 150 atmospheres. They report parameters somewhat different than recommended here, but their data are reproduced well by the recommended values. The work of Laguna and Baughcum [154] seems to be in the fall–off region. Results of Pratt and Wood [220] in Ar are consistent with this recommendation, although the measurements are indirect. Their T dependence is within our estimate. As can be seen from Patrick and Golden [211], the above value leads to a very small β

, ~0.02, and thus temperature dependence is hard to calculate. The suggested value accommodates the values of Keiffer et al. [140], who measured the process in Ar between 20 and 600 Torr and in the range

334 

### ≤ T/K 

### ≤ 582. Ryan and Plumb [230] suggest that the same type of calculation as employed by Patrick and Golden yields a reasonable value of β

. We have not been able to reproduce their results. The high-pressure rate constant fits the data of Cobos et al. [58]. The temperature dependence is an estimate. (Data of van den Bergh and Callear [266], Hochanadel et al. [121], Basco et al. [23], Washida and Bayes [282], Laufer and Bass [156], and Washida [281] are also considered.) The fit to Keiffer et al. [140] is very good, suggesting that the temperature dependence for the high pressure limit is also reasonable. Kaiser [134] has determined values in reasonable agreement (±30%) w ith the recommended values.

D2. C 2 H 5 + O 2 . A relative rate study by Kaiser et al. [136] yields k
∞ = (9.2 ± 0.9) × 10 –12 cm 3 molecule –1 s –1 and k o = (6.5 ± 2.0) × 10 –29 cm 6 molecule –2 s –1 in He at 298 K and pressures between 3 and 1500 Torr. Their k
∞ agrees with the value calculated by Wagner et al. [269] (k
∞ = 7 × 10 –12 cm 3 molecule –1 s –1 ) using variational RRKM theory. The extrapolation to the low-pressure limit is difficult due to the complex potential energy surface, but agrees with a Patrick a nd Golden–type calcu lation [211] using 0

o 

### H ∆ = 32.4 kcal mol –1

. The recommended values use the calculated temperature depende nce and a 2.5 times higher rate constant for air as the bath gas.

D3. OH + C 2 H 2 . The rate constant for this complex process has been re-examined by Smith et al. [249] in the temperature range from 228 to 1400 K, and in the pressure range 1 to 760 Torr. Their analysis, which is cast in similar terms to those used here, is the source of the rate constants and temperature dependences at both limits. The negative value of m reflects the fact that their analysis includes a 1.2 kcal/mol barrier for the addition of OH to C 2 H 2 . The data analyzed include those of Pastrana and Carr [210], Perry et al. [213], Michael et al. [181], and Perry and Williamson [214]. Other data of Wilson and Westenberg [285], Breen and Glass [35], Smith and Zellner [252], and Davis et al. [79] were not included. Studies by Liu et al. [168] and Lai et al. [155] are in general agreement with the recommendation. Calculations of k o via the methods of Patrick and Golden [211] yield values compatible with those of Smith et al. [249].

D4. OH + C 2 H 4 . Experimental data of Tully [262], Davis et al. [79], Howard [122], Greiner [109], Morris et al. [186], and Overend and Paraskevopoulos [ 200] in helium, Atkinson et al. [17] in argon, and Lloyd et al. [169] and Cox [64] and Klein et al. [146] in nitrogen/oxyge n mixtures, have been considered in the evaluation. This well–studied reaction is considerably more complex than most others in this table. The parameters recommended here fit exactly the same curve proposed by Klein et al. [146] at 298 K. Discrepancies remain and the effect of multiple product channels is not well understood. Kuo and Lee [150] report very strong temperature dependence for the low-pressure limit (n=4). Calculations of the type in Patrick and Golden [211] yield the recommended value. The high-pressure limit temperature dependence has been determined by several workers. Almost all obtain negative activation energies, the Ze llner and Lorenz [298] value being equivalent to m = +0.8 over the range (296<T/K<524) at about 1 atmosphere. Although this could theoretically arise as a result of reversibility, the equilibrium constant is too high for this possibility. If there is a product channel that proceeds with a low barrier via a tight transition state, a complex rate cons tant may yield the observed behavior. The actual addition process (OH + C 2 H 4 ) may even have a small positive barrier. The recommended limits encompass the reported values. A new high temperature measurement has been reported by Diau and Lee [84].

### 2-11 D5. CH 3 O + NO. The recommended values are taken from the results of Frost and Smith [103] in argon. Temperature dependences are from their higher temperature results. The low pressure rate constant is consistent with the measurement of McCaulley et al. [179] and Daele et al. [73] in helium and half the value from Troe– type calculations. A bimolecular (chemical activation) path also exists, forming HNO + CH 2 O (Frost and Smith [103]). Studies by Ohmori et al. [195] and Dobé et al. [86] are in general agreement with Frost and Smith with respect to both the addition and bimolecular pathways. (See the note in Table 1-1 for the bimolecular pathway.)

D6. CH 3 O + NO 2 . The recommended values are from the work of Wollenhaupt and Crowley [289]. Agreement is good with earlier work at 298 K from the study of Frost and Smith [102] in argon (corrected by Frost and Smith [104] and that of Biggs et al [28] in He. Low pressure results agree within a factor of two with the measurements of McCaulley et al. [178] in helium. A minor bimolecular (chemical activation) pathway is also observed. (See Table 1-1.)

D7 C 2 H 5 O + NO. High-pressure data at 298 K in Ar from Frost and Smith [103] and low-pressure measurements in He by Daele et el. [74] are scaled to N 2 and fit with an expression summing the bimolecular and termolecular channels. The low pressure value agrees with theory. The bimolecular channel with an estimated rate of about 10 –12 needs to be verified by direct studies. The temperature dependence is estimated.

D8. C 2 H 5 O + NO 2 . High-pressure rate constant at 298 K from Frost and Smith [102]. Other values estimated from similar reactions.

D9. CH 3 O 2 + NO 2 . Parameters from a reasonable fit to the temperatur e- and pressure-depende nt data in Sander and Watson [235] and Ravishankara et al. [221]. These references report F c = 0.4, and their parameters are a somewhat better fit at all temperat ures than those recommended here. We do not adopt them since they are not much better in the stratospheric range, and they would require both a change in our F c = 0.6 format and the adoption of a quite large negative activation energy for 

### k

∞ . A study of the reverse reaction by Zabel et al. [295]
also uses F c = 0.4. The values recommended herein, taken with the value of the equilibrium constant in Table 3- 1, fit the data in Zabel et al. [295] very well. Destriau and Troe [83] have fit the above data with 

### k

∞ independent of temperature and F c = 0.36. Bridier et al. [37] are in good agreement with this recommendation at one atmosphere and 298 K.

D10. C 2 H 5 O 2 + NO 2 . The only experimental study is that of Elfers et al. [91] who measured the rate constant relative to the C 2 H 5 O 2 + NO reaction between 10 and 1000 mbar. Elfers et al. used a value of k = 8.9 × 10 –12 cm 3 molecule –1 s –1 for the reference reaction. By comparison th e recommended rate constant for the reference reaction from Table 1-1 of this evaluation is 1.1 × 10 –11 cm 3 molecule –1 s –1 at 254 K. There are three data points. An evaluation of the Elfers et al. work by Destriau and Troe [83] cast the da ta in the format used in the IUPAC evaluation [14]. The parameters in Table 2–1 are adjusted to agree with the data corrected for the change in the reference reaction, using the simpler formula employed in this recommendation.

D11. CH 3 C(O)O 2 + NO 2 . The recommended parameters are from the data of Bridier et al. [36], who report in the format represented here, but using F c = 0.3. Their values are: 300

o k = (2.7 ± 1.5) × 10 –28

, 

### k ∞

300 = (12.1 ± 2.0) × 10 –12 , with n = 7.1 ± 1.7 and m= 0.9 ± 0.15. Studies of the decomposition of
CH 3 C(O)O 2 NO 2 [PAN] by Roberts and Bertman [226], Grosjean et al. [110], and Orlando et al. [198] are in accord with Bridier et al. [36]. In the former study it was shown that PAN decomposition yields only peroxyacetyl radical and NO 2 ; no methyl nitrate.

D12. CH 3 CH 2 C(O)O 2 + NO 2 . This reaction, forming peroxypropionyl nitrate (PPN), has been studied in the reverse direction by Schurath and Wipprecht [238], Mineshos and Glavas [182], Grosjean et al. [110] and Kirchner et al. [144]. The measured values are very similar to those for CH 3 C(O)O 2 + NO 2 forming peroxyacetyl nitrate (PAN). Group additivity considerations indi cate that the equilibrium constant for both PAN and PPN will be the same (both sides of the equilibrium for PPN di ffer from those for PAN by the group C-(C)(CO)(H) 2 .) Therefore, the recommended value for the association reaction is taken from the decomposition studies multiplied by the same equilibrium constant as for PAN. Conservative error limits are estimated.

D13. CH 3 COCH 2 + O 2 . Cox et al. [69] reported a value of k = (1.5+/– 0.3) × 10 –12 cm 3 molecule –1 s –1 at 298 K and 1 atm of SF 6 in which a pulse radiolysis study was modeled. This should be close to the high-pressure limit, but Cox et al point out that it is a bit low. (Using group additivity to calculate the entropy change yields about 10 14.3 s –1 for the decomposition A-factor. This compares with almost 10 15 s –1 for C 2 H 5 O 2 decomposition.)

E1. F + O 2 . A study by Pagsberg et al. [206] reports k o in argon = 4.38 × 10 –33 (T/300) –1.2

. This is in good agreement with earlier values of Smith and Wrigley [251], Smith and Wrigley [250], Shamonina and Kotov [241],

### 2-12 Arutyunov et al. [9] and slightly lower than the values of Chen et al. [54] and Chegodaev et al. [53]. Wallington and Nielsen [278], Wallingt on et al. [277] and Ellerman et al. [92] confirm the valu e of Pagsberg et al. [206]. Lyman and Holland [172] report a slightly lower value in Ar at 298K. We assume that β Ar = β N 2 at all temperatures. Pagsberg et al. [206], also determined the equilibrium constant and thus ∆ H f (FO 2 ). See F + O 2 , Table 2–1. A calculation such as described in Patrick and Golden [211], using the new value yields: k o = 1.06 × 10 –33 (T/300) –1.5 using β N2 = 0.3 (i.e., 〈∆ E 〉 = 2 kJ mol –1 ). This is not good agreement.

E2. F + NO. A study by Pagsberg et al [203], taking into account data from Zetzsch [299], Skolnik et al . [246], Kim et al. [142], Pagsberg et al . [205] and Wallington et al. [ 275], reports rate constants fo r this reaction in several bath gases. Converting their values to the form used in this compilation yields the recommended parameters.

E3. F + NO 2 . A study by Pagsberg et al. [204], taking into account the experimental data of Fasano and Nogar [95] and Zetzsch [299], was used to determine bot h the high and low pressure limits at 300 K. Converting their values to the form used in this compilation yields the recommended parameters. Treatment of the data for this system requires knowledge of the relative stabilities of FNO 2 and FONO. Patrick and Golden [211] assumed that the difference between these woul d be the same as between the ClNO 2 isomers. Theoretical work by Dixon and Christie [85], Lee and Rice [159] and Amos et al. [3] indicates that FNO 2 is 35–40 kcal mol –1 more stable than FONO, and therefore the m easured rate refers to FNO 2 formation. The value of n = 2 is from Patrick and Golden, but consistent with Pagsberg et al. The value of m is a rough estimat e from similar reactions, but is also consistent with Pagsberg et al.

E4. FO + NO 2 . Low pressure limit from strong collision calculation and β = 0.33. T dependence from resultant 〈 ∆ E 〉 = 0.523 kcal mol –1

, high-pressure limit and T dependence estimated. A theoretical study by Rayez and Destriau [225] indicates that the product is the single isomer FONO 2 . Bedzhanyan et al. [27] report a value extracted from a complex mixture of bath gases.

E5. CF 3 + O 2 . Caralp et al. [49] have measured the rate constant in N 2 between 1 and 10 Torr. This supplants the value from Caralp and Lesclaux [48]. Kaiser et al. [137] have extended the pressure range to 580 Torr. They both recommend different parameters, but the data are well represented by the currently recommended values. Data of Ryan and Plumb [229] are in agreement.

E6. CF 3 O + NO 2 . Fockenberg et al. [98] report values in nitrogen with 250<T/K<302 and 7<p/mbar<107. They report large error limits. Their values, including two sigma errors, using the previous format are: k 0 =(3.1 ± 3.0)×10 –28 ; n = (2.0 ± 2.0) k
∞ =(1.5 ± 0.5)×10 –28 ; m = (2.8 ± 2.0). The reaction products agree with those reported by Chen et al. [55], who used photolysis of CF 3 NO to prepare CF 3 O 2 and subsequently CF 3 O in 700 Torr of air at 297 + 2 K. They considered two product channels: (a) CF 3 ONO 2 obtained via three–body recombination and (b) CF 2 O + FNO 2 obtained via fluorine transfer. Both products were observed and found to be thermally stable in their reactor. They report k a /(k a +k b ) > 90% and k b /(k a +k b ) < 10%, thus the formation of CF 3 ONO 2 is the dominant channel at 700 Torr and 297 K.

E7. CF 3 O 2 + NO 2. Based on experiments in O 2 of Caralp et al. [50], who s uggest a somewhat different fitting procedure, but the values recommended here fit the data just as well. Destriau and Troe [83] use yet a different fitting procedure that does not represent the data quite as well as that recommended here. Reverse rate data are given by Köppenkastrop and Zabel [148].

E8. CF 3 O + CO. Values taken from Turnipseed et al. [263]. The numbers were obtained for Ar as the bath gas and are assumed to hold for N 2 as well. The temperature dependence of the high-pressure rate constant was determined over the range 233<T/K<332 in SF 6 . No temperature dependence of the low-pressure-limiting rate constant was reported. Wallington and Ball [273] report values in good agreement with Turnipseed et al.

E9. CF 3 O + M. The activation energy for thermal decomposition of CF 3 O to CF 2 O + F has been reported to be 31 kcal mol –1 by Kennedy and Levy [141]. Thermochemical data yield ∆ H o (298) = 23 kcal mol –1

. This implies an intrinsic barrier of about 8 kcal mol –1 to elimination of F from CF 3 O. Electronic structure calculations by Li and Francisco [166] support this observation. Adopting the A-factor for unimolecular dissociation, A = 3 × 10 14 s –1 and E = 31 kcal mol –1 from Kennedy and Levy, k
∞ (298 K) is about 6 × 10 –9 s –1

. This corresponds to a lifetime of about 6 years; therefore, thermal decomposition of CF 3 O is unimportant throughout the atmosphere.

F1. Cl + O 2 . Nicovich et al. [189] measure k o = (9 ± 3) 10 –33 cm 6 molecule –2 s –1 at T = 187 ± 6 K in O 2 . Using the methods described in Patrick and Golden [211], but adjusting the thermochemistry of ClO 2 such that

o 298 K 

### S = 64.3 cal mol –1 K –1 and ∆ H f,298 = 23.3 ± 0.6 kcal mol –1 (Cl + O 2 , Table 3), we calculate

k o = 5.4 × 10 –33 cm 6 molecule –2 s –1 at T = 185 K. The collisional efficien cy of the bath gas is taken from the

### 2-13 formula [ β /(1– β 1/2 )] = 〈∆ E 〉 /F E kT and 〈∆ E 〉 ~ 0.5 kcal mol –1 (i.e., β 185 = 0.42 and β 300 = 0.30). Since O 2 may be particularly efficient for this process, we use this calculation with broader error limits. The value from the calculation at 300 K (i.e., 2.7 × 10 –33 cm 6 molecules –2 s –1 ) compares with an older value of Nicholas and Norrish [187] of 1.7 × 10 –33 in an N 2 + O 2 mixture. The temperature dependence is from the calculation. Baer et al. [18] report a value at 298 K in good agreement with the value recommended here, but the temperature dependence is strikingly different, as noted by the authors.

F2. Cl + NO. Low-pressure limit is from Lee et al. [158], Clark et al. [57], Ashmore and Spencer [10], and Ravishankara et al. [222]. Temperature dependence is from Lee et al. [158] and Clark et al. [57].

F3. Cl + NO 2 . Low-pressure limit and T dependence from Leu [164]. (Assuming similar T dependence in N 2 and He.) Leu [164] confirms the observation of Niki et al. [192] that both ClONO and ClNO 2 are formed, with the former dominating. This has been explained by Chang et al. [52], with detailed calculations in Patrick and Golden [211]. The temperature dependence is as predicted in Patrick and Golden [211]. Leu’s results are in excellent agreement with those reported in Ravishankara et al. [223]. The latter work extends to 200 Torr, and the high-pressure limit was chosen to fit these measurements. The temperature dependence of the high-pressure limit is estimated. A turbulent flow study by Seeley et al. [239] that extends results to 250 Torr of Ar is in agreement with earlier work.

F4. Cl + CO. From Nicovich et al. [190], who measured the process in N 2 for 185 ≤ T/K ≤ 260.

F5. Cl + C 2 H 2 . The recommended values are taken from the work of Kaiser [133] and Kaiser and Wallington [132], which extends the pressure range to 0.3–6000 Torr. The data are in reasonabl e agreement with earlier measurements of Brunning and Stief [40] and Walli ngton et al. [271] , although the derived temperature dependence is much less than obtained by Brunning and Stief [40]. These values are comp atible with earlier studies of Poulet et al . [219], Atkinson and Aschma nn [12], Lee and Rowland [ 157] and Wallington et al. [279]. Using FTIR, Zhu et al. [300] reported branching of 16% and 84% to the trans and cis adduct isomers, respectively, at 700 Torr N 2 and 295 K.

F6. Cl + C 2 H 4 . Values at 300K are from a relative ra te study by Walli ngton et al. [271]. A relative rate study by Kaiser and Wallington [132] extends the pressure range to 0.3–6000 Torr and is compatible with earlier studies. Temperature dependence of k o is taken from Kaiser and Wallington [135]. The temperature dependence of k
∞ is estimated. Values are in reasonable agreement with studies by Maricq et al. [175], Lee and Rowland [157], Iyer et al. [129], Atkinson a nd Aschmann [12], Atkinson and Aschmann [13] and Wallington et al. [280]. A study in He by Stutz et al. [255] is noted, as is a comment on it by Kaiser and Wallington [135]. Knyasev et al. [147] have done an extensive experimental and theoretical analysis. Their values agree with this recommendation.

F7 Cl + C 2 Cl 4 . Recommendation is from the flash-photolysis study of Nicovich et al. [191] done at 231–390 K in 3–700 Torr N 2 . A study by Thuner et al. is in agreement [257].

F8. ClO + NO 2 . The low-pressure-limit recommendation and uncertainties are based on temperature-dependent values from Zahniser et al. [296], Lee et al. [161], Birks et al . [31], Leu et al. [165] , Wallington and Cox [274], Cox et al. [65] and Molina et al. [183]. All of these data were collected in N 2 bath gas, except for several points from Lee et al. [161] collected in O 2 . The high-pressure-limit recommendation is based on the RRKM calculations of Smith and Golden . There are several pressure-dependent data sets in the literature, su ch as Percival et al. [212] , Handwerk and Zellner [113], Dasch et al. [77] and Cox and Lewis [68]; however, they are too disparate to extract unambiguous values. These data are all reproduced within two-sigma error limits by the current recommendation.

F9. OClO + NO 3. Friedl et al. [101], studied this system at 1 ≤ P/Torr ≤ 5 for helium and 220 ≤ T/K ≤ 298. They deduced values for the rate constant consistent with their data of k o ≈ 10 –31 and k
∞ ≈ 10 –11

. They also suggest a value for the equilibrium constant: K/cm 3 molecule –1 = 1 × 10 –28 exp (9300/T). However, Boyd et al. [34] have raised the question of possible heterogeneous effects in this system, and further work is needed.

F10. ClO + ClO. The recommendation is based on a simultaneous fit to data from Bloss et al. (183–245 K) [33], (which supersedes earlier work of Sander et al. (194–247 K) [231]), Nickolaisen et al. (260–390 K) [188] and Trolier et al. (200–263 K) [261]. The latter data have been corrected for the effect of Cl 2 as third body, as suggested by Nickolaisen et al. With this adjustment all the da ta are in reasonable agreement. Error limits are from the statistical fit. The k o value for N 2 is not in accord with a Patric k and Golden–type calculation [211]. This may be due to uncertainty in the ClOOCl thermochemistry, which is based on the equilibrium constants reported by Nickolaisen et al. and Cox and Hayman [67] (See Table 3.). Other previous rate constant measurements, such as those of Hayman et al. [116], Cox and Derwent [66], Basco and Hunt [22], Walker

### 2-14 [270], and Johnston et al. [131], range from 1–5 × 10 –32 cm 6 s –1 , with N 2 or O 2 as third bodies. The major dimerization product is chlorine peroxide (Birk et al. [30], DeMore and Tschuikow-Roux [82], Slanina and Uhlik [247], Stanton et al. [253] and Lee et al. [160]).

F11. ClO + OClO. Data are from Burkholder et al. [43], who measured the rate constant in N 2 at 200 ≤ T/K ≤ 260 and densities from (1.1–10.9) × 10 18 molecules cm –3

. They also measured the equilibrium constant. Parr et al. [208] also report a value for the rate constant in reasonable agreement w ith the recommendation.

F12. O + OClO. The recommendation is based on data of Colussi et al. [61] and Colussi [60], who measured the pressure dependence between 248 and 312 K. Their results are consistent with calculations. A zero-pressure rate constant of (1.6 ± 0.4) × 10 –13 cm 3 s –1 is reported for the chemical activation channel producing ClO + O 2 , and their value

of ∆ H o f (ClO 3 ) = 52 kcal mol –1 is derived at 298 K. A low-pressure study by Gleason et al. [107] suggests a

direct abstraction as well. See Table 1-1.

F13. CH 2 Cl + O 2 . Measured by Fenter et al. [96] over the range 298 ≤ T/K ≤ 448 and 1 ≤

 P/Torr ≤ 760 in nitrogen. Two different techniques were employed: laser photol ysis/photoionization mass spectrometry in the range 1–10 Torr and laser photolysis/UV absorption for the range 20–760 Torr. A study by Bilde et al. [29] in N 2 relative to the reaction CH 2 Cl + Cl 2 → CH 2 Cl 2 + Cl is in excellent agreement.

F14. CHCl 2 + O 2. Measured by Fenter et al. [96] over the range 298 ≤ T/K ≤ 383 and 1 ≤ P/Torr ≤ 760 in nitrogen. Two different techniques were employed: laser photol ysis/photoionization mass spectrometry in the range 1–10 Torr and laser photolysis/UV absorption for the range 20–760 Torr. A study by Nottingham et al. [194], in He, is in agreement.

F15. CCl 3 + O 2 . The recommendation incorporates studies by Fenter et al. [97], Danis et al. [76] and Luther et al. [171]. Experimental data of Ryan and Plumb [230] have been considered in the evaluation. A study by Nottingham et al. [194], in He, is in agreement. A Patrick and Golden–type calculation using the thermochemistry of Russell et al. [228] yields k 0 300 = 1.5 × 10 –30 , with β = 0.3. A value of k
∞ 300 = 5 × 10 –12 has been reported by Cooper et al. [63]. The value of the high-pressure-limiting rate constant recommended here is slightly below that of Luther et al., but within their error limits. If we use their value the fit to lower-pressure data in the atmospherically important regions is less good.

F16. CFCl 2 + O 2 . Values for both low- and high-pressure limits at 300 K are from Caralp and Lesclaux [48]. Temperature dependences are rough estimates based on calculations a nd similar reactions.

F17. CF 2 Cl + O 2 . Values estimated from other reactions in this series.

F18. CCl 3 O 2 + NO 2. Based on experiments in O 2 of Caralp et al. [50], who s uggest a somewhat different fitting procedure, but the values recommended here fit the data as well. Destriau and Troe [83] use yet a different fitting procedure that does not represent the data quite as well as that recommended herein. Reverse rate data are given by Köppenkastrop and Zabel [148].

F19. CFCl 2 O 2 + NO 2. Based on experiments in O 2 of Caralp et al. [50], who s uggest a somewhat different fitting procedure, but the values recommended here fit the data as well. Destriau and Troe [83] use yet a different fitting procedure that does not represent the data quite as well as that recommended herein. Reverse rate data are given by Köppenkastrop and Zabel [148].

F20. CF 2 ClO 2 + NO 2 . A study by Wu and Carr [291] supersedes the earlier work of Moore and Carr [184] and is recommended here. Reverse rate data are given by Köppenkast rop and Zabel [148] and Xiong and Carr [292].

G1. Br+NO 2 . The recommended values are from a study by Kreutter et al. [149]. Their k o value agrees with the measurement of Mellouki et al. [180] at 300 K. A Patrick-and-Golden-type calculation using the known structure of the more stable BrNO 2 isomer and the measured equilibrium by Kreutter et al. [149] underpredicts k o by an order of magnitude. Participation by other electronic states and isomers such as BrONO as suggested in JPL 97-4, in keeping with the chlorine analog, has been shown in studies by Broske and Zabel [38] and Orlando and Burkholder [196].

G2. BrO + NO 2 . Values from a study by Thorn et al. [256] that is in excellent agreement with Sander et al. [234] are recommended. Error limits are from a reanalysis of the data. Danis et al. [75] give slightly lower values for the low-pressure-limiting rate constant and a smaller temp erature dependence as well. This latter study may be hampered by heterogeneous effects. A theoretical study by Rayez and Destriau [225] suggests that the bonddissociation energy in BrONO 2 is higher than that in ClONO 2 , thus rationalizing the relative values of the low-

### 2-15 pressure-limiting rate constants for these two processes. This is confirmed by a more detailed study by Parthiban and Lee. [209] as well as by Orlando and Tyndall [197], who measured BrONO 2 decomposition and thus an equilibrium constant.

H1. I + NO. Evaluation taken from IUPAC [128]. The data is from van den Bergh et al. [264] and Basco and Hunt [21]. Although IUPAC recommends F c = 0.75, any differences will be insigni ficant, since this reaction is in the low pressure limit under atmospheric conditions.

H2. I + NO 2 . Evaluation taken from IUPAC [128]. The data is from van den Bergh et al. [264], Mellouki et al. [180], Buben et al. [41] and van den Bergh and Troe [265]. IUPAC uses F c = 0.63, which is the same as the universal value adopted here of F c = 0.6. (No evidence of possible isomers [INO 2 or IONO] is reported.)

H3. IO + NO 2 . Data taken from Daykin and Wine [81]. They suggest k o = 7.7 × 10 –31 (T/300) –5.0 , k
∞ = 1.5 × 10 –11 and F c = 0.4. The values recommended here fit the data as well.

I1. HS + NO. Data and analysis are from the work of Black et al. [32]. The temperature dependence of k has been estimated.

I2. CH 3 S + NO. The recommended values are from the study by Balla et al. [19] at 296K in nitrogen. Temperature dependences are derived from the higher temperature results of the same study.

I3 O + SO 2. The recommendation is taken from Atkinson et al. [15] and was transformed to the format used herein.

I4. OH + SO 2 . Values of the rate constant as a function of pressure at 298 K are from Leu [163], Paraskevopoulos et al. [207], and Wine et al. [287]. The value of the low-pressure limit is from Leu [163], corrected for fall–off. The high-pressure limit is from a fit to all the data. The value of n comes from the above data combined with calculations such as those of Patrick and Golden [211], except that the heat of formation of HOSO 2 is raised by 4 kcal mol –1 , as suggested by the work of Margitan [173]. The value of m is estimated. This is not a radical– radical reaction and is unlikely to have a positive value of m. The limit of m = –2 corresponds to a real activation energy of ~1 kcal mol –1

. Earlier data listed in Baulch et al. [26] and Baulch et al. [25] are noted. Work of Martin et al. [177], Barnes et al. [20], and Lee et al. [162] confirm the current evaluation.

I5. CH 3 SCH 2 + O 2

. Wallington et al. [276] have employed a pulse ra diolysis technique, allowing the derivation of k = 5.7 ± 0.4 × 10 –12 in 992 mbar of SF 6 at room temperature.

I6 SO 3 + NH 3 . Recommendation is from Lovejoy and Hanson [170], who studied this reaction from 10–400 Torr N 2 at 295 K. They observe that the adduct isomerizes rapidly to sulfamic acid and clusters efficiently with itself and sulfuric acid. Observed sulfamic acid dimeriza tion rate constant exceeds 5 × 10 –11

. Measurements of Shen et al. [243] made at 1–2 Torr He are much higher than those of Lovejoy and Hanson. Temperature dependences are rough estimates.

J1. Na + O 2. A study by Plane and Rajasekhar [217] finds k o = (2.9 ± 0.7) × 10 –30 at 300 K with n = 1.30 ± .04. They also estimate k
∞ to be about 6 × 10 –10, with a small positive temperature dependence. Another study by Helmer and Plane [117] yields k o = (3.1 ±0.2) × 10 –30 at 300 K with n = 1.52±0.27. The recommended values are taken from these studies. They are consistent with values measured by Marshall et al. [176] at 600 K and those measured by Vinckier et al. [268] at higher temperature. The k o value is about 60% higher than that of Silver et al. [244].

J2. NaO + O 2 . Ager and Howard [1] have measured the low- pre ssure limit at room temperature in several bath
gases. Their value in N 2 is used in the recommendation. They performed a Troe calcu lation, as per Patrick and Golden [211], to obtain collision effi ciency and temperature dependence. They obtained a high-pressure-limit rate constant by use of a simple model. The temperature dependence is estimated.

J3. NaO + CO 2 . Ager and Howard [1] have measured the rate cons tant for this process in the “fall–off” regime. Their lowest pressures are very close to the low-pressure limit. The temperature dependence is an estimate. Ager and Howard calculate the high-pressure rate constant from a simple model.

J4. NaOH + CO 2 . Ager and Howard [2] have measured th e low-pressure-limiting rate constant. The temperature dependence is an estimate. Ager and Howard have calculated the high-pressure limit using a simple model.

### 2-16 2.8 References

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## SECTION 3. EQUILIBRIUM CONSTANTS

Table of Contents SECTION 3. EQUILIBRIUM CONSTANTS ............................................................................................... ......... 3-1 3.1 Format ......................................................................................................................... .............................. 3-1 3.2 Definitions.................................................................................................................... ............................. 3-1 3.3 Notes to Table 3 ............................................................................................................... ......................... 3-3 3.4 References..................................................................................................................... ............................ 3-5



### Tables Table 3-1. Equilib rium Constants............................................................................................... ............................. 3-2



### 3.1 Format

Some of the three-body reactions in Table 2-1 form products that are thermally unstable at atmospheric temperatures. In such cases the ther mal decomposition reaction may compete w ith other loss processes, such as photodissociation or radical attack. Table 3-1 lists the equilibrium cons tants, K(T), for several reactions which may fall into this category. The table has three column entries, the first two being the parameters A and B which can be used to express K(T): K(T)/cm 3 molecule –1 = A exp(B/T) (200 < T < 300 K) The third column entry in Table 3-1 is the calculated value of K at 298 K. The data sources for K(T) are described in the individual notes to Table 3-1.



### 3.2 Definitions

When values of the heats of formation and entropies of all species are known at the temperature T, we note that:

o o 3 -1 T T 10 10 

### S H log K(T) / cm molecule = log (T) - 21.87 2.303R 2.303RT

∆ ∆   − +  

Where the superscript “o” refers to a standard stat e of one atmosphere. In some cases K values were calculated from this equation, using thermochemical data. In other cases the K values we re calculated directly from kinetic data for the forward and revers e reactions. When available, JANAF va lues were used for the equilibrium constants. The following equations were then used to calculate the parameters A and B: 

## ( ) ( ) o 200 200 10 10
300 300 

### 300 200 K K B/ K = 2.303 log = 1382 log 300 200 K K        

−     i



## ( ) 10 10 B log (A) = log K(T) 2.303 T −

The relationships between the parameters A and B and the quantities ∆ S o (298 K) and ∆ H o (298 K) are as follows:

o o 22

av 

### eR T S S A = exp 3.7x10 T exp NR R − 

### ′   ∆ ∆

=    

where R ′ = 82.1 cm 3 atm mole –1 K –1 , and N av = 6.02 × 10 23 molecule mole –1 and

o

o 

### H B/ K = - R ∆3-2 Table 3-1. Equilibrium Constants

Reaction A/cm 3 molecule –1 B/°K K eq (298 K) f(298 K) a g Note

HO 2 + NO 2 → HO 2 NO 2 2.1×10 –27 10900 1.6×10 –11 5 1000 1

NO + NO 2 → N 2 O 3 3.3×10 –27 4667 2.1×10 –20 2 100 2

NO 2 + NO 2 → N 2 O 4 5.9×10 –29 6643 2.8×10 –19 1.2 250 3

NO 2 + NO 3 → N 2 O 5 3.0×10 –27 10990 3.1×10 –11 1.2 500 4

CH 3 O 2 + NO 2 → CH 3 O 2 NO 2 1.3×10 –28 11200 2.7×10 –12 2 1000 5

CH 3 C(O)O 2 + NO 2 → CH 3 C(O)O 2 NO 2 9.0×10 –29 14000 2.3×10 –8 2 200 6

CH 3 CH 2 C(O)O 2 + NO 2 → CH 3 CH 2 C(O)O 2 NO 2 9.0×10 –29 14000 2.3×10 –8 10 800 7

CH 3 C(O)CH 2 + O 2 → CH 3 C(O)CH 2 O 2 7×10 –27 13000 6×10 –8 10 800 8

F + O 2 → FOO 3.2×10 –25 6100 2.5×10 –16 1 0 1200 9

Cl + O 2 → ClOO 5.7×10 –25 2500 2.5×10 –21 2 750 10

Cl + CO → ClCO 1.6×10 –25 4000 1.1×10 –19 5 500 11

ClO + O 2 → ClO

. O 2 2.9×10 –26 <3700 <7.2×10 –21 12

ClO + ClO → Cl 2 O 2 1.27×10 –27 8744 7.0×10 –15 1.3 500 13

ClO + OClO → Cl 2 O 3 1.1×10 –24 5455 9.8×10 –17 3 300 14

OClO + NO 3 → O 2 ClONO 2 1×10 –28 9300 3.6×10 –15 5 1000 15

OH + CS 2 → CS 2 OH 4.5×10 –25 5140 1.4×10 –17 1.4 500 16

CH 3 S + O 2 → CH 3 SO 2 1.8×10 –27 5545 2.2×10 –19 1.4 300 17

K/cm3 molecule–1 = A exp (B/T) [200 < T/K < 300] a f(298 K) is the uncertainty factor at 298 K, and g is a m easure of the uncertainty in the quantity B . To calculate the uncertainty at temperatures other than 298 K, use the expression: 

## () ( ) 1 1 f T f 298 K exp g T 298    

= −        

Shaded areas indicate changes or additions since JPL 97-4 and/or JPL 00-33-3 

### 3.3 Notes to Table 3

1. HO 2 + NO 2 . The value was obtained by combining the data from Table 1-1 for the rate constant of the reaction as written and that of Graham et al. [ 27] and Zabel [56] for the reverse reac tion. Values for the entropy and heat of formation of pernitric acid may be extracted. These values are: S(298 K) = 71.7 cal mole –1 K –1 and ∆ H f (298 K) = –12.9 kcal mole –1 . If the entropy is calculated from the frequencies and moments of inertia given by Chen and Hamilton [19], the value becomes 71.0 and the heat is –13.1. The values in the Appendix to this report reflect these results.

2. NO + NO 2 . The data are from JANAF [33] and Chao et al. [17]. This process is included because a measurement of the rate constant by Smith and Yarwood [50] and Markwalder et al. [36] shows that it is too slow to be an important process in most atmospheric and laboratory systems.

3. NO 2 + NO 2. The data are from JANAF [33] and Vosper [54], Chao et al. [18] and Amoruso et al. [1]. Rate data for this process are reported by Brunning et al. [11], Borrell et al. [8] Gozel et al. [25] and Markwalder et al. [35]. A direct study by Harwood and Jones [28] at low temperatures is in agreement with the recommendation. Re-evaluation of the data suggests lower error limits than recommended in JPL 97-4. A typographical error in JPL 97-4 has been corrected.

4. NO 2 + NO 3 . The recommendation is from Cantrell et al. [15]. They report rate constants for the decomposition reaction, which they combine with the rate constants of Orlando et al. [42] to obtain the e quilibrium constant. Agreement is quite good with the data of Burrows et al. [13] and Cantrell et al. [14], and the room temperature data of Tuazon et al. [51], Perner et al. [44] and Hjorth et al. [30]. An evaluation by Pritchard [47] is also in excellent agreement with the recommendation. Pritchard [47] examined the data of Cantrell et al. [14], Burrows et al. [13], Graham and Johnston [26], Wangberg et al [55], Schott and Davidson [48], and the room temperature data of Tuazon et al. [51] , Perner et al. [44] and Hjorth et al. [30]. He also included the values given by Smith et al. [49], and Kircher et al. [34], who combined data on the forward reaction, tabulated in Table 2-1, with decomposition data of by Connell and Johnston [20] and Viggiano et al. [53]. The latter was used as the basis for the value in JPL 00-3, but some uncertainties in the entropies of NO 3 and N 2 O 5 justify the reversion to the JPL 97-4 basis. Wa ngberg et al. [55] measured the e quilibrium constant between 280 and 294 K and report results in agreement with this recommendation.

5. CH 3 O 2 + NO 2 . Thermochemical values at 300 K for CH 3 O 2 NO 2 and CH 3 O 2 are from Baldwin [6]. In the absence of data, ∆ H° and ∆ S° were assumed to be independent of temperature. Bahta et al. [5] have measured k(dissociation) at 263 K. Using the values of k(recombination) suggested in this evaluation, they compute K(263 K) = (2.68 ± 0.26) × 10 –10 cm 3 . Our values predict 3.94 × 10 –10 cm 3 , in good agreement. Zabel et al. [57] have measured k(dissociation) as a function of pressure and temperature. (CH 3 O 2 + NO 2 , Table 2-1). Their values are in good agreement with Bahta et al. [5] and, taken together with k(recombination), would lead to A = 5.2 × 10 –28 and B = 10,766. This is sufficiently close to the value in Table 3-1 to forego any change in parameters, but the uncertainty has been reduced. Bridier et al. [10] m easure an equilibrium constant in good agreement with this recommendation.

6. CH 3 C(O)O 2 + NO 2 : From measurements of the rate constants in both directions by Bridier et al. [9].

7. CH 3 CH 2 C(O)O 2 + NO 2 . Assumed to be the same as for PAN (Note 6). Both sides of the of the reaction differ from PAN by the group C–(C)(CO)(H) 2 . Error limits are estimated and expanded from those for PAN.

8. CH 3 COCH 2 + O 2 . Estimated values of the entropy and enthalpy changes for the reaction are: ∆ S = –33 e.u. and ∆ H = –26 kcal/mole. The entropy is from group additiv ity and the enthalpy fro m group additivity for the hydroperoxide followed by assuming that the O–H bond dissociation energy is 88 kcal/mole. Error limits are estimated from the uncertainties in this procedure.

9. F + O 2 . Calculated from JANAF thermo chemical values except for ∆ H f,298 (FO 2 ) = 6.24 ± 0.5 kcal mol –1 . The latter was taken from Pagsberg et al. [43]. This direct measurement, which falls between the earlier disputed values, would seem to settle that controversy, but the calculated value of k o is not in good agreement with the experiment (see F + O 2 of Table 2-1).

10. Cl + O 2 . Baer et al. [4] determined K in the temperature range 180 to 300 K. Their value at 185.4 K (5.23 × 10 –19 cm 3 molecule –1 ) compares well with the Nicovi ch et al. [40] measurement K = 4.77 × 10 –19 cm 3 molecule –1 , and within error with the Mauldin et al. [37] value of 2.55 × 10 –19 cm 3 molecule –1 . A different expression for K by Avallone et al. [3] gives S° 298 (ClOO) = 61.8 cal K –1 moleculr –1 and ∆ H° f,298 (ClOO) = 23.3 kcal mol –1

. Using known thermochemistry3-4 for Cl and O 2 and computed entropy values for ClOO, ∆ H f,298 (ClOO) = 23.3 ±0.6 kcal mole –1 is obtained from the Nicovich et al. [40] data. The value of S° 298 (ClOO) = 64.3 cal mole –1 K –1 used is computed from a structure with a 105° bond angle and Cl–O and O–O bond lengths of 0.173 and 0.130 nm respectively. Frequencies of 1441, 407, and 373 cm –1 are from Arkell and Schwager [2]. Symmetry number is 1 and degeneracy is 2. 11. Cl + CO. From Nicovich et al. [41] who measured both k and K between 185 and 260 K in N 2 . They report ∆ H f,298 (ClCO) = –5.2 ± 0.7 kcal mole –1

. 12. ClO + O 2 . DeMore [22] reports K < 4 × 10 –18 cm 3 molecule –1 at 197 K. His temperature dependence of the equilibrium constant is estimated using S° 298 (ClO·O 2 ) = 73 cal mol –1 K –1 and ∆ H° 298 <7.7 kcal mol –1 . A higher value of K has been proposed by Prasad [45], but it requires S°(ClO·O 2 ) to be about 83 cal mol –1 K –1 , which seems unreasonably high. Carter and Andrews [16] found no experimental evidence for ClO·O 2 in matrix experiments. Prasad and Lee [46] discuss these issues and question the validity of the upper limit reported by DeMore. 13. ClO + ClO. The value is from a third-law calculation based on the data from Cox and Hayman [21] (except for the two lowest temperature points) and Nickolaisen et al. [39]. The entropy of ClOOCl, the value of which is 72.2 cal mol –1 K –1 at 300 K, is calculated from structural and spectroscopic data given by Birk et al. [7]. The heat of formation at 300 K is ∆ H° f,300 = 30.8 kcal mol –1 . A study of branching ratios of ClO + ClO channels in Cl 2 /O 2 /O 3 mixtures by Horowitz et al.[31] also finds the equilibrium constant in O 2 at 285 K to be in agreement with the recommendation. 14. ClO + OClO. The value in Table 3-1 is that of Burkholder et al. [12] who report a second law value combining their own data and those of Hayman and Cox [29] except for the lowest temperature point from the latter study. They deduce ∆ H f (Cl 2 O 3 ) ≈ 37 kcal mol –1 and S° (Cl 2 O 3 ) ≈ 95 cal mol –1 K –1 . The value from Hayman and Cox [29] is in agreement with entropy calculations based on molecular properties (3rd law). All calculations assume the chlorine chlorate structure (ClOCl(O) 2 ). The deviation that Burkholder et al. [12] observe from third law behavior may indicate that the reaction is more complex than written. Other structures might be stable at the lowest temperatures (i.e., ClOOClO, OClOClO, OClCl(O) 2 ).

15. OClO + NO 3 . Deduced by Friedl et al. [24].

16. OH + CS 2 . Average of the concordant recent measurements of Murrells et al. [38] and Diau and Lee [23] between 249 and 298 K. The measurements of Hynes et al. [32] indicate a less stable adduct, but agree within combined experimental error.

17. CH 3 S + O 2 . Turnipseed et al. [52] report the equilibrium constant for 216 ≤ T/K ≤ 258. From a third law analysis using ∆ S° 237 = –36.8 ± 2.6 eu, they obtain ∆ H o 237 = –11.5 ± 0.9 kcal/mole.3-5 

### 3.4 References

1. Amoruso, A., L. Crescentini, G. Fiocco and M. Volpe, 1993, J. Geophys. Res., 98 , 16857-16863. 2. Arkell, A. and I. Schwager, 1967, J. Amer. Chem. Soc., 89 , 5999-6006. 3. Avallone, L. M., D. W. Toohey and J. G. Anderson. 4. Baer, S., H. Hippler, R. Rahn, M. Siefke, N. Seitzinger and J. Troe, 1991, J. Chem. Phys., 95 , 6463-6470. 5. Bahta, A., R. Simonaitis and J. Heicklen, 1982, J. Phys. Chem. , 86 , 1849. 6. Baldwin, A. C. Thermochemistry of Peroxides. In Chemistry of Functional Groups ; Patai, S., Ed.; John Wiley and Sons Inc.: New York, 1982. 7. Birk, M., R. R. Friedl, E. A. Cohen, H. M. Pickett and S. P. Sander, 1989, J. Chem. Phys., 91 , 6588-6597. 8. Borrell, P., C. J. Cobos and K. Luther, 1988, J. Phys. Chem., 92 , 4377-4384. 9. Bridier, I., F. Caralp, H. Loirat, R. Lesclaux, B. Veyret, K. H. Becker, A. Reimer and F. Zabel, 1991, J. Phys. Chem., 95 , 3594-3600. 10. Bridier, I., R. Lesclaux and B. Veyret, 1992, Chem. Phys. Lett., 191 , 259-263. 11. Brunning, J., M. J. Frost and I. W. M. Smith, 1988, Int. J. Chem. Kinetics, 20 , 957. 12. Burkholder, J. B., R. L. Mauldin, R. J. Yokelson, S. Solomon and A. R. Ravishankara, 1993, J. Phys. Chem., 97 , 7597-7605. 13. Burrows, J. P., G. S. Tyndall and G. K. Moortgat, 1985, Chem. Phys. Lett., 119 , 193-198. 14. Cantrell, C. A., J. A. Davidson, A. H. McDaniel, R. E. Shetter and J. G. Calvert, 1988, J. Chem. Phys., 88

, 4997-5006. 15. Cantrell, C. A., R. E. Shetter, J. G. Calvert, G. S. Tyndall and J. J. Orlando, 1993, J. Phys. Chem., 97 , 9141- 9148. 16. Carter, R. O. and L. Andrews, 1981, J. Phys. Chem., 85 , 2351. 17. Chao, J., R. C. Wilhoit and B. J. Zwolinski, 1974, Thermochim. Acta, 10 , 359-360. 18. Chao, J., R. C. Wilhoit and B. J. Zwolinski, 1974, Thermochim. Acta, 10 , 361-371. 19. Chen, Z. and T. P. Hamilton, 1996, J. Phys. Chem., 100 , 15731-15734. 20. Connell, P. S. and H. S. Johnston, 1979, Geophys. Res. Lett., 6 , 553-556. 21. Cox, R. A. and G. D. Hayman, 1988, Nature, 332 , 796-800. 22. DeMore, W. B., 1990, Geophys. Res. Lett., 17 , 2353-2355. 23. Diau, E. W.-G. and Y.-P. Lee, 1991, J. Phys. Chem., 95 , 379. 24. Friedl, R. R., S. P. Sander and Y. L. Yung, 1992, J. Phys. Chem., 96 , 7490-7493. 25. Gozel, P., B. Calpani and H. van den Bergh, 1984, Isrl. J. Chem., 24 , 210. 26. Graham, R. A. and H. S. Johnston, 1978, J. Phys. Chem., 82 , 254-268. 27. Graham, R. A., A. M. Winer and J. N. Pitts, Jr., 1977, Chem. Phys. Lett., 51 , 215. 28. Harwood, M. H. and R. L. Jones, 1994, J. Geophys. Res., 99 , 22995-22964. 29. Hayman, G. D. and R. A. Cox, 1989, Chem. Phys. Lett., 155 , 1-7. 30. Hjorth, J., J. Nothholt and G. Re stelli, 1992, Int. J. Chem. Kinet., 24 , 51-65. 31. Horowitz, A., J. N. Crowley and G. K. Moortgat, 1994, J. Phys. Chem., 98 , 11924-11930. 32. Hynes, A. J., P. H. Wine and J. M. Nicovich, 1988, J. Phys. Chem., 92 , 3846-3852. 33. JANAF JANAF Thermochemical Tables , Third ed.; National Bureau of Standards, 1985. 34. Kircher, C. C., J. J. Margitan and S. P. Sander, 1984, J. Phys. Chem., 88 , 4370-4375. 35. Markwalder, B., P. Gozel and H. van den Bergh, 1992, J. Chem. Phys., 97 , 5472-5479. 36. Markwalder, B., P. Gozel and H. van den Bergh, 1993, J. Phys. Chem., 97 , 5260-5265. 37. Mauldin, R. L., III, J. B. Burkholder and A. R. Ravishankara, 1992, J. Phys. Chem., 96 , 2582-2588. 38. Murrells, T. P., E. R. Lovejoy and A. R. Ravishankara, 1990, J. Phys. Chem., 94 , 2381-2386. 39. Nickolaisen, S. L., R. R. Friedl and S. P. Sander, 1994, J. Phys. Chem., 98 , 155-169. 40. Nicovich, J. M., K. D. Kreutter, C. J. Shackelford and P. H. Wine, 1991, Chem. Phys. Lett., 179 , 367-373. 41. Nicovich, J. M., K. D. Kreutter and P. H. Wine, 1990, J. Chem. Phys., 92 , 3539-3544. 42. Orlando, J. J., G. S. Tyndall, C. A. Cantrell and J. G. Calvert, 1991, J. Chem. Soc. Far. Trans., 87 , 2345-2349. 43. Pagsberg, P. B., E. Ratajczak, A. Sillese n and J. T. Jodkowski, 1987, Chem. Phys. Lett., 141 , 88-94. 44. Perner, D., A. Schmeltekopf, R. H. Winkler, H. S. Johnst on, J. G. Calvert, C. A. Cantrell and W. R. Stockwell, 1985, J. Geophys. Res., 90 , 3807-3812. 45. Prasad, S. S., 1980, Nature, 285 , 152. 46. Prasad, S. S. and T. J. Lee, 1994, J. Geophys. Res., 99 , 8225-8230. 47. Pritchard, H. O., 1994, Int. J. Chem. Kinet., 26 , 61-72. 48. Schott, G. and N. Davidson, 1958, J. Amer. Chem. Soc., 80 , 1841-1853.3-6 49. Smith, C. A., A. R. Ravishankara and P. H. Wine, 1985, J. Phys. Chem., 89 , 1423-1427. 50. Smith, I. W. M. and G. Yarwood, 1986, Chem. Phys. Lett., 130 , 24-28. 51. Tuazon, E. C., E. Sanhueza, R. Atkinson, W. P. L. Carter, A. M. Winer and J. N. Pitts, Jr., 1984, J. Phys. Chem., 88 , 3095-3098. 52. Turnipseed, A. A., S. B. Baron and A. R. Ravishankara, 1992, J. Phys. Chem., 96 , 7502-7505. 53. Viggiano, A. A., J. A. Davidson, F. C. Fehsenfeld and E. E. Ferguson, 1981, J. Chem. Phys., 74 , 6113-6125. 54. Vosper, A. J., 1970, J. Chem. Soc. A, 1970 , 625. 55. Wangberg, I., T. Etzkorn, I. Barnes, U. Platt and K. H. Becker, 1997, J. Phys. Chem. A, 101 , 9694-9698. 56. Zabel, F., 1995, Zeitschrift fur Physikalische Chemie, 188 , 119-142. 57. Zabel, F., A. Reimer, K. H. Becker and E. H. Fink, 1989, J. Phys. Chem., 93 , 5500-5507.4-1 

## SECTION 4. PHOTOCHEMICAL DATA

Table of Contents
SECTION 4. PHOTOCHEMICAL DATA.................................................................................................. ............4-1

4.1 Format and E rror Estim ates..................................................................................................... ................ 4-3 4.2 Halocarbon Absorption Cross Secti ons and Quantum Yields................................................................. 4-3 4.3 References ..................................................................................................................... ...................... 4-102



### Tables Table 4-1. Photoc hemical Reactions ............................................................................................. .......................... 4-4 Table 4-2. Combined Uncertainties for Cross Sections and Quantum Yields........................................................ . 4-6 Table 4-3. Absorption Cross Sections of O 2 Between 205 and 240 nm.................................................................. 4-7 Table 4-4. Absorption Cross Sections of O 3 at 273 K............................................................................................. 4-8 Table 4-5. Parameters for the Calculation of O( 1 D) Quantum Yields..................................................................... 4-9 Table 4-6. Absorption Cross Sections of HO 2 ....................................................................................................... 4-10 Table 4-7. Absorption Cross Sections of H 2 O Vapor............................................................................................ 4-11 Table 4-8. Absorption Cross Sections of H 2 O 2 Vapor .......................................................................................... 4-11 Table 4-9. Mathematical Expression for Absorption Cross Sections of H 2 O 2 as a Function of Temperature ...... 4-12 Table 4-10. Absorption Cross Sections of NO 2 ..................................................................................................... 4-13 Table 4-11. Quantum Yields for NO 2 Photolysis.................................................................................................. 4-14 Table 4-12. Absorption Cross Sections of NO 3 at 298 K...................................................................................... 4-16 Table 4-13. Mathematical Expression for Absorption Cross Sections of N 2 O as a Function of Temperature * .... 4-16 Table 4-14. Absorption Cross Sections of N 2 O at 298 K...................................................................................... 4-17 Table 4-15. Absorption Cross Sections of N 2 O 5 ................................................................................................... 4-18 Table 4-16. Absorption Cross Sections of HONO .................................................................................. .............. 4-19 Table 4-17. Absorption Cross Sections and Temperature Coefficients of HNO 3 Vapor ...................................... 4-20 Table 4-18. Absorption Cross Sections of HO 2 NO 2 Vapor................................................................................... 4-20 Table 4-19. Absorption Cross Sections and Quantum Yields for Photolysis of CH 2 O......................................... 4-21 Table 4-20. Absorption Cross Sections of CH 3 O 2 , C 2 H 5 O 2 , and CH 3 C(O)O 2 ...................................................... 4-22 Table 4-21. Absorption Cross Sections of CH 3 OOH ............................................................................................ 4-23 Table 4-22. Absorption Cross Sections of PAN................................................................................... ................. 4-25 Table 4-23. Absorption Cross Sections of FNO................................................................................... ................. 4-26 Table 4-24. Absorption Cross Sections of CCl 2 O, CClFO, and CF 2 O at 298 K ................................................... 4-27 Table 4-25. Absorption Cross Sections of Cl 2 ....................................................................................................... 4-28 Table 4-26. Absorption Cr oss Sections of ClOO .................................................................................. ................ 4-29 Table 4-27. Absorption Cross Secti ons of OClO at the Band Peaks................................................................ ..... 4-30 Table 4-28. Absorption Cross Sections of Cl 2 O.................................................................................................... 4-32 Table 4-29. Absorption Cross S ections of ClOOCl at 200–250 K................................................................... ..... 4-33 Table 4-30. Absorption Cross Sections of Cl 2 O 3 .................................................................................................. 4-34 Table 4-31. Absorption Cross Sections of Cl 2 O 4 .................................................................................................. 4-34 Table 4-32. Absorption Cross Sections of Cl 2 O 6 .................................................................................................. 4-34 Table 4-33. Absorption Cro ss Sections of HCl Vapor............................................................................. ............. 4-35 Table 4-34. Absorption Cr oss Sections of HOCl .................................................................................. ................ 4-36 Table 4-35. Absorption Cr oss Sections of ClNO .................................................................................. ................ 4-37 Table 4-36. Absorption Cross Sections of ClNO 2 ................................................................................................. 4-37 Table 4-37. Absorption Cross Sections of ClONO at 231 K ........................................................................ ........ 4-38 Table 4-38. Absorption Cross Sections of ClONO 2 .............................................................................................. 4-39 Table 4-39. Absorption Cross Sections of CCl 4 at 295–298 K ............................................................................. 4-41 Table 4-40. Absorption Cross Sections of CH 3 OCl .............................................................................................. 4-42 Table 4-41. Absorption Cross Sections of CHCl 3 at 295–298 K .......................................................................... 4-43 Table 4-42. Absorption Cross Sections of CH 2 Cl 2 at 295–298 K ......................................................................... 4-44 Table 4-43. Absorption Cross Sections of CH 3 Cl at 295–298 K .......................................................................... 4-46 Table 4-44. Absorption Cross Sections of CH 3 CCl 3 at 295–298 K....................................................................... 4-47 Table 4-45. Absorption Cross Sections of CH 3 CH 2 Cl at 298 K ........................................................................... 4-47 Table 4-46. Absorption Cross Sections of CH 3 CHClCH 3 at 295 K...................................................................... 4-48 Table 4-47. Absorption Cross Sections of CFCl 3 at 295–298 K........................................................................... 4-49 Table 4-48. Absorption Cross Sections of CF 2 Cl 2 at 295–298 K.......................................................................... 4-504-2 Table 4-49. Absorption Cross Sections of CF 3 Cl at 295 K................................................................................... 4-51 Table 4-50. Absorption Cross Sections of CF 2 ClCFCl 2 at 295–298 K ................................................................. 4-52 Table 4-51. Absorption Cross Sections of CF 2 ClCF 2 Cl at 295 K ......................................................................... 4-53 Table 4-52. Absorption Cross Sections of CF 3 CF 2 Cl at 295–298 K..................................................................... 4-53 Table 4-53. Absorption Cross Sections of CHFCl 2 at 295–298 K ........................................................................ 4-54 Table 4-54. Absorption Cross Sections of CHF 2 Cl at 295–298 K ........................................................................ 4-55 Table 4–55. Absorption Cross Sections of CH 2 FCl at 298 K ............................................................................... 4-55 Table 4-56. Absorption Cross Sections of CF 3 CHCl 2 at 295 K ............................................................................ 4-56 Table 4-57. Absorption Cross Sections of CF 3 CHFCl at 295 K ........................................................................... 4-57 Table 4-58. Absorption Cross Sections of CF 3 CH 2 Cl at 298 K ............................................................................ 4-58 Table 4-59. Absorption Cross Sections of CH 3 CFCl 2 at 295–298 K .................................................................... 4-59 Table 4–60. Absorption Cross Sections of CH 3 CF 2 Cl at 295–298 K ................................................................... 4-60 Table 4-61. Absorption Cross Sections of CF 3 CF 2 CHCl 2 and CF 2 ClCF 2 CFCl at 298 K...................................... 4-61 Table 4-62. Absorption Cross Sections at the Peak of Various Bands in the A ← X Spectrum of BrO............... 4-62 Table 4-63. Absorption Cross Sections of BrO................................................................................... .................. 4-62 Table 4-64. Absorption Cr oss Sections of HOBr.................................................................................. ................ 4-65 Table 4-65. Absorption Cross Sections of BrONO 2 at 298 K............................................................................... 4-66 Table 4-66. Absorption Cross S ections of BrCl at 298 K ......................................................................... ............ 4-67 Table 4-67. Absorption Cross Sections of CH 3 Br at 295–296 K .......................................................................... 4-69 Table 4-68. Absorption Cross Sections of CH 2 Br 2 at 295–298 K......................................................................... 4-70 Table 4-69. Absorption Cross Sections of CHBr 3 at 295–296 K .......................................................................... 4-71 Table 4-70. Absorption Cross Sections of CH 2 BrCH 2 Br at 295 K ....................................................................... 4-72 Table 4-71. Absorption Cross Sections of C 2 H 5 Br at 295 K................................................................................. 4-72 Table 4-72. Absorption Cross Sections of CH 2 ClBr at 295 K .............................................................................. 4-73 Table 4-73. Absorption Cross Sections of CHClBr 2 at 296 K .............................................................................. 4-74 Table 4-74. Absorption Cross Sections of CHCl 2 Br at 298 K .............................................................................. 4-75 Table 4-75. Absorption Cross Sections of CCl 3 Br at 298 K ................................................................................. 4-75 Table 4-76. Absorption Cross Sections of CHF 2 Br at 298 K................................................................................ 4-76 Table 4-77. Absorption Cross Sections of CF 2 Br 2 at 295–296 K ......................................................................... 4-78 Table 4-78. Absorption Cross Sections of CF 2 ClBr at 295–298 K....................................................................... 4-80 Table 4-79. Absorption Cross Sections of CF 3 Br at 295–298 K........................................................................... 4-82 Table 4-80. Absorption Cross Sections of CF 3 CH 2 Br at 295 K............................................................................ 4-82 Table 4-81. Absorption Cross Sections of CF 3 CHClBr at 295–298 K ................................................................. 4-84 Table 4-82. Absorption Cross Sections of CF 3 CHFBr at 295 K........................................................................... 4-84 Table 4-83. Absorption Cross Sections of CF 2 BrCF 2 Br at 296 K......................................................................... 4-86 Table 4-84. Absorption Cross Sections of CF 3 CF 2 Br at 298 K............................................................................. 4-87 Table 4-85. Absorption Cross Sections of CH 3 I at 296–298 K and Temperat ure Coefficients ............................ 4-88 Table 4-86. Absorption Cross Sections of CH 2 I 2 at 298 K ................................................................................... 4-89 Table 4-87. Absorption Cross Sections of C 2 H 5 I at 298 K and Temperat ure Coefficients................................... 4-90 Table 4-88. Absorption Cross Sections of CH 3 CHI 2 at 298 K.............................................................................. 4-91 Table 4-89. Absorption Cross Sections of C 3 H 7 I at 298 K and Temperat ure Coefficients................................... 4-92 Table 4-90. Absorption Cross Sections of (CH 3 ) 3 CI at 298 K .............................................................................. 4-93 Table 4-91. Absorption Cross Sections of CF 3 I at 295–300 K ............................................................................. 4-95 Table 4-92. Absorption Cross Sections of CF 2 I 2 at 294 K .................................................................................... 4-96 Table 4-93. Absorption Cross Sections of C 2 F 5 I at 323 K .................................................................................... 4-96 Table 4-94. Absorption Cross Sections of 1-C 3 F 7 I at 295–298 K......................................................................... 4-97 Table 4-95. Absorption Cross Sections of CH 2 ICl at 298 K and Temperat ure Coefficients ................................ 4-98 Table 4-96. Absorption Cross Sections of CH 2 BrI at 298 K and Temperat ure Coefficients ................................ 4-99 Table 4-97. Absorption Cr oss Sections of OCS................................................................................... ............... 4-100 Table 4-98. Absorption Cross Sec tions of NaCl Vapor at 300 K ................................................................... .... 4-101



### Figures Figure 4-1. Absorption Spectrum of NO 3 .............................................................................................................. 4-15 Figure 4-2. Absorption Spectrum of ClO......................................................................................... ..................... 4-29 Figure 4-3. Absorption Spectrum of OClO ........................................................................................ ................... 4-31 Figure 4-4. Absorption Spectrum of BrO......................................................................................... ..................... 4-634-3 

### 4.1 Format and Error Estimates

In Table 4-1 we present a list of photochemical reacti ons considered to be of stratospheric interest. The absorption cross sections of O 2 and O 3 largely determine the extent of penetration of solar radiation into the stratosphere and troposphere. Some comments and references to these cro ss sections are presented in the text, but only a sample of the data is listed here. (See, for example, WMO Report No. 11 [1]; WMO Report No. 16 [434]) The photodissociation of NO in the O 2 Schumann-Runge band spectral range is another important process requiring special treatment and is not discussed in this evaluation (see, for example, Frederick and Hudson [123]; Allen and Frederick [8]; WMO Report No. 11 [1], and Minschwaner and Siskind [259]). For some other species having highly structured spectra, such as CS 2 and SO 2 , some comments are given in the text, but the photochemical data are not presented. The species CH 2 O, NO 2 , NO 3 , ClO, BrO, and OClO also have complicated spectra, but in view of their importan ce for atmospheric chemistry a sample of the data is presented in the evaluation; for more detailed information on their high-resolution spectra and temperature dependence, the reader is referred to the original literature. Table 4-2 gives recommended reliability factors fo r some of the more important photochemical reactions. These factors represent the combin ed uncertainty in cross sections and quantum yields, taking into consideration the atmospherically important wavelength re gions, and they refer to the total dissociation rate regardless of product identity. The exception is O( 1 D) production from photolysis of O 3 : the reliability factor applies to the quantum yield at the indicated wavelengths. The error estimates are not rigorous numbers resu lting from a detailed error propagation analysis of statistical manipulations of th e different sets of literature values; they merely represent a consensus among the panel members as to the reliability of the data for atmos pheric photodissociation calculati ons, taking into account the difficulty of the measurements, the agreement among the results reported by various groups, etc. The absorption cross sections are defined by the following expression of Beer’s Law:

I = I o exp(– σ nl),

where I o and I are the incident and transmitted light intensity, respectively; σ is the absorption cross section in

cm 2 molecule –1 ; n is the concentration in molecule cm –3 ; and l is the pathlength in cm. The cross sections are room temperature values at the specific wavelengths listed in the table, and the expected photodissociation quantum yields are unity, unless otherwise stated.


### 4.2 Halocarbon Absorption Cross Sections and Quantum Yields

The primary process in the photodissociation of chlorinated hydrocarbons is well established: absorption of ultraviolet radiation in the lowest frequency band is interpreted as an n– σ * transition involving excitation to a repulsive electronic state (antibonding in C–Cl), which dissociates by breaking the carbon-chlorine bond (Majer and Simons [228]). As expected, the chlorofluoromethanes, which are a particular type of chlorinated hydrocarbons, behave in this fashion (Sandorfy [361]). Hence, the quantum yield for photodissociation is expected to be unity for these compounds. There are several studies that show sp ecifically that this is the case for CF 2 Cl 2 , CFCl 3, and CCl 4 . These studies, which have been review ed in CODATA [82], also indicate that at shorter wavele ngths, two halogen atoms can be released simultane ously in the primary process.4-4 Table 4-1. Photochemical Reactions

_______________________________________________________________________ O x Photochemistry A1. O 2 + h ν → O + O A2. O 3 + h ν → O 2 + O O 3 + h ν → O 2 + O( 1 D)

HO x Photochemistry B1. HO 2 + h ν → products B2. H 2 O + h ν → H + OH B3. H 2 O 2 + h ν → OH + OH

NO x Photochemistry C1. NO 2 + h ν → NO + O C2. NO 3 + h ν → NO 2 + O NO 3 + h ν → NO + O 2 C3. N 2 O + h ν → N 2 + O( 1 D) C4. N 2 O 5 + h ν → products NH 3 + h ν → NH 2 + H (1) C5. HONO + h ν → OH + NO C6. HNO 3 + h ν → OH + NO 2 C7. HO 2 NO 2 + h ν → products

Organic Photochemistry CO + h ν → C + O (1) CO 2 + h ν → CO + O (1) CH 4 + h ν → products (2) D1. CH 2 O → H 2 + CO CH 2 O → H + HCO D2. CH 3 O 2 + h ν → products D3. C 2 H 5 O 2 + h ν → products D4. CH 3 OOH + h ν → products D5. HCN + h ν → products D6. CH 3 CN + h ν → products D7. CH 3 C(O)O 2 + h ν → products D8. CH 3 C(O)O 2 NO 2 + h ν → products

FO x Photochemistry E1. HF + h ν → H + F E2. FNO + h ν → F+ NO E3. CF 4 + h ν → products E4. C 2 F 6 + h ν → products E5. CF 2 O + h ν → products E6. CF 3 OH + h ν → products

ClO x Photochemistry F1. Cl 2 + h ν → Cl + Cl F2. ClO + h ν → Cl + O F3. ClOO + h ν → products F4. OClO + h ν → O + ClO F5. ClO 3 + h ν → products F6. Cl 2 O + h ν → products F7. Cl 2 O 2 + h ν → products F8. Cl 2 O 3 + h ν → products F9. Cl 2 O 4 + h ν → products F10. Cl 2 O 6 + h ν → products F11. HCl + h ν → H + Cl F12. HOCl + h ν → OH + Cl F13. ClNO + h ν → Cl + NO F14. ClNO 2 + h ν → products F15. ClONO + h ν → products F16. ClONO 2 + h ν → products F17. CCl 4 + h ν → products F18. CH 3 OCl + h ν → products F19. CHCl 3 + h ν → products F20. CH 2 Cl 2 + h ν → products F21. CH 3 Cl + h ν → products F22. CH 3 CCl 3 + h ν → products F23. CH 3 CH 2 Cl + h ν → products F24. CH 3 CHClCH 3 + h ν → products F25. CH 2 ClCH 2 Cl + h ν → products F26. CH 2 ClCH 2 CH 2 Cl + h ν → products F27. CH 2 Cl(CH 2 ) 2 CH 2 Cl + h ν → products F28. CCl 2 O + h ν → products F29. CClFO + h ν → products F30. CFCl 3 (CFC-11)+ h ν → products F31. CF 2 Cl 2 (CFC-12)+ h ν → products F32. CF 3 Cl (CFC-13)+ h ν → products F33. CF 2 ClCFCl 2 (CFC-113) + h ν → products F34. CF 2 ClCF 2 Cl (CFC-114) + h ν → products F35. CF 3 CF 2 Cl (CFC-115)+ h ν → products F36. CHFCl 2 (HCFC-21) + h ν → products F37. CHF 2 Cl (HCFC-22) + h ν → products F38. CH 2 FCl (HCFC-31) + h ν → products F39. CF 3 CHCl 2 (HCFC-123) + h ν → products F40. CF 3 CHFCl (HCFC-124) + h ν → products F41. CF 3 CH 2 Cl (HCFC-133) + h ν → products F42. CH 3 CFCl 2 (HCFC-141b) + h ν → products

F43. CH 3 CF 2 Cl (HCFC-142b) + h ν → products F44. CF 3 CF 2 CHCl 2 (HCFC-225ca) + h ν → products F45. CF 2 ClCF 2 CHFCl (HCFC-225cb) + h ν → products

BrO x Photochemistry G1. BrO + h ν → products G2. HOBr + h ν → products G3. BrONO 2 + h ν → products G4. BrCl + h ν → Br + Cl G5. CH 3 Br + h ν → products G6. CH 2 Br 2 + h ν → Products G7. CHBr 3 + h ν → Products G8. CH 2 BrCH 2 Br + h ν → Products G9. C 2 H 5 Br + h ν → Products G10. CH 2 ClBr (Halon-1011) + h ν → Products G11. CHClBr 2 (Halon-1012) + h ν → Products4-5 G12. CHCl 2 Br (Halon-1021) + h ν → Products G13. CCl 3 Br (Halon-1031) + h ν → Products G14. CHF 2 Br (Halon-1201) + h ν → Products G15. CF 2 Br 2 (Halon-1202) + h ν → Products G16. CF 2 ClBr (Halon-1211) + h ν → Products G17. CF 3 Br (Halon-1301) + h ν → Products G18. CF 3 CH 2 Br (Halon-2301) + h ν → Products G19. CF 3 CHClBr (Halon-2311) + h ν → Products G20. CF 3 CHFBr (Halon-2401) + h ν → Products G21. CF 2 BrCF 2 Br (Halon-2402) + h ν → Products G22. CF 3 CF 2 Br (Halon-2501) + h ν → Products

IO x Photochemistry H1. CH 3 I + h ν → CH 3 + I( 2 P 3/2 ) H2. CH 3 I + h ν → CH 3 + I*( 2 P 1/2 ) H3. CH 2 I 2 + h ν → CH 2 I + I( 2 P 3/2 ) H4. CH 2 I 2 + h ν → CH 2 I + I*( 2 P 1/2 ) H5. C 2 H 5 I + h ν → C 2 H 5 + I( 2 P 3/2 ) H6. C 2 H 5 I + h ν → C 2 H 5 + I*( 2 P 1/2 ) H7. CH 3 CHI 2 + h ν → Products H8. CH 3 CH 2 CH 2 I + h ν → Products H9. CH 3 CHICH 3 + h ν → Products H10. C 4 H 9 I + h ν → C 4 H 9 + I( 2 P 3/2 ) H11. C 4 H 9 I + h ν → C 4 H 9 + I*( 2 P 1/2 ) H12. (CH 3 ) 2 CHCH 2 I + h ν → (CH 3 ) 2 CCH 2 + I( 2 P 3/2 ) H13. (CH 3 ) 2 CHCH 2 I + h ν → (CH 3 ) 2 CCH 2 + I*( 2 P 1/2 ) H14. CH 3 ) 3 CI + → (CH 3 ) 3 C + I( 2 P 3/2 ) H15. (CH 3 ) 3 CI + → (CH 3 ) 3 C + I*( 2 P 1/2 ) H16. C 5 H 11 I + h ν → C 5 H 11 + I( 2 P 3/2 ) H17. C 5 H 11 I + h ν → C 5 H 11 + I*( 2 P 1/2 ) H18. CF 3 I + h ν → CF 3 + I( 2 P 3/2 ) H19. CF 3 I + h ν → CF 3 + I*( 2 P 1/2 ) H20. CF 2 I 2 +h ν → CF 2 I + I( 2 P 3/2 ) H21. CF 2 I 2 +h ν → CF 2 I + I*( 2 P 1/2 ) H22. CF 2 I 2 +h ν → CF 2 + I( 2 P 3/2 ) + I( 2 P 3/2 ) H23. CF 2 I 2 +h ν → CF 2 + I( 2 P 3/2 ) + I*( 2 P 1/2 ) H24. C 2 F 5 I + h ν → C 2 F 5 + I( 2 P 3/2 ) H25. C 2 F 5 I + h ν → C 2 F 5 + I*( 2 P 1/2 ) H26. C 3 F 7 I + h ν → C 3 F 7 + I( 2 P 3/2 ) H27. C 3 F 7 I + h ν → C 3 F 7 + I*( 2 P 1/2 ) H28. C 4 F 9 I + h ν → C 4 F 9 + I( 2 P 3/2 ) H29. C 4 F 9 I + h ν → C 4 F 9 + I*( 2 P 1/2 ) H30. C 6 F 13 I + h ν → C 6 F 13 + I( 2 P 3/2 ) H31. C 6 F 13 I + h ν → C 6 F 13 + I*( 2 P 1/2 ) H32. CH 2 ICl + h ν → CH 2 Cl + I H33. CH 2 BrI + h ν → CH 2 I + Br H34. CH 2 BrI + h ν → CH 2 Br + I H35. CF 2 BrCF 2 I + h ν → CF 2 BrCF 2 + I H36. CF 2 BrCF 2 I + h ν → CF 2 ICF 2 + Br

SO x Photochemistry I1. SO 2 + h ν → SO + O H 2 S + h ν → HS + H (1) I2. CS 2 + h ν → CS + S I3. OCS + h ν → CO + S I4. SF 6 + h ν → products

Metal Photochemistry J.1 NaOH + h ν → Na + OH J2. NaCl + h ν → Na + Cl

_______________________________________________________________________ (1) Hudson and Kieffer [170]. (2) Turco [405]. (3) Shaded areas indicate changes or additions since JPL 97-4/JPL 00-3.4-6 Table 4-2. Combined Uncertainties fo r Cross Sections and Quantum Yields

Species Uncertainty Notes
O 2 (Schumann-Runge bands) 1.2 O 2 (Continua) 1.2 O 3 (Cross Sections Only) 1.1
O 3 → O( 1 D), λ >310 nm 1.3

O 3 → O( 1 D), 290 < λ < 310 nm 1.2
H 2 O 2 1.3 NO 2 1.2 NO 3 1.5 N 2 O 1.2 N 2 O 5 2.0 HNO 3 1.3 HO 2 NO 2 2.0 CH 2 O 1.4 CH 3 OOH 1.5 CH 3 C(O)O 2 NO 2 1.3 λ < 300 nm CH 3 C(O)O 2 NO 2 2.0 λ ≥ 300 nm HCl 1.1 HOCl 1.4 ClOOCl 1.5 λ < 300 nm ClOOCl 3.0 λ ≥ 300 nm Cl 2 O 3 1.5 λ < 300 nm Cl 2 O 3 3.0 λ ≥ 300 nm ClONO 2 1.3 CCl 4 1.1 CCl 3 F 1.1 CCl 2 F 2 1.1 CH 3 Cl 1.1 CF 2 O 2.0 CF 3 Br 1.3 CF 2 ClBr 2.0 CF 2 Br 2 2.0 C 2 F 4 Br 2 2.0 HOBr 2.0 λ < 350 nm HOBr 10 λ ≥ 350 nm BrONO 2 1.44-7 A1. O 2 + h ν → O + O. The photodissociation of molecular oxygen in the stratosphere is due primarily to absorption of solar radiation in the 200–220 nm wavelength re gion, i.e., within the Herzberg continuum. The 185–200-nm region—the O 2 Schumann-Runge band spectral range—is also very important, since solar radiation penetrates efficiently into the stratosphere at those wavelengths.
Frederick and Mentall [124] Herman and Mentall [158] and Anderson and Hall [14,15] estimated O 2 absorption cross sections from balloon measurements of solar irradiance in the stratosphere. These authors find the cross sections in the 200–210 nm range to be ~35% smaller than the smallest of the older laboratory results, which are those of Shardanand and Prasad Rao [373]. The more recent laboratory st udies (Johnston et al. [190]; Cheung et al. [73,74], Jenouvrier et al. [183]) confirm the lower values obtained from solar irradiance
measurements. The recommended absorption cross section values between 205 and 240 nm are listed in Table 4-3; they are taken from Yoshino et al. [438] and are based on the latter set of laboratory measurements. Amoruso et al. [11] have also carried out cross secti on measurements in this wavelength range (the Herzberg continuum); their values are ~15% lower than those reported by Yoshino et al.

Table 4-3. Absorption Cross Sections of O 2 Between 205 and 240 nm

λ (nm) 10 24 σ (cm 2 ) λ (nm) 10 24 σ (cm 2 )

205 7.35 223 3.89 206 7.13 224 3.67 207 7.05 225 3.45 208 6.86 226 3.21 209 6.68 227 2.98 210 6.51 228 2.77 211 6.24 229 2.63 212 6.05 230 2.43 213 5.89 231 2.25 214 5.72 232 2.10 215 5.59 233 1.94 216 5.35 234 1.78 217 5.13 235 1.63 218 4.88 236 1.48 219 4.64 237 1.34 220 4.46 238 1.22 221 4.26 239 1.10 222 4.09 240 1.01

The studies of the penetration of solar radiation in the atmosphere in the Schumann-Runge wavelength region were based originally on laboratory measurements of cr oss sections that were a ffected by instrumental parameters due to insufficient spectral resolution. Yoshino et al. [446] reported high resolution O 2 cross section measurements at 300 K, between 179 and 202 nm, obtaining th e first set of results, which is independent of the instrument width. Additional studies at other temperatures, wave lengths, and isotopic compositions have been carried out by Yoshino et al. [439,442–445], Lewis et al. [214,215], Cheung et al. [72], and Chiu et al. [75]. More recently, Yoshino et al. [440] reported cross sections of the Schumann-Runge bands in the window region between the rotational lines for wavelengths between 180 and 195 nm; these measurements supersede their earlier ones. Minschwaner et al. [258] have fit temperature-dependent O 2 cross sections between 175 and 204 nm with polynomial expressions , providing accurate means of dete rmining the Schumann-Runge band cross sections with a model that incor porates the most recent laboratory data. Coquart et al. [86] have reported Herzberg continuum absorption cross sections in the wavelength region 196–205 nm of the Schumann-Runge bands.
For parameterizations of the O 2 absorption in the Schumann-Runge bands used in atmospheric modeling calculations, see, e.g., the review in WMO Report No. 16 [434]. More recent work by Murtagh [285], Nicolet and Kennes, [294] and Minschwaner et al. [258] incorporates results of the later laboratory measurements into efficient schemes for computing broad-band transmission and photolysis rates. Transmission values obtained by Murtagh [285] agree well with the WMO [434] recommendations, although the high-resolution calculations of Minschwaner and Salawitch differ with the WMO valu es by as much as 10–20% at some wavelengths.4-8 In view of the quality of the high-resolution laboratory measurements, the primary source of uncertainty in modeling O 2 photolysis in the Schumann-Runge bands (other than the issue of absolute solar irradiance) has shifted to the choice of broadband parameterization.

A2. O 3 + h ν → O + O 2 . The O 3 absorption cross sections and their temperature dependence have been measured by several groups. An earlier review is presented in WMO Report No . 16 [434]; this reference should be consulted to obtain data for atmospheric modeling calculations. Table 4-4 lists merely a sample of the data taken from this review, namely the 273 K cross section values averaged over the wavelength intervals commonly employed in modeling calculations, except for the wavelength range 185 to 225 nm, where the present recommendation incorporates the averaged values from the work of Molina and Molina [270]; the older values were based on the work of Inn and Tanaka [179]. More recently, Daumont et al. [101] a nd Brion et al. [ 43] reported ozone absorption cross section measurements between 195 and 345 nm, in the temperature range 200–300 K; and Yoshino et al. [441] measured the cross sections in the 185 to 254 nm wavelength range at 195, 228, and 295 K; the results of these studies yield values in very good agreement with those reported by Molina and Molina [270]. Cacciani et al. [63] reported measurements of the ozone cross sections in the wavelength range from 339 to 355 nm, in reasonable agreement with the present recommendation; the same group has measured also the cross sections in the 590–610 nm region, at 230 K and at 299 K (Amoruso et al. [9]). The temperature effect on the cross sections is negligible for wavelengths shorter than ~260 nm. Recent work by Mauersberger et al. [245,246] yields a value of 1137 × 10 –20 cm 2 for the cross section at 253.7 nm, the mercury line wavelength; it is about 1% smaller than the commonly accepted value of 1147 × 10 –20 cm 2 reported by Hearn [156]; about 2% smaller than the value obtained by DeMore a nd Raper [106] and Molina and Molina [270], 1157 × 10 –20 cm 2 ; and 0.5% larger than the value obtained by Daumont et al. [101]. The reason for the small discrepancy, which appears to be beyond experimental precision, is unclear.
Malicet et al. [229] report cross section measurements in the 195–345 nm range, at temperatures between 218 and 295 K, with a spectral bandwidth of 0.01–0.02 nm.; the results are in good agreement with the recommended values. Their data are presented in graphical form, and are also available in electronic format.

Table 4-4. Absorption Cross Sections of O 3 at 273 K

λ (nm) 10 20 σ (cm 2 )
average λ (nm) 10 20 σ (cm 2 )
average 175.439–176.991 81.1 238.095–240.964 797 176.991–178.571 79.9 240.964–243.902 900 178.571–180.180 78.6 243.902–246.914 1000 180.180–181.818 76.3 246.914–250.000 1080 181.818–183.486 72.9 250.000–253.165 1130 183.486–185.185 68.8 253.165–256.410 1150 185.185–186.916 62.2 256.410–259.740 1120 186.916–188.679 57.6 259.740–263.158 1060 188.679–190.476 52.6 263.158–266.667 965 190.476–192.308 47.6 266.667–270.270 834 192.308–194.175 42.8 270.270–273.973 692 194.175–196.078 38.3 273.973–277.778 542 196.078–198.020 34.7 277.778–281.690 402 198.020–200.000 32.3 281.690–285.714 277 200.000–202.020 31.4 285.714–289.855 179 202.020–204.082 32.6 289.855–294.118 109 204.082–206.186 36.4 294.118–298.507 62.4 206.186–208.333 43.4 298.507–303.030 34.3 208.333–210.526 54.2 303.030–307.692 18.5 210.526–212.766 69.9 307.692–312.5 9.80 212.766–215.054 92.1 312.5–317.5 5.01 215.054–217.391 119 317.5–322.5 2.49 217.391–219.780 155 322.5–327.5 1.20 219.780–222.222 199 327.5–332.5 0.617 222.222–224.719 256 332.5–337.5 0.274 224.719–227.273 323 337.5–342.5 0.1174-9 λ (nm) 10 20 σ (cm 2 )
average λ (nm) 10 20 σ (cm 2 )
average 227.273–229.885 400 342.5–347.5 0.0588 229.885–232.558 483 347.5–352.5 0.0266 232.558–235.294 579 352.5–357.5 0.0109 235.294–238.095 686 357.5–362.5 0.00549 The recommendation for the O( 1 D) quantum yield from ozone photolysis as a function of wavelength and temperature is given by the expression,



### Φ ( λ

, T ) = q 1 

### q

1 

### + q 2 

###         × A 1 

### × exp

− X 1 

### − λ

ω

1 

###         4 

###           + q 2 

### q

1 

### + q 2 

###         × A 2 

### × T
300       2



### × exp

− X 2 

### − λ

ω

2 

###         2 

###          

+ A 3 

### × T
300       1.5



### × exp

− X 3 

### − λ

ω

3 

###         2 

###           + c

where 

### q i 

### = exp

− ν i 

### RT         and X 1–3 , A 1–3 , ω 1–3 , ν 1–2 and c are best-fit parameters given in Table 4-5, λ is in nm, T is

in K, and R = 0.695 (cm –1 /K). The parameter c is assumed to be te mperature and wavelength independent. This expression is valid only for the wavelength range 306–328 nm and temperature range 200–320 K.

Table 4-5. Parameters for the Calculation of O( 1 D) Quantum Yields

Parameter i = 1 i = 2 i = 3

X i (nm) 304.225 314.957 310.737

ω i (nm) 5.576 6.601 2.187 A i 0.8036 8.9061 0.1192

ν i (cm –1 ) 0 825.518 – c 0.0765 – –

At room temperature (298 K) the uncertainties of the quantum yield values calculated with the above expression are estimated to be ± 10 % (1 σ ) for Φ(λ, 298 Κ) ≥ 0.4, while the uncertainties are estimated to be

± 0.04 for Φ(λ, 298 Κ) < 0.4. At temperatures other than room temper ature, the uncertaintie s are estimated to be ± 15 % for Φ(λ, Τ) ≥ 0.4 and ± 0.06 for Φ(λ, Τ) < 0.4.
In the wavelength range 329–340 nm we recommend the value of Φ (O 1 D) = 0.08 ± 0.04, independent of temperature. For λ > 340 nm, the quantum yield may be non-zero but no recommendation is made. For λ < 306 nm. the recommended quantum yield is 0.90, independent of temperature.
The recommendation for the temperature and wavelength dependences of the quantum yield for O( 1 D) production, Φ (O 1 D), is taken from the review of Matsumi et al. [244]. Matsumi et al. derived the recommended values using the following procedure: The measured O( 1 D) quantum yields at 298 K between 306 and 328 nm from eight studies (Talukdar et al. [398], Takahashi et al. [392], Ball et al. [19], Armerding et al. [16], Bauer et al. [28], Brock and Watson [44], Trolier and Wiesenfeld [403] and Smith et al. [383], were normalized using Φ (O 1 D) = 0.79 at 308 nm. This value was derived from the studies listed in Table 1 of Matsumi et al. [244]. The resulting renormalized data were averaged. The wavelength dependence quantum yield data at various temperatures reported by Talukdar et al. [396,398], Ta kahashi et al. [392], Hancock and Hofzumahaus [149] (this includes all the data from the Oxford group), Bauer et al. [28] and Smith et al. [383] were normalized to the value at 308 nm given above. These normalized data were used to obtain the best-fit parameters for eqn. 4-1 for the wavelength range 306–328 nm and temperature range 200–320 K. Because of the large number of studies upon which the 298 K evaluation is based, the averaged 298 K data were given a larger weight in the fitting procedure than the data at other temperatures.
The major differences between this recommendation and that of JPL 00-3 [358] are: (1) inclusion of more recent data from Smith et al., Hancock a nd Hofzumahaus, and Bauer et al., (2) selective deletion of data from4-10 the previous data from some of the groups, especially the use of data from Bauer et al. [28] which superseded the data of Silvente et al. [375] from the same group, (3 ) correcting for small differences in the absorption cross sections of ozone used by various gr oups, and (4) the normalization of all data to the selected value at 308 nm.

B1. HO 2 + h ν → OH + H. The absorption cross sections of the hydroperoxyl radical, HO 2 , in the 190–260 nm region have been measured at room temperature by Paukert and Johnston [311], Hochanadel et al. [161], Cox and Burrows [89], McAdam et al. [250], Kurylo et al. [206], Moortgat et al. [280], Dagaut and Kurylo [99], Lightfoot and Jemi-Alade [218], who measured the cross sections up to 777 K, Crowley et al. [97], Maricq and Szente [238], Roehl et al. [342] and Sander et al. [359] at 227.5 nm. The absorption cross sections have been evaluated in earlier reviews by Li ghtfoot et al. [217] a nd Wallington et al. [426] who noted significant discrepancies in both the shapes of the spectra and the absolute magnitudes of the cross section values, particularly around 200 nm. The published ultraviolet abso rption spectra have recently been reevaluated by Tyndall et al. [408]. Herein, the spectra were fitted to an analytical equa tion suggested by Ma ric et al. [237]:



## ( ) 2 ln 

### exp 1 med b
a b med



### b ν

ν 

### σ σ ν    

−

−    

−  

   



### =

−

where σ med = 1.84 × 10 –18 cm 2 molecule –1 , a = 4.91, b = 30612 cm –1 and ν med = 50260 cm –1 . Absolute cross sections were based on relative measurements of absorption cross sections of HO 2 , CH 3 O 2 and C 2 H 5 O 2 at 240 nm taken under identical conditions, combined with i ndependent calibrations by Cr owley et al. [97]. Table 4-6 lists the recommended cross sections, which are taken from the review by Tyndall et al. [408].
Lee [212] has detected O( 1 D) as a primary photodissociation product at 193 and at 248 nm, with a quantum yield that is about 15 times larger at the longer wavelength. The absolute quantum yield for O( 1 D) production has not been reported yet.
Photolysis of HO 2 in the stratosphere and troposphere is slow and can be neglected, but the UV absorption cross sections are important in laboratory studies of reaction kinetics.
Table 4-6. Absorption Cross Sections of HO 2

λ (nm) 10 20 σ (cm 2 ) 190 368 195 402 200 423 205 427 210 415 215 385 220 341 225 288 230 230 235 173 240 122 245 79.7 250 48.0 255 26.3 260 12.9

B2. H 2 O + h ν → H + OH. Water vapor has a continuum absorption spectrum at wavelengths longer than 145 nm, with a maximum around 165 nm, the cross sections fa lling off rapidly toward longer wavelengths; the photodissociation threshold occurs at 246 nm. Below 69 nm the spectrum is also a continuum, and between 69 and 145 nm it consists of diffuse bands. In the atmosphere water vapor is photodissociated mainly by the solar Lyman alpha line (121.6 nm).
The absorption cross sections and the photochemistry of water vapor have been reviewed, for example, by Hudson [168,169], by Hudson and Ki efer [170], by Calvert and P itts [65], and by Okabe [300].
The recommended absorption cross sections are taken from the review by Hudson and Kiefer [170] and are listed in Table 4-7 between 175 and 190 nm. At these wavelengths the quantum yield for production of H and4-11 OH is unity. At shorter wavelengths H 2 and O are also formed as primary products. Stief et al. [388] report a quantum yield of 0.11 for this process between 105 and 145 nm.

Table 4-7. Absorption Cross Sections of H 2 O Vapor

λ( nm) 10 20 σ (cm 2 ) 175.5 262.8 177.5 185.4 180.0 78.1 182.5 23.0 185.0 5.5 186.0 3.1 187.5 1.6 189.3 0.7

B3. H 2 O 2 + h ν → OH + OH. The recommended 298 K absorption cross section values, listed in Table 4-8, are the mean of the data of Lin et al. [221], Molina and Molina [267], Nicovich and Wine [295], and Vaghjiani and Ravishankara [414]. Molina and Molina [267] supersedes the earlier results of Molina et al. [273]. Nicovich and Wine measured the cross sections at λ ± 230 relative to the values at 202.6, σ = 4.32 × 10 –19 cm 2 , and at 228.8 nm, σ = 1.86 × 10 –19 cm 2

. The values are within 2% of the recommended value.

Table 4-8. Absorption Cross Sections of H 2 O 2 Vapor

10 20 σ (cm 2 ) 10 20 σ (cm 2 ) λ ( nm) 298 K 355 K λ ( nm) 298 K 355 K

190 67.2 270 3.3 3.5 195 56.4 275 2.6 2.8 200 47.5 280 2.0 2.2 205 40.8 285 1.5 1.6 210 35.7 290 1.2 1.3 215 30.7 295 0.90 1.0 220 25.8 300 0.68 0.79 225 21.7 305 0.51 0.58 230 18.2 18.4 310 0.39 0.46 235 15.0 15.2 315 0.29 0.36 240 12.4 12.6 320 0.22 0.27 245 10.2 10.8 325 0.16 0.21 250 8.3 8.5 330 0.13 0.17 255 6.7 6.9 335 0.10 0.13 260 5.3 5.5 340 0.07 0.10 265 4.2 4.4 345 0.05 0.06 350 0.04 0.05

Nicovich and Wine have measured the temperature dependence of these cross sections. They expressed the measured cross sections as the sum of two components: σ 1 , due to absorption from H 2 O 2, which has the O–O stretch excited; and σ 0 , due to absorption by ground state molecules. For atmospheric calculations the expression given in Table 4-9 may be used. The photodissociation quantum yield is believed to be unity. At and above 248 nm, the major photodissociation process is that leading to OH, i.e., the quantum yield for OH production is 2 (Vaghjiani and Ravishanka ra [415] and Vaghjiani et al. [416]). At 193 nm this quantum yield decreases to about 1.5 (Vaghjiani et al. [416]; Schiffman et al. [364]), and the quantum yield for O-atom production increases to about 0.16 (Vaghjiani et al. [416]).4-12 Table 4-9. Mathematical Expression fo r Absorption Cross Sections of H 2 O 2 as a Function of Temperature

_________________________________________________________________ 10 21 σ ( λ ,T) = χ

n = 

### ∑

0 7 A n λ n + (1 – χ )

n = 

### ∑

0 4 B n λ n

Where T: temperature K; λ : nm; χ = (1 + exp (–1265/T)) –1

A 0 = 6.4761 × 10 4 B 0 = 6.8123 × 10 3
A 1 = –9.2170972 × 10 2 B 1 = –5.1351 × 10 1
A 2 = 4.535649 B 2 = 1.1522 × 10 –1
A 3 = –4.4589016 × 10 –3 B 3 = –3.0493 × 10 –5
A 4 = –4.035101 × 10 –5 B 4 = –1.0924 × 10 –7
A 5 = 1.6878206 × 10 –7
A 6 = –2.652014 × 10 –10
A 7 = 1.5534675 × 10 –13

_________________________________________________________________ Range 260–350 nm; 200–400 K

C1. NO 2 + h ν → NO + O. Earlier recommendations for the absorp tion cross sections of nitrogen dioxide were taken from the work of Bass et al. [26]. More recent measurements have b een reported by Schneider et al. [367], at 298 K, for the wavelength range from 200 to 700 nm, and by Davidson et al. [103], from 270 to 420 nm, in the 232–397 K temperature range. At room temperature the agreemen t between these three sets of measurements is good (within 5% between 305 and 345 nm and w ithin 10% at the longer wavelengths). The agreement is poor below room temperature, as well as at the shorter wavelengths. A possible cause for the discrepancies is the presence of N 2 O 4 . The corrections needed to account fo r the presence of this species are largest around 200 nm, where it absorbs strongly. The corrections are also large at the lowest temperatures, because a significant fraction of the NO 2 forms N 2 O 4 . On the other hand, there is no error apparent in the corrections carried out by Bass et al., so that the reason for the discrepancy is not clear. Measurements of the absorption cross sections in the visible (440 to 460 nm), between 273 and 404 K, have been reported by Amoruso et al. [10], and Corcoran et al. [87] carried out high-resolution measurem ents at a few selected wavelength ranges between 470 and 616 nm, at 295, 573, and 673 K. Additional high-resolution studies of the cross sections, mainly aimed at improving the accuracy of atmospheric measurements, have been reported by Harwood and Jones [152], Coquart et al. [85], Mérienne et al. [257], Frost et al. [125], and Harder et al. [150].
Table 4-10 lists the recommended absorption cross secti ons, averaged over the wavelength intervals used for atmospheric photodissociation calculations. For the wavelength range from 200 to 274 nm the values are taken from Schneider et al. [367]; in this range the temperature effect is negligible. For the 274-to-420-nm region the temperature-dependent values are taken from Davidson et al. [103].4-13 Table 4-10. Absorption Cross Sections of NO 2

λ (nm) 10 20 σ , average at 25°C (cm 2 molecule –1 ) λ ( nm) 10 20 σ , average at 0°C (cm 2 molecule –1 ) 10 22 a* (cm 2 molecule –1 degree –1 )
202.02–204.08 41.45 273.97–277.78 5.03 0.075 204.08–206.19 44.78 277.78–281.69 5.88 0.082 206.19–208.33 44.54 281.69–285.71 7.00 –0.053 208.33–210.53 46.41 285.71–289.85 8.15 –0.043 210.53–212.77 48.66 289.85–294.12 9.72 –0.031 212.77–215.06 48.18 294.12–298.51 11.54 –0.162 215.06–217.39 50.22 298.51–303.03 13.44 –0.284 217.39–219.78 44.41 303.03–307.69 15.89 –0.357 219.78–222.22 47.13 307.69–312.50 18.67 –0.536 222.22–224.72 37.72 312.5–317.5 21.53 –0.686 224.72–227.27 39.29 317.5–322.5 24.77 –0.786 227.27–229.89 27.40 322.5–327.5 28.07 –1.105 229.89–232.56 27.78 327.5–332.5 31.33 –1.355 232.56–235.29 16.89 332.5–337.5 34.25 –1.277 235.29–238.09 16.18 337.5–342.5 37.98 –1.612 238.09–240.96 8.812 342.5–347.5 40.65 –1.890 240.96–243.90 7.472 347.5–352.5 43.13 –1.219 243.90–246.91 3.909 352.5–357.5 47.17 –1.921 246.91–250.00 2.753 357.5–362.5 48.33 –1.095 250.00–253.17 2.007 362.5–367.5 51.66 –1.322 253.17–256.41 1.973 367.5–372.5 53.15 –1.102 256.41–259.74 2.111 372.5–377.5 55.08 –0.806 259.74–263.16 2.357 377.5–382.5 56.44 –0.867 263.16–266.67 2.698 382.5–387.5 57.57 –0.945 266.67–270.27 3.247 387.5–392.5 59.27 –0.923 270.27–273.97 3.785 392.5–397.5 58.45 –0.738 397.5–402.5 60.21 –0.599 402.5–407.5 57.81 –0.545 407.5–412.5 59.99 –1.129 412.5–417.5 56.51 0.001 417.5–422.5 58.12 –1.208

* The quantity a is the temperature coefficient of σ as defined in the equation:

σ (t) = σ (0° C.) + aT,
where T is in degrees Celsius.
The earlier recommendation for quantum yields was based on the work of Harker et al. [151] and of Davenport [102] for the atmospherically important 375–470 nm region. The work by Gardner et al. [129] yields values that are in much better agreement with the values reported earlier by Jones and Bayes [193]. The recommended quantum yield values, listed in Table 4-11, are in agreement with the recommendation of Gardner et al. [129]; they are based on a smooth fit to the data of Gardner et al. [129] for the wavelength range from 334 to 404 nm; Harker et al. [151] for 397–420 nm (corrected for cr oss sections); Davenport [102] for 400–420 nm; and Jones and Bayes [193] for 297–412 nm. Direct measurements of the solar photodissociation rate of NO 2 in the troposphere by Parrish et al. [310] and by Shetter et al . [374] agree better with theoretical estimates based on this recommendation than with the earlier one.4-14 Table 4-11. Quantum Yields for NO 2 Photolysis

λ , nm Φ λ , nm Φ <285 1.000 393 0.953

290 0.999 394 0.950 295 0.998 395 0.942 300 0.997 396 0.922 305 0.996 397 0.870 310 0.995 398 0.820 315 0.994 399 0.760 320 0.993 400 0.695 325 0.992 401 0.635 330 0.991 402 0.560 335 0.990 403 0.485 340 0.989 404 0.425 345 0.988 405 0.350 350 0.987 406 0.290 355 0.986 407 0.225 360 0.984 408 0.185 365 0.983 409 0.153 370 0.981 410 0.130 375 0.979 411 0.110 380 0.975 412 0.094 381 0.974 413 0.083 382 0.973 414 0.070 383 0.972 415 0.059 384 0.971 416 0.048 385 0.969 417 0.039 386 0.967 418 0.030 387 0.966 419 0.023 388 0.964 420 0.018 389 0.962 421 0.012 390 0.960 422 0.008 391 0.959 423 0.004 392 0.957 424 0.000

C2. NO 3 + h ν → NO + O 2 ( Φ 1 )

NO 3 + h ν → NO 2 + O ( Φ 2 ). The absorption cross sections of the nitrate free radical, NO 3 , have been studied by (1) Johnston and Graham [188], (2) Gr aham and Johnston [144], (3) Mitchell et al. [262], (4) Marinelli et al. [242], (5) Ravishankara and Wine [330], (6) Cox et al. [88], (7) Burrows et al. [60], (8) Ravishankara and Mauldin [327], (9) Sander [356], (10) Cantrell et al. [69], (11) Canosa-Mas et al. [67], and (12) Yokelson et al. [437]. The 1st and 4th studies required calculation of the NO 3 concentration by modeling a complex kinetic system. The other studies are more direct, a nd the results in terms of integrat ed absorption coefficients are in good agreement. The recommended value at 298 K and 662 nm, (2.00 ± 0.25) × 10 –17 cm 2 , is the average of the results of studies (4), (5), and (7) through (11). The values in the wavelength range 600–670 nm, shown in Figure 4-1 and listed in Table 4-12, were calculated using the spectra measured in studies (8), (9), and (11), and with the 662 nm value normalized to the above average. The spectra obtained in other studies are consulted for a more extended wavelength range. The temperature dependence of the 662 nm band has been studied by Ravishankara and Mauldin, Sander, Cantrell et al., and Yokelson et al. Except for Cantrell et al., these studies all showed that the cross section at 662 nm increases with decreasing temperature. The reason for this discrepancy is not clear.
The quantum yields Φ 1 and Φ 2 have been measured by Graham and Johnston [144], and under higher resolution by Magnotta and Johnston [227], who report the product of the cross section times the quantum yield in the 400-to-630-nm range. The total quantum yield value, Φ 1 + Φ 2 , computed from the results of this latter study4-15 and the cross sections of Graham and Johnston [144], is above unity for λ <610 nm, which is, of course, impossible. Hence, there is some systematic error, and it is most likely in the primary quantum yield
measurements. More recently, Orlando et al. [306] measured the photolysis quantum yields between 570 and 635 nm. Johnston et al.[186] have recently re-analyzed the available la boratory data relevant to NO 3 photolysis, including quantum yield studies, chemiluminescence, LIF studies, and molecular-beam-scattering experiments. Their model reproduces the wavelength-dependent quantum yield data reasonably well. The new recommendation is based on the J-values calculated by J ohnston et al. for overhead sun in the stratosphere:

J 1 (NO + O 2 ) = 0.0201 s –1

J 2 (NO 2 + O) = 0.156 s –1

Wavelength-specific quantum yields over the temperature range 190–298 K may be found in the tabulation by Johnston et al.
The spectroscopy of NO 3 has been reviewed by Wayne et al. [431]. The reader is referred to this work for a more detailed discussion of the cross section and quantum yield data and for estimates of the photodissociation rates as a function of zenith angle.

Figure 4-1. Absorption Spectrum of NO 34-16 Table 4-12. Absorption Cross Sections of NO 3 at 298 K λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

600 258 625 796 648 60 601 263 626 703 649 51 602 302 627 715 650 49 603 351 628 702 651 52 604 413 629 672 652 55 605 415 630 638 653 61 606 322 631 470 654 76 607 225 632 344 655 93 608 170 633 194 656 131 609 153 634 142 657 172 610 192 635 128 658 222 611 171 636 159 659 356 612 202 637 191 660 658 613 241 638 193 661 1308 614 242 639 162 662 2000 615 210 640 121 663 1742 616 190 641 99 664 1110 617 189 642 91 665 752 618 208 643 93 666 463 619 229 644 92 667 254 620 292 645 85 668 163 621 450 646 72 669 113 622 941 647 69 670 85 623 1407 624 1139

C3. N 2 O + h ν → N 2 + O( 1 D). The recommended values are taken from the work of Selwyn et al. [371], who measured the temperature dependence of the absorption cross sections in the atmospherically relevant wavelength region. They have fitted their data with the expression shown in Table 4-13; Table 4-14 presents the room temperature data. Hubrich and Stuhl [165] remeasured the N 2 O cross sections at 298 K and 208 K and Merienne et al. [256] in the range from 220 K to 296 K. The results of these two sets of measurements are in very good agreement with those of Selwyn et al. The quantum yield for photodissociation is unity, and the products are N 2 and O( 1 D) (Zelikoff and Aschenbrand [448], Para skevopoulos and Cvetanovic [307], Preston and Barr [320], Simona itis et al. [381]). The yield of N( 4 S) and NO( 2 Π ) is less than 1% (Greenblatt and Ravishankara [147]).

Table 4-13. Mathematical Expression fo r Absorption Cross Sections of N 2 O as a Function of Temperature *

________________________________________________________ 

## ( ) 4 3

0 0 

### ln( ( , )) A 300 exp B n n

n n

n n 

### T T σ λλ λ

= = 

###  
= +−     

# ∑ ∑

Where T: temperature K; λ : nm; A 0 = 68.21023 B 0 = 123.4014 A 1 = –4.071805 B 1 = –2.116255 A 2 = 4.301146 × 10 –2 B 2 = 1.111572 × 10 –2
A 3 = –1.777846 × 10 –4 B 3 = –1.881058 × 10 –5
A 4 = 2.520672 × 10 –7

________________________________________________________ * Ranges of applicability: 173 nm < λ < 240 nm; 194 K < T < 320 K4-17 Table 4-14. Absorption Cross Sections of N 2 O at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

173 11.3 196 6.82 219 0.115 175 12.6 198 5.35 221 0.0739 176 13.4 199 4.70 222 0.0588 177 14.0 200 4.09 223 0.0474 178 13.9 201 3.58 224 0.0375 179 14.4 202 3.09 225 0.0303 180 14.6 203 2.67 226 0.0239 181 14.6 204 2.30 227 0.0190 182 14.7 205 1.95 228 0.0151 183 14.6 206 1.65 229 0.0120 184 14.4 207 1.38 230 0.00955 185 14.3 208 1.16 231 0.00760 186 13.6 209 0.980 232 0.00605 187 13.1 210 0.755 233 0.00478 188 12.5 211 0.619 234 0.00360 189 11.7 212 0.518 235 0.00301 190 11.1 213 0.421 236 0.00240 191 10.4 214 0.342 237 0.00191 192 9.75 215 0.276 238 0.00152 193 8.95 216 0.223 239 0.00123 194 8.11 217 0.179 240 0.00101 195 7.57 218 0.142

Several groups have investigated the isotopic fractionation of N 2 O resulting from photolysis in the UV. Fractionation factors have been measured by several gr oups following photolysis at several wavelengths in the 193–213 nm range: Turatti et al. [404] employed high resolution FTIR sp ectroscopy; Rockmann et al. [340] used a modified isotope ratio mass sp ectrometric technique; and Rahn et al . [321] utilized conventional isotope ratio mass spectrometry. Zhang et al. [450] employed a low-resolution FTIR technique with N 2 O photolysis at 213 nm, and Rockmann et al. [341] utilized a br oadband photolysis source centered around 200 nm and simulating stratospheric actinic fluxes. The results are in reasonably good agreement, and indicate that the fractionation factors increase with photolysis wavelength from 193 to 213 nm. Furthermore, the fractionation factors show a clear dependence on the position of the 15 N atom, in agreement with the theoretical model of Yung and Miller [447]; however, the th eoretical calculations underestimate the laboratory results by about a factor of two. Analysis of the isotopic composition of stratospheric air samples yields results that are in qualitative agreement with th e laboratory results, confirming that phot olysis is the predominant sink for N 2 O [148,341]. On the other hand, the fractionation factors measur ed in the atmospheric samples are smaller than those reported from the laboratory studies, indicating the influence of atmospheric diffusion and mixing [341].

C4. N 2 O 5 + h ν → Products. The absorption cross sections of dinitrogen pentoxide, N 2 O 5 have been measured at room temperature by Jones and Wulf [192] between 285 and 380 nm, by Johnston and Graham [188] between 210 and 290 nm, by Graham [143] between 205 and 380 nm, and for temperatures in the 223 to 300 K range by Yao et al. [436], between 200 and 380 nm. The agreement is good, particularly considering the difficulties in handling N 2 O 5 . The recommended cross section values, listed in Table 4-15, are taken from Yao et al. [436]. For wavelengths shorter than 280 nm there is little or no temperature dependence, and between 285 and 380 nm the temperature effect is best computed with the expression listed at the bottom of Table 4-15. Recent measurements of the cross sections and their temperature dependence by Harwood et al. [153] yield values in excellent agreement with this recommendation except at the longest wavelengths (380 nm) and lowest temperatures (233 K), where the new values are about 30% lower. However, the contribution to solar photodissociation from these longer wavelengths is neg ligible, and the differences between the predicted photolysis rates from the two sets of data are smaller than 3% (Harwood et al. [153]).
There are several studies on the primary photolysis products of N 2 O 5 : Swanson et al. [391] have measured the quantum yield for NO 3 production at 249 and at 350 nm, obtaining a value close to unity, which is consistent with the observations of Burrows et al. [59] for photolysis at 254 nm. Barker et al. [21] report a quantum yield4-18 for O( 3 P) production at 290 nm of less than 0.1, and near unity for NO 3 . For O-atom production Margitan (private communication, 1985) measured a quantum yiel d value of 0.35 at 266 nm, and Ravishankara et al. [331] report values of 0.72, 0.38, 0.21 and 0.15 at 248, 266, 287, and 289 nm, respectively, with a quantum yield near unity for NO 3 production at all these wavelengths. It appears, then, that NO 3 is produced with unit quantum yield while the O-atom, and hence the NO yield, increases at shorter wavelengths, with a consequent decrease in the NO 2 yield. The study of Oh et al. [299] indicates that, besides NO 3 , the primary photolysis products are a wavelength-dependent mixture of NO 2 , NO 2 * and NO + O, where NO 2 * represents one or more excited electronic states, most likely the 2 B 1 state.

Table 4-15. Absorption Cross Sections of N 2 O 5

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

205 820 250 40 210 560 255 32 215 370 260 26 220 220 265 20 225 144 270 16.1 230 99 275 13.0 235 77 280 11.7 240 62

Note: For 285 nm < λ < 380 nm; 300 K > T > 225 K: 10 20 σ = exp(2.735 + ((4728.5 – 17.127 λ )/T)) where σ is in cm 2 /molecule; λ in nm; and T in K. C5. HONO + h ν → OH + NO. The ultraviolet spectrum of HONO between 300 and 400 nm has been studied by Stockwell and Calvert [389] by examination of its equilibrium mixtures with NO, NO 2 , H 2 O, N 2 O 3 and N 2 O 4 ; the possible interferences by thes e compounds were taken into account. More recently, Vasudev [421] measured relative cross sections by monitoring the OH photodissociation product with laser-induced fluorescence; and Bongartz et al. [38] determined absolute cross section values at 0.1 nm resolution in a system containing a highly diluted mixture of NO, NO 2 , H 2 O, and HONO, by measuring total NO
x (NO and NO 2)
. There are some discrepancies between these two recent sets of results in terms of relative peak heights; however, both yield essentially the same photodissociation rate provided Vasudev's relative data are normalized to match the cross section value reported by Bongartz et al. at 354 nm. At this wavelength the value reported earlier by Stockwell and Calvert is about 20% smaller. The recommended values, listed in Table 4-16, are taken from Bongartz et al.4-19 Table 4-16. Absorption Cross Sections of HONO

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

310 1.3 339 18.8 368 52.0 311 1.9 340 10.0 369 38.8 312 2.8 341 17.0 370 17.8 313 2.2 342 38.6 371 11.3 314 3.6 343 14.9 372 10.0 315 3.0 344 9.7 373 7.7 316 1.4 345 10.9 374 6.2 317 3.1 346 12.3 375 5.3 318 5.6 347 10.4 376 5.3 319 3.6 348 9.1 377 5.0 320 4.9 349 7.9 387 5.8 321 7.8 350 11.2 379 8.0 322 4.9 351 21.2 380 9.6 323 5.1 352 15.5 381 11.3 324 7.1 353 19.1 382 15.9 325 5.0 354 58.1 383 21.0 326 2.9 355 36.4 384 24.1 327 6.6 356 14.1 385 20.3 328 11.7 357 11.7 386 13.4 329 6.1 358 12.0 387 9.0 330 11.1 359 10.4 388 5.6 331 17.9 360 9.0 389 3.4 332 8.7 361 8.3 390 2.7 333 7.6 362 8.0 391 2.0 334 9.6 363 9.6 392 1.5 335 9.6 364 14.6 393 1.1 336 7.2 365 16.8 394 0.6 337 5.3 366 18.3 395 1.0 338 10.0 367 30.2 396 0.4

C6. HNO 3 + h ν → products. The recommended absorption cross sections and their temperature dependency, listed in Table 4-17, are taken from the work of Burkholder et al. [56]. The temperature effect is very important for estimates of atmospheric photodissociati on; the results of Burkholder et al. agree well with those of Rattigan et al. [322,323], except at 238 K, where these latter authors report significantly smaller values.
The new cross section values agree reasonably well at room temperature with the data of Molina and Molina [267], which provided the basis for the earlier recommendation. These data are also in good agreement throughout the 190–330 nm range with the values reported by Biaume [32]. They are also in very good agreement with the data of Johnston and Graham [ 187], except towards both ends of the wavelength range. Okabe [301] has measured the cross sections in th e 110–190 nm range and his results are 20–30% lower than those of Biaume and of Johnston and Graham around 185–190 nm.
Johnston et al. [185] measured a quantum yield value of ~1 for the OH + NO 2 channel in the 200–315 nm range, using end product analysis. The quantum yield for O-atom production at 266 nm has been measured to be 0.03, and that for H-atom production less than 0.002, by Margitan and Watson [234], who looked directly for these products using atomic resonance fluorescence. Jolly et al. [191] measured a quantum yield for OH production of 0.89 ± 0.08 at 222 nm. Turnipseed et al. [407] have measured a quantum yield near unity for OH production at 248 and 222 nm. However, at 193 nm they report this quantum yield to be only ~0.33, and the quantum yield for production of O-atoms to be about 0.8. Thus, it appears that HONO is a major photolysis product at 193 nm. These results are qualitatively in agreement with those reporte d by Schiffman et al. [364], namely a quantum yield for OH production of 0.47 at 193 nm, and of 0.75 at 248 nm.4-20 Table 4-17. Absorption Cross Sections and Temperature Coefficients of HNO 3 Vapor

λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 )
192 1225 0 246 2.06 1.61 300 0.263 3.10 194 1095 0 248 2.00 1.44 302 0.208 3.24 196 940 1.70 250 1.97 1.34 304 0.167 3.52 198 770 1.65 252 1.96 1.23 306 0.133 3.77 200 588 1.66 254 1.95 1.18 308 0.105 3.91 202 447 1.69 256 1.95 1.14 310 0.0814 4.23 204 328 1.74 258 1.93 1.12 312 0.0628 4.70 206 231 1.77 260 1.91 1.14 314 0.0468 5.15 208 156 1.85 262 1.87 1.14 316 0.0362 5.25 210 104 1.97 264 1.83 1.18 318 0.0271 5.74 212 67.5 2.08 266 1.77 1.22 320 0.0197 6.45 214 43.9 2.17 268 1.70 1.25 322 0.0154 6.70 216 29.2 2.17 270 1.62 1.45 324 0.0108 7.16 218 20.0 2.21 272 1.53 1.49 326 0.00820 7.55 220 14.9 2.15 274 1.44 1.56 328 0.00613 8.16 222 11.8 2.06 276 1.33 1.64 330 0.00431 9.75 224 9.61 1.96 278 1.23 1.69 332 0.00319 9.93 226 8.02 1.84 280 1.12 1.78 334 0.00243 9.60 228 6.82 1.78 282 1.01 1.87 336 0.00196 10.5 230 5.75 1.80 284 0.909 1.94 338 0.00142 10.8 232 4.87 1.86 286 0.807 2.04 340 0.00103 11.8 234 4.14 1.90 288 0.709 2.15 342 0.00086 11.8 236 3.36 1.97 290 0.615 2.27 344 0.00069 9.30 238 2.93 1.97 292 0.532 2.38 346 0.00050 12.1 240 2.58 1.97 294 0.453 2.52 348 0.00042 11.9 242 2.34 1.88 296 0.381 2.70 350 0.00042 9.30

σ ( λ , T) = σ ( λ , 298) exp (B ( λ ) (T – 298)); T in K

C7. HO 2 NO 2 + h ν → Products. There are five studies of the UV spectrum of HO 2 NO 2 vapor: Cox and Patrick [91], Morel et al. [282], Graham et al. [145], Molina and Molina [267], and Singer et al. [382]. The latter three studies are the only ones covering the gas phase spectru m in the critical wavelength range for atmospheric photodissociation ( λ ≥ 290 nm). The recommended values, listed in Table 4- 18, are an average of the work of Molina and Molina [267] and of Singer et al. [382], which are the more direct studies. The cross sections appear to be temperature independent between 298 and 253 K (Singer et al. [382]). MacLeod et al. [226] report that photolysis at 248 nm yields one third OH and NO 3 and two thirds HO 2 + NO 2 . Table 4-18. Absorption Cross Sections of HO 2 NO 2 Vapor

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 1010 260 28.5 195 816 265 23.0 200 563 270 18.1 205 367 275 13.4 210 239 280 9.3 215 161 285 6.2 220 118 290 3.9 225 93.5 295 2.4 230 79.2 300 1.4 235 68.2 305 0.9 240 58.1 310 0.5 245 48.9 315 0.3 250 41.2 320 0.2 255 35.0 325 0.14-21 D1. CH 2 O + h ν → H + HCO ( Φ 1 )

CH 2 O + h ν → H 2 + CO ( Φ 2 ). The earlier recommendation for the formaldehyde absorption cross sections was based on the work carried out by Bass et al. [25] with a resolution of 0.05 nm at 296 K and 223 K, and by Moortgat et al. [277,279] with a resolution of 0.5 nm in the 210–360 K temperature range. More recently, Cantrell et al. [68] measured the cross sections in the 300–360 nm range between 223 K and 293 K, and Rogers [345] measured the cross sections in the 235–365 nm range at 296 K, both groups using Fourier transform spectrometry at a resolution of up to 0.011 nm ( 1 cm –1 ). The agreement between these two reports is very good. The recommended values are those given by Cantrell et al. as a function of temperature; the reader is referred to the original article to obtain the high-resolution data. Table 4-19 lists the low-resolution cross sections taken from that work, that are suitable for atmospheric photodissociation calculations.
The quantum yields have been reported with good agreement by Horowitz and Calvert [162], Clark et al. [79], Tang et al. [400], Moortgat and Warneck [281], and Moortgat et al. [277,279]. The recommended values listed in Table 4-19 are based on the results of these investigators, as evaluated by S. Madronich (private communication, 1991). The quantum yield for the production of H 2 and CO is pressure- and temperaturedependent for wavelengths longer than about 330 nm (Moortgat et al. [279]). Table 4-19 gives the values at atmospheric pressure and room temperature; the reader is referred to the Moortgat et al. publication for information on values at lower pressures and temperatures. Table 4-19. Absorption Cross Sections and Quantum Yields for Photolysis of CH 2 O

10 20 σ (cm 2 ) T-Parameters* λ (nm) 223 K 293 K A B Φ 1 (H + HCO) (H 2 + CO)

301.25 1.38 1.36 1.37 –0.21 0.749 0.251 303.75 4.67 4.33 4.43 –4.73 0.753 0.247 306.25 3.32 3.25 3.27 –1.06 0.753 0.247 308.75 2.27 2.22 2.24 –0.724 0.748 0.252 311.25 0.758 0.931 0.882 2.48 0.739 0.261 313.75 3.65 3.40 3.47 –3.64 0.724 0.276 316.25 4.05 3.89 3.94 –2.30 0.684 0.316 318.75 1.66 1.70 1.69 0.659 0.623 0.368 321.25 1.24 1.13 1.16 –1.52 0.559 0.423 323.75 0.465 0.473 0.471 0.118 0.492 0.480 326.25 5.06 4.44 4.61 –8.86 0.420 0.550 328.75 2.44 2.29 2.34 –2.15 0.343 0.634 331.25 1.39 1.28 1.31 –1.53 0.259 0.697 333.75 0.093 0.123 0.114 0.432 0.168 0.739 336.25 0.127 0.131 0.130 0.050 0.093 0.728 338.75 3.98 3.36 3.54 –8.96 0.033 0.667 341.25 0.805 0.936 0.898 1.86 0.003 0.602 343.75 1.44 1.26 1.31 –2.64 0.001 0.535 346.25 0.004 0.071 0.052 0.957 0 0.469 348.75 0.009 0.040 0.031 0.438 0 0.405 351.25 0.169 0.235 0.216 0.948 0 0.337 353.75 1.83 1.55 1.63 –4.05 0 0.265 356.25 0.035 0.125 0.099 1.27 0 0.197

Note: The values are averaged for 2.5 nm intervals centered on the indicated wavelength. * Cross section for –50°C < T < 20°C calculated as σ (T) = A + B × 10 –3 T; T in °C, and σ in 10 –20 cm 2

.

D2. CH 3 O 2 + h ν → Products. The absorption cross sections of the methylperoxy radical, CH 3 O 2 , in the 195–310-nm region have been measured at room temperature by Parkes et al. [309], Hochanadel et al. [160], Parkes [308], Anastasi et al. [12], Kan et al. [197], Cox and Tyndall [93,94] at 250 nm only; Adachi et al. [5], Sander and Watson [360] at 250 nm onl y; Pilling and Smith [316] at 254 nm only, Kurylo et al. [206], McAdam et al. [250], Jenkin et al. [181], Wallington et al . [425], Moortgat et al. [280], Dagaut and Kurylo [99], Simon et al. [377], Jenkin and Cox [180], Lightfoot and Jemi-Alade [218] who measured the cross sections up to 777 K., Maricq and Wa llington [240], Wallington et al. [427], Roehl et al. [342], and Fahr et al.4-22 [114]. The absorption cross sections have been evaluated in earlier reviews by Lightfoot et al. [217] and Wallington et al. [426], who noted significant discrepancies in the both the shapes of the spectra and the absolute magnitude of the cross section values. Th e ultraviolet absorption sp ectra have recently been reevaluated by Tyndall et al . [408], who fitted the absorption spectra to a semilogarithmic Ga ussian distribution function suggested by Lightfoot et al. [217] and Maric et al. [237] using:

2

max ln

max 

### exp a λ
λ 

### σ σ    

−        



### =
Screening of the data suggested that most spectra published before 1987 did not constrain the shape of the spectrum very well as indicated by the large relative uncertainty of the width parameter a. The shape was determined by averaging th e individual fitting parameters from McAdam et al., Moortgat et al. [280], Simon et al. [377], Lightfoot and Je mi-Alade [218], Jenkin and Cox [180] and Maricq and Wallington [240], which were judged to be most reliable by Tyndall et al. [408]. Absolu te cross sections were based on relative measurements of absorption cross sections of CH 3 O 2 and C 2 H 5 O 2 at 240 nm taken under identi cal conditions (Wallington et al. [426], Maricq and Wallingt on [240], Fenter et al. [120] and Roehl et al. [342]), combined with independent calibrations by Dagaut and Kurylo [99], Simon et al. [377] and Lightfoot and Jemi-Alade [218]. The fitting parameters are: σ max = 4.26 × 10 –18 cm 2 molecule –1 ; a = 44.4; λ max = 237.3 nm. Table 4-20 lists the recommended cross sections, which are taken from the review by Tyndall et al.
Photolysis of CH 3 O 2 in the stratosphere and troposphere is slow and can be neglected, but the UV absorption cross sections are important in laboratory studies of reaction kinetics.

Table 4-20. Absorption Cross Sections of CH 3 O 2 , C 2 H 5 O 2 , and CH 3 C(O)O 2

10 20 σ (cm 2 ) λ (nm) CH 3 O 2 C 2 H 5 O 2 CH 3 C(O)O 2 195.0 389 200.0 564 205.0 165 665 210.0 219 195 656 215.0 276 257 564 220.0 330 319 451 225.0 376 374 366 230.0 408 418 326 235.0 424 444 319 240.0 424 452 326 245.0 407 440 330 250.0 378 412 322 255.0 339 372 300 260.0 294 324 268 265.0 248 273 229 270.0 203 222 187 275.0 162 176 147 280.0 126 136 111 285.0 96.1 102 81.2 290.0 71.5 74.6 57.3 295.0 52.0 53.3 300.0 37.3

D3. C 2 H 5 O 2 + h ν → Products. The absorption cross sections of the ethylperoxy radical, C 2 H 5 O 2 , in the 200–310-nm region have been measured at room temperature by Adachi et al. [4], Anastasi et al . [13], Cattell et al. [70], Wallington et al. [426], Bauer et al. [27], Maricq and Wa llington [240], Fenter et al . [120], Munk et al. [284]. The absorption cross sections have b een evaluated in earlier reviews by Li ghtfoot et al. [217] and Wallington et al. [426], who noted significant discrepancies in the both the shapes of the spectra and the absolute magnitude of the cross section values. The ultr aviolet absorption spectra have recently been reeval uated by Tyndall et al.4-23 [408], who fitted the absorption spectra to a semiloga rithmic Gaussian distribu tion function suggested by Lightfoot et al. and Maric et al. [237] using:

2

max ln

max 

### exp a λ
λ 

### σ σ    

−        



### = The shape was determined by averaging the individual fitting parameters from Wallington et al., Bauer et al., Maricq and Wallington and Fenter et al., which were judged to be most reliable by Tyndall et al. Absolute cross sections were based on relative measurements of absorption cross sections of CH 3 O 2 and C 2 H 5 O 2 at 240 nm taken under identical conditions (Walli ngton et al. [426], Maricq and Wallington [240], Fent er et al. [120] and Roehl et al. [342]), combined with indepe ndent calibrations. The fitting parameters are σ max = 4.52 × 10 –18 cm 2
molecule –1 ; a = 49.0; λ max = 239.4 nm. Table 4-20 lists the recommended cross sections, which are taken from the review by Tyndall et al.
Photolysis of C 2 H 5 O 2 in the stratosphere and troposphere is slow and can be neglected, but the UV absorption cross sections are important in laboratory studies of reaction kinetics.

D4. CH 3 OOH + h ν → Products. Vaghjiani and Ravishankara [414] measured the cross sections of CH 3 OOH by monitoring the CH 3 OOH concentration via trapping and titration. These results are recommended and are listed in Table 4-21. The earlier results of Molina and Arguello [274] are consistently 40% higher than the values shown in Table 4-21; this difference is belie ved to be due to difficulty in trapping CH 3 OOH and measuring its concentration. CH 3 OOH dissociates upon light absorption to give CH 3 O with unit quantum yield (Vaghjiani and Ravishankara, [415]); these authors also obser ved some production of H and O atoms at shorter wavelengths (i.e., 193 nm). Thelen et al. [401] report unit quantum yield for OH production at 248 and 193 nm, in agreement with the results of Vaghjiani and Ravishankara.

Table 4-21. Absorption Cross Sections of CH 3 OOH

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

220 15.4 300 0.41 230 9.62 310 0.24 240 6.05 320 0.14 250 3.98 330 0.079 260 2.56 340 0.047 270 1.70 350 0.027 280 1.09 360 0.016

D5. HCN + h ν → Products. Herzberg and Innes [159] have studied th e spectroscopy of hydrogen cyanide, HCN, that starts absorbing weakly at λ < 190 nm. The solar photodissociation rate for this molecule is rather small, even in the upper stratosphere; estimates of this rate would require additional studies of the abso rption cross sections and quantum yields in the 200-nm region.

D6. CH 3 CN + h ν → Products. McElcheran et al. [251] have reported the spectrum of acetonitrile or methyl cyanide, CH 3 CN; the first absorption band appears at λ < 220 nm. More recently, Suto and Lee [390] and Zetzsch [449] have measured the cross sections around 200 nm; solar photodissociation is unimportant compared to reaction with OH radicals.

D7 CH 3 C(O)O 2 + h ν → Products. The UV absorption spectru m of the acetylperoxy radical, CH 3 C(O)O 2 , exhibits two absorption maxima in the 185–285 nm region: a strong band near 207 nm, and a feature at 245 nm that is weaker by a factor of 2. The absorp tion cross sections have been measured at room temperature by Addison et al. [6], Basco and Parmer [24], Moortgat et al. [280], Maricq and Szente [239], and Roehl et al. [342]. The absorption cross sections have been evaluated in earlier reviews by Lightf oot et al. [217] a nd Wallington et al. [426], who noted significant discrepancies in the both the shapes of the spectra and the absolute magnitude of the cross section values. Th e ultraviolet abso rption spectra have recently been reevaluated by Tyndall et al. [408], who fitted the absorption spectra to the sum of two Gaussian-shaped absorption bands:4-24 2 2 max1 max 2 1 2

ln ln

max1 max 2 

### exp exp a a λ λ

λ λ 

### σσ σ   

  

− −

  

         

### = +

The shape was determined by averaging the individual fitting parameters from Maricq and Szente and Roehl et al., which were judged to be the most reliable to date; th e data by Maricq and Szente were adjusted for their overcorrection for the contribution of CH 3 O 2 . Absolute cross sections were based on relative measurements of absorption cross sections of C 2 H 5 O 2 at 240 nm taken under identical c onditions. The fitting parameters are

σ max1 = 6.29 × 10 –18 cm 2 molecule –1 ; λ max1 = 206.0 nm; a 1 = 168.0; σ max2 = 3.26 × 10 –18 cm 2 molecule –1 ; λ max2 = 246.1 nm; a 2 = 64.2. Table 4-20 lists the recommended cross sections, which are taken from the review by Tyndall et al.
Photolysis of CH 3 C(O)O 2 in the stratosphere and troposphere is slow and can be neglected, but the UV absorption cross sections are important in laboratory studies of reaction kinetics.

D8. CH 3 C(O)O 2 NO 2 + h ν → Products. Absorption spectra of CH 3 C(O)O 2 NO 2 (PAN) have been measured by Senum et al. [372] over the range 200–300 nm, Libuda and Zabel [216] over the range 220–325 nm, and Talukdar et al. [395] over the spectral range 195–345 nm and temperature range 250–298 K. The three studies are in excellent agreement over their range of overlap, w ith the values of Senum et al. being slightly smaller (15–20%) beyond 250 nm. Libuda and Zabel carried out simu ltaneous infrared absorption studies that showed that the measured cross sections need to be corrected for impurities that are transparent in the ultraviolet but contribute to the sample pressure in the absorption cell. These corrections are on the order of 20%. The recommended cross sections (Table 4-22) are based on th e measurements of Talukdar et al. because of the good agreement with Libuda and Zabel and the wider spectral coverage and temperature range of this study. The uncertainties in the reported cross sections are probably quite large (on the order of a factor of 2), decreasing to about 30% at shorter wavelengths. The only PAN quantum yield studies are those of Mazely et al. [248,249]. In these studies, PAN was photolyzed at 248 nm, with NO 2 and NO 3 products being observed by laser-induced fluorescence at 298 K. Quantum yields of 0.83 ± 0.09 were obtained for the CH 3 C(O)O 2 + NO 2 channel and 0.3 ± 0.1 for the CH 3 C(O)O + NO 3 channel.4-25 Table 4-22. Absorption Cross Sections of PAN

λ (nm) 10 20 σ(298Κ) (cm 2 ) 10 3 B (K –1 ) λ (nm) 10 20 σ(298Κ) (cm 2 ) 10 3 B (K –1 )

196 430 2.02 274 2.4 5.55 198 400 1.73 276 2.1 5.76 200 360 1.36 278 1.7 5.98 202 320 1.07 280 1.5 6.20 204 290 0.86 282 1.2 6.43 206 260 0.75 284 1.0 6.67 208 230 0.71 286 0.81 6.90 210 200 0.75 288 0.65 7.15 212 170 0.84 290 0.54 7.39 214 140 0.97 292 0.45 7.63 216 120 1.12 294 0.37 7.86 218 100 1.29 296 0.30 8.08 220 90 1.47 298 0.24 8.27 222 78 1.64 300 0.19 8.44 224 68 1.81 302 0.15 8.61 226 59 1.98 304 0.12 8.76 228 52 2.14 306 0.10 8.87 230 46 2.30 308 0.082 9.01 232 40 2.46 310 0.067 9.13 234 35 2.63 312 0.054 9.3 236 31 2.80 314 0.046 9.46 238 28 2.96 316 0.036 9.57 240 24 3.11 318 0.030 9.75 242 21 3.25 320 0.025 10.0 244 19 3.39 322 0.020 10.2 246 17 3.52 324 0.017 10.4 248 15 3.64 326 0.014 10.6 250 13 3.76 328 0.012 10.7 252 11 3.87 330 0.011 10.9 254 10 3.98 332 0.0086 11.2 256 8.9 4.10 334 0.0068 11.5 258 7.8 4.23 336 0.0061 11.7 260 6.8 4.38 338 0.0053 11.9 262 6.0 4.53 340 0.0050 12.2 264 5.2 4.68 342 0.0036 12.4 266 4.5 4.82 344 0.0024 12.5 268 3.9 4.97 346 0.0023 270 3.4 5.14 348 0.0025 272 2.9 5.34 350 0.0016 Cross sections in the temperature range 250–298 K are calculated using the equation, ln( σ(Τ)/σ(298Κ)) = Β(Τ−298).

E1. HF + h ν → H + F. The ultraviolet absorption spectrum of HF has been studied by Safary et al. [354]. The onset of absorption occurs at λ < 170 nm, so that photodissociation of HF should be unimportant in the stratosphere.

E2. FNO + h ν → F + NO. The absorption cross sections have been measured by Burley et al. [58], who report their results in graphical form as well as in tabular form in 1-nm intervals, between 180 and 350 nm. The spectrum shows vibronic structure at wavelengths longer than 250 nm. The cross section values are listed in Table 4-23 in 2-nm intervals. The quantum yield for decomposition is expected to be unity (Brandon et al., [39]; Reid et al., [336]).4-26 Table 4-23. Absorption Cross Sections of FNO

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

180 52.4 236 3.09 292 11.9 182 51.7 238 2.76 294 7.11 184 50.7 240 2.25 296 9.15 186 49.4 242 2.08 298 22.0 188 47.5 244 1.74 300 15.6 190 45.1 246 1.65 302 25.4 192 42.7 248 1.41 304 8.85 194 40.0 250 1.54 306 11.8 196 37.3 252 1.25 308 32.2 198 33.8 254 1.23 310 15.5 200 30.5 256 1.36 312 31.6 202 27.7 258 1.58 314 12.3 204 24.8 260 1.30 316 11.0 206 22.2 262 1.64 318 25.5 208 19.9 264 2.03 320 15.2 210 17.6 266 1.96 323 40.2 212 15.8 268 2.10 324 17.8 214 13.9 270 2.81 326 12.1 216 12.3 272 4.47 328 9.39 218 10.7 274 3.97 330 12.9 220 9.35 276 4.24 332 13.0 222 8.32 278 3.41 334 19.3 224 7.22 280 8.26 336 13.1 226 6.30 282 7.58 338 8.96 228 5.44 284 7.26 340 5.65 230 4.68 286 5.17 342 3.81 232 4.10 288 10.4 344 2.68 234 3.52 290 17.0 346 1.96

348 1.48 350 1.18

E3. CF 4 +h ν → products. See Note E4.

E4. C 2 F 6 + h ν → products. CF 4 and C 2 F 6 do not absorb in the ultraviolet at wavelengths longer than 105 and 120 nm, respectively (Sauvageau et al. [362,363]; Inn, [178]); therefore, they are not expected to photodissociate until they reach the mesosphere.

E5. CF 2 O + h ν → Products. The recommended absorption cross sections for CF 2 O, CCl 2 O and CClFO are listed in Table 4-24, as averages over the 500 cm –1 intervals commonly employed for atmospheric modeling (the wavelength given in the table is the center of the interval). The values for CCl 2 O are based on the work of Gillotay et al. [139], who measured the cross sections between 170 and 320 nm at temperatures ranging from 210 to 295 K; the temperature effect is significant only at wavelengths longer than 250 nm. These cross section values are in good agreement with those recommended earlier, which were based on the data of Chou et al. [76]. For CClFO the recommended values are based on this latter work between 184 and 199 nm, and they are taken from the work of Nölle et al. [296] at the longer wavelengths. These workers measured the cross sections at temperatures ranging from 223 to 298 K; the temperature effect is not important for atmospheric photodissociation calculations, as is the case with CCl 2 O. For CF 2 O the cross section values are taken from Molina and Molina [268] between 184 and 199 nm, and from Nölle et al. [297] at the longer wavelengths. These authors measured the cross sections at 296 K between 200 and 230 nm.
The photodissociation quantum yield for CCl 2 O is unity (Calvert and Pitts [ 65]); the spectrum is a continuum. Similarly, the quantum yield for CClFO is taken as unity; the spectrum shows little structure. In contrast, the CF 2 O spectrum is highly structured. Nevertheless, its photodissociation quantum yield is also taken as unity, as4-27 reported by Nölle et al. [297]. The self-reaction of the CFO photodissociation product regenerates CF 2 O, and hence the apparent quantum yield is less than unity.

Table 4-24. Absorption Cross Sections of CCl 2 O, CClFO, and CF 2 O at 298 K

10 20 σ (cm 2 ) λ (nm) CCl 2 O CClFO CF 2 O
184.4 234 – – 186.0 186 15.6 5.5 187.8 146 14.0 4.8 189.6 116 13.4 4.2 191.4 90.3 12.9 3.7 193.2 71.5 12.7 3.1 195.1 52.4 12.5 2.6 197.0 39.3 12.4 2.1 199.0 31.2 12.3 1.6 201.0 25.2 12.5 1.3 203.0 20.9 12.0 0.95 205.1 17.9 11.5 0.74 207.3 15.8 10.8 0.52 209.4 14.3 9.9 0.40 211.6 13.3 9.0 0.28 213.9 12.6 7.9 0.20 216.2 12.3 6.8 0.12 218.6 12.2 5.8 0.08 221.0 12.2 4.8 0.049 223.5 12.4 3.8 0.035 225.7 12.7 2.9 0.024 228.6 13.1 2.2 0.018

E6. CF 3 OH + h ν → Products

. An upper limit of 10 –21 cm 2 has been determined experimentally by Molina and Molina [271] for the absorption cross sections of CF 3 OH in the 190–300-nm wavelength range. This upper limit is in agreement with estimates based on similarities between CF 3 OH and CH 3 OH, as well as with quantum chemistry calculations, as reported by Schneider et al. [368].

F1. Cl 2 + h ν → Cl + Cl. The recommended absorption cross sections are taken from the work of Maric et al. [235]; they can be calculated at various temperatures with the expression given at the bottom of Table 4-25. For convenience, some room temperature values are also listed in the table. Ganske et al. [128] have also measured the cross sections at room temperature, and the agreement with th e recommended values is excellent. These two sets of data also agree well with the earlier recommendation, which was based on the work of Seery and Britton [370], which is in turn in good agreement with the results reported by Gibson and Bayliss [131], Fergusson et al. [121], and Burkholder and Bair [51]. The estimated atmospheric photodissociation rate is only weakly affected by the temperature de pendency of the cross sections.4-28 Table 4-25. Absorption Cross Sections of Cl 2

λ (nm) 10 20 σ , 298K (cm 2 ) λ (nm) 10 20 σ , 298K (cm 2 )

260 0.20 370 8.4 270 0.82 380 5.0 280 2.6 390 2.9 290 6.2 400 1.8 300 11.9 410 1.3 310 18.5 420 0.96 320 23.7 430 0.73 330 25.5 440 0.54 340 23.5 450 0.38 350 18.8 460 0.26 360 13.2 470 0.16

2 2

20 0.5 329.5 406.5 10 27.3exp 99.0 ln 0.932exp 91.5 ln σα α α λ λ −            = − +−                    

where α = tanh (402.7/T); λ in nm, and T in K; 300 K > T > 195 K.

F2. ClO + h ν → Cl + O. The absorption cross sections of chlorine monoxide, ClO, have been reviewed by Watson [430]. There are more recent measurements yielding results in reasonable agreement w ith the earlier ones, (1) Mandelman and Nicholls [232] in the 250–310 nm region; (2) Wine et al. [433] around 283 nm; (3) Rigaud et al. [337], (4) Jourdain et al. [194], (5) Sander and Friedl [357], (6) Trolier et al. [402] in the 270–310-nm region, and (7) Simon et al. [378] between 240 and 310 nm. The peak cross section at the top of the continuum is 5.2 × 10 –18 , based on the average of studies (4)–(7) and Johnston et al. [189]. Figure 4-2 shows a spectrum of ClO. It should be noted that the cross sections on the structured part are extremely dependent on instrument resolution, and the figure is only a guide to the line positions and approximate shapes. The cross sections of the continuum are independent of temperature (Trolier et al. [402]), while the structured part is extremely temperature dependent. The bands sharpen and grow with a decrease in temperature.
The calculations of Coxon et al. [ 95] and Langhoff et al. [210] indicate that phot odecomposition of ClO accounts for at most 2 to 3% of the total destruction rate of ClO in the stratosphere, which occurs predominantly by reaction with oxygen atoms and nitric oxide.4-29 Figure 4-2. Absorption Spectrum of ClO

F3. ClOO + h ν → ClO + O. Johnston et al. [189] measured the absorption cross sections of the ClOO radical using a molecular modulation technique that required interpretation of a complex kinetic scheme. More recently, Mauldin et al. [247] reported cross section measurements in the range from 220 to 280 nm, and Baer et al. [17] from 240 to 300 nm. These two studies are in very good agreement, yielding cross section values that are more than twice as large as the older Johnston et al. values. The recommended cross sections are listed in Table 4-26, and are taken from the work of Mauldin et al.

Table 4-26. Absorption Cross Sections of ClOO

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

220 611 252 2630 222 670 254 2370 224 747 256 2120 226 951 258 1890 228 1100 260 1610 230 1400 262 1370 232 1650 264 1120 234 1960 266 905 236 2240 268 725 238 2520 270 596 240 2730 272 435 242 2910 274 344 244 2960 276 282 246 2980 278 210 248 2950 280 200 250 28004-30 F4. OClO + h ν → O + ClO. The spectrum of OClO is characterized by a series of well-developed progressions of bands extending from ~280 to 480 nm. The spectroscopy of this molecule ha s been studied extensively, and the quantum yield for photodissociation appears to be unity throughout the above wavelength range. See for example, the review by Watson [430]. Birks et al. [35] have estimated a half-life against atmospheric photodissociation of OClO of a few seconds. The recommended absorption cross section values are those reported by Wahner et al. [424], who measured the spectra with a resolution of 0.25 nm at 204, 296, and 378 K, in the wavelength range 240 to 480 nm. Table 4-27 lists the cross section values at th e peak of the bands (a(0) to a(26)). Figure 4-3, from Wahner et al., shows the OClO spectrum at 204 K and at room temperature. Hubinger and Nee [163] have extended the measurements of OClO cross sections over the spectral range 125–470 nm. Frost et al. [126] have studied the spectrum at very high spectral resolution (0.1 cm –1 ) and at low temperature (200 K) in molecular beam expansion. In both of these studies, cross sections were measured relative to values obtained by Wahner et al. The photochemistry of OClO is extremely complex, with several electronic excited states involved in the photodissociation dynamics. Several channe ls have been observed at wavelengt hs important in the stratosphere, including O + ClO, Cl + O 2 and isomerization to ClOO. Colussi [83] measured the quantum yield for chlorine atom production to be less than 0.01, and for oxygen atom production to be unity (within experimental error), both at 308 nm. Vaida et al. [417] and Ruhl et al. [352] reported chlorine atom production at 362 nm; and Bishenden et al. [36,37] measured the quantum yield for this process to be 0.15±0.10 around that same wavelength. In contrast, Lawrence et al. [211] report a quantum yield for Cl-atom production in the 359–368-nm region of less than 5 × 10 –4

. This conclusion is supported by photofragment studies of Davis and Lee [105], who report Cl yields <0.2% below 370 nm, rising to a maximum of 4% near 404 nm. The recommendation is to use a quantum yield value of unity for the production of O-atoms. While accurate absorption cross section values are valuable for atmospheric measurements of OClO levels, the identity of the photodissociation products is only of minor importance in the context of atmospheric processes. Table 4-27. Absorption Cross Sections of OClO at the Band Peaks

10 20 σ (cm 2 ) λ (nm) 204 K 296 K 378 K
475.53 – 13 – 461.15 17 17 16 446.41 94 69 57 432.81 220 166 134 420.58 393 304 250 408.83 578 479 378 397.76 821 670 547 387.37 1046 844 698 377.44 1212 992 808 368.30 1365 1136 920 359.73 1454 1219 984 351.30 1531 1275 989 343.44 1507 1230 938 336.08 1441 1139 864 329.22 1243 974 746 322.78 1009 791 628 317.21 771 618 516 311.53 542 435 390 305.99 393 312 291 300.87 256 219 216 296.42 190 160 167 291.77 138 114 130 287.80 105 86 105 283.51 089 72 90 279.64 073 60 79 275.74 059 46 – 272.93 053 33 –4-31 Figure 4-3. Absorption Spectrum of OClO4-32 F5. ClO 3 + h ν → Products. The previous recommendation for absorption cross sections was based on the work of Goodeve and Richardson [141]. Lopez and Sicre [224] have shown that the spectrum reported by Goodeve and Richardson is most likely that of Cl 2 O 6 . Thermochemical estimates by Colussi et al. [84] further corroborate this assignment. No recommendation is given at present for the ClO 3 cross sections.
Grothe and Willner (1994; 1995) have reported UV and IR spectra of ClO 3 trapped in a neon matrix. By monitoring the amount of ClO formed as a photolysis product, they estimated UV absorption cross sections of the order of 2 × 10 –18 cm 2 around 400–450 nm.

F6. Cl 2 O + h ν → Products. The preferred absorption cross sections, listed in Table 4-28, are those reported by Knauth et al. [202] at 298 K. They are in very good agreement with the cross sections measured by Lin [220] and by Molina and Molina [265]; the discrepanc y is largest at the longest wavelengths. Nee [288] has recently reported cross section measurements in the 150–200 nm wavelength region.
Sander and Friedl [357] have measured the quantum yi eld for production of O-atoms to be 0.25±0.05, using a broadband photolysis source extending from 180 nm to beyond 400 nm. The main photolysis products are Cl and ClO. Using a molecular beam technique, Nelson et al. [289] found Cl + ClO to be the primary photodissociation channel at 193, 248, and 308 nm. More recently, Nickolaisen et al . [292] reported that broadband photolysis at wavelengths beyond 300 nm results in pressure-dependent ClO quantum yields. Furthermore, these authors detected a transient ab sorption spectrum, that they assigned to a metastable triplet state of Cl 2 O; the implication is that the photodecomposition quantum yi eld is less than unity at atmospherically relevant wavelengths, in spite of the continuous nature of the absorption spectrum. Additional experimental work is needed to corroborate this interpretation.

Table 4-28. Absorption Cross Sections of Cl 2 O

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

200 71.0 330 8.40 210 23.8 340 3.58 220 8.6 350 1.54 230 28.1 360 0.73 240 103 370 0.40 250 191 380 0.36 260 195 390 0.51 270 151 400 0.79 280 126 420 1.26 290 103 440 1.11 300 71.0 460 0.63 310 40.3 480 0.32 320 19.5 500 0.22

F7. ClOOCl + h ν → Cl + ClOO. Recommended absorption cross sections in the wavelength range 190–450 nm for ClOOCl are listed in Table 4-29. The values for the wavelength range 200–360 nm are the average of experimental results reported by Cox and Hayman [ 90], DeMore and Tschuikow-Roux [107], Permien et al. [313], and Burkholder et al. [53]. For the 190–200-nm range the data are from DeMore and Tschuikow-Roux [107], these being the only data available in that range. Data at wavelengths greater than 360 nm were obtained from a linear extrapolation of the logarithm of the cross sections, using the expression log(10 20 σ (cm 2 )) = –0.01915 × λ (nm) + 7.589. For λ > 360 nm the extrapolated data are considered to be more reliable than the experimental measur ements because of the very small di mer cross sections in this region.
While the results of Cox and Hayman, DeMore and Tsc huikow-Roux, Permien et al., and Burkholder et al. are in good agreement at wavelengths below 250 nm, there are significant discrepancies at longer wavelengths, which may be attributed to uncertainties in the spectral subtraction of impurities such as Cl 2 O, Cl 2 , and Cl 2 O 2 . Huder and DeMore [167] measured ClOOCl cross s ections over the 190–310-nm range using a method that minimized the corrections required for impurities such as Cl 2 O. The cross sections from this study are significantly smaller (up to a factor of 2) than the current recommendation, particularly when extrapolated beyond 400 nm. Additional measurements are needed, par ticularly at the longer wa velengths, to check the results of Huder and DeMore.4-33 These studies also indicate that only one stable species is produced in th e recombination reaction of ClO with itself, and that this species is dichlorine peroxide, ClOOCl, rather than ClOClO. Using submillimeter wave spectroscopy, Birk et al. [34] have further established the structure of the recombination product to be ClOOCl. These observations are in agreement with the results of quantum mechan ical calculations (McGrath et al. [254,255]; Jensen and Odershede [184]; Stanton et al. [387]).

Table 4-29. Absorption Cross Sections of ClOOCl at 200–250 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 565.0 256 505.4 322 23.4 388 1.4 192 526.0 258 463.1 324 21.4 390 1.3 194 489.0 260 422.0 326 19.2 392 1.2 196 450.0 262 381.4 328 17.8 394 1.1 198 413.0 264 344.6 330 16.7 396 1.0 200 383.5 266 311.6 332 15.6 398 0.92 202 352.9 268 283.3 334 14.4 400 0.85 204 325.3 270 258.4 336 13.3 402 0.78 206 298.6 272 237.3 338 13.1 404 0.71 208 274.6 274 218.3 340 12.1 406 0.65 210 251.3 276 201.6 342 11.5 408 0.60 212 231.7 278 186.4 344 10.9 410 0.54 214 217.0 280 172.5 346 10.1 412 0.50 216 207.6 282 159.6 348 9.0 414 0.46 218 206.1 284 147.3 350 8.2 416 0.42 220 212.1 286 136.1 352 7.9 418 0.38 222 227.1 288 125.2 354 6.8 420 0.35 224 249.4 290 114.6 356 6.1 422 0.32 226 280.2 292 104.6 358 5.8 424 0.29 228 319.5 294 95.4 360 5.5 426 0.27 230 365.0 296 87.1 362 4.5 428 0.25 232 415.4 298 79.0 364 4.1 430 0.23 234 467.5 300 72.2 366 3.8 432 0.21 236 517.5 302 65.8 368 3.5 434 0.19 238 563.0 304 59.9 370 3.2 436 0.17 240 600.3 306 54.1 372 2.9 438 0.16 242 625.7 308 48.6 374 2.7 440 0.15 244 639.4 310 43.3 376 2.4 442 0.13 246 642.6 312 38.5 378 2.2 444 0.12 248 631.5 314 34.6 380 2.1 446 0.11 250 609.3 316 30.7 382 1.9 448 0.10 252 580.1 318 28.0 384 1.7 450 0.09 254 544.5 320 25.6 386 1.6

F8. Cl 2 O 3 + h ν → Products. The absorption cross sections of Cl 2 O 3 have been measured by Hayman and Cox [155], Burkholder et al. [52], and Harwood et al. [154]. The results from these studies are significantly different in the spectral regions below 240 nm and in the l ong-wavelength tail beyond 300 nm. Table 4-30 lists the recommended values. These are derived by averaging the spectra of Burkholder et al. and Harwood et al., which are obtained by the most direct methods. Additional work is needed, particularly in the spectral region beyond 300 nm.4-34 Table 4-30. Absorption Cross Sections of Cl 2 O 3

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

220 1200 275 1470 225 1130 280 1240 230 1060 285 990 235 1010 290 760 240 1020 295 560 245 1120 300 400 250 1270 305 290 255 1450 310 210 260 1610 315 160 265 1680 320 140 270 1630

F9. Cl 2 O 4 + h ν → Products. The absorption cross sections of Cl 2 O 4 have been measured by Lopez and Sicre [223]; their results are given in Table 4-31.

Table 4-31. Absorption Cross Sections of Cl 2 O 4

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

200 161 255 42 205 97 260 31 210 72 265 22 215 64 270 14 220 71 275 8.8 225 75 280 5.5 230 95 285 4.0 235 95 290 2.7 240 87 295 2.2 245 72 300 1.7 250 56 305 1.2

310 0.7

F10. Cl 2 O 6 + h ν → Products. The absorption cross sections for Cl 2 O 6 are listed in Table 4-32 and are taken from the work of Lopez and Sicre [224]. These authors show that the spectrum originally attributed to ClO 3 by Goodeve and Richardson [141] was most likely that of Cl 2 O 6 . The cross section values measured by Lopez and Sicre are several times larger than those reported by Goodeve and Richardson, but the shape of the spectrum is similar. Table 4-32. Absorption Cross Sections of Cl 2 O 6

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

200 1230 300 980 210 1290 310 715 220 1230 320 450 230 1080 330 285 240 1010 340 180 250 1010 350 112 260 1290 360 59 270 1440 370 28 280 1440 380 12 290 12904-35 F11. HCl + h ν → H + Cl. The absorption cross sections of HCl, listed in Table 4-33, are taken from the work of Inn [177].

Table 4-33. Absorption Cross Sections of HCl Vapor

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

145 281 190 14.5 150 345 195 6.18 155 382 200 2.56 160 332 205 0.983 165 248 210 0.395 170 163 215 0.137 175 109 220 0.048 180 58.8

F12. HOCl + h ν → OH + Cl. The absorption cross sections of HOCl vapor have been measured by several groups. Molina and Molina [265] and Knauth et al. [202] produced this species us ing equilibrium mixtures with Cl 2 O and H 2 O; their results provided the basis for the earlier r ecommendation. More recently, Mishalanie et al. [261] and Permien et al. [313] used a dynamic source to gene rate the HOCl vapor. The cross section values reported by Molina and Molina [265], Mishalanie et al. [261], and Permien et al. [313] are in reasonable agreement between 250 and 330 nm. In this wavelength range, the valu es reported by Knauth et al. [202] are significantly smaller, e.g., a factor of 4 at 280 nm. Beyond 340 nm, the cross sections of Mishalanie et al. are much smaller than those obtained by the other three groups. At 365 nm , the discrepancy is about an order of magnitude.
Burkholder [50] has remeasured the absorption spect rum of HOCl over the wavelength range 200 to 380 nm, following photolysis of equilibrium mixtures of Cl 2 O-H 2 O-HOCl. The obtained spectrum displays two absorption maxima at 242 and 304 nm, and is in excellent agreement with the work of Knauth et al. [202], but in poor agreement with the measurements of Mishalanie et al. [261] and Permien et al. [313]. The discrepancies can be attributed mostly to difficulties in correcting the measured absorptions for the presence of Cl 2 and Cl 2 O. In the study by Burkholder, several control experiment s were carried out in order to check the internal consistency of the data. Moreover, Barnes et al. [23] examined the near-UV spectrum of HOCl by monitoring the OH fragments resulting from photodissociation, and revealed a third weak band centered at 387 nm extending down to 480 nm. The recommended cross sections up to 420 nm, calculated from an analytical expression provided by Barnes et al. [23] and based on the values of Burkholder [50] and Barnes et al. [23], are listed in Table 4-34. The work by Jungkamp et al. [196] yields cross section values in excellent agreement with this recommendation for wavelengths shorter than 350 nm.
Molina et al. [275] observed production of OH radicals in the laser photolysis of HOCl around 310 nm, and Butler and Phillips [62] found no evidence for O-atom production at 308 nm, placing an upper limit of ~0.02 for the primary quantum yield for the HCl + O channel. Vogt and Schindler [422] used broadband photolysis in the 290–390 nm wavelength range, determining a quantum yield for OH production of >0.95.4-36 Table 4-34. Absorption Cross Sections of HOCl

λ

(nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )
200 7.18 274 5.26 348 1.55 202 6.39 276 4.94 350 1.43 204 5.81 278 4.74 352 1.33 206 5.46 280 4.64 354 1.24 208 5.37 282 4.62 356 1.17 210 5.54 284 4.68 358 1.11 212 5.98 286 4.79 360 1.06 214 6.68 288 4.95 362 1.02 216 7.63 290 5.13 364 0.985 218 8.81 292 5.33 366 0.951 220 10.2 294 5.52 368 0.919 222 11.6 296 5.71 370 0.888 224 13.2 298 5.86 372 0.855 226 14.7 300 5.99 374 0.822 228 16.2 302 6.08 376 0.786 230 17.5 304 6.12 378 0.748 232 18.7 306 6.12 380 0.708 234 19.6 308 6.07 382 0.667 236 20.2 310 5.97 384 0.624 238 20.5 312 5.84 386 0.580 240 20.6 314 5.66 388 0.535 242 20.3 316 5.45 390 0.491 244 19.8 318 5.21 392 0.447 246 19.0 320 4.95 394 0.405 248 18.1 322 4.67 396 0.364 250 17.0 324 4.38 398 0.325 252 15.8 326 4.09 400 0.288 254 14.6 328 3.79 402 0.254 256 13.3 330 3.50 404 0.222 258 12.1 332 3.21 406 0.194 260 10.9 334 2.94 406 0.168 262 9.73 336 2.68 410 0.144 264 8.68 338 2.44 412 0.124 266 7.75 340 2.22 414 0.105 268 6.94 342 2.02 416 0.089 270 6.25 344 1.84 418 0.075 272 5.69 346 1.69 420 0.063

F13. ClNO + h ν → Cl + NO. Nitrosyl chloride has a continuous absorption extending beyond 650 nm. There is good agreement between the work of Martin and Gareis [243] for the 240-to-420-nm wavelength region, of Ballash and Armstrong [20] for the 185 to 540 nm region, of Illies and Takacs [175] for the 190-to-400-nm region, and of Tyndall et al. [409] for the 190-to-350-nm region except around 230 nm, where the values of Ballash and Armstrong are larger by almost a factor of two. Roehl et al. [344] measured the absorption cross sections between 350 and 650 nm at seve ral temperatures between 223 and 343 K. Their room temperature results agree to within 15% with those of Martin and Gareis [243], Ballash and Amstrong [20], and Tyndall et al. [409]. Table 4-35 lists the recommended cross sections: these are taken from the work of Tyndall et al. [409] between 190 and 350 nm (unchanged from the previous recommendation), and from Roehl et al. [344] beyond 350 nm. The quantum yield for the primary photol ytic process has been reviewed by Calvert and Pitts [65]. It is unity over the entire visible and near-ultraviolet bands.4-37 Table 4-35. Absorption Cross Sections of ClNO

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 4320 246 45.2 302 10.3 370 11.0 192 5340 248 37.7 304 10.5 375 9.95 194 6150 250 31.7 306 10.8 380 8.86 196 6480 252 27.4 308 11.1 385 7.82 198 6310 254 23.7 310 11.5 390 6.86 200 5860 256 21.3 312 11.9 395 5.97 202 5250 258 19.0 314 12.2 400 5.13 204 4540 260 17.5 316 12.5 405 4.40 206 3840 262 16.5 318 13.0 410 3.83 208 3210 264 15.3 320 13.4 415 3.38 210 2630 266 14.4 322 13.6 420 2.89 212 2180 268 13.6 324 14.0 425 2.45 214 1760 270 12.9 326 14.3 430 2.21 216 1400 272 12.3 328 14.6 435 2.20 218 1110 274 11.8 330 14.7 440 2.20 220 896 276 11.3 332 14.9 445 2.07 222 707 278 10.7 334 15.1 450 1.87 224 552 280 10.6 336 15.3 455 1.79 226 436 282 10.2 338 15.3 460 1.95 228 339 284 9.99 340 15.2 465 2.25 230 266 286 9.84 342 15.3 470 2.50 232 212 288 9.71 344 15.1 475 2.61 234 164 290 9.64 346 15.1 480 2.53 236 120 292 9.63 348 14.9 485 2.33 238 101 294 9.69 350 14.2 490 2.07 240 82.5 296 9.71 355 13.6 495 1.78 242 67.2 298 9.89 360 12.9 500 1.50 244 55.2 300 10.0 365 12.0

F14 ClNO 2 + h ν → Products. The absorption cross sections of nitryl chloride, ClNO 2 , have been measured between 230 and 330 nm by Martin and Gareis [243], between 185 and 400 nm by I llies and Takacs [175], and between 270 and 370 nm by Nelson and Johnston [291], and by Ganske et al. [128] between 200 and 370 nm. A major source of discrepancies in the data results from the presence of impurities. Table 4-36 lists the recommended values, which are taken from Ganske et al. Nelson and Johnston [291] report a value of one (within experimental error) for the quantum yield for production of chlorine atoms; they also report a negligible quantum yield for the production of oxygen atoms.

Table 4-36. Absorption Cross Sections of ClNO 2

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 2690 290 17.3 200 468 300 14.9 210 320 310 12.1 220 339 320 8.87 230 226 330 5.84 240 133 340 3.54 250 90.6 350 2.04 260 61.3 360 1.15 270 35.3 370 0.69 280 22.04-38 F15. ClONO + h ν → Products. Measurements in the near-ultraviolet of the cross sections of chlorine nitrite (ClONO) have been made by Molina and Molina [264]. Their results are listed in Table 4-37. The characteristics of the spectrum and the instability of ClONO strongly sugge st that the quantum yield for decomposition is unity. The Cl–O bond strength is only about 20 kilocalories, so that chlorine atoms are likely photolysis products.

Table 4-37. Absorption Cross Sections of ClONO at 231 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

235 215.0 320 80.3 240 176.0 325 75.4 245 137.0 330 58.7 250 106.0 335 57.7 255 65.0 340 43.7 260 64.6 345 35.7 265 69.3 350 26.9 270 90.3 355 22.9 275 110.0 360 16.1 280 132.0 365 11.3 285 144.0 370 9.0 290 144.0 375 6.9 295 142.0 380 4.1 300 129.0 385 3.3 305 114.0 390 2.2 310 105.0 395 1.5 315 98.1 400 0.6

F16. ClONO 2 + h ν → Products. The recommended cross sections are taken from the work of Burkholder et al. [55]; the values are listed in Table 4-38, together with the parameters needed to compute their temperature dependency. These values are in very good agreement with those reported by Molina and Molina [266], which provided the basis for the previous recommendation, and which supersedes the earlier work of Rowland, Spencer, and Molina [349].
The identity of the primary phot olytic fragments has been i nvestigated by several groups. Smith et al. [384] report O + ClONO as the most likely products, using end product analysis and steady-state photolysis. The results of Chang et al. [71], who employed the very low-pressure photolysis (VLPPh) technique, indicate that the products are Cl + NO 3 . Adler-Golden and Wiesenfeld [7], using a flash photolysis atomic absorption technique, find O-atoms to be the predominant photol ysis product and report a quantum yield for Cl-atom production of less than 4%. Marinelli and Johnston [241] re port a quantum yield for NO 3 production at 249 nm between 0.45 and 0.85, with a most likely value of 0.55; they monitored NO 3 by tunable dye-laser absorption at 662 nm. Margitan [233] used atomic resonance fluorescen ce detection of O- and Cl-atoms and found the quantum yield at 266 and at 355 nm to be 0.9 ± 0.1 for Cl-atom production and ~0.1 for O-atom production, with no discernible difference at the two wavelengths. These results were confirmed by Knauth and Schindler [203], who used end-product analysis to infer the quantum yields. Burrows et al. [61] report also Cl and NO 3 as the photolysis products at 254 nm, with a quantum yield of unity within experimental error. In contrast, Nikolaisen et al. [293] report relative branching ratios of 0.44 for production of ClO and NO 2 and 0.56 for production of Cl and NO 3 at wavelengths beyond 300 nm. Minton et al. [260], Nelson et al. [290], and Moore et al. [276] measured comparable yields for these two channels at 193, 248, and 308 nm, using a molecular beam technique.
The recommended quantum yield values for production of Cl + NO 3 ( φ 1 ) and ClO + NO 2 ( φ 2 ) are given at the bottom of Table 4-38 and are based on the work of Nelson et al. [290], Moore et al. [276], Nickolaisen et al. [293], and Ravishankara [326]. For wavelengths shorter than 308 nm the value of φ 1 is 0.6, and for φ 2 it is 0.4. For longer wavelengths φ 1 increases linearly to 0.9 at 350 nm, with the corresponding decrease in φ 2 to 0.1. There is no evidence for production of O + ClONO in the more recent work; the production of O-atoms reported in some of the earlier studies might have resulted from decomposition of excited NO 3 . Recent work by Nickolaisen et al. [293] indicates that the photodissociation quantum yi eld is less than unity at wavelengths longer than about 330 nm, because of the formation of a long-lived intermediate that might be4-39 quenched under atmospheric conditions (a situation analogous to that of Cl 2 O). Additional work is needed to address these issues, which have potentia lly important atmospheric consequences.

Table 4-38. Absorption Cross Sections of ClONO 2

λ (nm) 10 20 σ(λ,296) (cm 2 ) A1 A2 λ (nm) 10 20 σ(λ,296) (cm 2 ) A1 A2

196 310 9.90 (–5) –8.38 (–6) 316 1.07 5.07 (–3) 1.56 (–5) 198 294 6.72 (–5) –8.03 (–6) 318 0.947 5.24 (–3) 1.69 (–5) 200 282 –5.34 (–6) –7.64 (–6) 320 0.831 5.40 (–3) 1.84 (–5) 202 277 –1.19 (–4) –7.45 (–6) 322 0.731 5.55 (–3) 2.00 (–5) 204 280 –2.60 (–4) –7.50 (–6) 324 0.647 5.68 (–3) 2.18 (–5) 206 288 –4.12 (–4) –7.73 (–6) 326 0.578 5.80 (–3) 2.36 (–5) 208 300 –5.62 (–4) –8.05 (–6) 328 0.518 5.88 (–3) 2.54 (–5) 210 314 –6.96 (–4) –8.41 (–6) 330 0.466 5.92 (–3) 2.70 (–5) 212 329 –8.04 (–4) –8.75 (–6) 332 0.420 5.92 (–3) 2.84 (–5) 214 339 –8.74 (–4) –9.04 (–6) 334 0.382 5.88 (–3) 2.96 (–5) 216 345 –9.03 (–4) –9.24 (–6) 336 0.351 5.80 (–3) 3.05 (–5) 218 341 –8.86 (–4) –9.35 (–6) 338 0.326 5.68 (–3) 3.10 (–5) 220 332 –8.28 (–4) –9.38 (–6) 340 0.302 5.51 (–3) 3.11 (–5) 222 314 –7.31 (–4) –9.34 (–6) 342 0.282 5.32 (–3) 3.08 (–5) 224 291 –6.04 (–4) –9.24 (–6) 344 0.264 5.07 (–3) 2.96 (–5) 226 264 –4.53 (–4) –9.06 (–6) 346 0.252 4.76 (–3) 2.74 (–5) 228 235 –2.88 (–4) –8.77 (–6) 348 0.243 4.39 (–3) 2.42 (–5) 230 208 –1.13 (–4) –8.33 (–6) 350 0.229 4.02 (–3) 2.07 (–5) 232 182 6.18 (–5) –7.74 (–6) 352 0.218 3.68 (–3) 1.76 (–5) 234 158 2.27 (–4) –7.10 (–6) 354 0.212 3.40 (–3) 1.50 (–5) 236 138 3.72 (–4) –6.52 (–6) 356 0.205 3.15 (–3) 1.27 (–5) 238 120 4.91 (–4) –6.14 (–6) 358 0.203 2.92 (–3) 1.06 (–5) 240 105 5.86 (–4) –5.98 (–6) 360 0.200 2.70 (–3) 8.59 (–6) 242 91.9 6.64 (–4) –6.04 (–6) 362 0.190 2.47 (–3) 6.38 (–6) 244 81.2 7.33 (–4) –6.27 (–6) 364 0.184 2.22 (–3) 3.66 (–6) 246 71.6 8.03 (–4) –6.51 (–6) 366 0.175 1.93 (–3) 2.42 (–7) 248 62.4 8.85 (–4) –6.59 (–6) 368 0.166 1.62 (–3) –3.62 (–6) 250 56.0 9.84 (–4) –6.40 (–6) 370 0.159 1.33 (–3) –7.40 (–6) 252 50.2 1.10 (–3) –5.93 (–6) 372 0.151 1.07 (–3) –1.07 (–5) 254 45.3 1.22 (–3) –5.33 (–6) 374 0.144 8.60 (–4) –1.33 (–5) 256 41.0 1.33 (–3) –4.73 (–6) 376 0.138 6.73 (–4) –1.54 (–5) 258 37.2 1.44 (–3) –4.22 (–6) 378 0.129 5.01 (–4) –1.74 (–5) 260 33.8 1.53 (–3) –3.79 (–6) 380 0.121 3.53 (–4) –1.91 (–5) 262 30.6 1.62 (–3) –3.37 (–6) 382 0.115 2.54 (–4) –2.05 (–5) 264 27.8 1.70 (–3) –2.94 (–6) 384 0.108 2.25 (–4) –2.11 (–5) 266 25.2 1.78 (–3) –2.48 (–6) 386 0.103 2.62 (–4) –2.11 (–5) 268 22.7 1.86 (–3) –2.00 (–6) 388 0.0970 3.33 (–4) –2.08 (–5) 270 20.5 1.94 (–3) –1.50 (–6) 390 0.0909 4.10 (–4) –2.05 (–5) 272 18.5 2.02 (–3) –1.01 (–6) 392 0.0849 5.04 (–4) –2.02 (–5) 274 16.6 2.11 (–3) –4.84 (–7) 394 0.0780 6.62 (–4) –1.94 (–5) 276 14.9 2.02 (–3) 9.02 (–8) 396 0.0740 8.95 (–4) –1.79 (–5) 278 13.3 2.29 (–3) 6.72 (–7) 398 0.0710 1.14 (–3) –1.61 (–5) 280 11.9 2.38 (–3) 1.21 (–6) 400 0.0638 1.38 (–3) –1.42 (–5) 282 10.5 2.47 (–3) 1.72 (–6) 402 0.0599 1.63 (–3) –1.20 (–5) 284 9.35 2.56 (–3) 2.21 (–6) 404 0.0568 1.96 (–3) –8.97 (–6) 286 8.26 2.66 (–3) 2.68 (–6) 406 0.0513 2.36 (–3) –5.15 (–6) 288 7.24 2.75 (–3) 3.09 (–6) 408 0.0481 2.84 (–3) –6.64 (–7) 290 6.41 2.84 (–3) 3.41 (–6) 410 0.0444 3.38 (–3) 4.47 (–6) 292 5.50 2.95 (–3) 3.74 (–6) 412 0.0413 3.96 (–3) 1.00 (–5)4-40 λ (nm) 10 20 σ(λ,296) (cm 2 ) A1 A2 λ (nm) 10 20 σ(λ,296) (cm 2 ) A1 A2

294 4.67 3.08 (–3) 4.27 (–6) 414 0.0373 4.56 (–3) 1.60 (–5) 296 4.09 3.25 (–3) 5.13 (–6) 416 0.0356 5.22 (–3) 2.28 (–5) 298 3.57 3.45 (–3) 6.23 (–6) 418 0.0317 5.96 (–3) 3.07 (–5) 300 3.13 3.64 (–3) 7.36 (–6) 420 0.0316 6.70 (–3) 3.87 (–5) 302 2.74 3.83 (–3) 8.38 (–6) 422 0.0275 7.30 (–3) 4.58 (–5) 304 2.39 4.01 (–3) 9.30 (–6) 424 0.0242 7.82 (–3) 5.22 (–5) 306 2.09 4.18 (–3) 1.02 (–5) 426 0.0222 8.41 (–3) 5.95 (–5) 308 1.83 4.36 (–3) 1.11 (–5) 428 0.0207 9.11 (–3) 6.79 (–5) 310 1.60 4.53 (–3) 1.20 (–5) 430 0.0189 9.72 (–3) 7.52 (–5) 312 1.40 4.71 (–3) 1.30 (–5) 432 0.0188 9.96 (–3) 7.81 (–5) 314 1.22 4.89 (–3) 1.42 (–5)

σ ( λ , T) = σ ( λ , 296) (1 + A 1 (T – 296) + A 2 (T – 296) 2 ); T in K
Quantum yields: ClONO 2 + h ν → Cl + NO 3 φ 1 = 0.6 ( λ < 308 nm)
φ 1 = 7.143 × 10 –3 λ (nm) – 1.60 (308 nm < λ < 364 nm)
φ 1 = 1.0 ( λ > 364 nm)

ClONO 2 + h ν → ClO + NO 2 φ 2 = 1 – φ 1
F17. CCl 4 + h ν → Products. The absorption cross sections of CCl 4 have been measured at room temperature and 110–200 nm by Russell et al. [353]; at 204–250 nm by Gordus and Bernstein [142]; at 186–226 nm by Rowland and Molina [347]; at 170–230 nm by Roxlo and Mandl [350]; and at 160–275 nm by Hubrich andStuhl [165]; at 297–477 K and 250 nm by Currie et al. [98], at 279 and 296 K and 190–252 nm by VanlaethemMeurée et al. [418]; at 225–295 K and 174–250 nm by Simon et al. [379]; and at 220–300 K and 186–240 nm by Prahlad and Kumar [319]. The room temperature data agree within 10% between 190 and 235 nm and within 20% and 40% at 240 and 250 nm (except the value at 250 nm reported by Currie et al [98], which is lower than the half of the other values). The absorption curve based on the data (reported at 0.5-nm intervals) of Prahlad and Kumar [319] shows wiggles over the whole range 186–240 nm obviously due to experimental uncertainties. In the range 180–186 nm, the values reported by Hubrich and Stuhl [165] are higher by up to 25% than those reported by Simon et al. [379], and the value at 186 nm reported by Prahlad and Kumar [319] is lower by 18% than the value of Simon et al. [379]. In the maximum near 176 nm, the absorption cross section is 1.01 × 10 –17 cm 2 , as reported by Hubrich and Stuhl [165] and Simon et al. [379], whereas the plotted spectrum reported by Roxlo and Mandl [350] shows a lower value of ~7 × 10 –18 cm 2 . For a wavelength of 313 nm, an absorption cross section of ≤ 3.7 × 10 –26 cm 2 was derived by Rebbert and Ausloos [332] from the C 2 H 5 Cl yield in the photolysis of CCl 4 -C 2 H 6 mixtures. The preferred absorption cross sections at room temperature, listed in Table 4-39, are the mean of the values reported by Hubrich and Stuhl [165] and Simon et al. [379] at 174–192 nm, the values of Simon et al. [379] at 194–250 nm, and the data of Hubrich and Stuhl [165] at 255–275 nm. The temperature dependence of the absorption cross sections becomes significant at wavelengths above 205 nm, where the cross sections decrease with decreasing temperature between 300 and 210 K as observed in good agreement by Simon et al. [379] and Prahlad and Kumar [319]. Simon et al. [379] parameterized the cross sections and the temperature dependence by the polynomial expansion

log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n

and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 194–250 nm are as follows:4-41 A 0 = –37.104 B 0 = 1.0739 A 1 = –5.8218 × 10 –1 B 1 = –1.6275 × 10 –2
A 2 = 9.9974 × 10 –3 B 2 = 8.8141 × 10 –5
A 3 = –4.6765 × 10 –5 B 3 = –1.9811 × 10 –7
A 4 = 6.8501 × 10 –8 B 4 = 1.5022 × 10 –10
Quantum yields ≥ 0.9 and ~0.75 for the photodissociative processes CCl 4 + h ν → CCl 3 + Cl at 213.9 nm and CCl 4 + h ν → CCl 2 + 2Cl at 163.3 nm, respectively, were derived from the gas-phase photolysis of CCl 4 in the presence of HCl, HBr, and C 2 H 6 by Rebbert and Ausloos [332]. A quantum yield for Cl*( 2 P 1/2 ) atom formation in the broad band photolysis of CCl 4 , Φ (Cl*) = 0.78 ± 0.27, was reported by Clark and Husain [80].

Table 4-39. Absorption Cross Sections of CCl 4 at 295–298 K
λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

174 956 204 61.0 234 2.20 176 1010 206 57.0 236 1.60 178 982.5 208 52.5 238 1.16 180 806 210 46.9 240 0.830 182 647 212 41.0 242 0.590 184 478.5 214 34.5 244 0.413 186 338.5 216 27.8 246 0.290 188 227 218 22.1 248 0.210 190 145.5 220 17.5 250 0.148 192 99.6 222 13.6 255 0.0661 194 76.7 224 10.2 260 0.0253 196 69.5 226 7.60 265 0.0126 198 68.0 228 5.65 270 0.00610 200 66.0 230 4.28 275 0.00239 202 63.8 232 3.04 Notes:
174–192 nm: mean of Hubrich and Stuhl [165] and Simon et al. [379] 194–250 nm: Simon et al. [379] 255–275 nm: Hubrich and Stuhl [165].

F18. CH 3 OCl + h ν → Products. The absorption cross sections of CH 3 OCl have been determined by Crowley et al. [96] and by Jungkamp et al. [196]. The preferred cross sections, listed in Ta ble 4-40, are the mean of the values reported by these two groups. The agreement between the two sets of m easurements is excellent at wavelengths longer than 250 nm; at the maximum near 230 nm the results of Jungkamp et al. are about 15% smaller.4-42 Table 4-40. Absorption Cross Sections of CH 3 OCl

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

230 14.9 290 1.32 350 0.662 232 15.4 292 1.34 352 0.611 234 15.7 294 1.35 354 0.574 236 15.9 296 1.37 356 0.529 238 15.8 298 1.40 358 0.482 240 15.5 300 1.43 360 0.445 242 14.9 302 1.45 362 0.411 244 14.2 304 1.47 364 0.389 246 13.2 306 1.48 366 0.356 248 12.2 308 1.49 368 0.331 250 11.1 310 1.49 370 0.298 252 9.96 312 1.48 372 0.273 254 8.86 314 1.47 374 0.246 256 7.77 316 1.46 376 0.225 258 6.80 318 1.43 378 0.209 260 5.87 320 1.41 380 0.202 262 5.05 322 1.37 382 0.186 264 4.31 324 1.33 384 0.17 266 3.69 326 1.30 386 0.16 268 3.16 328 1.24 388 0.15 270 2.71 330 1.20 390 0.13 272 2.35 332 1.14 392 0.14 274 2.06 334 1.09 394 0.13 276 1.83 336 1.04 278 1.64 338 0.980 280 1.53 340 0.918 282 1.42 342 0.875 284 1.37 344 0.822 286 1.33 346 0.760 288 1.32 348 0.709

F19. CHCl 3 + h ν → Products. The absorption cross sections of CHCl 3 have been measured at room temperature and in the far UV region at 113–182 nm by Lucazeau et al. [225]; at the Lyman- α line at 121.6 nm by Brownsword et al. [46]; and at 110–200 nm by Russell et al. [353]; at room temperature and 222.7 nm by Gordus and Bernstein [142]; at 160–255 nm by Hubrich and Stuhl [165]; at 279 and 296 K and 190–230 nm by Vanlaethem-Meurée et al. [418]; and at 225–295 K and 174–240 nm by Simon et al. [379]. The room temperature data of Vanlaethem- Meurée et al. [418] and Simon et al. [379] are identical at 190–210 nm and increasingly deviate up to ~15% at 212–240 nm. The data of Hubrich and Stuhl [165] and Simon et al. [379] agree within 10 % between 180 and 234 nm; however the values of Hubrich and Stuhl [165] become increasingly larger by up to~25% than those of Simon et al. [379] in the long-wavelength tail. In the region of the absorption maximum at ~176 nm, there is the largest spread: a cross sections of ~5 × 10 –18 cm 2 has been measured by Simon et al. [379] in contrast to values of 3.7 × 10 –18 cm 2 reported by Hubrich and Stuhl [165] and <2 × 10 –18 cm 2 given in a plot by Lucazeau et al. [225]. We therefore recommend absorption cross sections only for the region above 180 nm. The values, listed in Table 4-41, are the mean of the values reported by Hubrich and Stuhl [165] and Simon et al. [379] for the range 180–240 nm. For the range 242–256 nm, these have been extrapolated (log σ = –1.2277 – 0.0844 λ ) (in italics).
The temperature dependence of the absorption cross sections becomes significant at wavelengths above 194 nm, where the cross sections decrease with decreasing temperature between 295 and 210 K. Simon et al. [379] parameterized the cross sections and the te mperature dependence by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in4-43 stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 190–240 nm are as follows:

A 0 = 269.80 B 0 = 3.7973 A 1 = –6.0908 B 1 = –7.0913 × 10 –2
A 2 = 4.7830 × 10 –2 B 2 = 4.9397 × 10 –4
A 3 = –1.6427 × 10 –4 B 3 = –1.5226 × 10 –6
A 4 = 2.0682 × 10 –7 B 4 = 1.7555 × 10 –9 Quantum yields for H atom formation have been measured in the far UV by Brownsword et al. [46], [47]: Φ (H) = 0.23 ± 0.03 and 0.13 at 121.6 and 157.6 nm, respectively, whereas H atoms could not be detected in the photolysis at 193.3 nm.

Table 4-41. Absorption Cross Sections of CHCl 3 at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

180 372 206 20.7 232 0.158 182 317 208 15.1 234 0.107 184 248 210 10.7 236 0.0730 186 186 212 7.48 238 0.0503 188 144 214 5.24 240 0.0347 190 113 216 3.60 242 0.0223 192 89.9 218 2.48 244 0.0151 194 76.1 220 1.69 246 0.01023 196 64.2 222 1.13 248 0.00694 198 53.0 224 0.750 250 0.00470 200 42.6 226 0.503 252 0.00319 202 34.4 228 0.342 254 0.00216 204 27.2 230 0.234 256 0.00147 Note: 180–240 nm: mean of Hubrich and Stuhl [165] and Simon et al. [379] 242–256 nm: extrapolation of mean of Hubrich and Stuhl [165] and Simon et al. [379] data.

F20. CH 2 Cl 2 + h ν → Products. The absorption cross sections of CH 2 Cl 2 have been measured at room temperature and 110–200 nm by Russell et al. [353]; at the Lyman- α line at 121.6 nm by Brownsword et al. [46]; at 213 nm by Gordus and Bernstein [142], at 160–255 nm by Hubrich and Stuhl [165]; at 279 and 296 K and 176–216 nm by Vanlaethem-Meurée et al. [418]; and at 225–295 K and 176–220 nm by Simon et al. [379]. The room temperature data of Vanlaethem-Meurée et al. [418] and Simon et al. [379] are nearly identical. The data of Hubrich and Stuhl [165] agree with those of Simon et al. [379] within 12% at 176–206 nm and become increaseingly larger at 185–220 nm by up to 50%. The preferred absorption cross sections, listed in Table 4-42, are the mean of the values reported by Hubrich and Stuhl [165] and Simon et al. [379] at 176–220 nm. For wavelengths above 220 nm, the average of their data at 200–210 nm has been extrapolated (log σ = –2.1337 – 0.08439 λ ) (in italics) at wavelengths up to 256 nm. The measured values of Hubrich and Stuhl [165] are smaller by up to 7% below 230 nm and become larger by up to 50% between 235 and 255 nm than the extrapolated values.
The temperature dependence of the absorption cross sections becomes significant at wavelengths above 190 nm, where the cross sections decrease with decreasing temperature between 295 and 210 K. Simon et al. [379] parameterized the cross sections and the temp erature dependence by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 176–220 nm are as follows:

A 0 = –1431.8 B 0 = –3.1171 A 1 = 27.395 B 1 = 6.7874 × 10 –2
A 2 = –1.9807 × 10 –1 B 2 = –5.5000 × 10 –4
A 3 = 6.3468 × 10 –4 B 3 = 1.9649 × 10 –6
A 4 = –7.6298 × 10 –7 B 4 = –2.6101 × 10 –94-44 Quantum yields for H atom formation have been measured in the far UV by Brownsword et al. [46], [47]: Φ (H) = 0.28 ± 0.03, 0.23, and 0.002 ± 0.001 at 121.6, 157.6, and 193.3 nm, respectively.

Table 4-42. Absorption Cross Sections of CH 2 Cl 2 at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

176 186 204 4.41 232 0.0194 178 182 206 3.07 234 0.0132 180 173 208 2.13 236 0.00892 182 156 210 1.45 238 0.00605 184 135 212 0.978 240 0.00410 186 110 214 0.651 242 0.00278 188 84.2 216 0.435 244 0.00188 190 61.0 218 0.291 246 0.00128 192 43.9 220 0.190 248 0.000866 194 30.5 222 0.135 250 0.000587 196 20.6 224 0.0918 252 0.000398 198 14.1 226 0.0623 254 0.000270 200 9.48 228 0.0422 256 0.000183 202 6.40 230 0.0286 Note: 176–220 nm: mean of Hubrich and Stuhl [165] and Simon et al. [379] 222–256 nm: extrapolation of mean of Hubrich and Stuhl [165] and Simon et al. [379] data.

F21. CH 3 Cl + h ν → Products. The absorption cross sections of CH 3 Cl have been measured at room temperature and 110–200 nm by Russell et al. [353]; at the Lyman- α line at 121.6 nm by Brownsword et al. [46]; at 171.2 nm by Felps et al. [119]; and at 174–220 nm by Robbins [338]; at 208 and 298 K and 158–235 nm by Hubrich et al. [166]; at 255, 279, and 296 K and 186–216 nm by Vanlaethem-Meurée et al. [418]; and at 225–295 K and 174–216 nm by Simon et al. [379]. The room temperature data generally agree within 10% in the wavelength range 174–216 nm, those of Vanlaethem-Meurée et al. [418] and Simon et al. [379] are nearly identical. The value at 171 nm of Felps et al. [47] is smaller by ~15% than that of Hubrich et al. [166]. The preferred absorption cross sections, listed in4-45 Table 4-43, are the mean of the values reported by Robbins [338], Hubrich et al. [166], and Simon et al. [379] at 174–184 nm, the mean of the values reported by Robbins [338], Hubrich et al. [166], Vanlaethem-Meurée et al. [418], and Simon et al. [379] at 186–216 nm, and the mean of the values reported by Robbins [338] and Hubrich et al. [166] at 218–220 nm. The values for th e wavelength range 222–236 nm have been taken from an interpolation (at 2-nm intervals) of the 200–235-nm data of Hubrich et al. [166] (log σ = –0.24164 – 0.09743 λ ).
The temperature dependence of the absorption cross sections becomes significant at wavelengths above 194 nm, where the cross sections decrease with decreasing temperature between 295 and 210 K. There is very good agreement between the low-temperature values at 250–255 K of Vanlaethem-Meurée et al. [418] and Simon et al. [379]. The latter authors parameterized the cross sections and the temperature dependence by the polynomial expansion log 10 σ ( λ , T) = Σ A n λ n + (T – 273) × Σ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths correspondi ng to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ

= 174–216 nm are as follows: A 0 = –299.80 B 0 = –7.1727

A 1 = 5.1047 B 1 = 1.4837 × 10 –1

A 2 = –3.3630 × 10 –2 B 2 = –1.1463 × 10 –3

A 3 = 95805 × 10 –5 B 3 = 3.9188 × 10 –6

A 4 = –1.0135 × 10 –7 B 4 = –4.9994 × 10 –9

Quantum yields for H atom formation have been measured in the far UV by Brownsword et al. [46], [47]: Φ (H) = 0.53 ± 0.05 ̧ 0.29, 0.012 ± 0.006 at 121.6, 157.6, and 193.3 nm, respectively.4-46 Table 4-43. Absorption Cross Sections of CH 3 Cl at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

174 110 196 3.96 218 0.0345 176 93.9 198 2.68 220 0.0220 178 78.2 200 1.77 222 0.0135 180 63.6 202 1.13 224 0.00859 182 46.5 204 0.731 226 0.00549 184 35.0 206 0.482 228 0.00350 186 25.8 208 0.313 230 0.00224 188 18.4 210 0.200 232 0.00143 190 12.8 212 0.127 234 0.000911 192 8.84 214 0.0860 236 0.000582 194 5.83 216 0.0534

Note:
174–184 nm: mean of Robbins [338], Hubrich et al. [166], and Simon et al. [379]
186–216 nm: mean of Robbins [338], Hubrich et al. [166], Vanlaethem-Meurée et al. [418] and Simon et al. [379]
218–220 nm: mean of Robbins [338] and Hubrich et al. [166]
222–236 nm: extrapolation of Hubrich et al. [166] data.

F22. CH 3 CCl 3 + h ν → Products. The absorption cross sections of CH 3 CCl 3 have been measured at room temperature and 147 nm by Salomon et al. [355], and at 160–255 nm by Hubrich and Stuhl [165], who corrected (<10.7%) the absorption cross sections in the range 170–190 nm for the concentration and absorption cross sections of a 1,4-dioxane stabilizer present during the experi ments. Measurements at 220–295 K and 182–240 nm were carried out by Vanlaethem-Meurée et al. [420] and at 223–333 K and 160 240 nm by Nayak et al. [287]. The latter authors also measured the absorption cross sections in the liquid phase at 235–260 nm and used a wavelength-shift procedure to convert the liquid-phase da ta into gas-phase data. The agreement of the room temperature data is within 20% at 165–205 nm (at 160 nm, the value reported by Nayak et al. [287] is larger by 50% than that reported by Hubrich and Stuhl [165]). Between 210 and 240 nm, the data of Vanlaethem-Meurée et al. [420] and Nayak et al. [287] are within 15%, whereas those of Hubrich and Stuhl [165] are larger by 100– 150%. The preferred absorption cross sections, listed in Table 4-44, are the mean of the values reported by Hubrich and Stuhl [165] and Nayak et al. [287] at 170–180 nm, the mean of the values reported by Vanlaethem-Meurée et al. [420], Hubrich and Stuhl [165], and Nayak et al. [287] at 185–205 nm, and the mean of the values reported by Vanlaethem-Meurée et al. [420] and Nayak et al. [287] at 210–240 nm. For wavelengths above 240 nm, the average of their data at 220–240 nm has been extrapolated (log σ = –1.59792 – 0.08066 λ ) at wavelengths up to 255 nm. The measured values of Hubrich and Stuhl [165] are larger by up to ~140% at 250 nm and smaller by ~80% at 255 nm than the recommended values.
The temperature dependence of the absorption cross sections becomes significant at wavelengths above 210 nm, where the cross sections decrease with decreas ing temperature, as observed in good agreement at 333– 223 K by Nayak et al. [287] and at 295–210 K by Vanlaethem-Meurée et al. [420]. The latter authors parameterized the cross sections and the temper ature dependence by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumbe r intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 182–240 nm reported by Gillotay and Simon [138] are as follows:

A 0 = 341.085191 B 0 = –1.660090 A 1 = –7.273362 B 1 = 3.079969 × 10 –2
A 2 = 5.498387 × 10 –2 B 2 = –2.106719 × 10 –4
A 3 = –1.827552 × 10 –4 B 3 = 6.264984 × 10 –7
A 4 = 2.238640 × 10 –7 B 4 = –6.781342 × 10 –104-47 Table 4-44. Absorption Cross Sections of CH 3 CCl 3 at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 406 200 92.1 230 0.717 175 424 205 52.0 235 0.276 180 404 210 25.5 240 0.111 185 301 215 10.9 245 0.0437 190 212 220 4.47 250 0.0173 195 147 225 1.82 255 0.00682 Note: 170–180 nm: mean of Hubrich and Stuhl [165] and Nayak et al. [287] 185–205 nm: mean of Vanlaethem-Meurée et al. [420], Hubrich and Stuhl [165] and Nayak et al. [287] 210–240 nm: mean of Vanlaethem-Meurée et al. [420] and Nayak et al. [287] 245–255 nm: extrapolation of mean of Vanlaethem-Meurée et al. [420] and Nayak et al. [287] data.

F23. CH 3 H 2 Cl + h ν → Products. The absorption cross sections of CH 3 CH 2 Cl have been measured at room temperature and 147 nm by Ichimura et al. [173] and at 160–240 nm by Hubrich and Stuhl [165]. The data of Hubrich and Stuhl [165] are listed in Table 4-45.

Table 4-45. Absorption Cross Sections of CH 3 CH 2 Cl at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

160 189.0 190 6.85 220 0.0127 165 110.0 195 2.56 225 0.00463 170 70.5 200 1.17 230 0.00117 175 44.4 205 0.375 235 0.000395 180 30.4 210 0.147 240 0.000156 185 13.6 215 0.0433 Note: 160–240 nm, Hubrich and Stuhl [165].

F24. CH 3 CHClCH 3 + h ν → Products. In a compilation of ultraviolet absorption cross sections of halocarbons by Gillotay and Simon [355] results are reported for (erroneously) CH 3 CH 2 ClCH 3 , which presumably should be CH 3 CHClCH 3 . The data are listed in Table 4-46.4-48 Table 4-46. Absorption Cross Sections of CH 3 CHClCH 3 at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 31.7 192 4.67 214 0.0965 172 27.0 194 3.49 216 0.0652 174 24.3 196 2.58 218 0.0444 176 22.1 198 1.88 220 0.0308 178 20.3 200 1.34 222 0.0212 180 18.0 202 0.954 224 0.0144 182 15.0 204 0.671 226 0.0107 184 12.2 206 0.463 228 0.00752 186 9.99 208 0.311 230 0.00580 188 7.93 210 0.214 190 6.06 212 0.144

Note : 170–230 nm, Gillotay and Simon [138].

F25. CH 2 ClCH 2 Cl + h ν → Products.

F26. CH 2 ClCH 2 CH 2 Cl + h ν → Products.

F27. CH 2 Cl(CH 2 ) 2 CH 2 Cl + h ν → Products.
Absorption cross sections for these three dichloroalkanes at room temperature and 118–200 nm have been reported by Russell et al. [353].

F28. CCl 2 O + h ν → Products. See note for CF 2 O + h ν (Note E5).

F29. CClFO + h ν → Products. See note for CF 2 O + h ν (Note E5).

F30. CFCl 3 (CFC-11) + h ν → Products. The absorption cross sections of CFCl 3 have been measured at room temperature and 225 nm by Gordus and Bernstein [142], at 186–226 nm by Rowland and Molina [347], at 174– 226 nm by Robbins and Stolarski [339], at 186–209 nm by Greene and Wayne [146]; at 213–296 K and 185– 226 nm by Chou et al. [78]; at 208 and 298 K and 158–260 nm by Hubrich et al. [166] and Hubrich and Stuhl [165]; at 255, 279, and 296 K and 190–220 nm by Vanlaethem-Meurée et al. [419]; at 225–295 K and 174– 230 nm by Simon et al. [379]; and at 220, 240, and 296 K and 200–238 nm by Mérienne et al. [256]. The room temperature data are in good agreement, generally within 10–15%. Absorption cross sections at 148–225 nm have also been derived from electron energy-loss measurements by Huebner et al. [171], which are up to 30% higher than the values obtained by optical measurements. The preferred absorption cross sections, listed in Table 4-47, are the values of Simon et al. [379] at 174–198 nm, the mean of the values reported by Simon et al. [379] and Mérienne et al. [256] at 200–230 nm, and the data of Hubrich and Stuhl [165] at 235–260 nm. Measurements in the far UV at 60–145 nm have been reported by Gilbert et al. [132], and at 120–200 nm by Doucet et al. [110].
The temperature dependence becomes significant at wavelengths above 185 nm, where the cross sections decrease with decreasing temperature between 296 and 210 K (Hubrich et al. [166] observed such a behavior only above 200 nm). Simon et al. [379] parameterized the temperature dependence of the cross sections by the polynomial expansion log 10 σ ( λ , T) = Σ A n λ n + (T – 273) × Σ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wave lengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 174–230 nm are as follows:

A 0 =–84.611 B 0 = –5.7912 A 1 = 7.9551 × 10 –1 B 1 = 1.1689 × 10 –1
A 2 = –2.0550 × 10 –3 B 2 = –8.8069 × 10 –4
A 3 = –4.4812 × 10 –6 B 3 = 2.9335 × 10 –6
A 4 = 1.5838 × 10 –8 B 4 = –3.6421 × 10 –9

A similar polynomial expansion, log 10 σ ( λ , T) = Σ a n ( λ – 200) n + (T – 296) × Σ b n ( λ – 200) n , for the ranges T = 220–296 K and λ = 200–238 nm was used by Mérienne et al. [256] with the following parameters a n and b n :4-49 a 0 = –41.925548 b 0 = 3.58977 × 10 –4

a 1 = –1.142857 × 10 –1 b 1 = 3.02973 × 10 –4

a 2 = –3.12034 × 10 –3 b 2 = –1.13 × 10 –8

a 3 = 3.6699 × 10 –5

A quantum yield for Cl*( 2 P 1/2 ) atom formation in the broad band photolysis of CFCl 3 , Φ (Cl*) = 0.79 ± 0.27, was reported by Clark and Husain [80].

Table 4-47. Absorption Cross Sections of CFCl 3 at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

174 313.0 198 78.0 222 1.72 176 324.0 200 63.2 224 1.17 178 323.5 202 49.1 226 0.790 180 314.0 204 37.3 228 0.532 182 296.0 206 28.1 230 0.354 184 272.0 208 20.4 235 0.132 186 243.0 210 15.1 240 0.0470 188 213.0 212 10.7 245 0.0174 190 179.0 214 7.54 250 0.0066 192 154.0 216 5.25 255 0.0029 194 124.3 218 3.65 260 0.0015 196 99.1 220 2.51

Note : 174–198 nm: Simon et al. [379] 200–230 nm: mean of Simon et al. [379] and Mérienne et al. [256] 235–260 nm: Hubrich and Stuhl [165].

F31. CF 2 Cl 2 (CFC-12) + h ν → Products. The absorption cross sections of CF 2 Cl 2 have been measured at room temperature and 210 nm by Gordus and Bernstein [142], at 186–216 nm by Rowland and Molina [347], at 174– 216 nm by Robbins and Stolarski [339], at 186–206 nm by Greene and Wayne [146]; at 234–442 K and 213.9 nm by Rebbert and Ausloos [333]; at 212, 252, and 296 K and 184–221 nm by Chou et al. [78]; at 208 and 298 K and 159–240 nm by Hubrich et al. [166]; at 255, 279, and 296 K and 190–216 nm by Vanlaethem-Meurée et al. [419]; at 225–295 K and 174–230 nm by Simon et al. [379]; and at 220, 240, and 296 K and 200–231 nm by Mérienne et al. [256]. The room temperature data are in good agreement, generally within 10–15%, except the data of Green and Wayne [146] above 195 nm and the data of Rowland and Molina [347] around 210 nm. Absorption cross sections at 148–218 nm have also been derived from electron energy-loss measurements by Huebner et al. [171], which agree within 10% with the data obtained by optical measurements around the absorption maximum and become higher than the optical data by up to 100% above 196 nm. The preferred absorption cross sections, listed in Table 4-51, are the values of Hubrich et al. [166] at 170–172 nm, the mean of the values reported by Hubrich et al. [166] and Simon et al. [379] at 174–178 nm, the values of Simon et al. [379] at 180–198 nm, the mean of the values reported by Simon et al. [379] and Mérienne et al. [256] at 200– 226 nm, and the data of Mérienne et al. [256] at 228–230 nm. For the range 232–240 nm, the absorption curve above 210 nm of Mérienne et al. [256] has been extrapolated (log σ = 2.1448 – 0.1061 λ ). The measured values of Hubrich et al. [166] are lower by up to ~40% at 240 nm than the extrapolated values.
High-resolution absorption cross section measurements ha ve been carried out by S eccombe et al. [369] between 50 and 150 nm, and by Limao-Vieira et al. [219] betw een 113 and 225 nm using a synchrotron radiation light source. The results of Limao-Vieira et al. for the absorption band at 170–204 nm are in very good agreement with the recommendation in Table 4-48 (at wavelengths above 204 nm, noise effects become significant). The new cross section measurements for the far UV regi on from both recent studies si gnificantly improve upon the earlier data of Gilbert et al. [132] for the wavelength range 60–135 nm and of Doucet et al. [110] for the wavelength range 120–200 nm.
The temperature dependence becomes significant at wavelengths above 186 nm, where the cross sections decrease with decreasing temperature between 296 and 210 K. Simon et al. [379] parameterized the temperature dependence of the cross sections by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273)

× ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths4-50 corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 174–226 nm are as follows:

A 0 =–711.02 B 0 = 6.1648 A 1 = 12.490 B 1 = –1.2093 × 10 –1
A 2 = –8.2865 × 10 –2 B 2 = 8.8587 × 10 –4
A 3 = 2.4091 × 10 –4 B 3 = –2.8743 × 10 –6
A 4 = –2.6113 × 10 –7 B 4 = 3.4904 × 10 –9

A similar polynomial expansion, log 10 σ ( λ , T) = ∑ a n ( λ – 200) n + (T – 296) × ∑ b n ( λ – 200) n , for the ranges T = 220–296 K and λ = 200–231 nm was used by Mérienne et al. [256] with the following parameters a n and b n :

a 0 = –43.8954569 b 0 = 4.8438 × 10 –3

a 1 = –2.403597 × 10 –1 b 1 = 4.96145 × 10 –4

a 2 = –4.2619 × 10 –4 b 2 = –5.6953 × 10 –6

a 3 = 9.8743 × 10 –6

A quantum yield for Cl*( 2 P 1/2 ) atom formation in the broad band photolysis of CF 2 Cl 2 , Φ (Cl*) = 0.75 ± 0.26, was reported by Clark and Husain [80]. Table 4-48. Absorption Cross Sections of CF 2 Cl 2 at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 124.0 194 31.5 218 0.103 172 151.0 196 21.1 220 0.0624 174 168.0 198 13.9 222 0.0381 176 185.5 200 8.71 224 0.0233 178 189.5 202 5.42 226 0.0140 180 179.0 204 3.37 228 0.0090 182 160.0 206 2.06 230 0.0057 184 134.0 208 1.26 232 0.0034 186 107.0 210 0.762 234 0.0021 188 82.8 212 0.458 236 0.0013 190 63.2 214 0.274 238 0.0008 192 45.50 216 0.163 240 0.0005

Note : 170–172 nm, Hubrich et al. [166], 174–178 nm, the mean of Hubrich et al. [166] and Simon et al. [379], 180–198 nm, Simon et al. [379], 200–230 nm, mean of Simon et al. [379] and Mérienne et al. [256], 232–240 nm, extrapolation of Mérienne et al. [256] data.

F32. CF 3 Cl (CFC-13) + h ν → Products. The absorption cross sections of CF 3 Cl have been measured at roomtemperature and 184–203 nm by Chou et al. [77]; at 255, 279, and 296 K and 172–200 nm by VanlaethemMeurée et al. [419]; at 208 and 298 K and 160–220 nm by Hubrich and Stuhl [165]; and at 225–295 K and 172–200 nm by Simon et al. [379]. The values of Vanlaethem-Meurée et al. [419] and Simon et al. [379] are identical, the room temperature values of Hubrich and Stuhl [165] deviate from the latter by up to about ±25%, and the data of Chou et al. [77] are always larger by about 15–30% in the region 185–200 nm. The recommended absorption cross sections for CF 3 Cl, presented in Table 4-49, are taken from Simon et al. [379] for the range 172–200 nm. The values at 202–220 nm are obtained by extrapolation of the absorption curve above 200 nm (log σ = –5.048 – 0.0834 λ ) of Simon et al. [379].
Measurements in the far UV at 65–130 nm have been reported by Gilbert et al. [132] and at 120–160 nm by Doucet et al. [110]. Measurements at the Lyman- α line at 121.6 nm have been carried out by Ravishankara et al. [328].
Temperature effects, if any, could not be detected by Vanlaethem-Meurée et al. [419] and Simon et al. [379], whereas Hubrich and Stuhl [165] report a decrease of the absorption cross sections between 298 and 208 K by4-51 4% at160 nm to 74% at 205 nm. Simon et al. [379] parameterized the cross sections and the temperature dependence of the absorption cross sections by the polynomial expansion
log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n (with all B n = 0),
and reported smoothed values for T = 295 K, ever y 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratosphe ric photodissociation calculations. The parameters A n for the ranges T = 210–300 K and λ = 172–200 nm are:

A 0 =–1.55.88, A 1 = 2.0993, A 2 = –1.0486 × 10 –2 , A 3 = 1.6718 × 10 –5

. A quantum yield for Cl*( 2 P 1/2 ) atom formation in the broad band photolysis of CF 3 Cl, Φ (Cl*) = 0.86 ± 0.29, was reported by Clark and Husain [80].
Table 4-49. Absorption Cross Sections of CF 3 Cl at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

172 1.100 190 0.128 206 0.00595 174 0.970 192 0.0900 208 0.00406 176 0.825 194 0.0610 210 0.00276 178 0.681 196 0.0410 212 0.00188 180 0.542 198 0.0280 214 0.00128 182 0.425 200 0.0190 216 0.000872 184 0.326 200 0.0189 218 0.000594 186 0.244 202 0.0128 220 0.000405 188 0.175 204 0.00874 Note: 172–200 nm, Simon et al. [379], 202–220 nm, extrapolation of Simon et al. [379] data.

F33. CF 2 ClCFCl 2 (CFC-113) + h ν → Products. The absorption cross sections of CF 2 ClCFCl 2 have been measured at 298 K and 184–224 nm by Chou et al. [77]; at 208 and 298 K and 160–250 nm by Hubrich and Stuhl [165]; and at 225–295 K and 184–230 nm by Simon et al. [380]. The room temperature values agree within about 10% except in the region around 190 nm where the values of Hubrich and Stuhl [165] are smaller by up to 20 % than the other values. The preferred absorption cross sections, listed in Table 4-50, are the values of Hubrich and Stuhl [165] at 175–180 nm, a value at 184 nm interpolated between those of Hubrich and Stuhl [165] at 180 nm and Simon et al. [380] at 186 nm, and the values of Simon et al. [380] at 186–230 nm. For the range 232–250 nm, the absorption curve of Simon et al. [380] above 230 nm has been extrapolated (log σ = –0.9860 – 0.0894 λ ). The measured values of Hubrich and Stuhl [165] are larger than the extrapolated values by ~20–80% at 232–250 nm.
Measurements in the far UV at 110–200 nm have been carried out by Doucet et al. [111].
The temperature dependence becomes significant at wa velengths above 194 nm and below 170 nm, where the cross sections decrease with decreasing temperature. This was observed by Simon et al. [380] at 295–225 K and by Hubrich and Stuhl [165] at 298 and 208 K. Simon et al. [380] parameterized the temperature dependence of the cross sections by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 182–230 nm are as follows:

A 0 =–1087.9 B 0 = 12.493 A 1 = 20.004 B 1 = –2.3937 × 10 –1
A 2 = –1.3920 × 10 –1 B 2 = 1.7142 × 10 –3
A 3 = 4.2828 × 10 –4 B 3 = –5.4393 × 10 –6
A 4 = –4.9384 × 10 –7 B 4 = 6.4548 × 10 –8

.4-52 Table 4-50. Absorption Cross Sections of CF 2 ClCFCl 2 at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

175 192 204 5.80 228 0.0410 180 155 206 4.00 230 0.0270 184 123 208 2.65 232 0.0188 186 104 210 1.80 234 0.0124 188 83.5 212 1.15 236 0.00824 190 64.5 214 0.760 238 0.00546 192 48.8 216 0.505 240 0.00361 194 36.0 218 0.318 242 0.00239 196 26.0 220 0.220 244 0.00159 198 18.3 222 0.145 246 0.00105 200 12.5 224 0.0950 248 0.000696 202 8.60 226 0.0630 250 0.000461 Note : 175–180 nm: Hubrich and Stuhl [165] 184 nm: interpolation: Hubrich and Stuhl (180 nm) and Simon et al. (186 nm) 186–230 nm: Simon et al. [380] 232–250 nm: extrapolation of Simon et al. [380] data.

F34. CF 2 ClCF 2 Cl (CFC-114) + h ν → Products. The absorption cross sections of CF 2 ClCF 2 Cl have been measured at room temperature and 184–219 nm by Chou et al. [77]; at 208 and 298 K and 160–235 nm by Hubrich and Stuhl [165]; and at 225–295 K and 182–220 nm by Simon et al. [380]. The room temperature values of Simon et al. [380] and Chou et al. [77] agree within 5% except for a hump around 195 nm in the absorption curve reported by Chou et al. [77]. The values of Hubrich and Stuhl [165] are always larger than those of Simon et al. [380], around 190 nm by up to ~40% and between 200 a nd 220 nm up to ~50% with increasing wavelength. The recommended absorption cross sections, listed in Table 4-51, are the values of Simon et al. [380] at 172– 220 nm. For the range 222–235 nm, the absorption curve above 200 nm of Simon et al. [380] has been extrapolated (log σ = –1.8233 – 0.00913 λ ). The measured values of Hubrich et al. [165] are larger by ~40% in that range than the extrapolated values
Measurements at the Lyman- α line at 121.6 nm have been carried out by Ravishankara et al. [328]; and at 110– 190 nm by Doucet et al. [111].
The temperature dependence has been observed at wave lengths above 190 nm, where Simon et al. [380] report decreasing cross sections with decreasing temperature 295–210 K. Hubrich and Stuhl [165] report for the range 160–210 nm and between 298 and 208 K a small decrease of the cross sections (generally <10%, except two data points). Simon et al. [380] parameterized the temperature dependence of the cross sections by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wave lengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K, λ = 172–220 nm are as follows:

A 0 = –160.50 B 0 = –1.5296 A 1 = 2.4807 B 1 = 3.5248 × 10 –2
A 2 = –1.5202 × 10 –2 B 2 = –2.9951 × 10 –4
A 3 = 3.8412 × 10 –5 B 3 = 1.1129 × 10 –6
A 4 = –3.4373 × 10 –8 B 4 = –1.5259 × 10 –94-53 Table 4-51. Absorption Cross Sections of CF 2 ClCF 2 Cl at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

172 69.0 194 2.56 216 0.0290 174 55.0 196 1.75 218 0.0190 176 43.0 198 1.20 220 0.0122 178 34.0 200 0.800 222 0.00809 180 26.2 202 0.540 224 0.00531 182 19.8 204 0.370 226 0.00349 184 15.0 206 0.245 228 0.00229 186 11.0 208 0.160 230 0.00151 188 7.80 210 0.104 232 0.00099 190 5.35 212 0.0680 234 0.00065 192 3.70 214 0.0440 235 0.00053 Note : 172–220 nm: Simon et al. [380] 222–235 nm: extrapolation of Simon et al. [380] data.

F35. CF 3 CF 2 Cl (CFC-115) + h ν → Products. The absorption cross sections of CF 3 CF 2 Cl have been measured at room temperature and 184–207 nm by Chou et al. [77]; at 208 and 298 K and 160–230 nm by Hubrich and Stuhl [165]; and at 225–295 K and 172–204 nm by Simon et al. [380]. The room temperature data of Simon et al. [380] and Hubrich and Stuhl [165] agree within ~20%, where Hubrich and Stuhl [165] report the larger values over the range 172–204 nm. The data of Chou et al. [77] are larger by up to more than 50% than those of Simon et al. [380]. The preferred absorption cross sections, listed in Table 4-52, are the mean of the values reported by Hubrich and Stuhl [165] and Simon et al. [380] at 172–204 nm. The mean of the values measured by Hubrich and Stuhl [165] and those obtained by extrapolating the absorption curve of Simon et al. [380] (log

σ = –6.2191 – 0.0756 λ ) were taken for the range 205–230 nm (the extr apolated values become larger by up to nearly 50% with increasing wavelength than the measured values of Hubrich and Stuhl [165]).
Measurements at the Lyman- α line at 121.6 nm have been carried out by Ravishankara et al. [328]; and at 120– 175 nm by Doucet et al. [111].
Temperature effects, if any, could not be detected for this highly fluorinated species. Simon et al. [380] parameterized the absorption cross sections by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273)

× ∑ B n λ n (with all B n = 0), and reported smoothed values for T = 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n for the ranges T = 210–300 K and λ = 172–204 nm are

A 0 = 5.8281, A 1 = 2.900 × 10 –1 , A 2 = 1.325 × 10 –3 , A 3 = –2.6851 × 10 –6

.

Table 4-52. Absorption Cross Sections of CF 3 CF 2 Cl at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

172 5.50 188 0.403 204 0.0218 174 4.13 190 0.287 205 0.0187 176 3.08 192 0.203 210 0.00700 178 2.25 194 0.143 215 0.00273 180 1.58 196 0.0985 220 0.00107 182 1.13 198 0.0685 225 0.00046 184 0.790 200 0.0474 230 0.00018 186 0.563 202 0.0325 Note : 172–204 nm: mean of Hubrich and Stuhl [165] and Simon et al. [380] 205–230 nm: mean of Hubrich and Stuhl [165] and extrapolated Simon et al. [380] data.

F36. CHFCl 2 (HCFC-21) + h ν → Products. The absorption cross sections of CHFCl 2 have been measured at room temperature and 208 nm by Gordus and Bernstein [142]; at 174–222 nm by Robbins and Stolarski [339]; at 184–205 nm by and Green and Wayne [146]; and at 213.9 nm by Rebbert et al. [335]; at 208 and 298 K and 158–235 nm by Hubrich et al. [166]; and at 225–295 K and 174–222 nm by Simon et al. [379]. The results of4-54 these groups (except those of Green and Wayne [146] which deviate strongly) are in good agreement, generally within 15%, although the data of Hubrich et al. [166] show humps around 205 and 220 nm, where the agreement is only ~40%. The preferred absorption cross sections, listed in Table 4-53, are the values of Simon et al. [379] at 174–222 nm. For the range 224–236 nm, the absorption curve above 200 nm of Simon et al. 283] has been extrapolated (log σ = 0.9806 – 0.1014 λ ). The measured values of Hubrich et al. [166] deviate from the extrapolated values by up to ~–20% and +50%.
Measurements in the far UV at 60–120 nm have been reported by Gilbert et al. [132], measurements at 120– 200 nm by Doucet et al. [110], and a measurement at 147 nm by Rebbert et al. [335].
The temperature dependence becomes significant at wavelengths above 190 nm, where the cross sections decrease with decreasing temperature between 296 and 210 K. Simon et al. [379] parameterized the temperature dependence of the cross sections by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273)

× ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 174–222 nm are as follows:

A 0 = –514.56 B 0 = –3.0577 A 1 = 8.7940 B 1 = 6.6539 × 10 –2
A 2 = –5.6840 × 10 –2 B 2 = –5.3964 × 10 –4
A 3 = 1.5894 × 10 –4 B 3 = 1.9322 × 10 –6
A 4 = 1.6345 × 10 –7

Table 4-53. Absorption Cross Sections of CHFCl 2 at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )
174 166.0 198 8.10 222 0.0319 176 164.5 200 5.24 224 0.0195 178 155.0 202 3.35 225 0.0154 180 138.0 204 2.12 226 0.0122 182 116.0 206 1.34 228 0.00766 184 92.4 208 0.836 230 0.00480 186 71.5 210 0.522 232 0.00301 188 53.2 212 0.325 234 0.00189 190 38.4 214 0.203 235 0.00150 192 26.9 216 0.127 236 0.00119 194 18.4 218 0.0797 196 12.3 220 0.0503 Note : 174–222 nm: Simon et al. [379] 224–236 nm: extrapolation of Simon et al. [379] data.

F37. CHF 2 Cl (HCFC-22) + h ν → Products. The absorption cross sections of CHF 2 Cl have been measured at room temperature and 174–202 nm by Robbins and Stolarski [339] and at 181–194 nm by Green and Wayne [146]; at 208 K and 298 K and 158–220 nm by Hubrich et al. [166], and at 225–295 K and 174–204 nm by Simon et al. [379]. The results of Robbins and Stolarski [339], Hubrich et al. [166], and Simon et al. [379] are in good agreement generally within 15–20%, however those of Green and Wayne [146] deviate strongly. The preferred absorption cross sections, listed in Table 4-54, are the values of Hubrich et al. [166] at 170–172 nm and the values of Simon et al. [379] at 174–204 nm. For the range 206–220 nm, the absorption curve above 190 nm of Simon et al. [379] has been extrapolated (log σ = –4.1001 – 0.0870 λ ). The measured values of Hubrich et al. [166] deviate from the extrapolated values by up to 20%.
Measurements in the far UV at 60–160 nm have been reported by Gilbert et al. [132], and measurements at 120–200 nm by Doucet et al. [110].
A weak temperature dependence has been observed a bove 190 nm, where the cross sections decrease with decreasing temperature between 296 and 210 K. Simon et al. [379] parameterized the cross sections and the temperature dependence by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported4-55 smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratosphe ric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 174–204 nm are as follows:

A 0 = –106.029 B 0 = –1.3399 × 10 –1
A 1 = 1.5038 B 1 = 2.7405 × 10 –3
A 2 = –8.2476 × 10 –3 B 2 = –1.8028 × 10 –5
A 3 = 1.4206 × 10 –5 B 3 = 3.8504 × 10 –8

Table 4-54. Absorption Cross Sections of CHF 2 Cl at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 12.9 188 0.372 206 0.00842 172 9.79 190 0.245 208 0.00636 174 5.72 192 0.156 210 0.00426 176 4.04 194 0.103 212 0.00285 178 2.76 196 0.072 214 0.00191 180 1.91 198 0.048 216 0.00128 182 1.28 200 0.032 218 0.00086 184 0.842 202 0.0220 220 0.00057 186 0.576 204 0.0142

Note : 170–172 nm: Hubrich et al. [166] 174–204 nm: Simon et al. [379] 206–220 nm: extrapolation of Simon et al. [379] data.

F38. CH 2 FCl (HCFC-31) + h ν → Products. The absorption cross sections of CH 2 FCl have been measured at 208 and 298 K and 160–230 nm by Hubrich and Stuhl [165]. The room temperature data at 160–230 nm are listed in Table 4–55.
Measurements in the far UV at 60–120 nm have been reported by Gilbert et al. [132], and measurements at 120–200 nm by Doucet et al. [110].

Table 4–55. Absorption Cross Sections of CH 2 FCl at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

160 47.9 185 4.20 210 0.0188 165 55.9 190 1.95 215 0.00560 170 43.0 195 0.544 220 0.00215 175 23.3 200 0.209 225 0.00049 180 12.5 205 0.069 230 0.00026

Note : 160–230 nm: Hubrich and Stuhl [165].

F39. CF 3 CHCl 2 (HCFC-123) + h ν → Products. The absorption cross sections of CF 3 CHCl 2 have been measured at room temperature and 185–204 nm by Green and Wa yne [146]; at 225–295 K and 170–250 nm by Gillotay and Simon [136]; at 203–295 K and 190–230 nm by Orlando et al. [305]; and at 223–333 K and 160–230 nm by Nayak et al. [286]. The agreement between the results of the latter three groups is within 25% in the region below 220 nm. The results of Green and Wayne [146] are very different below 200 nm. The preferred absorption cross sections at 295 K, lis ted in Table 4-56, are the mean of the values reported by Gillotay and Simon [136] and Nayak et al . [286] at 170–188 nm and the mean of the values reported by Gillotay and Simon [136], Orlando et al. [305], and Nayak et al. [286] at 190–230 nm. For the range 232–250 nm, the absorption curve above 210 nm of Orlando et al. [305] has been extrapolated (log σ = –3.1097 – 0.0794 λ ).
The studies of the temperature dependence show a decr ease of the absorption cross sections with decreasing temperature at wavelengths above 178–180 nm and be low 170 nm. Between 170–180 nm, the reverse behavior was observed by Gillotay and Simon [ 136] and Nayak et al. [ 286]. An irregular temp erature dependence was reported by Orlando et al. [305] for the range 210–230 nm, where the absorption curves show wiggles.4-56 Various parameterized fits, i.e., polynomial expansions of the logarithm of the absorption cross section, have been proposed for the temperature de pendence. Gillotay and Simon [136] pa rameterized the cross sections and the temperature dependence by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 182–250 nm are as follows:

A 0 =–513.996354 B 0 = 1.757133

A 1 = 9.089141 B 1 = –3.499205 × 10 –2

A 2 = –6.136794 × 10 –2 B 2 = 2.593563 × 10 –4

A 3 = 1.814826 × 10 –4 B 3 = –8.489357 × 10 –7

A 4 = –1.999514 × 10 –7 B 4 = 1.037756 × 10 –9

. Nayak et al. [286] report sixth-order polynomial coefficients for the functions log 10 ( σ T ) = ∑ C n ( λ – 170) n at T = 223, 233, 253, 273, 295, 313, and 333 K and for the range 160–230 nm. The parameters C n are as follows:

223 K 273 K 295 K 333 K C 0 –17.6732 –17.6773 –17.6792 –17.6722 C 1 1.70233 × 10 –2 1.3636 × 10 –2 1.19392 × 10 –2 9.07941 × 10 –3
C 2 –7.39366 × 10 –4 –4.98553 × 10 –4 –3.71661 × 10 –4 –1.29566 × 10 –4
C 3 –1.83761 × 10 –4 –1.70566 × 10 –4 –1.61218 × 10 –4 –1.56667 × 10 –4
C 4 7.80778 × 10 –6 6.73373 × 10 –6 6.03101 × 10 –6 5.56409 × 10 –6
C 5 –1.29836 × 10 –7 –1.02726 × 10 –7 –8.76762 × 10 –8 –7.77379 × 10 –8
C 6 8.05415 × 10 –10 5.66688 × 10 –10 4.61745 × 10 –10 3.93859 × 10 –10 A double expansion in terms of twelve parameters, ln σ ( λ , T) = ∑ ( ∑ a ij (T–245.4) j–1 ) ( λ – 206.214) i–1 , i = 1–4, j = 1–3, T = 203–295 K, λ = 190–230 nm, was used by Orlando et al. [305]:

a 11 = –4.500 × 10 –1 a 12 = 3.529 × 10 –3 a 13 = –4.181 × 10 –8

a 21 = –1.985 × 10 –1 a 22 = 6.826 × 10 –5 a 23 = 1.555 × 10 –6

a 31 = –2.802 × 10 –4 a 32 = –1.018 × 10 –5 a 33 = 4.037 × 10 –8

a 41 = 6.312 × 10 –5 a 42 = –3.055 × 10 –7 a 43 = –2.473 × 10 –9

Table 4-56. Absorption Cross Sections of CF 3 CHCl 2 at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 192 198 17.1 226 0.0880 172 207 200 11.9 228 0.0599 174 214 202 8.24 230 0.0451 176 213 204 5.70 232 0.0295 178 202 206 3.89 234 0.0205 180 184 208 2.67 236 0.0142 182 161 210 1.82 238 0.0098 184 135 212 1.23 240 0.0068 186 109 214 0.838 242 0.0047 188 85.5 216 0.573 244 0.0033 190 62.2 218 0.384 246 0.0023 192 46.4 220 0.266 248 0.0016 194 33.9 222 0.180 250 0.0011 196 24.2 224 0.124 Note: 170–188 nm: mean of the values of Gillo tay and Simon [136] a nd Nayak et al. [286] 190–230 nm: mean of the values of Gillotay and Si mon [136], Orlando et al. [305] , and Nayak et al. [286] 232–250 nm: extrapolation of Orlando et al. [305] data.4-57 F40. CF 3 CHFCl (HCFC-124) + h ν → Products. The absorption cross sections of CF 3 CHFCl have been measured at 203–295 K and 190–230 nm by Orlando et al. [305]; and at 210–295 K a nd 170–230 nm by Gillotay and Simon [137]. The agreement is better than 10 % between 190 and 220 nm, whereas above 220 nm the values of Orlando et al. [305] become increasi ngly larger by up to 133% than thos e of Gillotay and Simon [137]. The preferred room temperature values, listed in Table 4- 57, are the values of Gillotay and Simon [137] at 170–188 nm and 222–230 nm and the mean of the values reported by Gillotay and Simon [137] and Orlando et al. [305] at 190–220 nm. The temperature dependence of the cross sections has been measured by both groups and a decrease of the absorption cross sections with d ecreasing temperature was observed at 170–230 nm by Gillotay and Simon [137] and at 190–215 nm by Orlando et al. [305]. An irregular temperature behavior was reported by Orlando et al. [305] for the range 215–230 nm, where the absorption curves show wiggles. Parameterized fits, i.e., polynomial expansions of the logarithm of the absorption cross section, have been derived. Gillotay and Simon [137] parameterized the cross sections and the te mperature dependence by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 170–230 nm are as follows:

A 0 =–101.230250 B 0 = –5.795712 × 10 –2

A 1 = 1.333519 B 1 = 1.053901 × 10 –3

A 2 = –6.888672 × 10 –3 B 2 = –6.530379 × 10 –6

A 3 = 1.114172 × 10 –5 B 3 = 1.382056 × 10 –8

A double expansion in terms of twelve parameters, ln σ ( λ , T) = ∑ ( ∑ a ij (T–251.7) j–1 ) ( λ – 206.214) i–1

, i = 1–4, j = 1–3, T = 203–295 K, λ = 190–230 nm, was used by Orlando et al. [305]:

a 11 = –4.967 × 10 –1 a 12 = 6.562 × 10 –3 a 13 = 1.735 × 10 –5

a 21 = –2.025 × 10 –1 a 22 = 2.788 × 10 –4 a 23 = –3.974 × 10 –6

a 31 = 6.839 × 10 –4 a 32 = 5.523 × 10 –6 a 33 = –3.092 × 10 –7

a 41 = 1.275 × 10 –4 a 42 = –2.959 × 10 –7 a 43 = –1.182 × 10 –8

Table 4-57. Absorption Cross Sections of CF 3 CHFCl at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 13.6 192 0.548 214 0.00859 172 11.1 194 0.387 216 0.00610 174 8.85 196 0.267 218 0.00431 176 6.93 198 0.185 220 0.00312 178 5.33 200 0.128 222 0.00214 180 4.03 202 0.0868 224 0.00153 182 3.00 204 0.0594 226 0.00111 184 2.20 206 0.0401 228 0.00082 186 1.60 208 0.0269 230 0.00061 188 1.14 210 0.0186 190 0.772 212 0.0126 Note : 170–188 nm, Gillotay and Simon [137], 190–220 nm, mean of the values of Gillotay and Simon [137] and Orlando et al. [305], 222–230 nm, Gillotay and Simon [137].

F41. CF 3 CH 2 Cl (HCFC-133) + h ν → Products. The absorption cross sections of CF 3 CH 2 Cl have been measured at room temperature and 147 nm ( σ = 1.35 × 10 –17 cm 2 ) by Ichimura et al. [174], and 186–203 nm by Green and Wayne [146], and at 208 and 298 K and 160–245 nm by Hubrich and Stuhl [165]. There is no good agreement between the results at wavelengths above 180 nm. Table 4-58 gives the recommended room temperature data of Hubrich and Stuhl [165].4-58 Table 4-58. Absorption Cross Sections of CF 3 CH 2 Cl at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

160 59.4 190 6.20 220 0.0887 165 64.6 195 2.95 225 0.0226 170 56.4 200 1.14 230 0.0147 175 37.3 205 0.598 235 0.00404 180 22.8 210 0.328 240 0.00181 185 11.6 215 0.169 245 0.00054
Note: 160–245 nm, Hubrich and Stuhl [165].

F42. CH 3 CFCl 2 (HCFC-141b) + h ν → Products. The absorption cross sections of CH 3 CFCl 2 have been measured at 210–295 K and 170–240 nm by Gillotay and Simon [136] ; at 203–295 K and 190–230 nm by Orlando et al. [305] (data of Orlando et al. reported by Gillotay and Simon [138]); at 203–295 K and 190–230 nm by Talukdar et al. [393]; and at room temperature and 190–240 nm by Fahr et al. [113], who investigated the spectrum both for the gas and liquid phases and used a wa velength-shift procedure to convert the liquid-phase data into gas-phase data. The agreem ent between the values reported by G illotay and Simon [136] and Fahr et al. [113] for the 190–240-nm region is very good (1–10% up to 236 nm); the results of Orlando et al. [305] are also in good agreement with these, but only in the region 190–210 nm. The agreement of the results of Talukdar et al. [393] is not as good, their absorption cross sections become smaller below 210 nm by up to ~20% and become larger above 210 nm by up to about 70% than the above mentioned data. The preferred absorption cross sections, listed in Table 4-59, are th e values of Gillotay and Simon [136] at 170–188 nm and the mean of the values reported by Gillotay a nd Simon [136] and Fahr et al. [113] at 190–240 nm.
A decrease of the absorption cross sections with decreasing temperature at wavelengths above 188 nm and below 172 nm and the reverse behavior between 172 a nd 188 nm was observed by Gillotay and Simon [136]. They parameterized the cross sections and the temperat ure dependence of the absorption cross sections using the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n . They derived the parameters

A 0 = –682.913042 B 0 = 4.04747

A 1 = 12.122290 B 1 = –8.05899 × 10 –2

A 2 = –8.187699 × 10 –2 B 2 = 5.946552 × 10 –4

A 3 = 2.437244 × 10 –4 B 3 = –1.945048 × 10 –6

A 4 = –2.719103 × 10 –7 B 4 = 2.380143 × 10 –9

for the ranges 210–300 K and 172–240 nm and list smoothed values for T = 210, 230, 250, 270, and 295 K at 2-nm intervals and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. A similar temperature behavior was observed by Orlando et al. [305] only between 190 and 210 nm, and by Talukdar et al. [393] only above 197 nm.4-59 Table 4-59. Absorption Cross Sections of CH 3 CFCl 2 at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 143.1 194 47.2 218 0.382 172 145.1 196 34.1 220 0.248 174 154.2 198 24.0 222 0.161 176 162.9 200 16.6 224 0.105 178 172.6 202 11.3 226 0.0680 180 172.3 204 7.56 228 0.0444 182 162.9 206 5.02 230 0.0290 184 146.4 208 3.30 232 0.0189 186 125.7 210 2.16 234 0.0123 188 103.6 212 1.40 236 0.00801 190 83.0 214 0.909 238 0.00518 192 63.6 216 0.589 240 0.00334 Note: 170–188 nm, Gillotay and Simon [136], 190–240 nm, mean of Gillotay and Sim on [136] and Fahr et al. [113].

F43. CH 3 CF 2 Cl (HCFC-142b) + h ν → Products. The absorption cross sections of CH 3 CF 2 Cl have been measured at room temperature and 120–180 nm by Doucet et al. [111]; at 184–210 nm by Green and Wayne [146]; at 298 and 208 K and 160–230 nm by Hubrich and Stuhl [165]; at 210–295 K and 170–230 nm by Gillotay and Simon [136]; at 203–295 K and 190–230 nm by Orlando et al. [305]; and at 223–333 K and 160–210 nm by Nayak et al. [286]. At wavelengths below 200 nm, the values of Hubrich and Stuhl [165] and Nayak et al. [286] are within 15%, those of Gillotay and Sim on [136] and Orlando et al . [305] are lower than the latter by up to 30%. At wavelengths between 200 and 215 nm, the values of Gillotay and Simon [136], Orlando et al. [305], and Nayak et al [286] agree within 15%. Above 215 nm, the absorption curve reported by Orlando et [305] shows wiggles with deviations by up to 100% from the data of Gillotay and Simon [136]. Also the values reported for the range 205–230 nm by Hubrich and Stuhl [165] become increasingly large by up to 600% than those of Gillotay and Simon [136] .The results of Green and Wa yne [146] are very different from all other data. The preferred room temperature absorption cross sections, listed in Table 4–60, are the mean of the values reported by Hubrich and Stuhl [165], Gillotay and Simon [136], and Naya k et al. [286] at 175–185 nm, the mean of the values reported by Gillotay and Si mon [136], Orlando et al. [305], and Nayak et al . [286] at 190–210 nm, and the values reported by Gillota y and Simon [136] at 212–230 nm.
A decrease of the absorption cross sections with decr easing temperature was observed by Gillotay and Simon [136] and Nayak et al. [286] over the wavelength ra nge 160–230 nm and by Orlando et al. [305] between 190 and 200 nm. An irregular temperature behavior was re ported by Orlando et al. [305] for the range 215–230 nm, where the absorption curves for the va rious temperatures show several crossings. Various parameterized fits for the temperature dependence of the abso rption cross sections have been offe red. Gillotay and Simon [136] used the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodisso ciation calculations. Their parameters A n and B n for the ranges T = 210–300 K and λ = 172–230 nm are as follows:

A 0 = –328.092008 B 0 = 4.289533 × 10 –1

A 1 = 6.342799 B 1 = –9.042817 × 10 –3

A 2 = –4.810362 × 10 –2 B 2 = 7.018009 × 10 –5

A 3 = 1.611991 × 10 –4 B 3 = –2.389065 × 10 –7

A 4 = –2.042613 × 10 –7 B 4 = 3.039799 × 10 –10

Nayak et al. [286] report fourth-order polynomial coefficients C n (T) for the functions log 10 ( σ T ) = ∑ C n ( λ – 160) n at T = 223, 233, 253, 273, 295, 313, and 333 K and for the range 160–210 nm. The parameters C n are as follows4-60 223 K 273 K 295 K 333 K C 0 –18.2361 –18.2441 –18.2406 –18.1777 C 1 –1.26669 × 10 –2 –7.37889 × 10 –3 –6.48269 × 10 –3 –2.39647 × 10 –2
C 2 –2.32945 × 10 –3 –2.66537 × 10 –3 –2.80923 × 10 –3 –7.23910 × 10 –4
C 3 2.81933 × 10 –5 4.19193 × 10 –5 5.01979 × 10 –5 –1.08049 × 10 –5
C 4 –1.37963 × 10 –7 –2.88472 × 10 –7 –3.96860 × 10 –7 1.37618 × 10 –7
A double expansion in terms of twelve parameters, ln σ ( λ , T) = ∑ ( ∑ a ij (T–245.4) j–1 ) ( λ – 206.214) i–1 , i = 1–4, j = 1–3, T = 203–295 K, λ = 190–230 nm, was used by Orlando et al. [305]:

a 11 = –4.973 × 10 –1 a 12 = 9.077 × 10 –3 a 13 = –4.651 × 10 –5

a 21 = –2.175 × 10 –1 a 22 = 4.712 × 10 –4 a 23 = –1.005 × 10 –5

a 31 = 4.133 × 10 –4 a 32 = –6.432 × 10 –5 a 33 = 1.141 × 10 –6

a 41 = 7.145 × 10 –5 a 42 = –5.396 × 10 –6 a 43 = 1.187 × 10 –7

Quantum yields for Cl ( 2 P 3/2 ) and Cl*( 2 P 1/2 ) atom formation in the photolysis of CH 3 CF 2 Cl at 193.3 nm have been measured by Brownsword et al. [49] and quantum yields for H atom formation in the photolysis at 121.6 and 193.3 nm by Brownsword et al. [48]: Φ (Cl + Cl*) = 0.90 ± 0.17 with Φ (Cl) = 0.65 ± 0.12 and Φ (Cl*) = 0.25 ± 0.05 at 193.3 nm, and Φ (H) = 0.53 ± 0.12 and 0.06 ± 0.02 at 121.6 and 193.3 nm, respectively.

Table 4–60. Absorption Cross Sections of CH 3 CF 2 Cl at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 27.1 200 0.145 218 0.00243 175 14.0 202 0.0949 220 0.00145 180 6.38 204 0.0622 222 0.000845 185 2.73 206 0.0399 224 0.000484 190 1.02 208 0.0256 226 0.000271 192 0.706 210 0.0161 228 0.000148 194 0.482 212 0.0105 230 0.0000783 196 0.324 214 0.00652 198 0.218 216 0.00401 Note: 170–185 nm: mean of Gillotay and Simon [136], Hubr ich and Stuhl [165], a nd Nayak et al. [286] 190–210 nm: mean of Gillotay and Simon [136], Or lando et al. [305], and Nayak et al. [286] 212–230 nm: Gillotay and Simon [136].

F44. CF 3 CF 2 CHCl 2 (HCFC-225ca) + h ν → Products

F45. CF 2 ClCF 2 CHFCl (HCFC-225cb) + h ν → Products. The absorption spectra of these compounds in the gaseous and liquid phases at 298 K have been measured by Braun et al. [40]. Table 4-61 lists the absorption cross sections for the gas phase taken from this work. The originally listed (0.5-nm intervals) absorption coefficients

ε in (atm, 298 K) –1 cm –1 ( σ = 4.06 × 10 –20 ε ) for both phases have been fitted with third-order polynomial expansions log 10 ε = ∑ a n ( λ – 160) n with

a 0 = 1.425, a 1 = 4.542 × 10 –2 , a 2 = –2.036 × 10 –3 , a 3 = 1.042 × 10 –5 for HCFC-225ca at 170–270 nm,

a 0 = 1.677, a 1 = –2.175 × 10 –2 , a 2 = –1.484 × 10 –3 , a 3 = 1.147 × 10 –5 for HCFC-225cb at 165–250 nm.4-61 Table 4-61. Absorption Cross Sections of CF 3 CF 2 CHCl 2 and CF 2 ClCF 2 CFCl at 298 K

λ (nm) 10 20 σ (cm 2 ) CF 3 CF 2 CHCl 2 CF 2 ClCF 2 CFCl (HCFC-225ca) (HCFC-225cb) λ (nm) 10 20 σ (cm 2 ) CF 3 CF 2 CHCl 2 CF 2 ClCF 2 CFCl (HCFC-225ca) (HCFC-225cb)
160 268.7 187.9 202 11.58 0.479 162 236.8 173.3 204 8.185 0.369 164 207.6 154.8 206 5.802 0.291 166 189.0 135.1 208 4.084 0.254 168 181.4 113.2 210 2.903 0.250 170 182.7 91.35 212 2.042 172 182.8 70.68 214 1.429 174 189.0 54.73 216 1.05 176 190.9 40.68 218 0.727 178 187.9 30.04 220 0.463 180 177.5 21.11 222 0.308 182 161.1 14.90 224 0.209 184 140.3 10.47 226 0.145 186 118.3 7.308 228 0.0987 188 96.51 5.075 230 0.0653 190 74.30 3.492 232 0.0434 192 57.08 2.412 234 0.0299 194 42.83 1.661 236 0.0193 196 31.75 1.165 238 0.0134 198 23.22 0.873 239 0.0119 200 16.24 0.633 Note: HCFC-225ca, 160–239 nm, Braun et al. [40],
HCFC-225cb, 160–210 nm, Braun et al. [40].

G1. BrO + h ν → Br + O. The BrO radical has a banded spectrum in the 290–380 nm range. The strongest absorption feature is around 338 nm. The measured cross sections are both temperature- and resolutiondependent. As an example, the spectrum measured by Wahner et al. [423] is shown in Figure 4-4. The bands are due to a vibrational progression in the A ← X system, and the location of the bands, along with the assignments and cross sections measured using 0.4 nm resolution, are shown in Table 4-62. BrO is expected to dissociate upon light absorption. As a guide, the cross sections averaged over 5 nm wavelength intervals are taken from the work of Cox et al. [92], and are listed in Table 4-63. These authors estimate a BrO lifetime against atmospheric photodissoci ation of ~20 seconds at the earth's su rface, for a solar zenith angle of 30°.
The earlier BrO cross section measurements were carried out mostly around 338 nm, and these have been reviewed by CODATA ([81,82]).4-62 Table 4-62. Absorption Cross Sections at the Peak of Various Bands in the A ← X Spectrum of BrO

10 20 σ (cm 2 ) ν ', ν " λ (nm) 298 K 223 K 13,0 313.5 712 938 12,0 317.0 1010 1360 11,0 320.8 1180 1570 10,0 325.0 1130 1430

9,0 329.1 1130 1390 8,0 333.5 1210 1470 7,0 338.3 1550 1950 6,0 343.7 935 1110 5,0 348.8 703 896 4,0 354.7 722 1050 3,0 360.4 264 344 2,0 367.7 145 154 1,0 374.5 90 96
Spectral resolution is 0.4 nm, fwhm.

Table 4-63. Absorption Cross Sections of BrO

λ (nm) 10 20 σ (cm 2 ) average
300–305 200 305–310 259 310–315 454 315–320 391 320–325 600 325–330 753 330–335 628 335–340 589 340–345 515 345–350 399 350–355 228 355–360 172 360–365 161 365–370 92 370–375 514-63 Figure 4-4. Absorption Spectrum of BrO4-64 G2. HOBr + h ν → Products. The absorption spectrum of HOBr has been measured by Orlando and Burkholder [304], Deters et al. [108], Be nter et al. [31], Rattigan et al. [324], and Ingham et al . [176]. The spectra cluster has been measured in two groups. Orlando and Burkholder [304], Deters et al. [108], and Benter et al. [31] observe between 240 and 400 nm two absorption bands with maxima near 284 and 351 nm; the spectra agree reasonably well in their shape, but show a sharp decrease in cross section above 400 nm. In contrast, the cross sections reported by Rattigan et al . [324] and Ingham et al . [176] are roughly 50 % larger between 300 and 400 nm. In addition, the spectrum obtained by Rattigan et al. shows a pronounced tail extending to 520 nm, whereas Ingham et al. observe unambiguously a third weaker absorption band ranging to 550 nm with a maximum at 457 nm. These last two studies confirm the observations of Barnes et al. [22], who showed that laser photolysis of HOBr between 440–600 nm gives rise to OH fragments. The presence of a weak band beyond 400 nm is attributable to the presence of a forbidden transition from the ground electronic to a triplet state predicted by the ab initio calculations of Francisco et al. [122]. The differences in the sp ectral shapes are probably attributable to impurities such as Br 2 O and Br 2 , and/or the use of different Br 2 O cross sections. However, the presence of impurities alone cannot explai n the large difference in cross secti ons at the peak of the absorption bands.
The recommended absorption cross sections are listed in , in the range from 250 to 550 nm; below 250 nm the data are uncertain and no recommendation is given. The cross section values in the table are based on the latest study by Ingham et al. [176]. These authors generated HOBr in situ by laser photolytic production of OH in the presence of Br 2 , and determined the HOBr spectrum using a gated diode camera shortly after the pulse, circumventing the problem associated with the presence of the strong absorbing impurity Br 2 O, which was encountered in previous studies. The calibration of the absorption cross sections was made relative to the established cross sections of Br 2 . The data presented in Table 4-64 are computed with the following expression taken from Ingham et al. [176], which is based on a combination of three Ga ussian fits, one for each absorption band:

22 2 284.01 350.57 457.38 ( ) 24.77 exp 109.80 ln 12.22 exp 93.63 ln 2.283exp 242.40 ln σ λ λλ λ               = − +− +−                        

σ ( λ ): 10 –20 cm 2 molecule –1 ; 250 < λ < 550 nm. Benter et al. [31] measured quantum yields for HOBr photolysis at 261 and 363 nm (near the peaks of the second absorption bands). The observed quantum yield for Br formation at 363 nm was greater than 0.95, and a unity quantum yield into the product channel OH + Br is recommended. The other channel O + HBr was not observed. The laser photofragment study of Barnes et al. [22] claimed that OH was the major photolysis product at wavelengths beyond 400 nm. Lock et al. [222] found that at 490 and 510 nm OH and Br fragments are in their respective vibrational and spin-orbit ground states. The assumption of unit quantum yield of OH formation should be confirmed experimentally.4-65 Table 4-64. Absorption Cross Sections of HOBr

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

250 4.15 355 12.1 460 2.28 255 6.19 360 11.5 465 2.14 260 10.5 365 10.5 470 1.91 265 14.6 370 9.32 475 1.62 270 18.7 375 7.99 480 1.30 275 22.1 380 6.65 485 0.993 280 24.3 385 5.38 490 0.723 285 25.0 390 4.22 495 0.502 290 24.0 395 3.23 500 0.333 295 21.9 400 2.43 505 0.212 300 19.1 405 1.80 510 0.129 305 16.2 410 1.36 515 0.076 310 13.6 415 1.08 520 0.042 315 11.8 420 0.967 525 0.023 320 10.8 425 0.998 530 0.012 325 10.5 430 1.15 535 0.0059 330 10.8 435 1.40 540 0.0029 335 11.3 440 1.68 545 0.0013 340 11.9 445 1.96 550 0.0006 345 12.3 450 2.18 350 12.4 455 2.29

G3. BrONO 2 + h ν → Products. The bromine nitrate cross sections have been measured at room temperature by Spencer and Rowland [386] in the wavelength region 186–390 nm, and by Burkholder et al. [54] from 200– 500 nm. The results from both studies are in excellent ag reement over the range of spectral overlap. The recommended cross sections (Table 4-65) are taken from Burkholder et al.
The only study of photolysis products is that of Nickolaisen and Sander [292]. In that study, quantum yields for the Br + NO 3 and BrO + NO 2 channels were measured using broadband photolysis in quartz ( λ >200 nm) and pyrex ( λ >300 nm) reaction cells with the assumption that th ese were the only reaction pathways. The quantum yields were Φ BrO+NO 2 = 0.71 and Φ Br+NO 3 = 0.29.4-66 Table 4-65. Absorption Cross Sections of BrONO 2 at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

200 680 305 16.2 410 1.81 205 520 310 14.2 415 1.66 210 361 315 12.4 420 1.50 215 293 320 11.0 425 1.38 220 258 325 9.82 430 1.30 225 231 330 8.94 435 1.20 230 205 335 8.22 440 1.11 235 174 340 7.64 445 1.04 240 139 345 7.17 450 0.930 245 106 350 6.66 455 0.834 250 79.5 355 6.21 460 0.743 255 60.1 360 5.69 465 0.652 260 47.1 365 5.17 470 0.566 265 38.9 370 4.66 475 0.461 270 33.8 375 4.16 480 0.390 275 30.5 380 3.69 485 0.275 280 27.9 385 3.23 490 0.243 285 25.6 390 2.88 495 0.214 290 23.2 395 2.53 500 0.135 295 20.7 400 2.25 300 18.4 405 1.994-67 G4. BrCl + h ν → Br + Cl. The recommended absorption cross sections are given by the expression listed at the bottom of Table 4-66, which is take from the work of Maric et al. [236]. For convenience, some room temperature values are also listed in the table. Hubinger and Nee [164] have also measured the cross sections at room temperature. Their results are in excellent agr eement with the recommended values.

Table 4-66. Absorption Cross Sections of BrCl at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

200 2.4 390 34.7 210 4.0 400 28.2 220 5.4 410 21.9 230 6.0 420 16.9 240 5.1 430 14.2 250 3.7 440 12.4 260 2.5 450 11.1 270 1.5 460 9.6 280 1.2 470 8.0 290 0.63 480 6.8 300 0.61 490 5.0 310 1.2 500 3.8 320 2.8 510 3.1 330 7.4 520 2.3 340 14.2 530 1.5 350 22.9 540 0.96 360 33.3 550 0.76 370 38.7 560 0.31 380 38.5

where 318.8 tanh T α  

=     , λ in nm and T in K, 200 nm < λ < 600 nm., 195 K < T < 300 K. 2 22
20 0.5 227.6 372.5 442.4 10 7.34exp 68.6 ln 43.5exp 123.6 ln 11.2exp 84.8 ln σα α α α λ λλ −            = − +− +−                    4-68 G5. CH 3 Br + h ν → Products. The absorption cross sections of CH 3 Br have been measured at room temperature and 205–270 nm by Davidson [104]; at 204–260 nm by Gordus and Bernstein [142]; at 174–270 nm by Robbins [338]; at 200–260 nm by Uthman et al. [413]; at 190–290 nm by Molina et al. [272]; at 201.6 nm by Felps et al. [119]; at 180–264 nm by Man et al . [230]; and at 210–295 K and 180–280 nm by Gillotay and Simon [133]. Above 180 nm and below 270 nm, the room temperature values of Gordus and Bernstein [142], Robbins [338], Uthman et al. [413], Molina et al. [272], Gillotay and Simon [133], and th e values of Davidson [104] above 210 nm are in very good agreement, i.e., generally within 10% and around the absorption maximum at 200– 202 nm within 2%. The value at 202 nm of Felps et al. [119] is lower by ~10% than the rest of the data. The data of Man et al. [230], given as a plot in their paper, are lower by 20–30% over the whole absorption band than the above mentioned agreeing data sets. The prefe rred absorption cross sections, listed in Table 4-67, are the values of Robbins [338] at 174–178 nm; the mean of the values reported by G illotay and Simon [133] and Robbins [338] at 180–188 nm; the mean of the values re ported by Gillotay and Sim on [133], Uthman et al. [413], and Robbins [338] at 190–198 nm; the mean of the values re ported by Gillotay and Simon [133], Molina et al. [272], Uthman et al . [413], and Robbins [ 338] at 200–260 nm; the mean of the values reported by Gillotay and Simon [133], Molina et al.[272], and Robbins [338] at 262–268 nm; the mean of the values reported by Gillotay and Simon [133] and Molina et al. [272] at 270–280 nm; and the da ta of Molina et al. [272] at 285–290 nm. A slight temperature dependence was observed above 220 nm, where the absorption cross sections decrease with decreasing temperature 295–210 K. Gillotay and Sim on [133] parameterized the cross sections and the temperature dependence by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and reported smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratosphe ric photodissociation calculations. The parameters A n and B n for the ranges T = 210–300 K and λ = 200–280 nm are as follows:

A 0 = 46.520 B 0 = 9.3408 × 10 –1

A 1 = –1.4580 B 1 = –1.6887 × 10 –2

A 2 = 1.1469 × 10 –2 B 2 = 1.1487 × 10 –4

A 3 = –3.7627 × 10 –5 B 3 = –3.4881 × 10 –7

A 4 = 4.3264 × 10 –8 B 4 = 3.9945 × 10 –10

Quantum yields for Br and H atom formation in the photodissociation of CH 3 Br were measured at 298 K by Talukdar et al. [399]. The quantum yields for Br atom formation were found to be close to unity, Φ (Br) = 1.05 ± 0.11, 1.10 ± 0.20, and 1.01 ± 0.16 at 193, 222, and 248 nm, respectively; the quantum yield for H atom formation in the photolysis at 193 nm was measured to be Φ (H) = 0.002 ± 0.001, whereas H atoms could not be detected in the photolysis at 222 and 248 nm. Broad band flash photolysis of CH 3 Br produced Br*( 2 P 1/2 ) atoms with a quantum yield Φ (Br*) = 0.15 ± 0.12 as reported by Ebenstein et al. [112].4-69 Table 4-67. Absorption Cross Sections of CH 3 Br at 295–296 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

174 533 212 59.9 250 0.921 176 1010 214 54.2 252 0.683 178 1280 216 47.9 254 0.484 180 44.6 218 42.3 256 0.340 182 19.8 220 36.6 258 0.240 184 21.0 222 31.1 260 0.162 186 27.8 224 26.6 262 0.115 188 35.2 226 22.2 264 0.0795 190 44.2 228 18.1 266 0.0551 192 53.8 230 14.7 268 0.0356 194 62.6 232 11.9 270 0.0246 196 69.7 234 9.41 272 0.0172 198 76.1 236 7.38 274 0.0114 200 79.0 238 5.73 276 0.00808 202 79.2 240 4.32 278 0.00553 204 78.0 242 3.27 280 0.00382 206 75.2 244 2.37 285 0.00110 208 70.4 246 1.81 290 0.00030 210 65.5 248 1.31 Note: 174–178 nm, Robbins [338], 180–188 nm, mean of Gillotay and Si mon [133] and Robbins [338], 190–198 nm, mean of Gillotay ad Simon [133], Uthman et al. [413] , and Robbins [338], 200–260 nm, mean of Gillotay and Simon [133], Mo lina et al. [272], Uthm an et al. [413] and Robbins [338], 262–268 nm, mean of Gillotay and Simon [ 133], Molina et al. [272] , and Robbins [338], 270–280 nm, mean of Gillotay a nd Simon [133] and Molina et al.[272], 285–290 nm, Molina et al. [272].

G6. CH 2 Br 2 + h ν → Products. The absorption cross sections of CH 2 Br 2 have been measured at room temperature and 200–300 nm by Molina et al. [272] ; at 210–295 K and 174–290 nm by Gillota y et al. [138], [135]; and at 250–348 K and 215–300 nm by Mössinger et al. [283]. The results are in good agreement, at 200–255 nm within 10% and up to 275 nm within 30%. The preferred room temperature values, listed in Table 4-68, are the values of Gillotay et al. [138], [ 1325] at 174–198 nm; the mean of the valu es reported by Molina et al. [272] and Gillotay et al. [138], [135] for the wavelength range 200–215 nm; the mean of the values reported by the three groups for the wavelength range 220–290 nm; and the values of Mössinger et al. [283] at 295–300 nm.
Both studies of the temperature dependence show a decr ease of the absorption cross sections with decreasing temperature at wavelength above ~235–239 nm, and th e reverse behavior around the absorption maximum down to 207 nm. At lower wavelengths, Gillotay et al. [135,138] report between 210 and 295 K a slight increase of σ at 175–189 nm and a slight decrease around the weaker absorption maximum at 198–201 nm. The latter group parameterized the cross sections and the temperature dependence by the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and report smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wa venumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges 210–290 nm and 210–300 K are as follows:

A 0 = –70.211776 B 0 = 2.899280 A 1 = 1.940326 × 10 –1 B 1 = –4.327724 × 10 –2
A 2 = 2.726152 × 10 –3 B 2 = 2.391599 × 10 –4
A 3 = –1.695472 × 10 –5 B 3 = –5.807506 × 10 –7
A 4 = 2.500066 × 10 –8 B 4 = 5.244883 × 10 –10
Mössinger et al. [283] list the temperature coefficients B( λ ) at 5-nm intervals for the ranges 215–300 nm and 250–348 K for the empirical relation ln σ ( λ , T) = ln σ ( λ , 298K) + B( λ )x(T–298). The formulae used by Gillotay et al. [135,138] and Mössinger et al. [283] produce cross sections which agree at 250 K within 5% in the range 215–265 nm and within 10% in the range 270–285 nm.4-70 Table 4-68. Absorption Cross Sections of CH 2 Br 2 at 295–298 K

λ (nm) 10 20

σ (cm 2 ) λ (nm) 10 20

σ (cm 2 ) 10 3 B (K –1 ) λ (nm) 10 20

σ (cm 2 ) 10 3 B (K –1 )

174 1170.9 198 226.0 255 14.10 3.91 176 662.4 200 225.6 260 6.607 5.16 178 377.2 205 215.3 265 3.037 6.33 180 241.0 210 234.5 270 1.347 7.75 182 178.4 215 263.2 –2.02 275 0.590 8.74 184 154.4 220 272.0 –1.79 280 0.255 11.6 186 153.5 225 247.4 –1.50 285 0.114 13.8 188 166.1 230 195.8 –0.96 290 0.0499 15.3 190 187.0 235 138.9 –0.04 295 0.0210 16.5 192 209.3 240 88.60 0.71 300 0.0090 21.9 194 222.5 245 51.90 1.80 196 228.3 250 28.03 2.70 Note: Absorption cross sections σ : 174–198 nm, Gillotay et al. [138], [135], 200–210 nm, mean of Molina et al. [272] and Gillotay et al. [138], [135], 215–290 nm, mean of Molina et al [272] , Gillotay et al. [138], [135], and Mössinger et al. [283], 295–300 nm, Mössinger et al.[283]. Temperature coefficients B: 215–300 nm, Mössinger et al.[283].

G7. CHBr 3 + h ν → Products. The absorption cross sections of CHBr 3 have been measured at 240–295 K and 170– 310 nm by Gillotay et al. [133] a nd at 256–296 K and 286–362 nm by Moortgat et al. [ 278]; the agreement in the overlap region is excellent. The recommended cross sections at room temperature, listed in Table 4-69, are the values of Gillotay et al. [133] for the range 170–284 nm ; the mean of the values reported by Gillotay et al. [133] and Moortgat et al. [278] for the range 286–310 nm; and the values of Moortgat et al. [278] at 286–362

nm. The studies of the temperature dependence show an incr ease of the absorption cross sections with decreasing temperature around the three absorption maxima at 178–189 nm, 194–208 nm, and 208–234 nm, and a decrease of the absorption cross sections below 179 nm , at 189–194 nm and above 235 nm . Gillotay et al. [133] parameterized the cross sections and the temper ature dependence by the polynomial expansion
log 10 ( σ ( λ , T)) = ∑ A n λ n + (T – 273) × ∑ B n λ n
and report smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges 240–310 nm and 210–300 K are given by Gillotay and Simon [135]:

A 0 = –110.2782 B 0 = –1.5312 × 10 –1
A 1 = 1.0281 B 1 = 1.6109 × 10 –3
A 2 = –3.6626 × 10 –3 B 2 = –5.8075 × 10 –6
A 3 = 4.1226 × 10 –6 B 3 = 7.2893 × 10 –9

For wavelengths longer than 290 nm, the atmospherically important range, Moortgat et al. [278] give the expression

σ ( λ ,T) = exp { (0.06183 – 0.000241 λ ) (273 – T) – (2.376 + 0.14757 λ ) } ( λ = 290–340 nm, T = 210–300 K)

These two formulae produce continuous absorption curves for the range 240–340 nm also at low temperatures
At wavelengths longer than 290 nm, the cross sections are relatively small; the presence of impurities as well as optical artifacts arising, e. g., from adsorption of CHBr 3 on the cell windows, complicate the measurements. Hence, additional investigations of the spectrum would be useful.4-71 Table 4-69. Absorption Cross Sections of CHBr 3 at 295–296 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 1603.8 236 323.9 302 0.534 172 1173.2 238 294.7 304 0.397 174 969.6 240 272.8 306 0.297 176 872.0 242 253.3 308 0.222 178 857.6 244 233.7 310 0.165 180 831.3 246 214.4 312 0.127 182 770.3 248 193.9 314 0.0952 184 683.3 250 174.1 316 0.0712 186 570.4 252 157.7 318 0.0529 188 470.8 254 136.1 320 0.0390 190 399.1 256 116.4 322 0.0289 192 360.2 258 98.6 324 0.0215 194 351.3 260 82.8 326 0.0162 196 366.1 262 68.9 328 0.0121 198 393.6 264 56.9 330 0.00916 200 416.4 266 46.7 332 0.00690 202 433.6 268 38.0 334 0.00525 204 440.6 270 30.8 336 0.00396 206 445.0 272 24.8 338 0.00307 208 451.4 274 19.8 340 0.00240 210 468.5 276 15.8 342 0.00176 212 493.4 278 12.5 344 0.00135 214 524.2 280 9.88 346 0.00102 216 553.5 282 7.77 348 0.00080 218 573.9 284 6.10 350 0.00064 220 582.6 286 4.79 352 0.00054 222 578.0 288 3.74 354 0.00046 224 557.8 290 2.89 356 0.00032 226 527.2 292 2.20 358 0.00024 228 486.8 294 1.69 360 0.00017 230 441.2 296 1.28 362 0.00013 232 397.4 298 0.956 234 361.8 300 0.719 Note: 170–284 nm, Gillotay et al. [133], 286–310 nm, mean of Gillotay et al. [ 133] and Moortgat et al. [278], 312–362 nm, Moortgat et al. [278].

G8. CH 2 BrCH 2 Br + h ν → Products. The absorption cross sections of CH 2 BrCH 2 Br have been measured at room temperature and 190–270 nm by Uthman et al. [413]. Their data are listed in Table 4-70.4-72 Table 4-70. Absorption Cross Sections of CH 2 BrCH 2 Br at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 230 218 170 246 9.3 192 250 220 150 248 7.1 194 270 222 130 250 5.9 196 290 224 110 252 4.4 198 300 226 89 254 4.0 200 310 228 75 256 2.8 202 310 230 62 258 2.1 204 300 232 50 260 1.9 206 290 234 41 262 1.7 208 280 236 32 264 1.4 210 260 238 26 266 1.1 212 230 240 20 268 0.9 214 210 242 16 270 0.7 216 190 244 11 Note: 190–270 nm, Uthman et al. [413].

G9. C 2 H 5 Br + h ν → Products. The absorption cross sections of C 2 H 5 Br have been measured at 295 K and 200– 260 nm by Zhang et al. [451]. This wavelength range shows part of an absorption band with a maximum of ~ 6 × 10 –19 cm 2 at ~200 nm. Estimated values at 5-nm intervals, read from a logarithmic plot, are presented in Table 4-71.

Table 4-71. Absorption Cross Sections of C 2 H 5 Br at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

200 60.5 225 23.7 250 1.12 205 59.5 230 14.9 255 0.53 210 53.5 235 8.30 260 0.23 215 44.5 240 4.30 220 34.0 245 2.28 Note: 200–260 nm, Zhang et al. [451], estimated values read from logarithmic plot.

G10. CH 2 ClBr (Halon-1011) + h ν → Products. The absorption cross sections of CH 2 ClBr have been measured at room temperature and 210–260 nm by Cadman and Simons [64], and at 187–290 nm by Orkin et al. [303]. The data of Cadman and Simons [64], which are given only on a plot in their paper, are smaller by ≤ 20% than the data of Orkin et al. [303]. The recommended absorption cross sections, listed in Table 4-72, are the data of Orkin et al. [303].
Quantum yields for Br ( 2 P 3/2 ) and Br*( 2 P 1/2 ) atom formation in the photolysis of CH 2 ClBr at 193–242 nm and 248–268 nm have been measured by Zou et al. [452] and McGivern et al. [253], respectively. Reported values are as follows:

193 nm 234 nm 248.5 nm 261.5 nm 266.7 nm:

Φ (Br ( 2 P 3/2 )) 0.82 ± 0.10 0.80 ± 0.10 0.86 ± 0.10 0.84 ± 0.10 0.91 ± 0.10

Φ (Br*( 2 P 1/2 )) 0.18 ± 0.10 0.20 ± 0.10 0.14 ± 0.10 0.16 ± 0.10 0.09 ± 0.104-73 Table 4-72. Absorption Cross Sections of CH 2 ClBr at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

187 151.1 222 57.4 258 1.45 188 126.4 224 50.5 260 1.09 190 104.6 226 44.1 262 0.807 192 100.5 228 38.2 264 0.596 194 104.7 230 32.8 266 0.440 196 111.8 232 28.0 268 0.322 198 119.4 234 23.6 270 0.235 200 124.7 236 19.7 272 0.170 202 127.1 238 16.3 274 0.123 204 126.3 240 13.4 276 0.089 206 122.5 242 10.8 278 0.064 208 116.3 244 8.73 280 0.046 210 108.4 246 6.94 282 0.033 212 99.6 248 5.46 284 0.024 214 90.5 250 4.24 286 0.0178 216 81.5 252 3.29 288 0.0129 218 72.9 254 2.52 290 0.0098 220 64.8 256 1.92 Note: 187–290 nm, Orkin et al. [303].

G11. CHClBr 2 (Halon-1012) + h ν → Products. The absorption cross sections of CHClBr 2 have been measured at room temperature and 106–200 nm by Ibuki et al. [172]; and at 240, 261, and 296 K and 200–310 nm by Bilde et al. [33]. Two absorption bands are apparent above 200 nm, one maximizing near 210 nm and the other near 240 nm. Near the band maxima, the cross sections at 240 K are approximately higher by 10% than those at room temperature. A positive temperature dependence of the cross sections is evid ent in the long-wavelength tail of the spectrum, the room temperature cross section being about 15% higher at 270 nm than that obtained at 240 K. The recommended absorption cross sections, listed in Table 4-73, are the room temperature data of Bilde et al. [33] (originally listed at 1-nm intervals); values at 2-nm intervals are given for wavelengths above 212 nm, and values at 1-nm intervals are given or the region of the first absorption maximum (200–212 nm), where the absorption curve shows a somewhat irregular behavior.4-74 Table 4-73. Absorption Cross Sections of CHClBr 2 at 296 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

200 274.6 230 141.4 272 9.415 201 282.8 232 136.4 274 7.552 202 293.9 234 131.4 276 5.950 203 306.7 236 126.8 278 4.687 204 314.2 238 122.2 280 3.691 205 320.6 240 116.0 282 2.884 206 324.9 242 109.2 284 2.261 207 323.7 244 101.2 286 1.734 208 322.9 246 92.70 288 1.331 209 324.6 248 83.52 290 1.016 210 317.8 250 74.04 292 0.7907 211 306.2 252 64.83 294 0.6116 212 297.4 254 55.95 296 0.4583 214 279.4 256 47.67 298 0.3489 216 261.7 258 39.92 300 0.2692 218 234.9 260 33.35 302 0.2076 220 215.1 262 27.50 304 0.1588 222 199.1 264 22.50 306 0.1208 224 184.5 266 18.28 308 0.0945 226 165.3 268 14.78 310 0.0742 228 151.7 270 11.82 Note: 200–310 nm, Bilde et al. [33]

G12. CHCl 2 Br (Halon-1021) + h ν → Products. The absorption cross sections of CHCl 2 Br have been measured at room temperature and 106–200 nm by Ibuki et al. [172]; at room temperature and 201–270 nm by Cadman and Simons [64]; and at 253, 273 and 298 K and 200–320 nm by Bilde et al. [33]. The data of Cadman and Simons [64], which are given only in a plot in their paper, agree between 200 and 260 nm within ≤ 15% with the room temperature data of Bilde et al. [33], the absorption maximum, however, is shifted to lower wavelengths. The recommended absorption cross sections, listed in Table 4-74, are those reported by Bilde et al. [33].
A decrease of the absorption cross sections with decreasing temperature was observed between 298 and 253 K over the whole spectrum. The cross section in the absorption maximum, which has been observed at 220 nm by Bilde et al. [33], is approximately 6% lower at 253 K than at room temperature. An increasingly positive temperature dependence was observed at longer wavelengt hs, the room temperature cross section at 320 nm becoming about four times larger than those at 253 K.4-75 Table 4-74. Absorption Cross Sections of CHCl 2 Br at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

200 115.0 230 58.1 276 1.63 202 93.8 232 54.6 278 1.32 204 81.1 234 50.0 280 1.07 206 73.6 236 45.8 282 0.865 208 69.0 238 41.6 284 0.694 209 69.8 240 37.3 286 0.573 210 68.8 242 33.0 288 0.454 211 67.4 244 29.3 290 0.384 212 68.4 246 25.8 292 0.317 213 70.0 248 22.2 294 0.265 214 70.1 250 19.2 296 0.217 215 70.2 252 16.5 298 0.176 216 71.1 254 13.6 300 0.146 217 71.0 256 11.5 302 0.118 218 70.7 258 9.75 304 0.0962 219 71.3 260 8.19 306 0.0761 220 71.6 262 6.82 308 0.0617 221 70.6 264 5.61 310 0.0496 222 69.3 266 4.68 312 0.0395 223 68.7 268 3.74 314 0.0317 224 68.2 270 3.01 316 0.0259 226 65.2 272 2.48 318 0.0210 228 62.2 274 2.02 320 0.0171 Note: 200–320 nm, Bilde et al. [33].

G13. CCl 3 Br (Halon-1031) + h ν → Products. The absorption cross sections of CCl 3 Br have been measured at room temperature and 170–230 nm by Roxlo and Mandl [350] and at 207–305 nm by Cadman and Simons [64]. Both groups report their results as plots only. Estimated absorption cross sections are listed in Table 4-75, which are the results of Roxlo and Mandl [350] at 170–200 nm; the mean of the results of both groups at 205–230 nm; and the results of Cadman and Simons [64] at 235 305 nm.
Quantum yields for Br*( 2 P 1/2 ) atom formation in the photolysis at 234 and 265 nm, Φ (Br*) = 0.31 ± 0.01 and 0.68 ± 0.02, respectively, were reported by Jung et al. [195].

Table 4-75. Absorption Cross Sections of CCl 3 Br at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 600 220 49 270 19 175 600 225 46 275 11 180 1050 230 52 280 7.2 185 1100 235 50 285 5.0 190 850 240 50 290 3.3 195 530 245 49 295 2.2 200 230 250 48 300 1.4 205 140 255 46 305 1.0 210 90 260 42 215 66 265 34 Note: 170–200 nm, Roxlo and Mandl [350], 205 230 nm, mean of Roxlo and Mandl [350] and Cadman and Simons [64], 235–305 nm, Cadman and Simons [64].4-76 G14. CHF 2 Br (Halon-1201) + h ν → Products. The absorption cross sections of CHF 2 Br have been measured at room temperature and 207–255 nm by Davidson [104]; at 190–280 nm by Talukdar et al. [394]; and at 190– 280 nm by Orkin and Kasim ovskaya [302]. Gillotay et al. [138] carri ed out measurements at 210–295 K and in the wavelength range 166–267 nm and report only smoothe d values for T = 210, 230, 250, 270, and 295 K and at wavelengths corresponding to the wavenumber interval s generally used in stratospheric photodissociation calculations. The results of Davidson [104], Orkin and Kasimovs kaya [302], and Gillotay et al. [138] are in excellent agreement at wavelengths below 240 nm; the va lues of Gillotay et al. [138] become increasingly smaller by up to about 40% at 260 nm, and those of Da vidson [104] become smaller by up to about 30% at 250 nm than the values of Orkin and Kasimovskaya [ 302]. The results of Talukdar et al. [394], who report a plot on a logarithmic scale for measured values at 190–280 nm and extrapolated values up to 360 nm, appear to be in agreement with the results of Orkin and Kasimovs kaya [302]. The preferred values, listed in Table 4-76, are the values of Gillotay et al. [138] at the centers of the 500-cm –1 intervals between 168 and 188 nm, and the values of Orkin and Kasimovskaya [302] at 190–280 nm.
With decreasing temperature 295–210 K, an increase of the absorption cross sections around the absorption maximum at 168–215 nm and a decrease at wavelengths above 215 nm was obs erved by Gillotay et al. [104] (the interpolation formula has not been reported for this molecule)

. Table 4-76. Absorption Cross Sections of CHF 2 Br at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) 168.10 3.97 206 23.2 246 0.299 170.95 8.21 208 21.2 248 0.220 173.15 12.5 210 19.0 250 0.161 174.65 15.6 212 16.8 252 0.117 176.20 18.8 214 14.6 254 0.0849 177.80 21.9 216 12.6 256 0.0615 179.40 24.5 218 10.6 258 0.0444 181.00 26.6 220 8.85 260 0.0319 182.65 28.3 222 7.25 262 0.0230 184.35 29.6 224 5.88 264 0.0166 186.05 30.6 226 4.71 266 0.0121 187.80 31.4 228 3.73 268 0.0087 190 32.5 230 2.91 270 0.0063 192 32.4 232 2.24 272 0.0046 194 31.8 234 1.71 274 0.0034 196 31.0 236 1.30 276 0.0024 198 29.9 238 0.982 278 0.0018 200 28.6 240 0.735 280 0.0012 202 27.0 242 0.547 204 25.2 244 0.405 Note: 168–188 nm, Gillotay et al. [138], 190–280 nm, Orkin and Kasimovskaya [302].

G15. CF 2 Br 2 (Halon-1202) + h ν → Products. The absorption cross sections of CF 2 Br 2 have been measured at room temperature and 215–290 nm by Davidson [104]; at 200–310 nm by Walton et al. [428]; at 190–340 nm by Molina et al. [272]; at 190–320 nm by Orkin and Kasimovskaya [302]; at 210–295 K and 170–304 nm by Gillotay and Simon [134]; and at 210–296 K and 190–320 nm by Burkholder et al. [57]. The room temperature data, except those of Walton [428], are in good agreement, i.e., better than 10%, over their common wavelength range from 190 to 300 nm. In the absorption maximum around 226 nm, the older data of Davidson [172] and Molina et al. [272] are the highest a nd lowest, respectively, and the more recent data agree within 5% (the absorption maximum reported by Walton [428] is larger by ~50%). At wavelengths above 300 nm, the values of Orkin and Kasimovskaya [302] and Burkholder et al. [57] agree within 15%, whereas those of Molina et al. [272] become increasingly larger by up to ~200% at 320 nm ( and larger by up to ~660% than the extrapolated values at 340 nm, see below). The preferred absorption cross sections, listed in Table 4-77, are the values of Gillotay and Simon [134] at 170–188 nm; the mean of the values reported by Gillota y and Simon [134], Orkin and Kasimovskaya [302], and Burkholder et al. [57] for the wavelength range 190–304 nm; and the mean of the values reported by the latter two groups for the range 306–320 nm. For wavelengths 322–340 nm, the mean4-77 of the values of Orkin and Kasimovskaya [302], and Burkholder et al.[57] for the range 306–320 nm have been extrapolated (log σ = 1.85109 – 0.07755 λ ).
Measurements in the far UV were reported by Doucet et al. [109] for the wavelength range 60–220 nm and by Seccombe et al. [369] for the wavelength range 55–175 nm.
Both studies of the temperature dependence show an increase of the absorption cr oss sections in the two absorption bands around 190 and 226 nm with decreasing temperature 296–210 K and the reverse effect at wavelengths above 240 nm and below 177 nm. Gillotay and Simon [134] observed a regular temperature behavior, i.e., an increase of the maximum absorption cross section at ~225 nm by ~0.09 × 10 –18 cm 2 molecule

–
1 per 20-K temperature decrease. Burkholder et al.[57] observed a less pronounced temperature behavior below 250 K (the maximum absorption cross sections agree within 1%), so that their maximum cross section at 210 K is lower by 5% than that observed by Gillotay and Sim on [134] (in contrast to th e cross sections at room temperature which are nearly identi cal). Different parameterizations for the temperature dependence of the absorption cross section have been proposed. Gillotay and Simon [134] give the polynomial expansion log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n and report smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wa venumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges 222–304 nm and 210–300 K are as follows:

A 0 = –206.2 B 0 = 1.0460 × 10 –1
A 1 = 2.3726 B 1 = –1.4124 × 10 –3
A 2 = –1.0527 × 10 –2 B 2 = 6.9015 × 10 –6
A 3 = 1.9239 × 10 –5 B 3 = –1.5164 × 10 –8
A 4 = –1.2242 × 10 –8 B 4 = 1.3990 × 10 –11

Burkholder et al. [57] give the expansion
log 10 σ ( λ , T) = ( ∑ A i ( λ – 268.7998) I ) (1 + (296–T) ∑ B i ( λ – 268.7998) I )
and report the following parameters A i and B i for the ranges 235–260 nm and 210–296 K:

A 0 = –44.42756 B 0 = 1.481886 × 10 –4
A 1 = –1.464955 × 10 –1 B 1 = 6.77182 × 10 –6
A 2 = –5.692188 × 10 –4 B 2 = 1.154347 × 10 –7
A 3 = 1.155366 × 10 –5 B 3 = –2.77145 × 10 –11
A 4 = –1.399502 × 10 –7 B 4 = –6.619515 × 10 –11

A parameterization for extrapolated absorption cross sections up to 400 nm,

log 10 σ ( λ , T) = ( ∑ A i ( λ – 301.0104) I ) + ( λ – 260) ( ∑ B i (T – 251.2) I )

has also been reported by Burkholder et al. [57].
The quantum yield for formation of CF 2 O and Br 2 in the photolysis of CF 2 Br 2 at 206, 248, and 302 nm, in the presence of O 2 has been measured to be unity by Molina and Mo lina [269], independent of pressure, in contrast to an earlier report by Walton [428] that the quantum yield at 265 nm decreases from unity when the system pressure is raised to 50 torr of CO 2 . Primary quantum yields for Br atom formation, Φ (Br) = 1.96 ± 0.27, 1.63 ± 0.19, and 1.01 ± 0.15, in the photodissociation of CF 2 Br 2 at 193, 222, and 248 nm, respectively, were measured at 298 K by Talukdar et al. [399]. A quantum yield for CF 2 formation, Φ (CF 2 ) = 1.15 ± 0.30, in the 193-nm photolysis was reported by Talukdar et al. [397].4-78 Table 4-77. Absorption Cross Sections of CF 2 Br 2 at 295–296 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 124.5 228 253.4 286 0.336 172 78.1 230 244.7 288 0.245 174 55.3 232 230.2 290 0.178 176 49.5 234 211.9 292 0.128 178 60.3 236 191.6 294 0.0926 180 75.0 238 169.3 296 0.0672 182 86.6 240 147.3 298 0.0487 184 100.9 242 125.8 300 0.0352 186 111.8 244 106.0 302 0.0253 188 118.0 246 87.8 304 0.0183 190 115.9 248 72.0 306 0.0130 192 110.3 250 58.3 308 0.00919 194 101.6 252 46.5 310 0.00650 196 91.4 254 36.8 312 0.00456 198 82.1 256 28.9 314 0.00319 200 74.9 258 22.4 316 0.00222 202 71.7 260 17.3 318 0.00157 204 73.4 262 13.1 320 0.00105 206 80.7 264 9.90 322 0.000759 208 93.0 266 7.47 324 0.000531 210 110.0 268 5.59 326 0.000371 212 131.0 270 4.17 328 0.000260 214 154.9 272 3.08 330 0.000182 216 180.4 274 2.27 332 0.000127 218 204.7 276 1.66 334 0.000089 220 226.0 278 1.21 336 0.000062 222 244.2 280 0.888 338 0.000044 224 253.3 282 0.647 340 0.000030 226 256.8 284 0.470 Note: 170 188 nm: Gillotay and Simon [134] 190–304 nm: mean of Gillotay and Sim on [134], Orkin and Ka simovskaya [302], and Burkholder et al. [57] 306–320 nm: mean of Orkin and Kasimovskaya [302] and Burkholder et al.[57] 322–340 nm: extrapolation of mean of Orkin and Kasimovskaya [302], and Burkholder et al. [57] data.

G16. CF 2 ClBr (Halon-1211) + h ν → Products. The absorption cross sections of CF 2 ClBr have been measured at room temperature and 191–307 nm by Giolando et al. [140]; at 190–330 nm by Molina et al. [272]; at 190– 304 nm by Orkin and Kasimovskaya [302]; at 210–295 K and 170–302 nm by G illotay and Simon [134]; and at 210–296 K and 190–320 nm by Burkholder et al. [57]. The agreement between the room temperature data of Orkin and Kasimovskaya [302], Gillota y and Simon [134], and Bu rkholder et al. [57] is very good in the region of the absorption band, i.e., within 10% over the range 190–240 nm and within 3% in the maximum at 205– 206 nm, with one exception: Gillotay and Simon [134] observed a structure near the absorption maximum, different from the other observations, which resulted in values higher by about 10% at 200–202 nm. Molina et al. [272] reported values for the range 190–240 nm which are lower by 10–20% than the above mentioned data. The few data points (at 10-nm intervals) of Giolando et al. [140] fit well to the absorption curves reported by Orkin and Kasimovskaya [302], Gillota y and Simon [134], and Bu rkholder et al. [57]. Th e deviations between the various data sets increase at longer wavelengths to ≤ 30% at 300 nm and up to 55% at 320 nm. The preferred absorption cross sections at 295–298 K, listed in Table 4-78, are the values of Gillotay and Simon [134] at 170–188 nm; the mean of the values reported by Molina et al. [272], Gillotay and Simon [134], Burkholder et al. [57] and Orkin and Kasimovskaya [ 302] at 190–302 nm; the mean of the values reported by Molina et al. [272], Burkholder et al. [57], and Orkin and Kasimovskaya [302] at 304 nm; and the mean of the values reported by Molina et al. [272] and Burkholder et al. [57] at 306–320 nm.
Measurements in the far UV at 60–220 nm were reported by Doucet et al. [109].4-79 Both studies of the temperature dependence show an incr ease of the absorption cross sections in the absorption band around 204–206 nm with decreasing temperature 296–210 K and the reverse effect at wavelengths above 233 nm and below 180 nm. Gillotay and Simon [134] observe d a regular temperature behavior, i.e., an increase of the maximum absorption cross section by ~0.05 × 10 –18 cm 2 molecule –1 per 20 K temperature decrease. Burkholder et al. [57] observed a less pronounced temperature behavior (the maximum absorption cross sections agree within 2.5%), so that their maximum cross section at 210 K is lower by 15% than that observed by Gillotay and Simon [134] (in contrast to the cross sections at room temperature which are within 4%). Different parameterizations for the temperature dependen ce of the absorption cross section have been proposed. Gillotay and Simon [134] give the polynomial expansion

log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n

and report smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges 200–302 nm and 210–300 K are as follows:

A 0 = –134.80 B 0 = 3.3070 × 10 –1

A 1 = 1.7084 B 1 = –5.0957 × 10 –3

A 2 = –9.1540 × 10 –3 B 2 = 2.9361 × 10 –5

A 3 = 2.1644 × 10 –5 B 3 = –7.6198 × 10 –8

A 4 = –1.9863 × 10 –8 B 4 = 7.6825 × 10 –11

Burkholder et al. [57] give the expansion

log 10 σ ( λ , T) = ( ∑ A i ( λ – 259.8989) I ) (1 + (296–T) ∑ B i ( λ – 259.8989) I )

and report the following parameters A i and B i for the ranges 220–260 nm and 210–296 K:

A 0 = –45.4087 B 0 = 1.528905 × 10 –4

A 1 = –1.304811 × 10 –1 B 1 = 6.024833 × 10 –6

A 2 = –6.995443 × 10 –4 B 2 = 1.030995 × 10 –7

A 3 = 6.159709 × 10 –6 B 3 = –6.387931 × 10 –11

A 4 = –9.384074 × 10 –9 B 4 = –3.718503 × 10 –11

A parameterization for extrapolated absorption cross sections up to 400 nm,
log 10 σ ( λ , T) = ( ∑ A i ( λ – 292.2083) I ) + ( λ – 260) ( ∑ B i (T – 251.2) I )
has also been reported by Burkholder et al. [57].
Quantum yields for Cl and Br atom formation in the photodissociation of CF 2 ClBr at 193, 222, and 248 nm, Φ (Cl) = 1.03 ± 0.14, 0.27 ± 0.04, and 0.18 ± 003, Φ (Br) = 1.04 ± 0.13, 0.86 ± 0.11, and 0.75 ± 0.13, respectively, and a quantum yield for CF 2 formation in the 193-nm photolysis, Φ (CF 2 ) = 0.91 ± 0.30, were measured at 298 K by Talukdar et al. [397].4-80 Table 4-78. Absorption Cross Sections of CF 2 ClBr at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 323.0 222 68.3 274 0.250 172 234.2 224 60.4 276 0.184 174 176.0 226 52.7 278 0.135 176 120.9 228 45.7 280 0.0991 178 84.7 230 39.2 282 0.0724 180 58.1 232 33.8 284 0.0527 182 41.9 234 28.8 286 0.0385 184 35.0 236 24.4 288 0.0282 186 34.1 238 20.4 290 0.0205 188 38.9 240 16.9 292 0.0148 190 46.1 242 13.9 294 0.0106 192 57.0 244 11.4 296 0.00764 194 69.1 246 9.28 298 0.00544 196 81.4 248 7.50 300 0.00391 198 93.5 250 5.99 302 0.00279 200 106.0 252 4.76 304 0.00207 202 113.3 254 3.76 306 0.00161 204 117.4 256 2.94 308 0.00113 206 118.7 258 2.29 310 0.000803 208 117.7 260 1.76 312 0.000569 210 114.2 262 1.36 314 0.000403 212 108.5 264 1.03 316 0.000288 214 101.5 266 0.784 318 0.000213 216 93.6 268 0.593 320 0.000159 218 85.3 270 0.447 220 76.8 272 0.336 Note: 170–188 nm: Gillotay and Simon [134] 190–302 nm: mean of Molina et al. [272], Gillotay and Simon [134], Burkhol der et al. [57], and Orkin and Kasimovskaya [302] 304 nm: mean of Molina et al. [272], Burkholder et al. [57], and Orkin and Kasimovskaya [302] 306–320 nm: mean of Molina et al. [272] and Burkholder et al. [57]. G17. CF 3 Br (Halon-1301) + h ν → Products. The absorption cross sections of CF 3 Br have been measured at room temperature and 207–255 nm by Davidson [172]; at 170–230 nm by Roxlo and Mandl [350]; at 180–400 nm by Pence et al. [312]; at 190–300 nm by Molina et al. [272]; at 190–270 nm by Orkin and Kasimovskaya [302]; at 210–295 K and 168–280 nm by Gillotay and Simon [134] ; and at 210–296 K and 190–285 nm by Burkholder et al. [57]. The agreement between the room temperature data is very good, i.e., 10% and better, in the region of the absorption band between 190 and 230 nm with the exception of the data of Davidson [253] below 210 nm and the whole data set of Roxlo and Mandl [350]. Pence et al. [312] report a plot of the absorbance (in arbitrary units) and give for 193 nm an absorption cross s ection smaller by one order of magnitude than the rest of the data for 193 nm. At wavelengths above 250 nm, Burkholder et al. [57] and Orkin and Kasimovskaya [302] measured higher values (up to ~ 35% at 270 nm) th an those reported by Molina et al. [272] and Gillotay and Simon [134]. The preferred absorption cross sections at 295–298 K, listed in Table 4-79, are the values of Gillotay and Simon [134] at 168–188 nm, the mean of the values reported by Molina et al. [272], Gillotay and Simon [134], Burkholder et al. [57], and Orkin and Kasimovskaya [302] at 190–270 nm, the mean of the values reported by Molina et al. [272], G illotay and Simon [134], and Burkholde r et al. [57] at 272–280 nm, and the values of Molina et al. [272] at 295–300 nm.
Measurements in the far UV at 60–220 nm were reported by Doucet et al. [109].
Both studies of the temperature dependence show an incr ease of the absorption cross sections in the absorption band between 174 and 216 nm with decreasing temperat ure 296–210 K and the reverse effect at wavelengths above 218 nm and below 174 nm. Gillota y and Simon [134] observed a regular temperature behavior, i.e., an increase of the maximum absorption cross section by ~0.06 × 10 –19 cm 2 molecule –1 per 20 K temperature decrease. Burkholder et al. [57] observed a less pronounced temperature behavior (the maximum absorption cross sections agree within 2%), so that their maximum cross section at 210 K is lower by ~25% than that4-81 observed by Gillotay and Simon [134] (i n contrast to the cross sections at room temperature which are within 6%). Different parameteriza tions for the temperature dependence of the absorption cross section have been proposed. Gillotay and Simon [134] give the polynomial expansion

log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n

and report smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges 178–280 nm and 210–300 K are as follows:

A 0 = 62.563 B 0 = –9.1755 × 10 –1

A 1 = –2.0068 B 1 = 1.8575 × 10 –2

A 2 = 1.6592 × 10 –2 B 2 = –1.3857 × 10 –4

A 3 = –5.6465 × 10 –5 B 3 = 4.5066 × 10 –7

A 4 = 6.7459 × 10 –8 B 4 = –5.3803 × 10 –10

Burkholder et al. [57] give the expansion

log 10 σ ( λ , T) = ( ∑ A i ( λ – 242.2466) I ) (1 + (296–T) ∑ B i ( λ – 242.266) I )

and report the following parameters A i and B i for the ranges 214–285 nm and 210–296 K:

A 0 = –46.70542 B 0 = 1.694026 × 10 –4

A 1 = –1.55047 × 10 –1 B 1 = 8.723247 × 10 –6

A 2 = –1.020187 × 10 –3 B 2 = 5.953165 × 10 –9

A 3 = 2.246169 × 10 –5 B 3 = –3.872168 × 10 –9

A 4 = –1.300982 × 10 –7 B 4 = –1.803325 × 10 –11

Quantum yields for Br (Br( 2 P 3/2 + Br*( 2 P 1/2 )) atom formation in the photodissociation of CF 3 Br at 193 and 222 nm, Φ (Br+Br*) = 1.12 ± 0.16 and 0.92 ± 0.15, respectivel y, were measured at 298 K by Talukdar et al. [399]. A quantum yield for Br*( 2 P 1/2 ) atom formation at 193 nm, Φ (Br*) = 0.56 ± 0.05, was reported by Pence et al. [312].4-82 Table 4-79. Absorption Cross Sections of CF 3 Br at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

168 0.517 210 12.1 252 0.107 170 0.696 212 11.4 254 0.0743 172 0.928 214 10.6 256 0.0516 174 1.22 216 9.71 258 0.0357 176 1.60 218 8.65 260 0.0248 178 2.05 220 7.56 262 0.0171 180 2.61 222 6.50 264 0.0118 182 3.26 224 5.47 266 0.00827 184 4.02 226 4.52 268 0.00580 186 4.88 228 3.69 270 0.00399 188 5.82 230 2.91 272 0.00271 190 6.56 232 2.32 274 0.00188 192 7.58 234 1.80 276 0.00129 194 8.63 236 1.39 278 0.00092 196 9.61 238 1.04 280 0.00064 198 10.5 240 0.766 285 0.00022 200 11.3 242 0.563 290 0.00008 202 11.9 244 0.414 295 0.00003 204 12.4 246 0.296 300 0.00001 206 12.5 248 0.212 208 12.4 250 0.149 Note: 170–188 nm: Gillotay and Simon [134] 190–270 nm: mean of Molina et al. [272], G illotay and Simon [134], Bu rkholder et al. [57] and Orkin and Kasimovskaya [302] 272–280 nm: mean of Molina et al.[272] and Burkholder et al. [57] 285–300 nm: Molina et al. [272].

G18. CF 3 CH 2 Br (Halon-2301) + h ν → Products. The absorption cross sections of CF 3 CH 2 Br have been measured at 295 K and 190–294 nm by Orkin and Kasimovskaya [302]. Their results are listed in Table 4-80.

Table 4-80. Absorption Cross Sections of CF 3 CH 2 Br at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 45.4 226 16.6 262 0.190 192 49.5 228 14.1 264 0.137 194 52.5 230 11.9 266 0.0983 196 54.4 232 9.85 268 0.0705 198 55.1 234 8.10 270 0.0504 200 54.7 236 6.58 272 0.0361 202 53.3 238 5.28 274 0.0258 204 51.2 240 4.20 276 0.0184 206 48.6 242 3.31 278 0.0132 208 45.7 244 2.58 280 0.0096 210 42.5 246 2.01 282 0.0069 212 39.1 248 1.53 284 0.0048 214 35.7 250 1.16 286 0.0034 216 32.2 252 0.876 288 0.0025 218 28.8 254 0.653 290 0.0018 220 25.5 256 0.484 292 0.0013 222 22.3 258 0.357 294 0.0011 224 19.4 260 0.261 Note: 190–294 nm, Orkin and Kasimovskaya [302].4-83 G19. CF 3 CHClBr (Halon-2311) + h ν → Products. The absorption cross sections of CF 3 CHClBr have been measured at room temperature and 190–310 nm by Orkin and Kasimovskaya [302]; at 210–295 K and 170–290 nm by Gillotay et al. [138]; and at 223–298 K and 200–310 nm by Bilde et al. [33]. The room temperature values are in good agreement within 5–15% at wavelengt hs below 280 nm, where Gillotay et al. [138], [135] report the lowest, Orkin and Kasimovskaya [302] the highe st values. At wavelengths above 280 nm, the data of Bilde et al. [33] become increasingly higher (up to 100% at 310 nm) than those of Orkin and Kasimovskaya [302]. The preferred absorption cross sections, listed in Ta ble 4-81, are the values of Gillotay et al. [138] at 170–188 nm; the mean of the values reported by Gillotay et al. [138] and Orkin a nd Kasimovskaya [302] at 190–198 nm; the mean of the values reported by the three groups at 200–290 nm; and the mean of the values reported by Orkin and Kasimovskaya [302] and Bilde et al. [33] at 292–310 nm.
The study of the temperature dependence by Gillotay et al. [138] shows an increas e of the absorption cross sections in the absorption band between 192 and 238 nm with decreasing temperature 295–210 K and the reverse effect at wavelengths a bove 238 nm and below 192 nm; the increase in the absorption maximum at ~202 nm is ~0.024 × 10 –18 cm 2 molecule –1 per 20 K temperature decrease, i.e., an increase by ~10% between 295 and 210 K. Bilde et al. [33] observed a less pronounced temperature behavior in the absorption band (the maximum absorption cross sections ag ree within 3%) and a decrease of th e absorption cross sections with decreasing temperature at wavelengths above 214 nm.
Gillotay and Simon [138] parameterized the cross secti ons and the temperature dependence of the absorption cross section by the polynomial expansion

log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n

and report smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges 190–290 nm and 210–300 K are as follows:

A 0 = –127.157358 B 0 = –7.959828 × 10 –2

A 1 = 1.635435 B 1 = 1.978026 × 10 –3

A 2 = –9.002683 × 10 –3 B 2 = –1.627866 × 10 –5

A 3 = 2.190678 × 10 –5 B 3 = 5.480744 × 10 –8

A 4 = 2.062651 × 10 –8 B 4 = –6.480935 × 10 –114-84 Table 4-81. Absorption Cross Sections of CF 3 CHClBr at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 702.6 218 78.7 266 0.980 172 614.6 220 71.0 268 0.765 174 496.8 222 63.3 270 0.575 176 379.8 224 56.3 272 0.444 178 281.1 226 49.5 274 0.339 180 206.1 228 43.3 276 0.258 182 153.3 230 37.3 278 0.196 184 118.4 232 32.2 280 0.149 186 97.1 234 27.6 282 0.111 188 86.6 236 23.6 284 0.0818 190 93.4 238 20.0 286 0.0606 192 99.8 240 16.8 288 0.0448 194 107.1 242 14.0 290 0.0331 196 114.3 244 11.7 292 0.0263 198 119.7 246 9.51 294 0.0198 200 121.5 248 7.79 296 0.0147 202 123.0 250 6.38 298 0.0109 204 122.3 252 5.15 300 0.00808 206 119.7 254 4.13 302 0.00583 208 115.1 256 3.31 304 0.00450 210 109.0 258 2.63 306 0.00313 212 102.0 260 2.06 308 0.00235 214 94.6 262 1.61 310 0.00180 216 86.7 264 1.26 Note: 170–188 nm, Gillotay et al. [138], [135], 190–198 nm, mean of Gillotay et al. [138][135] and Orkin and Kasimovskaya [302], 200–290 nm, mean of Gillotay et al. [138][135], Orkin and Ka simovskaya [302], and Bilde et al. [33], 292–310 nm, mean of Orkin and Kasimovskaya [302] and Bilde et al. [33].

G20. CF 3 CHFBr (Halon-2401) + h ν → Products. The absorption cross sections of CF 3 CHFBr have been measured at 295 K and 190–280 nm by Orkin and Kasimovskaya [302]. Their results are listed in Table 4-82.

Table 4-82. Absorption Cross Sections of CF 3 CHFBr at 295 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 24.9 222 11.0 254 0.226 192 26.1 224 9.38 256 0.166 194 27.0 226 7.91 258 0.121 196 27.5 228 6.58 260 0.0873 198 27.7 230 5.42 262 0.0628 200 27.4 232 4.42 264 0.0450 202 26.9 234 3.53 266 0.0325 204 26.0 236 2.79 268 0.0235 206 24.8 238 2.19 270 0.0171 208 23.4 240 1.69 272 0.0124 210 21.9 242 1.30 274 0.0093 212 20.2 244 0.991 276 0.0069 214 18.3 246 0.736 278 0.0053 216 16.5 248 0.556 280 0.0040 218 14.6 250 0.416 220 12.8 252 0.308 Note: 190–280 nm, Orkin and Kasimovskaya [302].4-85 G21. CF 2 BrCF 2 Br (Halon-2402) + h ν → Products. The absorption cross sections of CF 2 BrCF 2 Br have been measured at room temperature and 195–320 nm by Molina et al. [272] and at 190–300 nm by Orkin and Kasimovskaya [302]; at 210–295 K and 170–280 nm by Gillotay et al . [138], and at 210–296 K and 190–320 nm by Burkholder et al. [57]. The room temperature data are in very good agreement, in the absorption band at180–240 nm generally within 10%, in the absorption maximum at ~200 nm within 5%, and in the longwavelength tail up to 310 nm within 15 %. The preferred absorption cross sections at 295–298 K, listed in Table 4-83, are the values of Gillotay et al. [138] at 170–186 nm; the mean of the values reported by Molina et al. [40], Gillotay et al. [138], Bur kholder et al. [57], and Orkin and Kasimovskaya [302] at 196–280 nm; the mean of the values reported by Molina et al. [272], Burkholder et al. [57], and Orkin and Kasimovskaya [302] at 282–300 nm; and the mean of the values reported by Molina et al. [272] and Burkholder et al. [57] at 302– 320 nm. In the region around 190 nm, there is some uncer tainty, because there is no continuous transition between the absorption curve of Gillotay et al. [138] and th at obtained by averaging th e data of Gillotay et al. [138], Burkholder et al. [57], and Orkin and Kasimovskaya [302]. We therefore smoothed the absorption curve between 186 and 196 nm and give estimated values for 188, 190, 192, and 194 nm.
The results of the two temperature studies are rather controversial. A regular, but weak decrease of the absorption cross sections at 194–280 nm with decreasing temperature 295 to 210 K and the reverse effect below 194 nm was observed by Gillotay et al. [138]; th e decrease in the absorption maximum at ~200 nm is ~0.010 × 10 –18 cm 2 molecule –1 per 20-K temperature decrease, i.e., a decrease by ~4% between 295 and 210 K. Burkholder et al. [57] observed a strong increase over the whole absorption band (increase of the absorptionmaximum by 20%) with decreasing temperature 296–210 K, and the reverse effect above 230 nm. So, lowtemperature data of these two groups are not comparable Different parameterizations of the temperature dependence of the absorption cross section have been proposed. Gillotay and Simon [350] give the polynomial expansion

log 10 σ ( λ , T) = ∑ A n λ n + (T – 273) × ∑ B n λ n

and report smoothed values for T = 210, 230, 250, 270, and 295 K, every 2 nm, and at wavelengths corresponding to the wavenumber intervals generally used in stratospheric photodissociation calculations. The parameters A n and B n for the ranges 190–290 nm and 210–300 K are as follows:

A 0 = 34.026000 B 0 = 4.010664 × 10 –1
A 1 = –1.152616 B 1 = –8.358968 × 10 –3
A 2 = 8.959798 × 10 –3 B 2 = 6.415741 × 10 –5
A 3 = –2.9089 × 10 –5 B 3 = –2.157554 × 10 –7
A 4 = 3.307212 × 10 –8 B 4 = 2.691871 × 10 –10 Burkholder et al. [57] give the expansion

log 10 σ ( λ , T) = ( ∑ A i ( λ – 242.4015) i ) (1 + (296–T) ∑ B i ( λ – 242.4015) i )

and report the following parameters A i and B i for the ranges 190–320 nm and 210–296 K:

A 0 = –43.69218 B 0 = 3.301341 × 10 –5
A 1 = –1.124704 × 10 –1 B 1 = 4.695917 × 10 –6
A 2 = –1.213301 × 10 –3 B 2 = 6.128629 × 10 –8
A 3 = 5.275007 × 10 –6 B 3 = –5.443107 × 10 –10
A 4 = 6.936195 × 10 –8 B 4 = –1.035596 × 10 –11 Quantum yields for Br atom formation in the photodissociation of CF 2 BrCF 2 Br at 193, 233, and 266 nm, Φ (Br) = 1.9 ± 0.1, 1.9 ± 0.1, and 1.4 ± 0.1, respectively, were measured at room temperature by Zou et al. [453]. These values indicate bond breaking of both C–Br bonds in nearly all the CF 2 BrCF 2 Br molecules at 193 and 233 nm and in an appreciable fraction of the parent molecules still at 266 nm.4-86 Table 4-83. Absorption Cross Sections of CF 2 BrCF 2 Br at 296 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

170 50.9 222 59.6 274 0.112 172 56.4 224 52.6 276 0.0813 174 62.3 226 45.9 278 0.0592 176 68.5 228 39.7 280 0.0428 178 75.1 230 33.9 282 0.0300 180 81.8 232 28.8 284 0.0216 182 88.6 234 24.1 286 0.0152 184 95.3 236 19.9 288 0.0109 186 101.8 238 16.4 290 0.00784 188 107.0 240 13.2 292 0.00569 190 112.0 242 10.6 294 0.00410 192 116.5 244 8.45 296 0.00301 194 120.0 246 6.68 298 0.00219 196 122.3 248 5.25 300 0.00161 198 123.7 250 4.03 302 0.00124 200 124.3 252 3.12 304 0.00094 202 123.6 254 2.37 306 0.00071 204 120.3 256 1.78 308 0.00054 206 115.9 258 1.34 310 0.00042 208 110.4 260 0.973 312 0.00033 210 104.2 262 0.718 314 0.00026 212 97.4 264 0.529 316 0.00020 214 90.1 266 0.390 318 0.00016 216 82.4 268 0.287 320 0.00014 218 74.8 270 0.211 220 67.0 272 0.154 Note: 170–186 nm: Gillotay et al. [138] 188–194 nm: values estimated by smoothing the absorption curve 196–280 nm: mean of Molina et al. [272], Gillotay et al. [138], Burkholder et al. [57], and Orkin and Kasimovskaya [302] 282–300 nm: mean of Molina et al. [272], Burkholder et al. [57], and Orkin and Kasimovskaya [302] 302–320 nm: mean of Molina et al. [272] and Burkholder et al. [57].

G22. CF 3 CF 2 Br (Halon-2501) + h ν → Products. Table 4-84 lists the absorption cross sections of CF 3 CF 2 Br measured at room temperature and reported at 5-nm intervals by Molina et al. [272]. The results of Zhang et al. [451], who report a plot on a logarithmic scale for measured values at 200–250 nm, are about 30% larger over that wavelength range than the results of Molina et al. [272]. Pence et al. [312] measured the absorption cross sections at 180–400 nm, report a plot of the absorbance (in arbitrary units) and give for 193 nm an absorption cross section smaller by ~ 40% than that reported by Molina et al. [272].
Broad band flash photolysis of CF 3 CF 2 Br produced Br*( 2 P 1/2 ) atoms with a quantum yield Φ (Br*) = 0.48 ± 0.02 as reported by Ebenstein et al. [112]. A quantum yield for Br*( 2 P 1/2 ) atom formation at 193 nm, Φ (Br*) = 0.16 ± 0.08, was reported by Pence et al. [312].4-87 Table 4-84. Absorption Cross Sections of CF 3 CF 2 Br at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 18.1 230 3.83 270 0.0112 195 18.4 235 2.22 275 0.00505 200 18.1 240 1.20 280 0.00218 205 16.9 245 0.620 285 0.00100 210 14.8 250 0.305 290 0.00045 215 12.0 255 0.135 295 0.00020 220 8.94 260 0.0590 300 0.00009 225 6.13 265 0.0260 Note: 190–300 nm, Molina et al. [272].

H1. CH 3 I + h ν → CH 3 + I( 2 P 3/2 ).

H2. CH 3 I + h ν → CH 3 + I*( 2 P 1/2 ).
The absorption cross sections of CH 3 I have been measured at room temperature and 147 nm by Rebbert et al. [334], at 200–360 nm by Porret and Goodeve [317], at 200–310 nm by Baughcum and Leone [29], at 180– 400 nm by Pence et al. [312]; at 257.7 nm by Felps et al. [119], at 205–335 nm by Jenkin et al. [182], at 205– 360 nm by Man et al. [ 230], and at 192–225 nm by Kwok and Phillip s [208], who also measured the CH 3 I spectrum in cyclohexane solution. Measurements were also carried out at 223–333 K and 160–330 nm by Fahr et al. [116]; at 243–333 K and 235–365 nm by Rattigan et al. [325] ; and at 210–298 K and 200–350 nm by Roehl et al. [343]. Fahr et al. [116] also measured the absorption cross sections at 330–400 nm for the liquid phase and used a wavelength-shift procedure to convert th em into gas-phase values. The room temperature data for the absorption band at 210–305 nm are in reasonable to good agreement, whereb y Rattigan et al. [325] report the lowest values and Fahr et al. [116] the highe st values over the whole absorption band. The agreement generally is better than 15% except for the region around the absorption maximum where the spread is ~30%: Rattigan et al. [325] and Fahr et al. [116] report values of 1.07 × 10 –18 cm 2 and 1.4 × 10 –18 cm 2 , respectively, for the maximum at ~260 nm, and the rest of the data ranges between 1.15 × 10 –18 cm 2 and 1.22 × 10 –18 cm 2 . At wavelengths 305–330 nm, the agreement is still within 20% . At wavelengths below 210 nm, the few data points reported by Jenkin et al. [ 182] and Roehl et al. [343] and the abso rption curve reported by Kwok and Phillips [209] obviously fit into the strong and highly structured band system observed by Fahr et al. [116] between 160 and 205 nm. The preferred room temperature absorption cross sections for the wavelength range above 210 nm, listed in Table 4-85, are the mean of the values reported by Jenkin et al. [182], Fahr et al. [116], and Roehl et al. [343] at 210–230 nm; the mean of the values reported by Jenkin et al. [182], Fahr et al . [116], Rattigan et al. [325], and Roehl et al. [343] at 235–330 nm; the mean of the values reporte d by Fahr et al. [ 116], Rattigan et al. [325], and Roehl et al. [343] at 335–350 nm; and the values of Rattigan et al. [325] at 355–365 nm. The data of Man et al. [230] are given only as a plot in their paper and have therefore not been included in the evaluation.
The three temperature studies are in qualitative agreement. An increase of the absorption cross sections in the absorption band at 210–270 nm with decreasing temperature 333–210 K has been observed. Very small temperature effects are reported by Rattigan et al. [ 325] for the temperature range 243–333 K, and by Fahr et al. [116] and Roehl et al. [343] for the range between room temperature and ~240–250 K and at 313–333 K. At wavelengths above 270 nm and below 210 nm, the abso rption cross sections decrease with decreasing temperature. The low temperature absorption spectra observed by the three groups differ in the same manner as their room temperature spectra, i.e., Fahr et al. [116] report the highest and Rattigan et al. [325] the lowest values for the absorption band.
A simple analytical expression for the temperature dependence,

σ ( λ , T) = σ (298 K) (1 + a 1 (T–298) + a 2 (T–298) 2 )
and the fitting parameters a 1 ( λ ) and a 2 ( λ ) for λ = 200–350 nm and T = 210– 298 K give Roehl et al. [343]. Another simple parameterization, ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298), and parameters B( λ ) for λ = 235–355 nm and T = 243–333 K report Rattigan et al. [325]. The parameters a 1 , a 2 , and B are listed also in Table 4-85.
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of CH 3 I at several wavelengths between 222 and 333.5 nm have been reported: Φ (I*) = 0.63 ± 0.02, 0.79 ± 0.02, 0.69 ± 0.02, and 0.43 ± 0.02 at 222, 266, 280,4-88 and ~305 nm by Uma and Das [410], [411], [412]; Φ (I*) = 0.72 ± 0.08 at 248 nm by Gedanken [412], Φ (I*) = 0.81 ± 0.03 and ~ 0.05 at 248 and 308 nm by Pence et al. [312], Φ (I*) = 0.30 at 304 nm by Kang et al. [198]; and Φ (I*) = 0.47, 0.77, and 0.92 at 325.8, 329.4, and 333.5 nm by Ogorzalek Loo et al. [298]. The latter authors report also quantum yields for CD 3 I:

Φ (I*): 0.66 0.59 0.83 0.91 0.90 0.57 0.80 0.92 >0.95 0.61 0.84

λ , nm: 312.6 314.4 317.0 319.8 322.9 324.5 327.8 330.5 333.8 336.2 339.3 3

Brewer et al. [42] report Φ (I*) = 0.75 ± 0.02 at 248 nm for CD 3 I.
Quantum yields for I( 2 P 3/2 ) atom formation, Φ (I), can be derived from Φ (I) = 1 – Φ (I*).

Table 4-85. Absorption Cross Sections of CH 3 I at 296–298 K and Temperature Coefficients

λ (nm) 10 20 σ (cm 2 ) 10 3 a 1 (K –1 ) 10 5 a 2 (K –2 ) 10 3 B(K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 a 1 (K –1 ) 10 5 a 2 (K –2 ) 10 3 B(K –1 )

210 3.62 3.07 2.42 290 8.04 6.14 2.57 4.98 215 5.08 2.61 2.28 295 4.00 7.27 2.91 6.38 220 6.90 1.06 1.22 300 2.06 7.82 3.53 6.97 225 9.11 1.74 1.96 305 1.10 7.82 3.85 6.84 230 12.6 1.47 1.67 310 0.621 7.37 3.71 6.78 235 20.5 1.91 2.04 0.67 315 0.359 6.98 3.47 6.75 240 38.1 1.74 2.06 0.61 320 0.221 7.39 3.54 6.53 245 65.6 1.52 2.15 0.34 325 0.126 7.23 2.82 6.79 250 96.3 1.20 2.11 0.08 330 0.0684 8.93 3.74 7.82 255 117.7 0.890 1.95 –0.10 335 0.0388 10.88 4.88 9.34 260 119.7 0.882 1.93 –0.12 340 0.0212 11.30 4.46 10.95 265 102.9 1.21 2.00 0.10 345 0.0114 15.68 8.44 13.58 270 75.9 1.77 2.11 0.54 350 0.00609 15.94 8.22 16.83 275 49.6 2.52 2.12 1.33 355 0.00320 18.91 280 29.2 3.62 2.24 2.43 360 0.00190 17.28 285 15.6 4.84 2.38 3.74 365 0.00090 23.63 Note: Absorption cross sections σ : 210–230 nm: mean of Jenkin et al. [182], Fahr et al. [116], and Roehl et al. [343], 235–330 nm: mean of Jenkin et al . [182], Fahr et al. [116], Rattigan et al. [325], and Roehl et al. [343], 335–350 nm: mean of Fahr et al. [116], Rattigan et al. [325], and Roehl et al. [343], 355–365 nm: Rattigan et al. [325]. Temperature coefficients a 1 and a 2 : 210–298 K, Roehl et al. [343]: ( σ ( λ , T) = σ (298 K) [1 + a 1 (T–298) + a 2 (T–298) 2 ]), Temperature coefficients B: 243–333 K, Rattigan et al. [325] (ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298)).

H3. CH 2 I 2 + h ν → CH 2 I + I( 2 P 3/2 ).

H4. CH 2 I 2 + h ν → CH 2 I + I*( 2 P 1/2 ).
The absorption cross sections of CH 2 I 2 have been measured at room temperature and 180–400 nm by Pence et al. [312], at 220–360 nm by Schmitt and Comes [365], at 200–360 nm by Baughcum and Leone [29], at 265– 341 nm by Koffend and Leone [205] ; and at 220–400 nm by Kwok and Phillips [207], who measured the spectrum also in methanol and cyclohexane. Measur ements at 273 and 298 K and 205–380 nm have also been carried out by Roehl et al. [343]; and at 273, 298, and 348 K and 215–385 nm by Mössinger et al. [283]. There are absorption maxima at or below 215 nm, and around 250 and 290 nm. The room temperature data of the various teams (except those of Kwok and Phillips [207], which are presented only as a plot) are in very good agreement, i.e., generally within 5–10% between 230 a nd 380 nm, were the older data of Schmitt and Comes [365] and Koffend and Leone [205] for the prominent absorption band around 290 nm are higher than those of Roehl et al. [343] and Mössinger et al. [283]. The values of Kwok a nd Phillips [207] for the prominent absorption band around 290 nm are lower by 15–20% than the rest of the data. The preferred room temperature absorption cross sections, listed in Table 4-86, are the values of Roehl et al. [343] at 205–215 nm, the mean of4-89 the values reported by Roehl et al. [343] and Mössinger et al. [283] at 220–380 nm, which are very close, and the value of Mössinger et al. [283] at 385 nm.
Both temperature studies show, that decreasing the temperature from 298 or 348 K to 273 K causes a slight increase of the absorption cross sections between 275 and 300 nm (~2% in the maximum at 290 nm between 298 and 273 K) and a slight decrease outside this wavelength region. A simple empirical relation for the temperature dependence between 273 and 348 K, ln σ ( λ , T) = ln σ ( λ , 298K) + B( λ )·(T–298), and temperature coefficients B( λ ) for λ = 205–375 nm at 5-nm intervals are given by Mössinger et al. [283]. The temperature coefficients B are also listed in Table 4-86 (an erroneous B value at 305 nm has been corrected by Dr. Mössinger via a personal communication).
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of CH 2 I 2 at 193, 248, and 308 nm, Φ (I*) = ~0.05, 0.46 ± 0.04, and 0.25 ± 0.02, respectively, have been reported by Pence et al. [312]. Quantum yields for I( 2 P 3/2 ) atom formation, Φ (I), can be derived from Φ (I) = 1 – Φ (I*).

Table 4-86. Absorption Cross Sections of CH 2 I 2 at 298 K

λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 )

205 407.0 300 357.0 –0.37 210 404.0 305 338.5 –0.16 215 366.0 0.15 310 313.5 0.07 220 260.0 0.14 315 280.0 0.15 225 197.5 0.19 320 244.0 0.27 230 133.0 0.51 325 203.0 0.27 235 109.0 0.56 330 161.5 0.51 240 122.5 0.15 335 120.5 0.55 245 150.0 0.18 340 83.3 1.36 250 157.0 0.67 345 53.7 1.99 255 139.5 1.58 350 32.6 3.19 260 120.5 2.04 355 19.2 4.09 265 130.0 1.30 360 10.9 5.39 270 178.5 0.00 365 6.05 6.77 275 255.0 –0.71 370 3.45 8.25 280 328.5 –1.24 375 1.93 11.3 285 371.5 –1.21 380 1.17 290 380.5 –0.94 385 0.769 295 371.5 –0.58 Note: Absorption cross sections σ : 205–215 nm, Roehl et al. [343], 220–380 nm, mean of Roehl et al. [343] and Mössinger et al. [283], 385 nm, Mössinger et al. [283]. Temperature coefficients B: 273–348 K, Mössinger et al. [283] (ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298)).

H5. C 2 H 5 I + h ν → C 2 H 5 + I( 2 P 3/2 ).

H6. C 2 H 5 I + h ν → C 2 H 5 + I*( 2 P 1/2 ).
The absorption cross sections of C 2 H 5 I have been measured at room temperature and 147 nm ( σ = 1.48 × 10 –17 cm 2 ) by Rebbert et al. [334], at 205–360 nm by Porret and Goodeve [318]; at 223–298 K and 205–365 nm by Roehl et al. [343], at 243–333 K and 235–355 nm by Rattigan et al. [325], a nd at 323 K and 220–320 nm by Zhang et al. [451]. The room temperature data are in good agreement, the values of Roehl et al.[343] are higher by 5–15% at 235–325 nm and become increasingly higher up to 125% at 355 nm than the values of Rattigan et al. [325]. The latter authors f ound their data to agree with in 10–15% with the plotted values of Porret and Goodeve [318]. The preferre d absorption cross sections, listed in Table 4-87, are the mean of the values reported by Roehl et al. [343] and Rattigan et al. [325] in the common wavelength range 235– 355 nm, and the data of Roehl et al. [343] at 215–230 nm.
The temperature studies of Roehl et al . [343] and Rattigan et al. [325] show , that decreasing the temperature in the range 333–223 K causes an increase of the absorption cross section in the absorption band at ~230–270 nm and a decrease at longer wavelengths. The differences between the low-temperature data of the two groups are4-90 comparable with those between the room temperature data. The data for 323 K, reported by Zhang et al. [451] as a plot on a logarithmic scale, are larger by 10–40% around the absorption maximum and up to more than 200% in the long-wavelength tail than the data for 313 and 333 K reported by Rattigan et al. [325]. A simple analytical expression for th e temperature dependence, σ ( λ , T) = σ (298 K) [1 + a 1 (T–298) + a 2 (T–298) 2 ], and the fitting parameters a 1 ( λ ) and a 2 ( λ ) for λ = 205–365 nm and T = 223–298 K give Roehl et al. [343]. Another simple parameterization, ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298), and parameters B( λ ) for λ = 235–355 nm and T = 243–333 K is reported by Rattigan et al. [325]. The parameters a 1 , a 2 , and B are listed also in Table 4-87.
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of C 2 H 5 I at a few wavelengths between 222 and 305 nm have been reported: Φ (I*) = 0.57 ± 0.02, 0.72 (or 0.73) ± 0.02, 060 ± 0.02, and 0.39 ± 0.02 at 222, 266, 280, and ~305 nm by Uma and Das [410], [411], [412]; Φ (I*) = 0.78 ± 0.07 at 248 nm by Gedanken [130]; Φ (I*) = 0.68 ± 0.02 at 248 nm by Brewer et al. [42], Φ (I*) = 0.22 at 304 nm by Kang et al. [198]. Quantum yields for I( 2 P 3/2 ) atom formation, Φ (I), can be derived from Φ (I) = 1 – Φ (I*).
At 147 nm, the overall process C 2 H 5 I + h ν → C 2 H 4 + H + I was observed with a quantum yield of 0.75 by Rebbert et al. [334].

Table 4-87. Absorption Cross Sections of C 2 H 5 I at 298 K and Temperature Coefficients

λ (nm) 10 20 σ (cm 2 ) 10 3 a 1 (K –1 ) 10 5 a 2 (K –2 ) 10 3 B(K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 a 1 (K –1 ) 10 5 a 2 (K –2 ) 10 3 B(K –1 )

205 11.9 6.38 3.15 285 19.1 3.85 0.926 3.61 210 4.22 4.07 6.28 290 10.3 5.47 1.65 4.83 215 4.56 4.93 6.75 295 5.38 7.00 2.52 6.33 220 6.18 4.06 5.70 300 2.78 8.56 4.11 7.48 225 9.09 2.81 3.81 305 1.44 9.31 4.89 8.08 230 14.3 2.62 3.83 310 0.777 10.56 6.87 7.55 235 23.2 1.28 2.17 –0.27 315 0.416 10.83 6.81 7.92 240 41.7 0.876 1.96 –0.40 320 0.227 11.98 9.76 8.27 245 69.3 0.233 1.62 –0.62 325 0.127 12.98 11.3 8.81 250 99.3 –0.111 1.58 –0.79 330 0.0743 14.56 17.5 9.30 255 119.7 –1.03 0.606 –0.82 335 0.0403 18.81 24.6 10.20 260 121.8 –1.48 –0.0332 –0.75 340 0.0246 13.90 9.08 11.16 265 105.9 –1.09 1.2 × 10 –6 –0.44 345 0.0133 18.86 22.1 12.41 270 80.6 –0.538 –0.257 0.36 350 0.00840 20.19 20.1 11.28 275 54.4 0.770 0.0299 1.23 355 0.00488 –7.04 –40.5 12.20 280 33.5 2.01 0.110 2.36 Note: Absorption cross sections σ : 205–230 nm, Roehl et al. [343], 235–355 nm, mean of Roehl et al. [ 343] and Rattigan et al. [325]. Temperature coefficients a 1 and a 2 : 223–298 K, Roehl et al. [343] ( σ ( λ , T) = σ (298 K) [1 + a 1 (T–298) + a 2 (T–298) 2 ]), Temperature coefficients B: 243–333 K, Rattigan et al. [325] (ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298)).4-91 H7. CH 3 CHI 2 + h ν → Products. The absorption cross sections of CH 3 CHI 2 have been measured at 298 K and 220– 360 nm by Schmitt and Comes [365]. Thei r data are listed in Table 4-88.

Table 4-88. Absorption Cross Sections of CH 3 CHI 2 at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

220 304 270 183 320 222
225 240 275 243 325 201
230 181 280 304 330 175
235 144 285 352 335 138
240 138 290 374 340 107
245 151 295 366 345 75.7
250 157 300 339 350 49.3
255 143 305 305 355 31.7
260 133 310 273 360 19.1
265 145 315 247 Note: 220–360 nm, Schmitt and Comes [365].

H8. CH 3 CH 2 CH 2 I + h ν → Products.

H9. CH 3 CHICH 3 + h ν → Products.
The absorption cross sections of 1-C 3 H 7 I have been measured at 223–298 K and 205–335 nm, those of 2-C 3 H 7 I at 223–298 K and 205–380 nm by Roehl et al. [343]. The absorption cross sections of 2-C 3 H 7 I in the gas phase and in cyclohexane solution have al so been measured at room temper ature and 235–305 nm by Phillips et al. [315]. The gas-phase data repor ted by Phillips et al. [315] and given as a plot in th eir paper are larger by 30– 70% over the whole absorption band than the data of Roehl et al. [343]. Room temperature values at 147 nm for 1-C 3 H 7 I and 2-C 3 H 7 I have been reported by Rebbert et al. [334]. ].The recommended room temperature values for 1-C 3 H 7 I and 2-C 3 H 7 I, listed in Table 4-89, are taken from the paper of Roehl et al. [343].
Decreasing the temperature in the range 298–223 K causes an increase of the absorption cross sections around the absorption maximum, at 245–265 nm for 1-C 3 H 7 I and at 240–270 nm for 2-C 3 H 7 I, and a decrease in the long-wavelength tail. Decrease of the absorption cross sec tions with decreasing temperature generally has been observed in the short-wavelength tail of the absorpti on band except for slight increases between 273 and 248 K in the case of 1-C 3 H 7 I and between 248 and 223 K in the case of 2-C 3 H 7 I. At wavelengths below the minimum (~210 nm), the absorption cross sections decrease with decreasing temperature between 298 and 223 K. The temperature dependence has been parame terized by the anal ytical expression

σ ( λ , T) = σ (298 K) [1 + a 1 (T–298) + a 2 (T–298) 2 ]
and the fitting parameters a 1 ( λ ) and a 2 ( λ ) for T = 223–298 K and λ = 205–335 nm (1-C 3 H 7 I) and λ = 205– 380 nm (2-C 3 H 7 I) are reported by Roehl et al. [343]. These are listed also in Table 4-89.
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of C 3 H 7 I at a few wavelengths have been reported: Φ (I*) = 0.54 ± 0.02, 0.66 ± 002, 0.56 ± 0.02, and 0.35 ± 0.02 at 222, 266, 280, and ~305 nm by Uma and Das [410], [412]; Φ (I*) = 0.60 ± 0.02 at 248 nm by Brewer et al. [42], Φ (I*) = 0.20 at 304 nm by Kang et al. [198] for 1-C 3 H 7 I; Φ (I*) = 0.40 ± 0.02, 0.44 ± 0.03, and 0.19 ± 0.02 at 222, 266, and ~305 nm by Uma and Das [411], and Φ (I*) = 0.26 ± 0.02 at 248 nm by Brewer et al. [42] for 2-C 3 H 7 I. Quantum yields for I( 2 P 3/2 ) atom formation, Φ (I), can be derived from Φ (I) = 1 – Φ (I*).
At 147 nm, Rebbert et al. [334] observed the main overall processes 1-C 3 H 7 I + h ν → C 3 H 6 + H + I and

1-C 3 H 7 I + h ν → CH 3 + C 2 H 4 + I with quantum yields 0.38 and 0.47 and the processes

2-C 3 H 7 I + h ν → C 3 H 6 + H + I and 2-C 3 H 7 I + h ν → CH 3 + C 2 H 4 + I with quantum yields 0.80 and 0.07.4-92 Table 4-89. Absorption Cross Sections of C 3 H 7 I at 298 K and Temperature Coefficients

1-C 3 H 7 I 2-C 3 H 7 I λ (nm) 10 20 σ (cm 2 ) 10 3 a 1 (K –1 ) 10 5 a 2 (K –2 ) 10 20 σ (cm 2 ) 10 3 a 1 (K –1 ) 10 5 a 2 (K –2 )

205 15.6 7.60 4.37 44.9 15.14 8.46 210 5.05 0.283 1.57 4.53 7.84 7.23 215 5.14 –1.49 –2.46 3.57 4.96 5.08 220 6.84 –1.59 –2.97 4.20 1.55 1.27 225 10.4 –0.891 –2.14 6.45 2.21 1.99 230 17.7 –0.375 –1.26 11.0 1.60 1.80 235 32.8 –0.311 –1.04 20.4 0.480 0.681 240 58.1 –0.611 –0.804 38.2 –0.333 0.121 245 91.9 –0.949 –0.609 66.7 –0.680 0.0947 250 124 –1.22 –0.611 102 –0.795 0.289 255 141 –1.55 –0.776 133 –0.966 0.570 260 136 –1.44 –0.867 148 –1.14 0.512 265 113 –1.02 –1.04 143 –0.589 0.824 270 82.2 –0.306 –1.16 120 –0.439, 0.281 275 53.4 0.524 –1.50 90.2 0.792 0.873 280 32.0 1.68 –1.66 61.4 1.65 0.466 285 18.1 3.08 –1.44 38.6 2.88 0.534 290 9.96 5.56 0.812 22.6 4.13 0.559 295 5.42 6.76 2.05 12.8 5.71 1.04 300 2.96 7.16 2.90, 6.94 7.20 1.93 305 1.63 6.90 3.20 3.73 8.19 2.33 310 0.945 7.10 4.01 2.04 8.75 2.81 315 0.532 5.59 2.78 1.09 8.49 2.25 320 0.301 3.68 0.0140 0.627 10.79 4.36 325 0.177 4.23 0.0238 0.348 9.54 2.76 330 0.110 11.40 12.3 0.202 10.99 5.94 335 0.0627 15.76 25.8 0.115 12.37 7.58 340 0.0688 13.69 12.2 345 0.0402 16.32 17.1 350 0.0253 18.50 24.7 355 0.0150 19.41 24.3 360 0.0105 18.61 13.9 365 0.00666 29.85 50.9 370 0.00479 37.24 76.8 375 0.00535 36.71 80.7 380 0.00530 22.00 40.0
Note : Absorption cross sections σ : 205–380 nm, Roehl et al. [343], Temperature coefficients a 1 and a 2 : 223–298 K, Roehl et al. [343] ( σ ( λ , T) = σ (298 K) [1 + a 1 (T–298) + a 2 (T–298) 2 ]).

H10. C 4 H 9 I + h ν → C 4 H 9 + I( 2 P 3/2 ).

H11. C 4 H 9 I + h ν → C 4 H 9 + I*( 2 P 1/2 ).
H12. (CH 3 ) 2 CHCH 2 I + h ν → (CH 3 ) 2 CCH 2 + I( 2 P 3/2 ).
H13. (CH 3 ) 2 CHCH 2 I + h ν → (CH 3 ) 2 CCH 2 + I*( 2 P 1/2 ).
H14. (CH 3 ) 3 CI + → (CH 3 ) 3 C + I( 2 P 3/2 ).
H15. (CH 3 ) 3 CI + → (CH 3 ) 3 C + I*( 2 P 1/2 ).4-93 Absorption cross sections for n - and iso -C 4 H 9 I are not available. Absorption cross sections of tert -C 4 H 9 I have been measured at 323 K by Phillips et al. [315]. An absorptions band between 230 and 310 nm exhibits a maximum of ~2.1 × 10 –18 cm 2 at ~268 nm. Estimated values at 5-nm intervals, read from a logarithmic plot, are presented in Table 4-90.
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of n -C 4 H 9 I at several wavelengths between 222 and 305 nm have been reported: Φ (I*) = 0.51 ± 0.02, 0.64 ± 0.03, 0.50 ± 0.03, and 0.30 ± 0.02 at 222, 266, 280, and ~305 nm by Uma and Das [410], [412]; Φ (I*) = 0.53 ± 0.03 at 248 nm by Brewer et al. [42], Φ (I*) = 0.14 at 304 nm by Kang et al. [198].
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of i so -C 4 H 9 I, Φ (I*) = 0.71 ± 0.01, 0.56 ± 0.03, and 0.35 ± 0.02 at 266, 280, and ~305 nm, ha ve been reported by Uma and Das [412], Φ (I*) = 0.20 ± 0.02 at 248 nm by Brewer et al. [42].
Quantum yields for I atom formation in the photolysis of tert -C 4 H 9 I, Φ (I( 2 P 3/2 )+I*( 2 P 1/2 )) = 0.93 and 0.92 at 277 and 304 nm, have been reported by Kim et al. [201]. Quantum yields for I*( 2 P 1/2 ) atom formation, Φ (I*( 2 P 1/2 )) = 0.33 ± 0.03, 0.20 ± 0.03, and 0.12 ± 0.03, in the photolysis at 222, 266, and ~305 nm, have been reported by Uma and Das [411], I*( 2 P 1/2 ) = 0.41 ± 0.10 and 0.03 ± 0.02 at 248 nm by Gedanken [412] and Brewer et al. [42], respectively.

Table 4-90. Absorption Cross Sections of (CH 3 ) 3 CI at 298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

235 28.5 265 209 295 54.0 240 42.5 270 211 300 34.0 245 64.8 275 186 305 21.5 250 98.0 280 150 310 14.0 255 140 285 116 260 180 290 83.0 Note: 235–310 nm, Phillips et al. [315], estimated from logarithmic plot.

H16. C 5 H 11 I + h ν → C 5 H 11 + I( 2 P 3/2 ).

H17. C 5 H 11 I + h ν → C 5 H 11 + I*( 2 P 1/2 ).
Absorption cross sections for n -C 5 H 11 I are not available. A quantum yield for I*( 2 P 1/2 ) atom formation in the photolysis of n -C 5 H 11 I at 222 nm, Φ (I*) = 0.50 ± 0.03, has been measured by Uma and Das [410].

H18. CF 3 I + h ν → CF 3 + I( 2 P 3/2 )

H19. CF 3 I + h ν → CF 3 + I*( 2 P 1/2 )
The absorption cross sections of CF 3 I have been measured at room temperature and 170–230 nm by Roxlo and Mandl [350]; at room temperature and in shock waves at 625 and 1050 K and 220–360 nm by Brouwer and Troe [45]; at 200–298 K and 216–370 nm by Solomon et al. [385]; at 218–333 K and 160–350 nm by Fahr et al. [115]; and at 243–333 K and 235–390 nm by Rattigan et al. [325]. Measur ements in the long-wavelength tail of the absorption band up to 455 nm and at temperatures up to ~4000 K were also carried out with hot molecules excited by IR laser pulses by Bagratashvili et al. [18] and Abel et al. [2][3].
There is good agreement between the room temperature values above 200 nm, i.e., better than 20% around the absorption maximum at 265–270 nm and better than 15% below 255 nm and at 280–350 nm. Fahr et al. [115] report the highest absorption maximum of 7 × 10 –19 cm 2 , compared to 6.4 × 10 –19 , 6.2 × 10 –19 , and

5.9 × 10 –19 cm 2 reported by Solomon et al. [385], Brouwer and Troe [45] , and Rattigan et al. [325], respectively. The long-wavelength data of Solomon et al. [385] become increasingly higher by up to ~70% than those of Rattigan et al. [325]. The pref erred absorption cross sections, listed in Table 4-91, are the data of Fahr et al. [115] at 180–215 nm; the mean of the values reported by Brouwer and Troe [45], Solomon et al. [385], and Fahr et al. [115] at 220–230 nm; the mean of the values reported by Brouwer and Troe [45], Solomon et al. [385], Fahr et al. [115], and Rattigan et al. [325] at 235–310 nm; the mean of the values reported by Solomon et al. [385], Fahr et al. [115] , and Rattigan et al. [325] at 315–350 nm; and the values of Rattigan et al. [325] at 355–385 nm.4-94 Fahr et al. [115] observed in the short-wavelength regi on a band centered at about 171 nm with cross sections up to 3.6 × 10 –17 cm 2 , which shows vibrational structure, and a band with a maximum approaching values of 10 –16 cm 2 at or below 160 nm. The plotted spectrum at 170–230 nm reported by Roxlo and Mandl [350] is not in agreement with the results of Fahr et al. [115].
The temperature studies of Solomon et al. [385], Fahr et al . [115], and Rattigan et al. [325] agree in the observation, that the absorption cross sections increase in the region of the maximum (~240–280 nm) with decreasing temperature from 333 K or room temperature down to temperatures of 240–250 K; the ratios

σ (298 K)/ σ (~240 K) and σ (333 K)/ σ (~240 K) around the maximum are ~0.9, the ratios σ (333 K)/ σ (298 K) are ~1. Solomon et al. [385] observed a further increase of the cross sections down to 200 K, whereas Fahr at al. [115] observed a slight decrease between 253 and 218 K. A decrease of the absorption cross sections above 280 nm and between 333 and 200 K was observed by the three groups; the ratios σ (298 K)/ σ (~240 K) increase from ~1.0 to ~1.9 at 280–340 nm, the ratios σ (333 K)/ σ (298 K) are around 1.3. Thus, the temperature dependences reported by the three groups are compatible at least in the range 240–333 K.
Solomon et al. [385] and Rattigan et al. [ 325] fitted their spectra to the expression

ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298)
and report the temperature coefficients B( λ ) for T = 200–298 K and λ = 216–344 nm (at 2-nm intervals) and for T = 243–333 K and λ = 235–390 nm (at 5-nm intervals), respectively. The temperature coefficients B reported by Solomon et al. [385] are nearly constantly larger by ~0.8 × 10 –3 than those of Rattigan et al. [325] at 235–300 nm and become smaller by up to 1.75 × 10 –3 between 315 and 345 nm. The B values reported by Rattigan et al. [325] for the ranges 235–385 nm and 243–333 K are listed also in Table 4-91.
Fahr et al. [115] gave fits for the long-wavelength tail using the expressions σ ( λ ) = σ 0 ( λ ) exp (–L/ λ ) for λ > 320 nm and σ (T) = σ 0 (T) exp(– θ /T) and reported values for the parameters σ 0 ( λ ) and L at T = 218, 235, 253, 273, 295, and 333 K and for σ 0 (T) and θ at 300, 310, 320, 330, 340, and 350 nm.
In the short-wavelength region at 160–180 nm, a decrease of the absorption cross sections with decreasing temperature 333–218 K has been observed by Fahr et al. [115].

Since CF 3 I serves as model system for studying the dynamics of I*( 2 P 1/2 ) atom production by UV photolysis, there is a great number of studies which measure I*( 2 P 1/2 )/I( 2 P 3/2 ) branching ratios and I*( 2 P 1/2 ) quantum yields from CF 3 I photolysis in the wavelength region of the abso rption band. The following quantum yields were reported for the range between 248 and 308 nm:

Φ (I*) = 0.89 ± 0.01, 0.87 ± 0.04, and 0.88 at 248 nm by Brewer et al. [42], Gedanken et al. [130], and Felder [117], respectively;

Φ (I*) = 0.89 ± 0.05, 0.79 ± 0.03 and 0.63 ± 0.02 at 266, 280, and ~305 nm by Kavita and Das [199];

Φ (I*) = 0.87 at 277 nm by Kim et al. [200]; Φ (I*) = 0.69 at 304 nm by Kang et al. [198];

Φ (I*) = 0.21 at 308 nm by Felder [118], and

Φ (I*) = 0.99 ± 0.01 0.91 ± 0.01 0.89 ± 0.01 0.84 ± 0.01 0.81 ± 0.01 0.69 ± 0.01 λ (nm)= 275 279 283 290 293 295
Φ (I*) = 0.68 ± 0.01 0.63 ±0.02 0.61 ± 0.02 0.47 ± 0.01 0.41 ± 0.0 0.37 ± 0.01 λ (nm)= 296 297 298 300 302 303 by Furlan et al. [127].
Quantum yields for I( 2 P 3/2 ) atom formation, Φ (I), can be derived from Φ (I) = 1 – Φ (I*)4-95 Table 4-91. Absorption Cross Sections of CF 3 I at 295–300 K

λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 )

180 3.11 285 33.4 0.55 185 0.75 290 22.7 1.65 190 0.28 295 14.3 2.98 195 0.16 300 8.60 4.22 200 0.15 305 5.06 5.61 205 0.19 310 2.82 6.84 210 0.34 315 1.62 7.68 215 0.68 320 0.905 8.27 220 1.52 325 0.485 8.74 225 2.88 330 0.262 9.25 230 5.03 335 0.142 9.92 235 8.21 0.16 340 0.0750 10.27 240 13.6 –0.16 345 0.0407 11.71 245 21.8 –0.52 350 0.0210 12.85 250 32.4 –0.86 355 0.0115 13.26 255 45.2 –1.17 360 0.0064 14.65 260 56.9 –1.37 365 0.0036 14.63 265 63.4 –1.43 370 0.002 15.49 270 63.1 –1.30 375 0.0011 17.14 275 56.1 –0.94 380 0.0007 17.66 280 45.1 –0.62 385 0.0004 19.71 Note: Absorption cross sections σ : 180–215 nm: Fahr et al. [115] 220–230 nm: mean of Brouwer and Troe [45], Solomon et al. [385], and Fahr et al.[115] 235–310 nm: mean of Brouwer and Troe [45], Solomon et al . [385], Fahr et al. [115] ,and Rattigan et al. [325] 315–350 nm: mean of Solomon et al. [385], Fahr et al. [115], and Ra ttigan et al. [325] 355–385 nm: Rattigan et al. [325]. Temperature coefficients B: 243–333 K, Rattigan et al. [325] (ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298)).

H20. CF 2 I 2 +h ν → CF 2 I + I( 2 P 3/2 )

H21. CF 2 I 2 +h ν → CF 2 I + I*( 2 P 1/2 )

H22. CF 2 I 2 +h ν → CF 2 + I( 2 P 3/2 ) + I( 2 P 3/2 )

H23. CF 2 I 2 +h ν → CF 2 + I( 2 P 3/2 ) + I*( 2 P 1/2 )
The photodissociation of CF 2 I 2 has been studied at room temperature and wavelengths 248, 308, 337, and 351 nm by Wannenmacher et al. [429] and Baum et al. [30]. These authors report also plots of the absorption spectrum at room temperature and between 190 and 420 nm, which suggest the presence of at least two overlapping transitions corresponding to the different dissociation processes. Numerical absorption data belonging to Wannenmacher et al. and Baum et al. were obtained via personal communication by Pfister and Huber [314]. The absorption cross sections listed in Table 4-92 are normalized to a maximum value

σ = 2.929 × 10 –18 cm 2 ·molecule –1 at 300 nm, which was derived from fi ve different spectra and has an uncertainty of ±16%.4-96 Table 4-92. Absorption Cross Sections of CF 2 I 2 at 294 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

190 3163 270 203.1 350 66.24 195 4616 275 215.7 355 57.76 200 4070 280 224.3 360 49.81 205 2285 285 236.4 365 41.51 210 837.0 290 259.5 370 33.92 215 238.1 295 281.9 375 26.85 220 75.78 300 292.9 380 18.90 225 36.39 305 288.5 385 13.60 230 29.50 310 266.7 390 9.892 235 35.51 315 235.6 395 6.713 240 47.34 320 198.6 400 4.240 245 66.07 325 163.9 405 3.356 250 89.21 330 135.5 410 1.943 255 118.0 335 111.6 415 1.413 260 150.1 340 91.33 420 0.7066 265 180.5 345 78.25 Note: 190–420 nm, Wannenmacher et al. [429], Baum et al. [30], and Pfister and Huber [314].

H24. C 2 F 5 I + h ν → C 2 F 5 + I( 2 P 3/2 ).

H25. C 2 F 5 I + h ν → C 2 F 5 + I*( 2 P 1/2 ).
The absorption cross sections of C 2 F 5 I have been measured at 295 K and 268 nm ( σ = 6.39 × 10 –19 cm 2 ) by Pence et al. [312] and at 323 K and 220–320 nm by Zhang et al. [451]. The absorption band extending over the 220–320-nm range has a maximum of ~ 6.7 × 10 –19 cm 2 at ~269 nm Estimated values at 5-nm intervals, read from a logarithmic plot, are presented in Table 4-93.
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of C 2 F 5 I at 266, 288, and ~305 nm, Φ (I*) = 0.97 ± 0.03, 0.75 ± 0.03, and 0.83 ± 0.05, respec tively, have been reported by Kavita and Das [199]. Quantum yields for I( 2 P 3/2 ) atom formation, Φ (I), can be derived from Φ (I) = 1 – Φ (I*).

Table 4-93. Absorption Cross Sections of C 2 F 5 I at 323 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

220 1.95 255 49.8 290 35.3 225 3.27 260 60.0 295 25.0 230 5.60 265 65.5 300 16.3 235 9.40 270 66.8 305 10.4 240 16.0 275 63.2 310 6.4 245 25.3 280 56.1 315 3.9 250 37.5 285 46.5 320 2.3 Note: 235–310 nm, Zhang et al. [451], estimated from logarithmic plot.

H26. C 3 F 7 I + h ν → C 3 F 7 + I( 2 P 3/2 ).

H27. C 3 F 7 I + h ν → C 3 F 7 + I*( 2 P 1/2 ).
The absorption cross sections of 1-C 3 F 7 I have been measured at room temperature and 265–341 nm by Koffend and Leone [205] and at 180–400 nm by Pence et al. [312]. The latter authors report a plot of the absorbance (in arbitrary units), which shows an absorption band between ~220 and 340 nm with the maximum at ~268 nm, and absorption cross sections only for 248, 268, and 308 nm. The data for 268 and 308 nm are in good agreement with the corresponding data reported by Koffend and Leone [205]. The recommended absorption cross sections of 1-C 3 F 7 I, listed in Table 4-94, are the value for 248 nm reported by Pence et al. [312]; the mean of the values of Pence et al. [312] and Koffend a nd Leone [205] at 268 nm; and, for the range 270–340 nm,4-97 values obtained by interpolation and extrapolation at 5- nm intervals of the data reported at odd wavelength by Koffend and Leone [205].
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of C 3 F 7 I at 266, 288, and ~305 nm,

Φ (I*) = 0.83 ± 0.02, 0.89 ± 0.03, and 0.90 ± 0.05 for 1-C 3 F 7 I and

Φ (I*) = 0.83 ± 0.01, 0.80 ± 0.03, and 0.89 ± 0.02 for 2-C 3 F 7 I, have been reported by Kavita and Das [199].
Quantum yields for I( 2 P 3/2 ) atom formation, Φ (I), can be derived from Φ (I) = 1 – Φ (I*).

Table 4-94. Absorption Cross Sections of 1-C 3 F 7 I at 295–298 K

λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 ) λ (nm) 10 20 σ (cm 2 )

248 31.0 290 43.7 320 3.3
268 77.3 295 31.8 325 2.0
270 77.0 300 21.3 330 1.2
275 74.0 305 14.2 335 0.70
280 66.5 310 9.2 340 0.42
285 56.2 315 5.5 Note: 248 nm, Pence et al. [312], 268 nm, mean of Pence et al. [312] and Koffend and Leone [205] 270–340 nm, 5-nm inter- and extrapolati on of Koffend and Leone [205] data.

H28. C 4 F 9 I + h ν → C 4 F 9 + I( 2 P 3/2 ).

H29. C 4 F 9 I + h ν → C 4 F 9 + I*( 2 P 1/2 ).

H30. C 6 F 13 I + h ν → C 6 F 13 + I( 2 P 3/2 ).

H31. C 6 F 13 I + h ν → C 6 F 13 + I*( 2 P 1/2 ).
Absorption cross sections are not available for these perfluoroalkyl iodides.
Quantum yields for I*( 2 P 1/2 ) atom formation in the photolysis of both iodides at 266, 288, and ~305 nm,

Φ (I*) = 0.75 ± 0.03, 0.80 ± 0.03, and 0.87 ± 0.02 for n -C 4 F 9 I and

Φ (I*) = 0.82 ± 0.02, 0.74 ± 0.03, and 0.82 ± 0.01 for n -C 6 F 13 I, have been reported by Kavita and Das [199].
Quantum yields for I( 2 P 3/2 ) atom formation, Φ (I), can be derived from Φ (I) = 1 – Φ (I*).

H32. CH 2 ICl + h ν → CH 2 Cl + I. The absorption cross sections of CH 2 ICl have been measured at room temperature and 205–330 nm by Schmitt and Comes [366]; at 192–225 nm and 215–400 nm by Kwok and Phillips [208], [209], who also measured the CH 2 ICl spectrum in cyclohexane solution. M easurements have also been carried out at 223–298 K and 205–355 nm by Roeh l et al. [343] and at 243–333 K a nd 235–390 nm by Rattigan et al. [325]. The room temperature data of Roehl et al. [343] and Rattigan et al. [325] are in good agreement, where the values of Rattigan et al. [325] are lower by ≤ 10% between 240 and 345 nm. The older data of Schmitt and Comes [366] and the data of Kwok and Phillips [209] are higher with absorption maxima near 270 nm of 1.94 × 10 –18 and 1.5 × 10 –18 cm 2 , respectively, compared to 1.35 × 10 –18 and 1.21 × 10 –18 cm 2 reported by the other two groups. The data of Kwok and Phillips [208] at 205 and 210 nm are lower by more than 80 % than the data of Roehl et al. [343]. The preferred absorption cross sections, listed in Table 4-95, are the data of Roehl et al. [343] at 205–230 nm; the mean of the values reported by Roehl et al. [343] and Rattigan et al. [325] at 235–355 nm; and the data of Rattigan et al . [325] at 360–390 nm. The data of Schmitt and Comes [366] and Kwok and Phillips [208], [209] ar e given only as a plots in their pa pers and have therefore not been included in the evaluation.
Both temperature studies show an increase of the absorption cross sections around the absorption maximum (~250–285 nm) with decreasing temperature between 333 a nd 223 K and the reverse effect above 285 nm. The absorption maxima at ~250 K reported by the two groups agree within 15%. A simple analytical expression for4-98 the temperature dependence, σ ( λ , T) = σ (298 K) [1 + a 1 (T–298) + a 2 (T–298) 2 ], and the fitting parameters a 1 ( λ ) and a 2 ( λ ) for λ = 205–355 nm and T = 223– 298 K give Roehl et al. [343]. Another simple parameterization, ln

σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298), and parameters B( λ ) for λ = 235–390 nm and T = 243–333 K report Rattigan et al. [325]. The te mperature coefficients a 1 , a 2 , and B are given also in Table 4-95.

Table 4-95. Absorption Cross Sections of CH 2 ICl at 298 K and Temperature Coefficients

λ (nm) 10 20 σ (cm 2 ) 10 3 a 1 (K –1 ) 10 5 a 2 (K –2 ) 10 3 B(K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 a 1 (K –1 ) 10 5 a 2 (K –2 ) 10 3 B(K –1 )

205 132 –1.59 –3.83 300 25.9 2.38 –0.0473 2.56 210 42.1 8.47 3.76 305 16.7 3.13 0.394 3.08 215 11.1 6.12 4.30 310 10.9 3.13 0.303 3.50 220 7.50 0.232 0.129 315 7.16 2.74 –0.317 3.56 225 9.76 –0.0938 0.660 320 4.79 2.44 –0.533 3.46 230 14.9 –0.268

– 1.4 × 10

– 325 3.23 2.87 0.140 3.44 235 21.2 –0.512 –0.388 0.24 330 2.14 8.52 –4.21 3.72 240 32.1 –0.793 –0.664 0.12 335 1.40 2.02 –2.25 4.09 245 45.9 –0.929 –0.758 –0.02 340 0.906 5.20 4.54 4.87 250 63.3 –1.22 –1.13 –0.11 345 0.569 7.05 6.88 5.69 255 84.5 –1.25 –0.998 –0.28 350 0.350 9.12 11.7 6.88 260 106 –1.56 –1.14 –0.44 355 0.225 12.27 18.9 8.16 265 122 –1.05 –0.294 –0.55 360 0.133 9.01 270 128 –1.33 –0.593 –0.59 365 0.081 11.06 275 121 –1.07 –0.298 –0.47 370 0.048 11.47 280 104 –0.618 –0.309 –0.18 375 0.027 12.77 285 81.1 –0.326 –0.554 0.32 380 0.017 15.14 290 58.5 0.300 –0.711 0.99 385 0.008 19.12 295 39.9 1.55 –0.245 1.73 390 0.006 20.48 Note: Absorption cross sections σ : 205–230 nm, Roehl et al. [343], 235–355 nm, mean of Roehl et al. [ 343] and Rattigan et al. [325], 360–390 nm, Rattigan et al. [325]. Temperature coefficients a 1 and a 2 : 223–298 K, Roehl et al. [343] ( σ ( λ , T) = σ (298 K) [1 + a 1 (T–298)+ a 2 (T–298)2]). Temperature coefficients B: 243–333 K, Rattigan et al. [325] (ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298)).

H33. CH 2 BrI + h ν → CH 2 I + Br.

H34. CH 2 BrI + h ν → CH 2 Br + I. The absorption cross sections of CH 2 BrI have been measured at room temperature and 180–360 nm by Man et al. [230]; and at 273, 298, and 348 K and 215–390 nm by Mössinger et al. [283]. The spectrum exhibits two absorption bands with maxima near 210 and 267 nm wh ich can be assigned to electronic transitions to repulsive states antibondi ng in C–Br and C–I, respectiv ely. The results of the two studies are not in quantitative agreement: Mössinger et al. [283] report room temperature absorption cross sections of 5.7 × 10 –18 and 2.3 × 10 –18 cm 2 at 215 and 270 nm, whereas a plot in the paper of Man et al. [230] gives the larger values of ~1 × 10 –17 and 3.5 × 10 –18 cm 2 , respectively. We recommend the data of Mössinger et al. [283], which are listed in Table 4-96.
The absorption cross sections increase with decreasi ng temperature around the band maxima and decrease in their long-wavelength tails at 220–240 nm and above 290 nm. The temperature dependence was parameterized by Mössinger et al. [283] by the empirical relation ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298). The temperature coefficients B( λ ) are listed also in Table 4-96 (an erroneous B value at 280 nm has been corrected by Dr. Mössinger via a personal communication).4-99 Table 4-96. Absorption Cross Sections of CH 2 BrI at 298 K and Temperature Coefficients

λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 ) λ (nm) 10 20 σ (cm 2 ) 10 3 B (K –1 )

215 567

– 2 16 275 2 14

– 1 22 335 5 52 3 89 220 423 –0.12 280 184 –0.94 340 3.50 4.79 225 269 1.34 285 150 –0.53 345 2.24 5.74 230 155 2.06 290 110 0.10 350 1.41 6.73 235 97.9 2.05 295 82.5 0.63 355 0.817 9.47 240 80.9 1.01 300 60.6 1.03 360 0.498 11.5 245 93.7 0.00 305 42.9 1.13 365 0.303 11.6 250 125 –0.58 310 31.4 1.41 370 0.165 14.3 255 170 –1.16 315 23.1 1.52 375 0.098 17.4 260 207 –1.29 320 16.8 1.71 380 0.070 265 228 –1.45 325 11.5 2.36 385 0.039 270 229 –1.73 330 8.02 2.99 390 0.025 Note: Absorption cross sections σ : 205–380 nm, Mössinger et al. [283]. Temperature coefficients B: 273–348 K, Mössinger et al. [283] (ln σ ( λ , T) = ln σ ( λ , 298 K) + B(T–298)).

H35. CF 2 BrCF 2 I + h ν → CF 2 BrCF 2 + I.

H36. CF 2 BrCF 2 I + h ν → CF 2 ICF 2 + Br. The absorption spectrum of CF 2 BrCF 2 I has been measured at room temperature and 190– 350 nm by Pence et al. [312]. The spectrum, reported as a plot (with arbitr ary absorbance units), exhibits an absorption band with the maximum near 268 nm corresponding to the C–I bond and part of an absorption band with the maximum at or below 193 nm corresponding to the C–Br bond. A cross section σ = 2.36 × 10 –18 cm 2 and a quantum yield for Br*( 2 P 1/2 ) atom formation, Φ (Br*) = 0.07 ± 0.05, at 193 nm have been reported.

I1. SO 2 + h ν → Products
The UV absorption spectrum of SO 2 is highly structured, with a very weak absorption in the 340–390 nm region, a weak absorption in the 260–340 nm region, and a strong absorption extending from 180 to 235 nm; the threshold wavelength for photodissociation is ~220 nm. The atmospheric photochemistry of SO 2 has been reviewed by Heicklen et al. [157] and by Calvert and Stockwell [66]. Direct photo-oxidation at wavelengths longer than ~300 nm by way of the electronically excited states of SO 2 appears to be relatively unimportant.
The absorption cross sections have been measured by McGee and Burris [252] at 295 and 210 K, between 300 and 324 nm, which is the wavelength region commonly used for atmospheric monitoring of SO 2 . Manatt and Lane [231] have recently compiled and evaluated the earlier cross sec tion measurements between 106 and 403

nm.

I2. CS 2 + h ν → CS + S

The CS 2 absorption spectrum is rather complex. Its photochemistry has been reviewed by Okabe [300]. There are two distinct regions in the near UV spectrum: a strong absorption extending from 185 to 230 nm, and a weaker one in the 290–380 nm range. The threshold wavelength for photodissociation is ~280 nm. Absorption cross section measurements have been reported r ecently by Xu and Joens [435] between 187 and 230 nm.
The photo-oxidation of CS 2 in the atmosphere has been discussed by Wine et al. [432], who report that electronically excited CS 2 may react with O 2 to yield eventually OCS.

I3. OCS + h ν → CO + S The absorption cross sections of OCS have been meas ured by Breckenridge and Taube [41], who presented their 298 K results in graphical form, between 200 and 260 nm; by Rudolph and Inn [351] between 200 and ~300 nm (see also Turco et al. [406]), at 297 and 195 K; by Leroy et al. [213] at 294 K, between 210 and 260 nm, using photographic plates; and by Molina et al. [263] between 195 and 260 nm, in the 195 K to 403 K temperature range. The results are in good agreement in the regions of overlap, except for λ > 280 nm, where the cross section values reported by Rudolph and Inn [351] are significantly larger than those reported by Molina et al. [263]. The latter authors concluded that solar photodissociation of OCS in the troposphere occurs only to a negligible extent.4-100 The recommended cross sections, given in Table 4-97, are taken from Molina et al. [263]. (The original publication also lists a table with cross section values averaged over 1 nm intervals, between 185 and 300 nm.)
Rudolph and Inn [351] reported a quantum yield for photodissociation of 0.72, based on measurements of the quantum yield for CO production in the 220–254 nm range. Additional measurements would be useful.

Table 4-97. Absorption Cross Sections of OCS

10 20 σ (cm 2 ) 10 20 σ (cm 2 ) λ (nm) 295 K 225 K λ (nm) 295 K 225 K
186.1 18.9 13.0 228.6 26.8 23.7 187.8 8.33 5.63 231.2 22.1 18.8 189.6 3.75 2.50 233.9 17.1 14.0 191.4 2.21 1.61 236.7 12.5 9.72 193.2 1.79 1.53 239.5 8.54 6.24 195.1 1.94 1.84 242.5 5.61 3.89 197.0 2.48 2.44 245.4 3.51 2.29 199.0 3.30 3.30 248.5 2.11 1.29 201.0 4.48 4.50 251.6 1.21 0.679 203.1 6.12 6.17 254.6 0.674 0.353 205.1 8.19 8.27 258.1 0.361 0.178 207.3 10.8 10.9 261.4 0.193 0.0900 209.4 14.1 14.2 264.9 0.0941 0.0419 211.6 17.6 17.6 268.5 0.0486 0.0199 213.9 21.8 21.8 272.1 0.0248 0.0101 216.2 25.5 25.3 275.9 0.0119 0.0048 218.6 28.2 27.7 279.7 0.0584 0.0021 221.5 30.5 29.4 283.7 0.0264 0.0009 223.5 31.9 29.5 287.8 0.0012 0.0005 226.0 30.2 27.4 292.0 0.0005 0.0002 296.3 0.0002 –

I4. SF 6 + h ν → Products
The species SF 6 does not absorb at wavelengths longer than 130 nm; it is expected to have an atmospheric residence time of thousands of years (Ravishankara et al. [329]; Ko et al. [204]).

J1. NaOH + h ν → Na + OH The spectrum of NaOH vapor is poorly characterized. Rowland and Makide [346] inferred the absorption cross section values and the average solar photodissociation rate from the flame measurements of Daidoji [100]. Additional measurements are required.4-101 J2. NaCl + h ν → Na + Cl

There are several studies of the UV absorption spectra of NaCl vapor. For a review of the earlier work, which was carried out at high temperatures, see Rowland and Rogers [348]. The recommended cross sections, listed in Table 4-98, are taken from the work of Silver et al. [376], who measured spectra of gas phase NaCl at room temperature in the range from ~190 to 360 nm by directly monitoring the product Na atoms.

Table 4-98. Absorption Cross Sections of NaCl Vapor at 300 K

λ (nm) 10 20 σ (cm 2 )
189.7 612 193.4 556 203.1 148 205.3 90.6 205.9 89.6 210.3 73.6 216.3 151 218.7 46.3 225.2 146 230.4 512 231.2 947 234.0 1300 237.6 638 241.4 674 248.4 129 251.6 251 254.8 424 260.2 433 268.3 174 277.0 40 291.8 0.84-102 

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## SECTION 5. HETEROGENEOUS CHEMISTRY

Table of Contents
SECTION 5. HETEROGENEOUS CHEMISTRY............................................................................................. .... 5-1

5.1 Introduction ................................................................................................................... .......................... 5-1 5.2 Surface Types—Acid/Water , Liquids, and Solids.................................................................................. . 5-2 5.3 Surface Types—Soot and Alumina ................................................................................................. ........ 5-2 5.4 Surface Composition and Morphology............................................................................................. ....... 5-3 5.5 Surface Porosity ............................................................................................................... ....................... 5-4 5.6 Temperature Dependences of Parameters .......................................................................................... ..... 5-4 5.7 Solubility Li mitations......................................................................................................... ..................... 5-4 5.8 Data Orga nization.............................................................................................................. ...................... 5-4 5.9 Parameter De finitions.......................................................................................................... .................... 5-5 5.10 Mass Accommodation Coefficients fo r Surfaces Other Than Soot......................................................... 5-8 5.11 Notes to Table 5-1 ............................................................................................................. ...................... 5-9 5.12 Gas/Surface Reaction Probabilities for Surfaces Other Than Soot. ...................................................... 5-16 5.13 Notes to Table 5-2 ............................................................................................................. .................... 5-19 5.14 Soot Surface Uptake Coefficients............................................................................................... ........... 5-32 5.15 Notes to Table 5-3 ............................................................................................................. .................... 5-32 5.16 Henry’s Law Constants for Pure Water........................................................................................... ...... 5-35 5.17 Notes to Table 5-4 ............................................................................................................. .................... 5-36 5.18 Henry’s Law Constants for Acids ................................................................................................ ......... 5-40 5.19 Notes to Table 5-5 ............................................................................................................. .................... 5-40 5.20 References ..................................................................................................................... ........................ 5-44



### Tables Table 5-1. Mass Accommodation Coefficients ( α ) for Surfaces Other Than Soot. ................................................ 5-8 Table 5-2. Gas/Surface Reaction Probabilities ( γ ) for Surfaces Other Than Soot. ............................................... 5-16 Table 5-3. Soot Surface Uptake Coefficients. ................................................................................... .................... 5-32 Table 5-4. Henry’s Law C onstants for Pure Water. ............................................................................... ............... 5-35 Table 5-5. Henry’s Law Constants for Acids..................................................................................... ................... 5-40



### Figures Figure 5-1. Recommended reactive uptake coefficients as a function of temperature for key stratospheric heterogeneous processes on sulfuric acid aerosols.............................................................................. ............ 5-7



### 5.1 Introduction

We have evaluated and tabulated the currently av ailable information on heterogeneous stratospheric processes. In addition, because of the increasing level of interest in troposphe ric processes with a direct bearing on the fluxes of reactive species into th e stratosphere, such as heterogeneous loss processes for partially oxidized degradation products of hydrohalocarbons and heterogeneous contrail and cloud processing of exhaust species from aircraft, we have included kinetic data for selected hete rogeneous interactions relevant to modeling cloud droplet and aqueous aerosol chemistry in the free troposphere. Ho wever, both stratospheric a nd tropospheric heterogeneous chemistry are relatively new and rapidly developing fields , and further results can be expected to change our quantitative and even our qualitative understanding on a regul ar basis. The complexity is compounded by the difficulty of characterizing the chemi cal and physical properties of atmospheric heterogeneous surfaces and then reproducing suitable simulations in the laboratory [227]. New and/or updated evaluations in this document have focused on uptake measurements on binary liquid sulfuric acid/water, supplemented in a few cases by data on ternary liquid sulfuric acid/water solutions, on water ice, and on “soot” (see definitions below). No updates on solid acid/ice compositions are presented in this document, although evaluations for key nitrogen oxide sequestration and/or halogen activation r eactions on nitric acid trihydrate (NAT) surfaces were recently re-evaluated and presented in JPL 00-3 [306]. Uptake data on alumina, sa lt and aqueous salt solutions have not been updated since JPL 97-4 [102]. Henry’s law solubility data for reactive upper tropospheric/stra tospheric species in binary liquid sulfuric acid/water and, where available, in ternary liquid sulfuric acid/nitric acid/water solutions have also been updated and a much more extensive compilation of Henry’ s law parameters for pure water has been added.5-2 

### 5.2 Surface Types—Acid/Water, Liquids, and Solids

To a first approximation there are three major types of surfaces believed to be present at significant levels in the stratosphere. They are: (1) Type I polar stratospheric clouds (PSCs), nominally composed of nitric acid trihydrate (HNO 3 • 3H 2 O); (2) crystals of relatively pure water ice, de signated as Type II PSCs because they form at lower temperatures than Type I and are believed to be nuc leated by Type I (similar surfaces may form as contrails behind high-altitude aircra ft under some stratospheric c onditions); and (3) sulfuric aci d aerosol, which is nominally a liquid phase surface generally co mposed of 60–80 weight percent H 2 SO 4 and, concomitantly, 40–20 weight percent H 2 O. While PSCs, as their name suggests, are formed primarily in the cold winter stratosphere at high latitudes, sulfuric acid aerosol is present year round at all latitudes and may influence stratospheric chemistry on a global basis, particularly after large injections of volcanic sulfur episodi cally increase their abundance and surface area. There is also increas ing evidence that ternary H 2 SO 4 /HNO 3 /H 2 O liquid solutions may play a significant role in PSC formation. In addition to the major stratospheric surface types noted above, several other types of heterogeneous surfaces are found in the stratosphere a nd may play a significant role in some stratospheric processes. For instance, laboratory work has indicated that nitric acid dihydrate (NAD) may play an impor tant role in the nucleation of Type I PSCs (Worsnop et al. [358], Fox et al. [126]) and that mixtures of solid nitric acid hydrates and sulfuric acid tetrahydrate (SAT) (Molina et al. [261], Zhang et al. [370]) and/or a more complex sulfuric acid/nitric acid hydrate (Fox et al. [126]) may also be key to understanding Type I PSC nucleation and evolution. Analyses of the range of atmospheric conditions possible in the polar stratosphere have also led to inte rest in solid SAT surfaces and possibly other forms of frozen sulfuric acid aerosols (Toon et al. [334], Middlebrook et al. [256]), as well as liquid sulfuric acid aerosols significantly more dilute than the 60–80 weight percent normally present at lower latitudes (Wolff and Mulvaney [356], Hofmann and Oltmans [177], Toon et al. [334]). Some modeling studies also suggest that certain types of major volcanic eruptions transport significant levels of sodium chloride into the stratosphere (Michelangeli et al. [255]), so studies of stratospheric trace species interacting with so lid NaCl or similar salts, as well as salt solutions, have also been included. In the free troposphere the heterogeneous surfaces of interest include liqui d or solid water (cloud droplets, contrails), and aqueous sulfate solutions. Uptake data are compiled for liquid water for several reasons. First this surface is one asymptote of the aqueous acid aer osol continuum; second, the interactions of some trace species with liquid water and water ice (Type II PSC) surfaces are often similar, and third, the uptake of some trace species by liquid water surfaces in th e troposphere can play a key role in understanding their tr opospheric chemical lifetimes and thus, the fraction that may be transported into the stratosphere.


### 5.3 Surface Types—Soot and Alumina

Aircraft at cruise altit udes and rocket exhausts contribute small but measur able amounts of carbonaceous “soot” (Pueschel et al. [280]) and al uminized solid propellant rocket e xhausts and spacecraft debris produce increasing levels of alumina (Al 2 O 3 ) and similar metal oxide particles (Zolensky et al. [373]) in the stratosphere and upper troposphere. Soot lofted above from surface com bustion sources may also be present in the upper troposphere, and to a lesser extent in the lower stratosphe re. Alumina from rocket exhausts is generally emitted as liquid droplets from the rocket nozzle and deposited in the alpha or metastable gamma phases as it quickly solidifies in the exhaust plume. “Soot” refers to a material that is a combination of elemental and organic carbon, with proportions varying de pending on the source material and the combustion conditions. In st udies of soot directed to understanding the interaction with atmospheric gases, tw o types of soot have been used: carbon blacks having relatively small hydrogen and oxygen contents (e.g. Degussa FW2, Cabot Monarch 1000, ground charcoal and spark-generated soot) and organic combustion soots ha ving higher hydrogen, oxygen and nitrogen content (e.g. soots from the combustion of n-hexane, methane, propane, d ecane, ethylene, acetylene, tolu ene, stearic candles). In the case of organic combustion soots, even different fuels used to generate the soot have been reported to affect the chemistry; for example, the yiel ds of HONO from the reaction of NO 2 with acetylene, toluen e, ethylene and decane soots were observed to vary with the fuel used [14,134]. Polycyclic aromatic hydrocarbons (PAH) and oxyge nated polycyclic aromatic compounds (O-PAC) are major constituents of soots formed from the com bustion of liquid fuels [ 10-12,63,123,139,315]. The bulk composition of soot can have varying amounts of C, H, and O. For example, Chughtai et al. [77] report that the composition (in weight %) of n -hexane soot varies from 87 to 92 % C, 1.2 to 1.6 % H, and 11 to 6% oxygen. Stadler and Rossi [321] showed that the elemental composition of the soot as well as its surface area depended on whether the flame was rich or lean; in the case of the rich flame giving a gr ey-colored soot, the composition (weight %) was 97.3% C, 0.83% H, 1.65% O, and 0.20% N while th e lean flame gave a black soot comprised of 96.4% C, 0.19% H, 3.2% O, and 0.27% N.5-3 The functional groups on the soot surface are expected to be important in terms of the uptake and reaction of gases on the surface. XPS studies of n -hexane soot show surface carbon and oxygen, although the specific nature of the bonding could not be determined (A khter et al. [12]). The su rface functional groups on soot vary, depending on the fuel composition, method of genera tion and the post-treatment of the soot. For example, Degussa FW2 carbon black, which has been used in a number of studies of uptake and r eactions of gases on soots, is post-treated with NO 2 by the manufacturer and Cabot Monarch 1000 is post-treated with aqueous HNO 3 . There may be sufficient NO and NO 2 concentrations generated under some cond itions during the form ation of soots by spark generators that these may also have been reacted with these gases prior to collection and uptake studies. Studies of a number of gases interacti ng with soot surfaces suggest there are at least two and likely more, types of reactive surface sites; one type r eacts very rapidly, e.g. with O 3 , while others react more slowly. The first type may be most relevant to the reactions of soot particles in exhaust plumes from combustion sources, while the latter is most relevant to soot diluted in air. Fourier transform infrared (FTIR) , Raman and el ectron paramagentic resonance (EPR) spectroscopic studies of n-hexane soot show C–O functionalities assigned to anhydrides and aryl ethers, alkyl ketones, as well as =C–H, highly substituted aromatics a nd conjugated carbonyl-aromatic groups [10,315]. Kirchne r et al. [220] measured the FTIR spectra of soots fro m the combustion of diesel fuel and n -hexane (described as “flame deposited”) and soots collected from a commercial spark generator in Ar, from the emissions of a diesel automobile and Degussa FW2 soot (described as “filter deposited”). In all cases, absorption peaks due to –C–C–, –C=C–, –C– O, aromatic –C=O, and carboxylic –C=O groups (both aroma tic and aliphatic) were observed. However, the flamedeposited soot showed bands due to substituted aromatics while the filter-collected samples did not. The filterdeposited samples had bands due to ali phatic –C–H groups that were not observed for the flame-deposited soots. Only the spark-generated soot showed bands due to both –C=C–H and to –O–H. For soot formed from the combustion of liquid fuels, the location in the flame at which the soot is collected also changes the surface enough to alter its reactions. For example, A khter et al. [10] showed that the functional groups as well as particle size depend on the height of collection of soot from the base of the flame. Such changes appear to also alter the reactions of soot; for example, Gerecke et al. [134] measured HONO and NO yields from the reaction of NO 2 with ethylene soot and found that the HONO yield decreased with distance from the bottom of the flame that the soot was collected from, while the yield of NO increased. Kirchner et al. [220] reported much stronger infrared absorption bands due to substituted aromatics in soot samples collected from the combustion of n -hexane near the bottom of the flame compared to the t op; in addition, absorption bands due to the –O–H group were only observed in samples collect ed at the bottom of the flame. Not only can the surface groups directly affect its interaction with gases, but they determine the hygroscopic properties of the soot surf ace. Chughtai et al. [84,87] have shown that the hy dration of soot surfaces depends on the fuel composition (particul arly sulfur and trace metal content) and combustion conditions, as well as the extent of surface oxidation. A highly hygroscopic surface holding significant amounts of water may behave differently than a “dry” surface with re spect to the interaction with gases; for example, black carbon suspended in aqueous solutions with ozone and irradiated to generate OH has been shown to help assist in the initiation of bulk solution phase OH chemistry [195]. There are also free radi cal sites on soot surfaces whose EPR signals are strongly affected by the adsorption of paramagnetic species such as NO 2 (e.g. see Chughtai et al. [77]). These unpaired electrons in soot may contri bute to the surface reactivity.

The International Steering Committee for Black Carbon Reference Materials (http://www.du.edu/~dwismith/bcs teer.html) has issued preliminary r ecommendations for representative black carbon reference materials. They recommend that soot formed from the combustion of saturated hydrocarbons, preferably n -hexane, be used for soot black carbon. For aerosol black carbon, they recommend the use of Urban Dust Reference Material (SRM) 1649a, which is a sample collected in Washington, D.C. in a baghouse in 1976– 1977. However, for studies of the uptake and reactions of gases in the atmosphe re with combustion-generated soots, organic combustion generated soots, particularly n -hexane soot, appear to be the most reasonable surrogate.


### 5.4 Surface Composition and Morphology

The detailed composition and morphology of each surf ace type are uncertain and probably subject to a significant range of natural variability. Certain chemical and physi cal properties of these surfaces, such as their ability to absorb and/or solvate HCl and HNO 3 , are known to be strongly dependent on their detailed chemical composition. Moreover, most heteroge neous processes studied under laborat ory conditions (and in some cases proceeding under stratospheri c conditions) can change the chemical co mposition of the surface in ways that significantly affect the kinetic or thermodynamic proce sses of interest. Thus, a careful analysis of the timedependent nature of the active surface is required in th e evaluation of measured upt ake kinetics experiments.5-4 Experimental techniques which allo w the measurement of mass accommodati on or surface reaction kinetics with high time resolution and/or with low trace gas fluxes are ofte n more credible in establishing that measured kinetic parameters are not seriously comp romised by surface saturation or ch anging surface chemical composition. The measured kinetic uptake parameters, mass accommodation coefficients, and surface reaction probabilities are separately documented for relevant at mospheric trace gas species for the major and, where available, the minor stratospheric and upper tropospheric surfaces noted above . Since these parameters can vary significantly with surface composition (e.g., the H 2 SO 4 /H 2 O ratio for sulfate aerosol or the HNO 3 /H 2 O ratio for Type I PSC) the dependence of these parameters on surf ace composition is reviewed where sufficient data are available. Due to its chemical and morphological complexity, uptake values for soot are documented in a separate table.


### 5.5 Surface Porosity

The experimental techniques utili zed to measure mass accommodation, heterogeneous reaction, and other uptake coefficients ge nerally require knowledge of the surface ar ea under study. For solid surfaces, and most particularly for water and acid ice surfaces formed in situ , the determination of how the molecular scale ice surface differs from the geometrical surface of the supporting substrate is not easy. Keyser, Leu, and coworkers have investigated the structure of water and nitric acid ice films prepared under cond itions similar to those used in their flow reactor for uptake studies [215,216, 218]. They have demonstrated that i ce films grown in situ from the vapor can have a considerably larger availabl e surface than that represented by the ge ometry of the substrate; they have also developed a simple model to attempt to correct measured uptake rates for this effect [217,218]. This model predicts that correction factors are larg est for small uptake coefficients and thic k films. The application of the model to experimental uptake data remains controversial (Keyse r et al. [217], Hanson and Ravishakara [162], Kolb et al. [227]). Some experimenters prefer to attempt growing ice surfaces as smooth as possible and to demonstrate that their measured uptake coefficients are only weakly dependent on surface thickness (Hanson and Ravishankara [160]). Similar issues arise for uptake experiments performed on powered, fused and single crystal salt or oxide surfaces (Fenter et al. [120]; Hanning- Lee et al. [147]).The issue of surf ace area available for uptake is also important for interpreting uptake measur ements on soot and soot surrogate surfaces. The degree to which measured uptake parameters must be corrected for porosity effects will remain in so me doubt until a method is devised for accurately determining the effective surface area for the surfaces actually us ed in uptake studies. Most studies evaluated in this review assume that the effec tive ice or salt surface area is the geometrical area.


### 5.6 Temperature Dependences of Parameters

A number of laboratory studies have shown that mass accommodation coeffi cients and, to some extent, surface reaction probabilities can be temperature dependent. While these dependencies have not been characterized for many systems of interest, temperature effects on kinetic data are noted where availa ble. More work that fully separates heterogeneous kinetic temp erature effects from temperature cont rolled surface composition is obviously needed.


### 5.7 Solubility Limitations

The uptake of certain trace gases by atmospherically relevant surfaces is usua lly governed by solubility limitations rather than kinetic processe s. In these cases properly analyzed da ta can yield measurements of trace gas solubility parameters relevant to stra tospheric conditions. In general, such parameters can be strongly dependent on both condensed phase composition and te mperature. Such parameters may be very important in stratospheric models, since they can govern the ava ilability of a reactant for a bimolecu lar heterogeneous process (e.g., the concentration of HCl available for the HCl + ClONO 2 reaction on sulfuric acid aerosols) or the gas/condensed phase partitioning of a heterogeneous reaction product (e.g., the HNO 3 formed by the reaction of N 2 O 5 on sulfuric acid aerosols). Surface saturation limitations have also been obs erved in experimental uptak e studies on solid surfaces, including water and wa ter/acid ice surfaces.


### 5.8 Data Organization

Data for trace-gas heterogeneous interactions with relevant condensed-phase surfaces are tabulated in Tables 5-1 through 5-5. These are organized into

Table 5-1—Mass Accommodation Coefficien ts for Surfaces Other Than Soot.

Table 5-2—Surface Reaction Probabilitie s for Surfaces Other Than Soot.5-5 Table 5-3—Soot-Surface Uptake Coefficients.
Table 5-4—Solubility Data for Pure Water.
Table 5-5—Solubility Data for Acids.
This compilation provides updated evaluations based on published lite rature available through 2001 for water ice, liquid sulfuric acid/nitric acid/water, and soot/soot surrogate surf aces. The evaluations for alumina, solid alkali salt, aqueous alkali salt, and liquid water (with the exception of Henry’s law constants for liquid water) have not been re-evaluated since JPL P ublication 97-4 [102]. Eval uations and recommendations for the latter surfaces should be used with caution since new studies have been published in some cases that would alter the recommended values or extend their range of applicability.



### 5.9 Parameter Definitions

Mass accommodation coefficients ( α ), represent the probability of reversible uptake of a gaseous species colliding with the condensed surface of in terest. For liquid surfaces this process is associated with interfacial (gasto-liquid) transport and is generally followed by bulk liquid pha se solvation. Examples include: simple surface absorption, absorption followed by ionic dissociation and solvation (e.g., HCl + nH 2 O ↔ H + (aq) + Cl

– (aq)), and absorption followed by a reversible chemical r eaction with a condensed phase substituent (e.g., SO 2 + H 2 O ↔ H + + HSO 3 – or CH 2 O + H 2 O ↔ CH 2 (OH) 2 ). The term “sticking coefficient” is often us ed for mass accommodation on solid surfaces where physisorption or chemisorption takes the pl ace of true interfacial mass transport. Processes involving liquid surfaces ar e subject to Henry’s law, which limits the fractional uptake of a gas phase species into a liquid. If the gas phase species is simply solvated, a physical Henry’s law constraint holds; if the gas phase species reacts with a condensed phase s ubstituent, as in the sulfur dioxide or formaldehyde hydrolysis cases noted above, a “chemically modified” or “effective” Henry’s law constraint holds (Clegg and Brimblecombe [88], Schwartz [308], Watson et al. [348]). Henry's law constants relate the equilibrium concentration of a species in the gas pha se to the concentration of the same species in a liquid phase, and they have, in this report, units of M atm –1 . These are tabulated for liquid surfaces in Table 5-4 and Table 5-5. Effective Henry’s law constants are designated H*, while simple physical Henry’s law constants are represented by H. Effective Henry’s law constants are also employed to represent decreas ed trace gas solubilities in moderate ioni c strength acid or salt solutions with the use of a Setchenow coefficient formulation which relates H* to the concentration of the acid or salt [185]. Available Henry’s law constants for reactive upper tropospheri c/stratospheric species in binary sulfuric acid/water solutions, and for a few cases of ternar y sulfuric acid/nitric acid/water solutions, are tabulated as a function of acid weight percent and temperature. Temperature dependent Henr y’s law expressions for a larger set of gaseous species in pure water are presented in Table 5-4. It is presently unclear whether “s urface solubility” effects govern the uptake on nominally solid water ice or HNO 3 /H 2 O ice surfaces in a manner analogous to bulk solubility effects for liquid substrates and no solubility paramete rs for these “ice” systems are presented. For some trace species on some surfaces, experi mental data suggest that mass accommodation coefficients untainted by experimental saturation limitations have been obtained. These are tabulated in Table 5-1. In other cases experimental data can be shown to be subj ect to Henry’s law constraints, and Henry’s law constants, or at least their upper limits, can be determined. Some experimental data sets are insufficient to determine if measured “uptake” coefficients are true mass accommodation coefficients or if the m easurement values are lower limits compromised by saturation effects. These are curre ntly tabulated, with suitabl e caveats, in Table 5-1.
Surface reaction probabilities ( γ ) are kinetic values for generally i rreversible reactive uptake of trace gas species on condensed surfaces. The rates of such processes may not be limited by Henry’ s law constraints; however, the fate of the uptake reaction products may be subject to saturation limitations. For example, N 2 O 5 has been shown to react with sulfuric acid aeros ol surfaces. However, if the H 2 SO 4 /H 2 O ratio is too high, the product HNO 3 will be insoluble, and a large fraction will be expelled back into the gas phase. Surface reaction probabilities for substantially irreversible processes are presented in Table 5-2. Reaction products are identified where known. . The total experimental uptake coefficient measured in laboratory heterogeneous kinetic experiments are also often represented by the symbol γ . In those cases where surface and/or bulk reaction dominate the uptake, the total uptake coefficient ( γ

total ) and reactive uptake coefficient ( γ

rxn ) may well be identical. More formally, for cases where bulk liquid phase reaction is facile and there ar e no gas phase diffusion constraints, the total uptake coefficient for aerosol or cloud droplets can be approximated in terms of γ rxn and γ sol as [227]:5-6 

### 11 1

total sol rxn 

### γ αγ γ = + +

where

1/2

1/2 

### 8

sol 

### HRT D

c t γ π  

=    

and 

# ( ) 1/2 

### 4

rxn rxn 

### HRT Dk

c γ =

where t is the time integrated expos ure of the trace gas to the liquid su rface, R is the gas constant, D is the liquid phase diffusion coefficient, and 

### c is the mean trace gas molecular speed . In the limit of low solubility or long exposure time γ sol

becomes negligible and



### 1 11

total rxn 

### γ α γ = +

Discussion of how to use this approach to model chemical reactions in liquid stratospheric aerosols can be found in Hanson et al. [168] and Kolb et al. [227]. Note that these formulations are approximate. In cases where separate terms are competitive, more rigorous solution of the kinetic differential equations may be appropriate. For solid surfaces, bulk diffusion is ge nerally too slow to allow bulk so lubility or bulk kinetic processes to dominate uptake. For solids, reactiv e uptake is driven by chemisorption/ chemical reaction at the interface, a process that can also influence trace gas upt ake on liquids. For liquids, surface reaction ( γ

surf ) occurs in parallel, rather than in series with mass accommodation, thus:

1 

### 1 1

total surf
sol rxn 

### γ γ αγ γ − 

###  

= ++   +  

Examples where this more complex situation holds for liquid surfaces can be found in Hu et al. [181] and Jayne et al. [200]. In such cases γ may be significantly larger than α

. Uptake of gases on soot may occur due to thr ee different processes: (1) physisorption (e.g. SO 2 or HNO 3 at room temperature and low nitric acid pre ssures); (2) reaction with the surface (e.g. NO 2 ), and (3) catalytic decomposition/reactions of the gas on the surface. All three pr ocesses may occur in parallel, and the relative contributions of each of these three ma y vary during the course of the reacti on as the surface “ages.” As discussed above, there are different types of reac tive sites on soot, leading in some cases to a rapid initial uptake followed by a slower uptake; these are often charact erized as reactions on “fresh” and “aged” surfaces respectively. Another complexity is that in some cases the geometric surface areas were used to cal culate the uptake coefficients from the experimental data while in others, the availa ble reactive surface area was estimated and used. Because of these complexities with soot heteroge neous chemistry, uptake coefficients for soot interactions with gases have been broken out into a sepa rate Table 5-3 rather than being included with the other surfacesin Table 5-1 and Table 5-2. When the uncertainty is more than an order of magnitude, a recommendation is not given in Table 5-3 and the range of reported values is given in the Notes. In most cases, the available reactive surface area rather than the geometric areas have been used in obtaining th e uptake coefficients; in those cases where the geometric area was used but a higher availabl e surface area was involved in the measured uptake, the uptake coefficient is given as an upper limit. Data are most commonly available for room temperature or there are very limited data at lower temperatures characteristic of the upper troposphere.

The data in Table 5-1 and Table 5-2 for uptake on non-soot surfaces are organized by trace gas species, since some systematic variation ma y be expected for surface accommodation or reaction as the surface composition and/or phase is varied. Data presente d for one surface may be judged for “reas onableness” by comparing with data for a “similar” surface. In some cases it is not yet clear if surface uptake is truly re versible (accommodation) or irreversibly reactive in nature. In such cases the available uptake coefficients are generally tabulated in Table 5-1 as accommodation coefficients, a judgment that will be subject to change if more definitive data become available.5-7 Where a specific evaluated value for an accommodati on coefficient or reaction probability has been obtained, an estimated uncertainty fact or is also tabulated. However, when the data evaluation yielded only a lower or upper limit, no uncertainty factor can be reliably estimated and none is presented. Description of and reference citations to many of th e laboratory techniques used to obtain the data in the following tables can be found in Kolb et al. [227].

Reactions of N 2 O 5 , ClONO 2 , HOCl and BrONO 2 on/in sulfuric acid are generally dependent on the species’ Henry's law solubility and liquid phase diffusi on coefficient in the liquid acid as well as the surface and/or liquid phase reaction rate parameters. All of these pro cesses are generally functions of the acid composition and temperature (Hanson et al. [168], R obinson et al. [293]Shi et al. [313]. Thus, these reactions’ reactive uptake coefficients must be represented by a complex phenomenological or empirical models that defy simple entry into Table 5-2. The notes in Table 5-2 for these reactions discuss and present the models adopted. To aid in visualizing the resulting reactive uptake parameters the results for several reactions have been plotted in Figure 5-1 as a function of temperature for a background pressure of 50 mbar and background water vapor and HCl mixing ratios of 5 ppmv and 2 ppbv, respectiv ely. These calculations are presented for monodisperse background sulfate aerosol particles with a radius of 1×10 –5 cm (0.1 μ m).



### 10 -5 

### 10 -4 

### 10 -3 

### 10 -2 

### 10 -1 

### 10 0γo



### 230 220 210 200 190

T (K) 50 mbar 5 ppm H2O 2 ppb HCl 0.1 ppb ClONO 2 

### 50 60 70 80 H 2 

### SO 4 

### wt%

N 2 

### O 5 

### + H 2 

### O BrONO 2 

### + H 2 

### O

ClONO 2 

### + HCl ClONO 2 

### + H 2 

### O

HOCl + HCl

Figure 5-1. Recommended reactive uptake coefficients as a function of temperature for key stratospheric heterogeneous processes on sulfuric acid aerosols. For ClONO 2 and HOCl species, the aerosol radius used in the calculation is 10 –5 cm, a typical value in the stratosphere . Because the current uptake models for N 2 O 5 and BrONO 2 hydrolysis do not provide the informa tion about the reacto- diffusive length ( A ), the aerosol radius used in the calculation is assumed to be much larger than their reacto-di ffusive length (i.e. A for N 2 O 5 and BrONO 2 are set to zero.)5-8 

### 5.10 Mass Accommodation Coefficients for Surfaces Other Than Soot

Table 5-1. Mass Accommodation Coefficients ( α ) for Surfaces Other Than Soot.

Gaseous Species Surface Type Surface Composition T(K) α Uncertainty Factor Notes

O Sulfuric Acid H 2 SO 4 • nH 2 O(l) (97 wt.% H 2 SO 4 ) 298 See Note 1 O 3 Water Ice Liquid Water Nitric Acid Ice Sulfuric Acid H 2 O(s) H 2 O(l) HNO 3 • 3H 2 O(s) H 2 SO 4 • nH 2 O(l) (50–98 wt.% H 2 SO 4 ) 195–262 292 195 193–295 >0.04 >2 × 10 –3‡ 2.5 × 10 –4‡ See Note 3 2 3 2 4 OH Water Ice Liquid Water Sulfuric Acid

Alumina H 2 O(s) H 2 O(l) H 2 SO 4 • nH 2 O(l) (28 wt.% H 2 SO 4 ) (97 wt.% H 2 SO 4 ) Al 2 O 3 (s) 205–253 275

275 298 253–348 >0.1 >4 × 10 –3

>0.07 >5 × 10 –4‡

0.04 5 5 6

7 7 8 HO 2 Liquid Water Aqueous Salts Sodium Chloride Potassium Chloride H 2 O(l) NH 4 HSO 4 (aq) and LiNO 3 (aq) NaCl(s) KCl(s) 275 293 295 295 > 0.02 > 0.2 2 × 10 –2 2 × 10 –2 5 5 9 9 10 10 H 2 O Water Ice Liquid Nitric Acid Nitric Acid Ice Sulfuric Acid Sodium Chloride H 2 O(s) HNO 3 •nH 2 O(l) HNO 3 • 3H 2 O(s) H 2 SO 4 • nH 2 O (96 wt.% H 2 SO 4 ) NaCl(s) NaCl(aq) 200 278 197 298 ~298 ~299 ~298 0.5 >0.3 See Note > 2 × 10 –3‡ See Note

> 0.5 > 4 × 10 –4 2 11 12 13 14

15 16 H 2 O 2 Liquid Water Sulfuric Acid H 2 O(l) H 2 SO 4 • nH 2 O(l) (96 wt.% H 2 SO 4 ) 273 298 0.18* > 8 × 10 –4‡ 2 17 18 NO Water Ice Sulfuric Acid H 2 O(s) H 2 SO 4 • nH 2 O (70 wt.% H 2 SO 4 ) (97 wt.% H 2 SO 4 ) 195

193–243

298 See Note See Note See Note See Note 19

20 20 NO 2 Water Ice H 2 O(s) 195 See Note 21 HONO Water Ice H 2 O(s) 180–200 See Note 22 HNO 3 Water Ice Liquid Water Nitric Acid Ice Liquid Nitric Acid Sulfuric Acid

Sulfuric Acid Tetrahydrate H 2 O(s) H 2 O(l) HNO 3 • 3H 2 O(s) HNO 3 • nH 2 O(l) H 2 SO 4 • nH 2 O(l) (57.7 wt.% H 2 SO 4 ) (73 wt.% H 2 SO 4 ) (75 wt.% H 2 SO 4 ) (97 wt.% H 2 SO 4 ) H 2 SO 4 • 4 H 2 O(s) 200 268 191–200

278

191–200

283 230 295 ~192 0.3 0.2* 0.4 0.6

>0.3 0.1 >2 × 10 –3 >2.4 × 10 –3

>0.02* 3 2 2 2

2 23 24 25 26

27 27 27 27 27 HO 2 NO 2 Water Ice Sulfuric Acid H 2 O(s) H 2 SO 4 • nH 2 O(l) (97 wt.% H 2 SO 4 ) a200 298 0.1‡ See Note 3 28 29 NH 3 Liquid Water H 2 O(l) ~295 0.06* 3 30 CO 2 Liquid Water H 2 O(l) 293 See Note 31 CH 3 OH Liquid Water H 2 O(l) 260–291 0.12–0.02* 2 32 CH 3 CH 2 OH Liquid Water H 2 O(l) 260–291 0.13–0.02* 2 33 CH 3 CH 2 CH 2 OH Liquid Water H 2 O(l) 260–291 0.08–0.02* 2 34 CH 3 CH(OH)CH 3 Liquid Water H 2 O(l) 260–291 0.10–0.02* 2 34 HOCH 2 CH 2 OH Liquid Water H 2 O(l) 260–291 0.13–0.04* 2 35 CH 2 O Liquid Water Sulfuric Acid H 2 O(l) H 2 O•mHNO 3 •nH 2 O(l) 260–270 235–300 0.04 0.04 3 3 36 36 CH 3 O 2 Sodium Chloride NaCl(s) 296 >4 × 10 –3 37 CH 3 CHO Liquid Water H 2 O(l) 267 >0.03* 38 CH 3 C(O)CH 3 Liquid Water H 2 O(l) 260–285 0.07–0.01* 2 39 HC(O)OH Liquid Water H 2 O(l) 260–291 0.10–0.02* 2 405-9 Gaseous Species Surface Type Surface Composition T(K) α Uncertainty Factor Notes

CH 3 C(O)OH Liquid Water H 2 O(l) 260–291 0.15–0.03* 2 41 Cl 2 Water Ice H 2 O(s) 200 See Note 42 OClO Water Ice H 2 O(s) 100,189, 200 See Note 43 HCl Water Ice Liquid Water Nitric Acid Ice Sulfuric Acid

Sulfuric Acid Tetrahydrate H 2 O(s) H 2 O(l) HNO 3 • 3H 2 O(s) H 2 SO 4 • nH 2 O(l) (n ≥ 8, ≤ 40 wt.% H 2 SO 4 ) (n<8, >40 wt.% H 2 SO 4 ) H 2 SO 4 • 4H 2 O(s) 191– 211 274 191– 211

283 218

† 192–201 0.3 0.2* 0.3 0.15* >0.005* † See Note 3 2 3 2

† 44 45 46 47

48 CCl 2 O Liquid Water H 2 O(l) 260–290 See Note 49 CCl 3 CClO Liquid Water H 2 O(l) 260–290 See Note 49 HBr Water Ice Nitric Acid Ice H 2 O(s) HNO 3 • 3H 2 O(s) 200 200 > 0.2 > 0.3 50 50 HOBr Sulfuric Acid H 2 O(s) H 2 SO 4 in H 2 O(l) (58 wt. % H 2 SO 4) 190–239 228 >10 –3 >0.05‡ 51 52 CHBr 3 Water Ice Sulfuric Acid H 2 O(l) H 2 SO 4 • nH 2 O(l) (97 wt.% H 2 SO 4 ) 220 220 See Note >3 × 10 –3‡ 53 53 HOI Sulfuric Acid H 2 SO 4 • nH 2 O(l) (40 wt % H 2 SO 4 ) (40 wt % H 2 SO 4 ) (40 wt % H 2 SO 4 ) (50 wt % H 2 SO 4 ) (70 wt % H 2 SO 4 ) (70 wt % H 2 SO 4 ) 195 205 212 222–224 230–232

252 0.07 0.03 0.04 0.02 0.02 0.02 3 3 3 3 3 3 54

HF Water Ice Nitric Acid Ice H 2 O(s) HNO 3 • 3H 2 O(s) 200 200 See Note See Note 55 55 CF 2 O Water Ice Liquid Water Nitric Acid Ice Sulfuric Acid H 2 O(s) H 2 O(l) HNO 3 • 3H 2 O(s) H 2 SO 4 • nH 2 O(l) (40 wt.% H 2 SO 4 ) (60 wt.% H 2 SO 4 ) 192 260–290

192 215–230 See Note See Note See Note

>3 × 10 –6 ‡ >6 × 10 –5 ‡ 56 49 56

56 56 CF 3 CFO Liquid Water H 2 O(l) 260–290 See Note 49 CF 3 COOH Liquid Water H 2 O(l) 263–288 0.2–0.1* 2 57 CF 3 CClO Liquid Water H 2 O(l) 260–290 See Note 49 SO 2 Liquid Water Sulfuric Acid H 2 O(l) H 2 SO 4 • nH 2 O(l) (97 wt.% H 2 SO 4 ) 260–292 298 0.11 See Note 2 58 59 H 2 SO 4 Sulfuric Acid H 2 SO 4 • nH 2 O(l) (50–98 wt.% H 2 SO 4 ) 200–300 0.7 1.4 60 CH 3 S(O)CH 3 Liquid Water H 2 O(l) 262–281 0.16–0.08* 2 61 CH 3 S(O 2 )CH 3 Liquid Water H 2 O(l) 262–281 0.27–0.08* 2 61 CH 3 S(O 2 )OH Liquid Water H 2 O(l) 264–278 0.17–0.11* 2 61

* Varies with T, see Notes † No data—all measurements; limited by HCl solubility ‡ May be affected by surface saturation



### 5.11 Notes to Table 5-1

1. O on H 2 SO 4 • nH 2 O—Knudsen cell experiment of Baldwin and Golden [27] measured an uptake coefficient limit of <10 –6 ; this result probably cannot be equated with an accommodation coefficient due to surface saturation.

2. O 3 on H 2 O(s) and HNO 3 • nH 2 O

— Undoped ice surfaces saturate too quick ly for reliable measurements. When ice is doped with Na 2 SO 3 to chemically remove absorbed O 3 the apparent α increases to 1 × 10 –2 (0.1M) or up to 4 × 10 –2 (1M) (Dlugokencky and Ravishankara [105]). Limit of γ < 10 –6 for undoped ice is consistent with5-10 earlier measurement by Leu [233] of 

### ≤ 1 × 10 –4 and with < 6 × 10 –5 obtained by Kenner et al. [214]. Dlugokencky and Ravishankara also measured the tabulated value of an uptake coefficient for O 3 on a NAT “like” surface, but the data were difficult to reprodu ce and the surfaces were not well characterized. Kenner et al. also measured a lower limit for an uptake coefficient of 8 × 10 –5 on NAT at 183 K, but this measurement is also certainly limited by surface saturation.

3. O 3 on H 2 O(l)—Utter et al. [335] used a wetted wall flow tube technique with various chemical scavengers to measure a lower limit for α of 2 × 10 –3 . The stopped flow measurement technique using an SO 3 = scavenger (Tang and Lee [327]) is subject to saturation effects, so their quoted α of 5.3 × 10 –4 is also taken as a lower limit.

4. O 3 on H 2 SO 4 • nH 2 O—Flow tube measurements (Dlugokencky and Ravishankara [105]) of an uptake coefficient limit of <10 –6 on both 50 and 97 wt. % H 2 SO 4 surfaces are consistent with earlier, but probably less quantitative, static systems measurements of Olszyn a et al. [271] and aerosol chamber measurements of Harker and Ho [169], who report uptake coefficients of the order 10 –8 or less for a variety of sulfuric acid concentrations and temperatures. In these earlier experiments, doping the H 2 SO 4 with Ni 2+, Cr 2+ , Al 3+ , Fe 3+

, and NH 4 + (Olszyna et al. [271]) or Al 2 O 3 or Fe 2 O 3 (Harker and Ho [169]) did not significantly increase measured O 3 loss. An upper limit of 1 × 10 –6 was also reported by Baldwin and Golden [26]for 97 wt % H 2 SO 4 at 295 K. Il’in et al. [ 187] performed static tube reactor meas urements on 98 wt. % sulfuric acid at 239, 258, 273 K measuring uptake coefficients between 1.2 and 1.75 × 10 –6 . Although these measurements are slightly larger than the limits in the other studies, uptake values this small are extremely hard to quantify and these measurements are not seen to be in serious disagreement with other studies finding slightly lower upper limits. All measurements are subj ect to solubility limitations and pr obably do not reflect true limits on mass accommodation.

5. OH on H 2 O(s)—Cooper and Abbatt[91] analyzed uptake rates in a wall-coated flow tube to determine an initial γ ~ 0.1 over the temperature range of 205 – 230 K. Uptake coefficients decreased at longer exposure times, indicating surface saturati on. These data indicate that α is at least 0.1 and possibly much larger. This is confirmed by an earlier experiment using a coated in sert/flow tube technique by Gershenzon et al. [136], which yielded α > 0.4 at 253 K.

6. OH on H 2 O(l)—see Note for HO 2 on H 2 O(l). The OH and HO 2 measurements of Hanson et al. [151] are subject to the same analysis issues.

7. OH on H 2 SO 4 •nH 2 O—See Note for HO 2 on H 2 O(l) for measurement (28 wt.% H 2 SO 4 ) by Hanson et al. [151] and Note for O on H 2 SO 4 for measurement (97 wt. % H 2 SO 4 ) by Baldwin and Golden [27].

8. OH on Al 2 O 3 (s)—Measured value is from flow tube experiment with native oxide on aluminum as the active surface. An uptake coefficient of 0.4 ± 0.2 indepe ndent of temperature over the range of 253–348 K was measured (Gershenzon et al. [136]).

9. HO 2 on H 2 O(l)—Determination of α in liquid-wall flow tube (Hanson et al. [151]) is dependent on gas-phase diffusion corrections; measured limit ( α >0.02) is consistent with α = 1. In the aqueous salt aerosol measurements of Mozurkewich et al. [264], HO 2 was chemically scavenged by Cu ++ from added CuSO 4 to avoid Henry’s law constraints; the measured limit of >0.2 is also consistent with α = 1.

10. HO 2 on NaCl(s) and KCl(s)—Based on measured values of γ = 1.8 × 10 –2 for KCl and 1.6 × 10 –2 for NaCl, both at 295 K by Gershenzon et al. [135] supplementing an earlier value of γ – 8 × 10 –3 measured by Gershenzon and Purmal [137]. Re sults have not been calibrate d with a competitive technique.

11. H 2 O on H 2 O(s)—Measurements are available from Leu [232] giving 0.3 (+0.7, –0.1) at 200 K and Haynes et al. [172] (1.06 ± 0.1 to 0.65 ± 0.08) from 20 to 185 K. Brown et al.[59] used molecular beam reflection techniques to measure a value of α = 0.99 ± 0.03 between 85 and 150 K and optical interference methods to obtain α = 0.97 ± 0.10 between 97 and 145 K.

12. H 2 O on HNO 3 /H 2 O(l)—Rudolf and Wagner[302] used aerosol expansion chambe r techniques to illustrate that on liquid water/nitric acid aerosols α is greater than 0.3 and is consistent with 1.0 at 278 K.

13. H 2 O on HNO 3 •nH 2 O(s)—Middlebrook et al. [257] measured an uptake coefficient of .002 for water vapor co-depositing with nitric acid over NAT at 197 K.

14. H 2 O on H 2 SO 4 • nH 2 O—Baldwin and Golden [26] measured γ ~ 2 × 10 –3, which is almost certainly affected by surface saturation. See Note for H 2 O 2 on H 2 SO 4 • nH 2 O.5-11 15. H 2 O on NaCl(s)—Fenter et al. [ 118] used Knudsen cell/mass spectrometry methods to measure γ < 2 × 10 4 for H 2 O(g) uptake on NaCl powders, an observation confirmed by Beichert and Finlayson-Pitts [46], who found

γ < 1 × 10 –5 . However, Dai et al. [94] us ed FTIR spectroscopy on NaCl cr ystallite films at 240 and 296 K to determine that a water adlayer does adhere to dry salt and that a small fraction of surface sites (<1%) cause H 2 O dissociation. It is likely that the measurements of Fenter et al. and Beichert and Finlayson-Pitts were affected by surface saturation.

16. H 2 O on NaCl(aq)—Fung et al.[130] used Mie resonance scattering techniques to quantify aqueous NaCl droplet growth (5.8 to 7.8 μm), yielding fitted values of α > 0.5 and consistent with 1.0.

17. H 2 O 2 on H 2 O(l)—Measured accommodation coefficient (Wor snop et al. [359]) ha s a strong negative temperature dependence over the measured range of 260–292 K, with α = 0.3 at 260 K decreasing to 0.1 at 292 K.

18. H 2 O 2 on H 2 SO 4 •nH 2 O—Knudsen cell uptake measurements are s ubject to surface saturation, thus uptake coefficient value of 7.8 × 10 –4 quoted by Baldwin and Golden [26] is almost certainly a lower limit for α

. This effect is probably also responsible for the lack of measured uptake ( γ <10 –6 ) for NO, NO 2 , SO 2 , Cl 2 , and other species reported in this reference and Baldwin and Golden [27].

19. NO on H 2 O(s)—NO data (Leu [233], Saastad et al. [303]) subject to same concerns as NO 2 . See Note for NO 2 on H 2 O(s).

20. NO on H 2 SO 4 •nH 2 O—See Notes for H 2 O 2 on H 2 SO 4 • nH 2 SO 4 and NO 2 on H 2 SO 4 • nH 2 O. NO is subject to the same concerns as NO 2 for both reported measurements (Saastad et al. [303]; Baldwin and Golden [26]).

21. NO 2 on H 2 O(s)—In the absence of a chemical sink, Leu [233] measured no sustained uptake of NO 2 on ice yielding an apparent α ≤ 1 × 10 –4 . Saastad et al. [303] measured a lower limit of 5 × 10 –5 for temperatures between 193 and 243 K. However these values are probably influenced by surface saturation.

22. HONO on H 2 O(s)—Fenter and Rossi [120] measured reversible uptake on water ice between 180 and 200 K using a Knudsen cell technique. An initial uptake coefficient of 1 × 10 – 3 suggests that α equals or exceeds this value. Chu et al. [73] used a cylindrical flow reactor to measure th e uptake coefficient as a function of temperature, obtaining values ranging from 3.7 × 10 –3 at 178 K to 6.4 × 10 –4 at 200 K, in good agreement with the results of Fenter and Rossi. On the other hand, Chu et al. report significantly lower values after correction for the effects of surface porosity, i.e. 1.4 × 10 –4 at 178 K and 1.3 × 10 –5 at 200 K (see Keyser et al. [218]).

23. HNO 3 on H 2 O(s)—Leu [232] reports 0.3 (+0.7, –0.1). Some a dditional uncertainty is introduced by effective ice surface area in fast-flow measurement (see Keyser et al. [218]). Hanson [ 148] measured an uptake coefficient of > 0.3 at 191.5 and 200 K. Aguzzi and Rossi [9] measured an uptake coefficient of 0.3 over the temperature range from 180 to 190 K, the value decreasing at T < 195 K with an exponential temperature dependence of –(3400 ± 500)/T. They attributed this ch ange to an increasing evaporation rate, concluding that the accommodation coefficient most likely remains large. Abbatt [4] m easured equilibrium uptake values at 208–248 K on the order of 1 to 3 × 10 14 molecule cm –2 . Zondlo et al. [374] report the formation of a supercooled H 2 O/HNO 3 liquid layer at 185 K, forming NAT or NAD only after decreasing the relative humidity below the ice frost point.

24. HNO 3 on H 2 O(l)—Measured α has a strong negative temperature dependence varying from 0.19 ± 0.02 at 268 K to 0.07 ± 0.02 at 293 K (Van Doren et al. [338]). Ponche et al. [276] m easured an accommodation coefficient of 0.05 ± 0.01 at 297 K.

25. HNO 3 on HNO 3 • nH 2 O(s)—Hanson [148] measured uptake coefficien ts of >0.3 and >0.2 on NAT surfaces at 191 K and 200 K, respectively. Middlebrook et al. [257] measured an uptake coefficient of 0.7 on NAT at 197 K under conditions where both nitric aci d and water vapor were co-depositing.

26. HNO 3 on HNO 3 • nH 2 O(l)—Rudolf and Wagner [302] used aerosol expansion chamber techniques to deduce that α for HNO 3 on 278 K H 2 O/HNO 3 droplets is > 0.3 and probably close to 1. The consistency of this value with smaller (~0.2) values measured for uptake on pure water by Van Doren et al. [338] is unclear, since the mechanism of co-condensation is unknown and the com position of the surface in the aerosol expansion chamber experiments may be kinetically c ontrolled and has not been well determined.5-12 27. HNO 3 on H 2 SO 4• nH 2 O and H 2 SO 4 • 4H 2 O(s)—Initial uptake at 73 wt. % H 2 SO 4 allows a measurement of

α = 0.11 ± 0.01 at 283 K (Van Doren et al. [338]). This value is expected to increase at lower temperatures, in a manner similar to H 2 O(1) uptake (Van Doren et al. [337]). Total HNO 3 uptake is subject to Henry’s law solubility constraints, even at stra tospheric temperatures (Reihs et al . [283]). Solubility limitations also affected the earlier “sticking coefficient” measurements of Tolbert et al. [332] for 75 wt % H 2 SO 4 at 230 K. Hanson [148] measured an uptake coefficient of >0.3 for frozen 57.7 wt. % sulfuric acid at 191.5 and 200 K. Baldwin and Golden [26] reported a lower limit of 2.4 × 10 –4 on 97 wt. % H 2 SO 4 at 295 K, also reflecting solubility limits. Iraci et al. [191] m onitored nitric acid trihydrate growth on sulfuric acid tetrahydrate with infrared techniques, measuring HNO 3 uptake coefficient limits of >0.03 at 192.5 K and >0.08 at 192 K. These measurements involved co-deposition of water vapor.

28. HO 2 NO 2 on H 2 O(s)—Li et al. [237] measured an uptake coefficient of 0.15 ±0.10; uptake may be limited by surface saturation.

29. HO 2 NO 2 on H 2 SO 4 •nH 2 O(l)—Baldwin and Golden [26] measured γ = 2.7 × 10 –5, which is probably solubility limited; see Note for H 2 O 2 on H 2 SO 4 • nH 2 O.

30. NH 3 on H 2 O(l)—Ponche et al. [276] used a droplet train technique to obtain α = (9.7 ±0.9) × 10 –2 at 290 K, and Bongartz et al.[57] used a liquid jet technique to obtain α = 4.0 (+3.0, –0.05) × 10 –2 . Earlier levitated droplet evaporation experiments [328] on NH 4 Cl obtained a larger eva poration coefficient of α = 0.29 ± 0.03, which is discounted because of the i ndirect nature of the experiment.

31. CO 2 on H 2 O(l)—Noyes et al.[270] used a dynamic stirring technique to monitor pressure decreases in a closed cylinder. They inferred α = (5.5 ± 0.5) × 10 – 8 at 293 K. This technique is uncalibrated against more widely used procedures and probably suffers from surface sa turation effects. Measured α is probably many orders of magnitude too small.

32

. CH 3 OH on H 2 O(l)—Jayne et al. [197] measured uptake from 260–291 K and derived accommodation coefficients fitting α /(1– α ) = exp(– ∆ G ‡ obs /RT), where ∆ G ‡ obs = –8.0 kcal/mol + 34.9 cal mol –1 K –1 T(K).

33. CH 3 CH 2 OH on H 2 O(l)—Jayne et al. [197] measured uptake from 260–291 K and derived accommodation coefficients fitting α /(1– α ) = exp(– ∆ G ‡ obs /RT), where ∆ G ‡ obs = –11.0 kcal/mol + 46.2 cal mol –1 K –1 T(K). Similar, but somewhat larger values were reported for chloro-, bromo-, and iodo-ethanols.

34. CH 3 CH 2 CH 2 OH and CH 3 CH(OH)CH 3 on H 2 O(l)—Jayne et al. [197] measured uptake coefficients between 260 and 291 K and derived accomm odation coefficients fitting α /(1– α ) = exp (– ∆ G ‡ obs /RT), where ∆ G ‡ obs = –9.2 kcal mol –1 + 40.9 cal mol –1 K –1 T(K) for 1-propanol and –9.1 kcal mol –1 + 43.0 cal mol –1 K –1 T(K) for 2-propanol. Similar data for t-butanol were also reported.

35. HOCH 2 CH 2 OH on H 2 O(l)—Jayne et al. [197] measured uptake coefficients for ethylene gycol between 260 and 291 K and derived accomm odation coefficients fitting α /(1 – α ) = exp(– ∆ G ‡ obs /RT), where ∆ G ‡ obs = –5.3 kcal mol –1 + 24.5 cal mol –1 K –1 T(K).

36. CH 2 O + H 2 O(l), H 2 SO 4 • mHNO 3 • nH 2 O(l)—Jayne et al.[200] report uptake measurements for 0 – 85 wt %

H 2 SO 4 and 0 – 54 wt% HNO 3 over a temperature range of 241–300 K. Measured uptake coefficients vary from 0.0027–0.027, increasing with H + activity (Jayne et al ([200]; Tolbert et al., [330]), and with increasing pH above 7 (Jayne et al ., [198]). Reversible uptake is solub ility limited through reactions to form H 2 C(OH) 2 and CH 3 O + . A model of uptake kinetics (Jayne et al., [200]) is consistent with γ = 0.04 ± 0.01 for all compositions. A chemisorbed surface comple x dominates uptake at 10 – 20 wt % H 2 SO 4 , and CH 3 O + formation dominates above 20 wt % (Tolbert et al., [330]; Jayne et al. [200], Iraci and Tolbert [192]). Low temperature (197–214 K) uptake studies by Iraci and Tolbert [192] confir m that uptake is solubility limited for uptake coefficients in the 10 –3 to 10 –2 range even at low temperatures. These chemical mechanisms allow

γ to greatly exceed α for strong acidic and basic solutions. A full uptake model for acid solutions is presented in Jayne et al. [200], and for basic solutions in Jayne et al. [198]. XPS surface analysis by Fairbrother and Somorjai [114] failed to see CH 3 O + surface species reported by Jayne et al.; however, their sensitivity of 1% of surface coverage is too poor to see th e predicted amounts of the surface species.

37. CH 3 O 2 + NaCl(s)—Gershenzon et al. [135] measured the uptake of CH 3 O 2 on crystalline NaCl(s) in a central rod flow apparatus. They determined a value of γ = (4 ±1) × 10 –3 at 296 K, suggesting that α ≥ 4×10 –3

. 38. CH 3 CHO on H 2 O(l)—Jayne et al. [198] measured a lower accommodation coefficient limit of > 0.03 at 267 K. Uptake can be limited by Henry's law and hydrolysis kinetics effects—see reference.5-13 39. CH 3 C(O)CH 3 on H 2 O(l)—Duan et al. [108] measured uptake between 260 and 285 K, deriving α = 0.066 at the lower temperature and 0.013 at the higher, with seve ral values measured in between. Measured values fit

α /(1– α ) = exp(– ∆ G ‡ obs /RT), where ∆ G ‡ obs = –12.7 kcal/mol + 53.6 cal mol –1 K –1 T(K).
40. HC(O)OH on H 2 O(l)—Jayne et al. [197] measured uptake coefficients for formic acid between 260 and 291 K and derived accommodati on coefficients fitting α /(1 – α ) = exp(– ∆ G ‡ obs /RT), where ∆ G ‡ obs = –7.9 kcal mol –1 + 34.9 cal mol –1 K –1 T(K).

41. CH 3 C(O)OH on H 2 O(l)—Jayne et al. [197] measured uptake coefficients for acetic acid between 260 and 291 K and derived an accomm odation coefficient fitting α /(1– α ) = exp(– ∆ G ‡ obs /RT), where ∆ G ‡ obs = –8.1 kcal mol –1 + 34.9 cal mol –1 K –1 T(K).

42. Cl 2 on H 2 O(s)—Measurement of Leu [232] yielded a limit of <1 × 10 –4 for Cl 2 and is subject to same concern as NO 2 (see Note) A similar limit of <5 × 10 –5 has been measured by Kenner et al. [214], which is also probably limited by surface saturation.

43. OClO + H 2 O(s)—Brown et al.[60] and Graham et al.[142] used complementary ultra high-vacuum (UHV) and coated-wall flow tube techniques to show sub-monol ayer reversible absorption of OClO on water ice at 100 K (UHV) and 189 and 200 K (flow tube). No kinetic data are available at stratospheric temperatures but the mass accommodation coefficient for 100 K ice surfaces is near unity, with values of 0.8 ± 0.2 reported for amorphous ice and 0.6 ±0.2 for crystalline ice [142].

44. HCl on H 2 O(s)—Leu [232] (0.4; +0.6, –0.2) and Hanson and Ravishankara, [158] ( α ≥ 0.3) are in reasonable agreement at stratospheric ice temper atures. More recently, a great deal of experimental effo rt (Abbatt et al. [5], Koehler et al. [225], Chu et al. [75], Graham and Roberts [140], Graham and Roberts[141]; Rieley et al.[286]) has gone into unde rstanding the uptake of HCl by ice surfaces. Rieley et al. measured

α = 0.95 ± 0.05 at 80–120 K. Water ice at stratospheric temperatures can take up a large fraction of a monolayer even at HCl partial pressures typical of the stratosphere. Both the thermodynamic and spectroscopic properties of this absorb ed HCl indicate that it has dissociat ed to ions, forms ionic hydrates, and is highly reactive. These experimental results contrast with initial theoretical calculations that predicted undissociated HCl hydrogen bonde d to the ice surface and a very small adsorption probability at stratospheric temperatures (Kroes and Clary [228]); more recent simulations result in highe r adsorption energies and theoretical accommodation coefficients of one for 190-K surfaces (Wang a nd Clary [346]). Recent molecular dynamics calculations by Gertner and Hynes[138] also show that ionic absorption is thermodynamically favorable by about 5 kcal/mole. At HCl partial pressure s significantly above those typical of the stratosphere, a liquid surface layer forms on the ice, greatly enhanci ng the total amount of HCl th at the surface can absorb.

45. HCl on H 2 O(1)—Recommendation is based on Van Doren et al. [337]. Measured α ’s decrease from 0.18 ± 0.02 at 274 K to 0.064 ± 0.01 at 294 K, demonstr ating strong negative temperature dependence. Tang and Munkelwitz [328] have measured a larger (0.45 ±0.4) HCl evaporation coefficient for an aqueous NH 4 Cl droplet at 299 K.

46. HCl on HNO 3 • nH 2 O—There was previously severe disagreemen t between Hanson and Ravishankara [158] ( α ≥ 0.3) for NAT (54 wt. % HNO 3 ), and Leu and coworkers (Moore et al. [262], Leu et al. [234]). However, subsequent experiments at lower HCl concentrations by Leu and coworkers (Chu et al. [75]) as well as Abbatt and Molina [6] are generally consistent with Hanson and Ravishankara. In particular, Abbatt and Molina [6] report a larg e uptake coefficient ( α > 0.2). The measurements of Hanson and Ravishankara are consistent with α = 1. The experiments at stratospherically representative HCl concentrations show that HNO 3 -rich NAT surfaces adsorb si gnificantly less HCl than H 2 O-rich surfaces.

47. HCl on H 2 SO 4 •nH 2 O—Measurements by Watson et al. [348] at 284 K show α = 0.15±0.01 independent of n
for n ≥ 8. Experimental uptake and, therefore, apparent α falls off for n 

### ≤ 8 ( 

### ≥ 40 wt. % H 2 SO 4 ). This behavior is also observed at stratospheric temperat ure (218 K) by Hanson and Ravishankara [158]. More recent measurements by Robinson et al. [294] extend mass accommodation measurements to lower temperatures, yielding significantly higher values. Solubility constraints also controlled earlier low temperature uptake measurements of Tolbert et al. [332]. A review of the most recent solubility data is presented in Table 5-5.

48. HCl on H 2 SO 4 • 4H 2 O(s)—Uptake is a strong function of temperature and water vapor partial pressure (relative humidity) (Zhang et al . [370]), both of which affect adsorbed surface water.5-14 49. Halocarbonyls on H 2 O(l)—Uptake is limited by Henry's law solubility and hydrolysis rate constants (De Bruyn et al. [98,100] and Georg et al. [131,133]. See Table 5-4 and Table 5-5.

50. HBr on H 2 O(s) and HNO 3 • nH 2 O—Hanson and Ravishankara [159, 163] have reported large uptake coefficients for HBr on 200-K ice and NAT. Lower limits of >0.3 and >0.2 for ice are reported in the two referenced publications, respectively, and a limit of >0.3 is reported for NAT. No surface saturation was observed, leading to the supposition that HBr, like HCl, dissociates to i ons on ice surfaces at stratospheric temperatures. Abbatt [1] measured an uptake coefficient lower limit of >0.03 on water ice at 228 K consistent with Hanson and Ravishankara. Rieley et al. [286] measured an α of 1.0 ± 0.05 for water ice at 80–120 K. Flückiger et al. [124] report α values of ~0.2 at 210 K, increasing to ~0.3 at 190 K, while Percival et al. [274] measured an α of 0.03 ± 0.005 for water ice at T > 212 K, and α > 0.1 at T< 212 K, attributing the apparent increase in the uptake coeffi cient to an increase in th e surface area of the ice. Mo re definitive experiments will need to be carried out to resolve the discrepancy. Hudson et al. [183] report α = 0.61 ± 0.06 at 140 K, and

α = 0.24 ± 0.05 at 100 K, for HBr pressures ranging from 3 × 10 –8 to 1.4 × 10 –7 Torr. Equilibrium HBr coverages for ice are reported by Chu and Heron [74] at 188 and 195 K, and by Chu and Chu [71] at 180– 220 K. The latter authors also report the formation of various solid HBr hydrates.

51. HOBr on H 2 O(s)—Abbatt [1] measured an uptake co efficient for water ice of 2 × 10 –3 at 228 K. Chu and Chu [71] report an uptake coefficient corrected for porosity effects in the range 0.11 to 0.007 at 190–218 K, with an exponential temperature dependence of (3809 ± 76)/T, and in the range 2 × 10 –3 to 6 × 10 –4 at 223– 239 K, with an exponential temperature dependence of (4658 ± 456)/T. Chaix et al. [69] measured the uptake coefficient as a function of temperature on three diffe rent types of water-ice, obtaining values ranging from ~0.3 at 185 K to ~0.03 at 205 K, with an exponential temperature dependence of (4900 ± 500)/T. The three sets of results are in reasonable ag reement with each other, and the te mperature dependence is attributed predominantly to changes in the evaporation rate.

52. HOBr on H 2 SO 4 • nH 2 O(l)—Abbatt [1] measured an uptake coefficient of 0.06 ± 0.02 by measuring HOBr gas phase loss at 228 K. This result may well be a lower limit due to surface saturation effects.

53. CHBr 3 on H 2 O(s) and H 2 SO 4 •nH 2 O(l)—Hanson and Ravishankara [163] investigated the uptake of bromoform on ice and 58 wt.% sulfuric acid at 220 K. No uptake on ice was observed, with a measured uptake coefficient of <6 × 10 –5 . Reversible uptake by the sulfuric acid surface was observed with an initial uptake coefficient of >3 × 10 –3 ; both measurements are probably limited by surface saturation.

54. HOI on H 2 SO 4 •nH 2 O—Knudsen cell studies by Allanic and Rossi [18] measured uptake at several temperatures for 40, 50, and 70 acid wt. %. Time dependent studies show no sign of saturation, so uptake coefficients should correspond to ma ss accommodation coefficients. Some acid concentration data in the table have been averaged for similar temperatures and rounded to one significant figure. An uncertainty factor of three has been assigned due to the relatively small number of temperature/concentration points studied and a lack of confirming studies from other laboratories. The authors note evidence of HOI disproportionation to form I 2 , however, this second order reaction is unlikely to occur under atmospheric conditions.

55. HF on H 2 O(s) and HNO 3 • nH 2 O(s)—Hanson and Ravishankara [159] attempted to measure the uptake of HF by 200 K water ice and NAT surfaces but were unable to observe measurable adsorption. They surmise that, unlike HCl and HBr, HF does not disso ciate to ions on ice or NAT surfaces at 200 K. Lack of measurable uptake is probably due to surface saturation.

56. CF 2 O on H 2 O(s), HNO 3 • nH 2 O and H 2 SO 4 • nH 2 O—Uptake coefficient measurements by Hanson and Ravishankara [156] on stra tospheric surfaces are probably subject to surface and/or bulk saturation effects and may not represent accommodation coefficient measur ements, particularly the lower limits of >3 × 10 –6 reported for water and nitric acid ices.

57. CF 3 COOH on H 2 O(l)—Hu et al. [182] measured mass accommodati on coefficients for five haloacetic acids, including trifluoroacetic acid (TFA); the others were mono-, di-, trichl oro-, and chlorodifluoro-acetic acids. All displayed negative temperature dependence and values for α of about 0.1 at 273 K.

58. SO 2 on H 2 O(1)—Measured α of 0.11 ± 0.02 has no significant temperature variation over a temperature range of 260–292 K (Worsnop et al. [359]). Ponche et al. [276] measured 0.13 ± 0.01 at 298 K, in agreement with the earlier measurement. Shimono and Koda [314] estimated an α of 0.2 at 293.5 K from analysis of pH-dependent uptake coefficients in a novel liquid impi ngement technique that has not been calibrated with5-15 other gases. Donaldson et al. [106] have used second harmonic generation spectroscopy to detect a chemisorbed SO 2 surface species which was predicted from earlier uptake measurements by Jayne et al.[196]; this surface complex may play a role in SO 2 heterogeneous reacti ons on aqueous surfaces.

59. SO 2 on H 2 SO 4 • nH 2 O—See Note for H 2 O 2 on H 2 SO 4 • nH 2 O.

60. H 2 SO 4 on H 2 SO 4 •nH 2 O—Poschl et al. [277] measured 0.43< α < 1.0 for 73–98 wt. % H 2 SO 4 at 303 K in a wetted wall flow tube. Lower temperatures and acid con centrations would be expect ed to lead to larger values of α . As discussed in Poschl et al. [277] this contradicts an indirect measurement of 0.02 < α < 0.09 at 42.5 wt. % at 298 K by Van Dingenen and Raes [336] in a photochemical aerosol r eactor. The Poschl et al. [277] result is consistent with room temperature α values very near that measured for (NH 4 ) 2 SO 4 particles in an aerosol flow reactor by Jefferson et al. [201].

61. CH 3 S(O)CH 3 , CH 3 S(O 2 )CH 3 and CH 3 S(O 2 )OH on H 2 O(l)—De Bruyn et al. [99] measured uptake over the temperature range ~262–281 K and derived accommodati on coefficients fitting α / (1 – α ) = exp(– ∆ G ‡ obs /RT), where ∆ G ‡ obs = –0.12 kcal molecule –1 + 23.1 cal molecule –1 K –1 T(K) for dimethylsulfoxide

–10.7 kcal molecule –1 + 43.0 cal molecule –1 K –1 T(K) for dimethylsulfone

–3.50 kcal molecule –1 + 16.7 cal molecule –1 K –1 T(K) for methanesulfonic acid.5-16 

### 5.12 Gas/Surface Reaction Probabilit ies for Surfaces Other Than Soot.

Table 5-2. Gas/Surface Reaction Probabilities ( γ ) for Surfaces Other Than Soot.

Gaseous Species Surface Type Surface Composition T(K) γ Uncertainty Factor Notes

O 3 + Surface → Products O 3 Alumina Sodium Chloride Al 2 O 3 (s) NaCl(s) 210–300 300 See Note >2 × 15 –10 1 1 OH + Surface → Products OH Water Ice Hydrochloric Acid Nitric Acid Ice Sulfuric Acid Sodium Chloride H 2 O(s) HCl • nH 2 O(l) HNO 3 • 3HzO(s) H 2 SO 4 • nH 2 O(l) NaCl(s) 205–230 220 200–228 200–298 245–339 >0.01 >0.2 >0.2 >0.2 1.2 × 10 –5

exp 1750/T 3 2 3 4 5 6

HO 2 + Surface → Products Water Ice Sulfuric Acid H 2 O(s) H 2 SO4 • nH 2 O(l) (28 wt %) (55 wt %) (80–96 wt %) 223

275 223 243 0.025

>0.07 >0.05 >0.2 3 7 7

2NO 2 + H 2 O(l) → HONO + HNO 3 NO 2 Liquid Water Sulfuric Acid H 2 O(l) H 2 SO 4 • nH 2 O (40–98 wt. %) 250–325 See Note 5 × 10 –7 3 8 9 2NO 2 + NaCl(s) → ClNO + NaNO 3 2NO 2 + NaBr(s) → BrNO + NaNO 3 NO 2 Sodium Chloride Sodium Bromide NaCl(s) NaBr(s) 298 298 See Note See Note 10 10 NO 3 + H 2 O → HNO 3 + OH NO 3 Water Ice Liquid Water H 2 O(s) H 2 O(l) 170–200 273 <10 –3 2 × 10 –4 20 11 12 N 2 O 5 + H 2 O → 2HNO 3 N 2 O 5 Water Ice Liquid Water Nitric Acid Ice Sulfuric Acid Sulfuric Acid Monohydrate Sulfuric Acid Tetrahydrate Ternary Acid H 2 O(s) H 2 O(l) HNO 3 • 3H 2 O(s) H 2 SO 4 • nH 2 O(l) H 2 SO 4 • H 2 O(s) H 2 SO 4 • 4H 2 O(s) H 2 SO 4 • nHNO 3 •nH 2 O(l) 188–195 260–295

200 195–300 200–300 195–207 195–218 0.02 See Note 4 × 10 –4 See Note * See Note

0.006 See Note 2 See Note 3 See Note 3 2 13 14 15 16 17 18 16 N 2 O 5 + HCl(s) → ClNO 2 + HNO 3 N 2 O 5 Water Ice Nitric Acid Ice Sulfuric Acid Monohydrate H 2 O(s) • HCl(s) HNO 3 • 3H 2 O(s) •HCl(s) H 2 SO 4 • H 2 O(s) 190–220 200 195 0.03 0.003 <1 × 10 –4 See Note 2 19 20 21 N 2 O 5 + NaCl(s) → ClNO 2 + NaNO 3 (s) N 2 O 5 Sodium Chloride NaCl(s) NaCl(aq) –300 5 × 10 –4 >0.02 20 22 22 N 2 O 5 + HBr(s) → BrNO 2 + HNO 3 N 2 O 5 Water Ice Nitric Acid Ice H 2 O HNO 3 • 3H 2 O(s) 180–200 200 See Note 0.005 10 23 24 N 2 O 5 + MBr(s) → Products N 2 O 5 Sodium Bromide Potassium Bromide NaBr(s) KBr(s) ~300 ~300 4 × 10 –3 See Note 10 25 25 HONO + H 2 O → Products HONO Liquid Water H 2 O(l) 247–297 0.04 5 26 HONO + H 2 SO 4 → Products HONO Sulfuric Acid H 2 SO 4 • nH 2 O(l) 180–200 See Note 27 HONO + HCl → ClNO + H 2 O5-17 Gaseous Species Surface Type Surface Composition T(K) γ Uncertainty Factor Notes

HONO Water Ice Sulfuric Acid H 2 O(s) H 2 SO 4 • nH 2 O(l) 180–200 0.05 See Note 3 See Note 28 29 HONO + NaCl → Products HONO Sodium Chloride NaCl(s) ~300 <1 × 10 –4 30 HNO 3 + Na×(s) → H× + NaNO 3 HNO 3 Sodium Chloride Sodium Bromide Potassium Chloride Potassium Bromide NaCl(s) NaBr(s) KCl(s) KBr(s) 295–298 ~290 ~290 ~290 0.02 0.02 0.02 0.02 3 10 10 10 31 31 31 31 HO 2 NO 2 + HCl → Products HO 2 NO 2 Sulfuric Acid H 2 SO 4 • nH 2 O (50–75 wt. %) 200–225 <1 × 10 –4 32 NH 3 + H 2 SO 4 → NH 4 HSO 4 NH 3 Sulfuric Acid H 2 SO 4 • nH 2 O 288–300 0.4 2.5 33 CH 3 C(O)O 2 + H 2 O → CH 3 C(O)OH + HO 2 CH 3 C(O)O 2 Liquid Water Sulfuric Acid H 2 O(l) H 2 SO 4 • nH 2 O (84 wt % H 2 SO 4 ) (51 wt % H 2 SO 4 ) (71 wt % H 2 SO 4 ) 225

246 223 298 4 × 10 –3

3 × 10 –3 1 × 10 –3 1 × 10 –3 3

3 3 3 34 34

CH 3 C(O)O 2 NO 2 + HCl, Cl, ClO, and OClO → Products CH 3 C(O)O 2 NO 2 Sulfuric Acid H 2 SO 4 • nH 2 O (40–70 wt. %) 200–225 <1 × 10 –4 35 Cl + Surface → Products Cl Sulfuric Acid H 2 SO 4 • nH 2 O(l) 221–296 2 × 10 –4 10 36 Cl 2 + HBr(s) → BrCl + HCl Cl 2 Water Ice • HBr(s) H 2 O(s) 200 >0.2 37 Cl 2 + KBr(s) → BrCl + KCl(s) Cl 2 Potassium Bromide KBr(s) ~295 >0.1 38 Cl 2 + Na× (aq) → Cl× + NaCl (aq) Cl 2 Aqueous Sodium Bromide Aqueous Sodium Iodide NaBr(aq) NaI(aq) See Note See Note 39 39 ClO + Surface → Products ClO Water Ice Nitric Acid Ice Sulfuric Acid H 2 O(s) HNO 3 • 3H 2 O(s) H 2 SO 4 • nH 2 O(l) (60 to 95 wt.% H 2 SO 4 ) 190 183 221–296 See Note See Note See Note 40 40 41 HCl + HNO 3 → Products HCl + HNO 3 Sulfuric Acid H 2 SO 4 • mHNO 3 • nH 2 O(l) See Note See Note 42 HOCl + HCl(s) → Cl 2 + H 2 O HOCl Water Ice Nitric Acid Ice Sulfuric Acid H 2 O(s) • HCl(s) HNO 3 •3H 2 O(s)•HCl(s) H 2 SO 4 •nH 2 O(l) 195–200 195–200 198–209 0.2 0.1 See Note 2 2 See Note 43 43 44 HOCl + HBr(s) → BrCl + H 2 O HOCl Water Ice Sulfuric Acid H 2 O(s) H 2 SO 4 •nH 2 O(l) 189–220 228 See Note See Note See Note 45 46 ClNO + NaCl(s) → Products ClNO Sodium Chloride NaCl(s) 298 >1 × 10 –5 47 ClNO 2 + NaCl(s) → Products ClNO 2 Sodium Chloride NaCl(s) 298 <1 × 10 –5 47 ClONO 2 + H 2 O(s) → HOCl + HNO 3 ClONO 2 Water Ice Nitric Acid Ice Sulfuric Acid Sulfuric Acid Monohydrate Sulfuric Acid Tetrahydrate H 2 O(s) HNO 3 • 3H 2 O(s) H 2 SO 4 • nH 2 O(l) H 2 SO 4 • H 2 O(s) H 2 SO 4 • 4H 2 O(s) 180–200 200–202 200–265

195 196–206 0.3 0.004 See Note * <1 × 10 –3 See Note 3 3 See Note 48 49 50 51 51 ClONO 2 + HCl(s) → Cl 2 + HNO 35-18 Gaseous Species Surface Type Surface Composition T(K) γ Uncertainty Factor Notes

ClONO 2 Water Ice Nitric Acid Ice Sulfuric Acid Sulfuric Acid Monohydrate Sulfuric Acid Tetrahydrate Alumina H 2 O(s) HNO 3 •3H 2 O•HCl H 2 SO 4 •nH 2 O(l)•HCl(l) H 2 SO 4 •H 2 O(s) H 2 SO 4 • 4H 2 O(s) Al 2 O 3 180–200 185–210 195–235

195 195–206 180–200 0.3 0.2 See Note <1 × 10 –4 See Note 0.3 3 2 See Note

3 52 53 54 55 55 56 ClONO 2 + M×(s) → ×Cl + MNO 3 ClONO 2 Sodium Chloride Potassium Bromide Sodium Bromide NaCl(s) KBr(s) NaBr(s) 200–300 ~295 ~295 5 × 10 –2 5 × 10 –2 See Note 10 10 57 57 57 ClONO 2 + HBr(s) → BrCl + HNO 3 ClONO 2 Water Ice Nitric Acid Ice H 2 O(s) • HBr(s) HNO 3 •3H 2 O(s)•HBr(s) 200 200 >0.3 >0.3 58 58 ClONO 2 + HF(s) → Products ClONO 2 Water Ice Nitric Acid Ice H 2 O(s) • HF(s) H 2 O(s)•HNO 3 (s)•HF(s) 200 200 See Note See Note 59 59 CF × Cl y + Al 2 O 3 (s) → Products CCl 4 CFCl 3 CF 2 Cl 2 CF 3 Cl Alumina Alumina Alumina Alumina Al 2 O 3 (s) Al 2 O 3 (s) Al 2 O 3 (s) Al 2 O 3 (s) 120–300 120–300 120–300 120–300 1 × 10 –5 1 × 10 –5 1 × 10 –5 1 × 10 –5 10 10 10 10 60 60 60 60 BrCl + KBr(s) → Br 2 + KCl(s) BrCl Potassium Bromide KBr(s) ~295 >0.1 38 Br 2 + Nal(aq) → Brl + NaBr(aq) Br 2 Aqueous Sodium Iodide Nal(aq) See Note 39 2BrO → Br 2 + O 2 BrO Water Ice Sulfuric Acid

Aqueous Sodium Chloride H 2 O(s) H 2 SO 4 • nH 2 O (60 wt% H 2 SO 4 ) (70 wt % H 2 SO 4 ) NaCl(aq) (23 wt% NaCl) 213

213 213 53 See Note

See Note See Note See Note 61

61 61 61 HOBr + HCl(s) → BrCl + H 2 O HOBr Water Ice Sulfuric Acid H 2 O(s) • HBr(s) H 2 SO 4 • nH 2 O (60–69 wt% H 2 SO 4 ) 180–228 198–218 0.3 See Note 3 62 62 HOBr + HBr(s) → Br 2 + H 2 O HOBr Water Ice Sulfuric Acid H 2 O(s) • HBr(s) H 2 SO 4 • nH 2 O 228 228 0.1 See Note 3 63 63 BrONO 2 + H 2 O → HOBr + HNO 3 BrONO 2 Water Ice Sulfuric Acid H 2 O(s) H 2 SO 4 • nH 2 O 190–200 210–300 >0.3 See Note 2 See Note 64 65 BrONO 2 + HCl → BrCl + HNO 3 BrONO 2 /HCl Water Ice Sulfuric Acid H 2 O(s) H 2 SO 4 • nH 2 O 200 229 See Note 0.9 2 64 65 CF 2 Br 2 + Al 2 O 3 (s) → Products CF 2 Br 2 Alumina Al 2 O 3 210, 315 2 × 10 –5 10 60 CF 3 OH + H 2 O → Products CF 3 OH Water Ice Sulfuric Acid H 2 O(l) H 2 SO 4 • nH 2 O (40 wt% H 2 SO 4 ) 45 wt% H 2 SO 4 ) (50 wt% H 2 SO 4 ) (50 wt% H 2 SO 4 ) 274

210–250 210–250 210–250 210–250 >0.01

0.07 0.04 0.01 0.001 3 3 3 3 66

66 66 66 66 SO 2 + H 2 O 2 , O 3 , HONO, NO 2 and HNO 3 → Products SO 2 Sulfuric Acid H 2 SO 4 • nH 2 O (20–60 wt. % H 2 SO 4 ) 293 See Note 67 SO 3 + H 2 O → Products SO 3 Sulfuric Acid H 2 SO 4 • nH 2 O (78–92 wt. % H 2 SO 4 ) 300 1.0 +0.0, –0.3 68

* γ is temperature dependent5-19 

### 5.13 Notes to Table 5-2

1. O 3 + Al 2 O 3 (s) and NaCl(s). Very low ozone decomposition effi ciencies for reaction on coarse (3 μm dia.) and fine (0.1 μm dia., partially hydroxylated) γ -alumina and coarse (3 μm dia.) α -alumina were measured in flowing and static systems by Hanning-Lee et al.[147] at temperatures ranging between 212 and 473 K. Based on measured BET surface areas, γ s ranged from 2 × 10 –11 to 4 × 10 –10 over the 212 to 298 K temperature range. γ s for γ -alumina at lower temperatures exceeded those for α -alumina. Results are roughly consistent with earlier, unpublished flow tube data from L.F. Keyser and fro m fluidized bed r eactor studies of Alebi ć -Jureti ć et al. [15]. Note that γ s based on geometic surface particle surface areas would be significantly (10 4 –10 7 ) larger. Alebi ć -Jureti ć et al. also studied ozone decomposition on small (<180 μm) NaCl crystals in their fluidized bed reactor a nd observed no eff ect, indicating γ for O 3 decomposition on NaCl(s) is much smaller than that for α -alumina.

2. OH + H 2 O(s). Cooper and Abbatt [91] measured initial irreve rsible OH uptake coefficients of ~ 0.1 for water ice between 205–230 K; these decayed to γ = 0.03 ±0.02 after repeated expos ure to OH. Self-reaction to form H 2 O or H 2 O 2 was indicated by the lack of observable gas phase products despite observation of first-order OH loss.

3. OH + HCl • nH 2 O(l). Cooper and Abbatt [91] demonstrated significant enhancement of OH uptake (to γ > 0.2) after HCl doping of 220 K ice surfaces sufficient to melt the surface layer. It is unclear whether OH is lost to self-reaction or reaction with hydrated Cl

– ions.

4. OH + HNO 3 • 3H 2 O. Cooper and Abbatt [91] measured γ > 0.2 for nitric acid-doped ice surfaces under conditions suitable for NAT formation at 200 and 228 K. Increase over pure ice uptake rates is probably due to HNO 3 + OH → H 2 O + NO 3 reaction.

5. OH + H 2 SO 4 • nH 2 O. Lower limits of 0.2 for uptake coefficients on 45–65 wt % H 2 SO 4 between 220 and 230 K and for 96 wt % H 2 SO 4 at 230 and 298 K by Cooper and Abbatt [91] are consistent with a lower limit of 0.07 on 28 wt % H 2 SO 4 at 275 K in similar expe riments by Hanson et al. [151] and a probable surface saturated value of (4.9 ±0.5) × 10 –4 from Knudsen cell measurements by Baldwin and Golden [27] and an estimate of γ = 1 on ~96 wt % H 2 SO 4 at 298 K by Gerhenzon et al. [136] using a coated insert flow tube technique. Uptake is probably reactive with OH + HSO 4 – → H 2 O + SO 4 – the hypothesized process.
6. OH + NaCl(s). Ivanov et al. [193] used a fast flow reactor with a central salt coated rod to measure heterogeneous loss of OH between 245 and 339 K. Their fit for NaCl(s) yielded

γ = (1.2 ±0.7) × 10 –5 exp[(1750 ±200)/T]. Similar data for NH 4 NO 3 yielded

γ – (1.4 ±0.5) × 10 –4 exp [(1000 ±100)]. Since uptake was irreversible, it is assumed that the loss was selfreaction.

7. HO 2 on H 2 O(s) and H 2 SO 4 • nH 2 O(l). Uptake of HO 2 on ice and super-cooled 55 wt % sulfuric acid at 223 K has been demonstrated to be limited by HO 2 surface saturation by Cooper and Abbatt [91]. They argue that self-reaction, presumably 2HO 2 → H 2 O 2 + O 2 is limiting measured uptake coefficients of 0.025 ±0.005 for ice and 0.055 ±0.020 for 55 wt % H 2 SO 4 . However, Gershenzon et al. [135]measured γ > 0.2 for 80 and 96 wt % H 2 SO 4 at 243 K and Hanson et al. [151] measured a lower limit for 28 wt % H 2 SO 4 at 275 K of 0.07. However, large gas phase diffusion correc tions mean this value is consistent with γ = 1.

8. NO 2 + H 2 O(1). Value for γ of (6.3 ± 0.7) × 10 –4 at 273 K (Tang and Lee, [327]) was achieved by chemical consumption of NO 2 by SO 3 = ; their stopped-flow measurement wa s probably still affected by surface saturation, leading to the measurement of a lower limit. Ponche et al. [276] measured an uptake coefficient of (1.5 ± 0.6) × 10 –3 at 298 K, which was also probably subject to saturation limitations. Mertes and Wahner [254] used a liquid jet technique to measure a lower limit of γ ≥ 2 × 10 –4 at 278 K, and they observed partial conversion of the absorbed NO 2 to HONO. Msibi et al. [266] used a cylindrical/annular flow reactor to derive g = (8.7 ±0.6) × 10 –5 on pH = 7 deionized water surfaces and (4.2 ± 0.9) × 10 –4 on pH = 9.3 wet ascorbate surfaces; it seems likely th at these results are also subject to surface saturation given the gas/surface interaction times involved in the experiment. Data are consistent with an α ≥ 1 × 10 –3 for 278– 298 K and a liquid-phase second-order hydrolysis of NO 2 to HONO and HNO 3 which depends on temperature and pH. However, the interplay betw een accommodation, possible surface reaction, and bulk reaction may be complex.5-20 9. NO 2 + H 2 SO 4 • nH 2 O. Kleffman et al. [224] performed bubble tube reactor uptake measurements for 0–98 wt. % acid at 298 K and for 44.6 and 56.1 wt % from 250–325 K. At 298 K, measured uptake coefficients varied between 6 and 3 × 10 –7 with a minimum near 70 wt. %. Most measurements at 44.6 and 56.1 wt. % overlapped within their error limits and showed little temperature dependence although there is evidence that uptake increases at th e lowest temperatures. The data can all be captured with a recommended value of 5 × 10 –7 with an uncertainty factor of three.
This recommendation is consistent with earlier upper limits of 1 × 10 –6 by Baldwin and Golden [26] for 96 wt. % at 295 K and 5 × 10 –6 for 70 wt. % between 193 and 243 K by Saastad et al. [303]. Kleffman et al. [224] conclude that thei r uptake measurements are mass accommodation limited; however, it is not clear that their values are not influenced by bulk or surface reaction of two NO 2 with H 2 O to form HONO and HNO 3 at lower acid wt. % values and the formation of nitrosyl su lfuric acid at higher acid c oncentrations. Kleffman et. al. [224] did perform separa te static wetted wall reactor studies s howing the formation of gas phase HONO at acid concentrations below 60 wt. %. It is more likel y that reactive uptake is a controlling factor and the measured uptakes are solubility and/or reaction rate limited. Thus, the mass accommodation coefficient may be much larger than the recommended uptake values.

10. NO 2 + NaCl(s), NaBr(s). Vogt and Finlayson-Pitts [342,344] used diffuse reflectan ce infrared spectroscopy to study the reaction of NO 2 with NaCl(s) at 298 K, and Vogt et al. [341] used the same technique to study NO 2 + NaBr(s) at 298 K. Both reactions were s hown to be approximately second order in NO 2 . Assuming that adsorbed N 2 O 4 is the reactant leads to γ = (1.3 ± 0.6) × 10 –4 for NaCl(s) and 2 (+4, –1.3) × 10 –4 for NaBr(s). Peters and Ewi ng [275] measured reactive uptake for single-crystal NaCl(100) surfaces and observed both NO 3 – (c) and ClNO products. The value of γ( N 2 O 4 ) measured by Peters and Ewing at 298 K was only (1.3 ±0.3) × 10 –6 . They noted that small amounts of water vapor (9.5 mbar) cause γ to increase by two orders of magnitude.

11. NO 3 on H 2 O(s). Fenter and Rossi [121] measured an upper limit for γ of 10 –3 over the range from 170 to
200 K.

12. NO 3 + H 2 O(l). Rudich et al. [300,301] used wetted-wall flow tube techniques to measure uptake coefficients for NO 3 on pure water and aqueous NaCl, NaBr, NaI, and NaNO 2 solutions. These studies were extended to other aqueous solutions by Imamura et al. [189]. Uptake on pure water wa s consistent with reaction of NO 3 to produce HNO 3 and OH. Uptake coefficients with solutions containing I

– , Cl

– , Br
– , NO 2 – and other anions were larger and scaled with anion concentra tion, indicating electon transfer reactions to produce NO 3 – . The γ of (2.0 ±1.0 × 10 – 4 ) at 273 K determined for pure water by Rudich et al. is significantly lower than the lower limit of 2.5 × 10 –3 quoted by Mihelcic et al. [258]. A detailed analysis of uptake coefficients for KI aqueous solutions indicated that the NO 3 mass accommodation coefficient is >0.04 [301].

13. N 2 O 5 + H 2 O(s). Leu [232] and Hanson and Ravishankara [ 157] measured nearly identical values of 0.028 (±0.011) and 0.024 (±30%) in the 195–202 K range on relatively thick ice films in coated wall flow tubes. Quinlan et al. [281] measured a maximum value for γ on ice surfaces at 188 K of 0.03 in a Knudsen cell reactor. The average of these three studies is 0.027 with a st andard deviation of 0.003. Hanson and Ravishankara [158,160] presented new and re-analyzed data as a function of ice thickness, with a value of ~0.008 for the thinnest ice sample, rising to 0.024 for the thickest. From these data there would appear to be no strong dependence on temperature, at least over the 188–195 K range. It is unclear whether the measured dependence on ice film thickness is due to added porosity surface area in the thicke r films or decreased ice film integrity in thinner films. The error estimate in the table is driven by the possible systematic error due to unresolved film thickness effects rather than the small statistical error among the “thick film” values from the three groups.
Zondlo et al. [374] report the formation of a supercooled H 2 O/HNO 3 liquid layer at 185 K as a reaction product, forming NAT or NAD only after decreasing the relative humidity below the ice frost point. This effect is similar to that resulting from the interaction of gaseous HNO 3 or ClONO 2 with the ice surface. These authors measured γ = (7 ± 3) ×10 –4 at 185 K for the reaction of N 2 O 5 with this supercooled liquid layer.

14. N 2 O 5 + H 2 O(l). Reaction on liquid water has a negative temp erature dependence. Van Doren et al. [337] measured γ s of 0.057 ± 0.003 at 271 K and 0.036 ± 0.004 at 282 K using a droplet train uptake technique. George et al. [132] also used a droplet train technique to measure γ s of (3.0 ± 0.2) × 10 –2 (262 K), (2.9 ± 1.2) × 10 –2 (267 K), (2.0 ± 0.2) × 10 –2 (273 K), (1.6 ± 0.8) × 10 –2 (276 K), and (1.3 ± 0.8) × 10 –2 (277 K) on pure water, while Schweitzer et al. [310] used the same approach for pure water5-21 and salt solutions between 262 and 278 K, obtaining similar results. Mozurkewich and Calvert [263] studied uptake on NH 3 /H 2 SO 4 /H 2 O aerosols in a flow reactor. For their most water-rich aerosols (RH = 76%) they measured γ s of 0.10 ±0.02 at 274 and 0.039 ±0.012 at 293 K. However, similar studies by Hu and Abbatt [180] on (NH 3 ) 2 SO 4 aerosols at 297 K showed that uptake rises with decreasing relative humidity (RH); their 94% RH results agree very well with the temperature trend measured by Van Doren et al. Msibi et al.[265] measured a smaller γ of 2.5 × 10 –3 for water adsorbed on a denuder flow tube well under 66–96% relative humidity conditions at room temperature. The higher γ values of Van Doren et al., Mozurkewhich and Calvert, and Hu and Abbatt are quite consistent when temperature and RH effects are factored in. The lower values from the Louis Pasteur (George et al.; Schweitzer et al.) and Birmingham (Msibi et al.) groups appear to have much less pronounced temperature dependence and are inconsistent with the other measurements. The same function used to fit the N 2 O 5 uptake on sulfuric acid as a function of temperature and concentration, discussed in note 17 below, has been ex tended to the Van Doren et al. and Hu and Abbatt data for pure water and very high RH aerosols. See note 17 for the functional fit and its error discussion.

15. N 2 O 5 + HNO 3 • 3H 2 O(s). Hanson and Ravishankara [155] have measured γ = 0.0006 (± 30%) near 200 K. They presented re-analyzed and additional data as a function of ice thickness (Hanson and Ravishankara [158,160]), deriving a value of 3 × 10 –4 for the thinnest NAT covered ice layer, with values up to three times higher for thicker NAT-covered ice layers. As in the case of uptake on water ice this may be due to increased surface area from porosity in the thicker films, or less integrity in the thinner films. Th e uncertainty listed in Table A-1 is driven by this observed effect. All of the Hanson et al. data are in very poor agreement with the
γ = 0.015 (±0.006) reported by Quinlan et al. [281] from their Knudsen cell measurements; this measurement may have been biased by formati on of a super-cooled aqueous nitric acid surface and is judged to be unreliable.

16. N 2 O 5 + H 2 SO 4 • nH 2 O(l). This reaction has been intensively studied between 195 and 296 K for a wide range of H 2 SO 4 wt. % values using four complementary experimental techniques. Data are available from aerosol flow tube studies (Fried et al. [129], Hanson and L ovejoy [152], Hu and Abbatt [180], and Hallquist et al. [145]), coated wall flow tube studies (Hanson and Ravi shankara [155], Zhang et al. [365]), a stirred Knudsen cell (Manion et al. [249]) and droplet train studies (Van Doren et al. [337], Robinson et al. [293]). All studies have yielded γ s between ~0.05 and 0.20 with modest dependence on surface H 2 SO 4 wt. % and temperature. The Knudsen cell studies, aerosol flow tube studies at higher N 2 O 5 exposure and the ternary H 2 SO 4 /HNO 3 /H 2 O studies of Zhang et al. [365] all illu strate that significant levels of HNO 3 in the
H 2 SO 4 /H 2 O solutions will reduce γ measurably; this fact explains some of the scatter in aerosol flow tube studies and the surface saturation evident in the Knudsen cell st udies. The effect of 5.0 × 10 –7 Torr HNO 3 on γ as a function of temperature at two water vapor concentrations are plotted in Zhang et al. [365]; the decrease in γ is greatest at low temperatures, approaching a factor of 2–5 between 200 and 195 K.
Experimental data on sulfuric acid surfaces between 40 and 80 wt. % sulfuric acid deemed to be free of saturation effects, plus the pure water uptake data of Van Doren et al. [337] and high relative humidity ammonium sulfate aerosol uptake data of Hu and Abba tt [180] were all fit to a polynomial expression to yield a single model describing γ for N 2 O 5 uptake valid between 0 and 80 wt. % H 2 SO 4 and 180 to 300 K (Robinson et al. [293]). The form of this function is: γ o =exp (k o +k 1 /T+k 2 /T 2 ), where T is the temperature in K. The parameters k o , k 1 , and k 2 obtained from the best-fit are:

k o = –25.5265 – 0.133188wt + 0.00930846wt 2 – 9.0194×10 –5 wt 3

k 1 = 9283.76 + 115.345wt – 5.19258wt 2 + 0.0483464wt 3

k 2 = –851801– 22191.2wt + 766.916 wt 2 – 6.85427wt 3

where wt is the weight percentage of H 2 SO 4 . The overall error of applying the uptake function provi ded here consists of two components. One is the standard deviation of the model-calculated value with respect to measured data, σ m , which is given by

model 

### 2

1 1
1 m 

### N i

i N γ

γ
σ  

−   ∑

=  

=

− .5-22 The other is the standard deviation of relativ e experimental measurement error from the mean, σ d , which is given by



## ( ) 2

1 d 

### N i

i l i

N N γ

γ

σ   ∆   ∑  

=  

=

− .

The overall error is

2 2 m d 

### σ σ σ = +

. (These formulations are also applied below in the error estimation for the ClONO 2 + H 2 O and HCl, BrONO 2 + H 2 O, and HOCl + HCl reaction system. For N 2 O 5 , the error is estimated to be 15% (one sigma), with σ m =14.7% and σ d =2.9%).

17. N 2 O 5 + H 2 SO 4 • H 2 O(s). Zhang et al. [366] used coated flow tube techniques to measure the uptake of N 2 O 5 on solid sulfuric acid monohydrate over a temperature range of 200 to 225 K. The measurement values of γ were significantly higher at 200 K ( γ ~ 1 × 10 –3 ) than at 225 K ( γ ~10 –4 ) and were well fit by log γ = [4.78 – 0.0386T(K)]. Acid-rich H 2 SO 4 • H 2 O surfaces had a lower γ than water rich surfaces (log γ = [0.162 – 0.789 × log p H2O ] where p H2O is their experimental water vapor partial pressure).

18. N 2 O 5 on H 2 SO 4 • 4H 2 O(s). Hanson and Ravishankara [162] studied N 2 O 5 uptake by frozen 57.5 and 60 wt % H 2 SO 4 as a function of temperature and relative humidity. The 57.5 wt % surface was not sensitive to relative humidity and was slightly more reactive ( γ = 0.008 vs 0.005) at 205 K than at 195 K. Reaction probabilities on the 60 wt % su rface dropped off with temperature and relative humidity.

19. N 2 O 5 + HCl on H 2 O(s). Leu [233] measured γ = 0.028 (±0.011) at 195 K, while Tolbert et al. [331] measured a lower limit of 1 × 10 –3 at 185 K. These experiments were done at high HCl levels probably leading to a liquid water/acid surface soluti on (Abbatt et al. [5]). Seis el et al. [311] measured γ ~ 0.03 at 200 K using a Knudsen flow reactor with a range of HCl flows. The uptake coefficient at low HC l flows is only slightly enhanced compared to the uptake on a pure ice surface.

20. N 2 O 5 + HCl on HNO 3 • 3H 2 O(s). Hanson and Ravishankara [155] measured γ = 0.0032 (±30%) near 200 K.

21. N 2 O 5 + HCl on H 2 SO 4 • H 2 O(s). Zhang et al. [366] saw no increase in N 2 O 5 uptake on sulfuric acid monohydrate at 195 K upon e xposure to HCl, setting γ < 10 –4

. 22. N 2 O 5 + NaCl (s,aq). Using FTIR analys is, Livingston and Finlay son-Pitts [241] have demonstrated that N 2 O 5 reacts with crystalline NaCl to form NaNO 3 (s), and they report γ > 2.5 × 10 –3 at 298 K. However, Leu et al.[235] used flow tube/mass spectrometric techniques to obtain γ < 1 × 10 –4 for dry salt at 223 and 296 K; they also noted that exposing sa lt surfaces to small amounts of H 2 O vapor increased γ significantly. Fenter et al.[119] measured γ = (5.0 ±0.2) × 10 –4 on fused salt surfaces at room temp erature, assuming the geometrical surface area is the only surface accessed. Msibi et al. [265] measured NO 3 – deposition on an annular flow reactor to determine γ = 1 × 10 –3 for salt surfaces between 45 and 96% re lative humidity at room temperature, rising to γ = 1.5 × 10 –2 at 96–97% relative humidity, but they argue th at most of the uptake is due to reaction with H 2 O. On aqeous NaCl solutions, Zetzsch, Behnke, a nd co-workers [43,44,362] ha ve studied the reaction of N 2 O 5 with aqueous NaCl aerosols in an aerosol chamber. The relative yields of ClNO 2 and HNO 3 rise with the NaCl concentration. A reaction probability of ~0.03 is measured with a 50% ClNO 2 yield at the deliquescence point (Zetsch and Behnke). This picture is confirmed by droplet uptake studies on 1 M NaCl solutions reported by George et al. [132] which confirm that uptake on salt solutions in the 263–278 K temperature range is larger than that on pure water droplets.

23. N 2 O 5 + HBr on H 2 O(s). Seisel et al. [311] report γ values ranging from ~3 × 10 –3 to 0.1, depending on the HBr concentrations employed; the measurements we re conducted at 180 and 200 K. These authors report Br 2 and HONO in 80% yield as products with respect to N 2 O 5 taken up, generated presumably by the secondary reaction of the primary product BrNO 2 with HBr.5-23 24. N 2 O 5 + HBr on HNO 3 • 3H 2 O(s). This reaction, yielding γ ~0.005, was investigated on NAT surfaces near 200 K by Hanson and Ravisha nkara [159]. Under some conditions a much higher reaction coefficient of ~0.04 was observed.

25. N 2 O 5 + MBr. Finlayson-Pitts et al. [122] used FTIR techniques to demonstrate that BrNO 2 (ads) is a major product of the N 2 O 5 (g) + NaBr(s) reaction. However, Fenter et al. [119] failed to measure gas-phase evolution of BrNO 2 using Knudsen cell/mass spectro metry techniques, detecting Br 2 (g) instead. They propose that BrNO 2 reacts with KBr(s) to yield KNO 2 (s) + Br 2 (g). A γ of (4.0 ±2.0) × 10 –3 at room temperature was determined for fused KB r surfaces with well-defined surface areas.

26. HONO + H 2 O(l). Bongartz et al. [56] present uptake measurements by two independent techniques, the liquid jet technique of Schurath and co-workers and the droplet train/flow tube technique of Mirabel and coworkers (Ponche et al. [276]). With a surface temper ature of ~245 K the droplet train techniques yielded 0.045< γ <0.09, while the liquid jet operating with a surface temperature of 297 K obtained 0.03 < γ < 0.15. Mertes and Wahner used a liquid jet technique to measure 4 × 10 – 3 < γ < 4 × 10 –2 at 278 K. Since HONO uptake by liquid water proba bly involved hydrolysis, an increase in Henry’s law solubility with decreasing temperature may be offset by a decreasing hydrolys is rate constant, leavi ng the uptake coefficient’s temperature trend uncertain. Meas ured uptake coefficients will not correspond to the mass accommodation coefficient.

27. HONO + H 2 SO 4 • nH 2 O(l). Zhang et al. [368] measured uptake coefficients for HONO on sulfuric acid that increased from (1.6 ±0.1) × 10 –2 for 65.3 wt. % H 2 SO 4 (214 K) to (9.1 ±1.6) × 10 –2 for 73 wt. % H 2 SO 4 (226 K). Fenter and Rossi [120] measured uptake coefficients rising from 1.8 × 10 –4 for 55 wt. % H 2 SO 4 (220 K) to 3.1 × 10 –1 for 95 wt. % H 2 SO 4 (220 K and 273 K). Baker et al. [24] measured much smaller uptake coefficients for 60 wt. % at 298 K. In general, the values measured by Zhang et al. [368] are a factor of 2 to 5 higher than those of Fent er et al. [120] for comparable aci d concentrations. Since the reaction probably depends on both temperature and acid concentr ation and since the data scatter is high in both experiments, further independent data will be required to define γ as a function of acid concentration and temperature. These data are generally consistent with the effective Henry’ law constant measurements of Becker et al. [42] who illustrate that HONO solubility decreases exponentially with H 2 SO 4 concentration until ~53 wt %, at which point reac tion to form nitrosyl sulfuric aci d increases H* dramatically as H 2 SO 4 concentration increases. Baker et al. [24] invoke surface decompositi on of HONO to explain their room temperature data, since they separately determine that the bulk second-order disproportionation rate for HONO is too slow to account for even their small uptake co efficients. It is possible that surface formation of nitrosyl sulfuric acid and not HONO disproportionation is responsible for much of their measured uptake. The Zhang et al. [368] and Fenter and Rossi [120] data have been combined and fit with a four-term polynomial as a function of acid wt. % (these data did not show an obvious temperature dependence):

ln γ = a + b wt + c wt 2 + d wt 3

where wt is the H 2 SO 4 wt. %, and

a = –155.7 ± 29.7

b = 5.663 ± 1.232

c = –0.07061 ± 0.01679

d = 0.000297 ± 0.000076
This parameterization should be used only within the 55–95-wt.-%-H 2 SO 4 range and the 214-to-273-K temperature range.

28. HONO + HCl + H 2 O(s). Knudsen cell uptake studies for HONO/HCl co-deposited on ice (180–200 K) and for HONO on 0.1 to 10 m HCl frozen solutions (~190 K) by Fenter and Rossi [120] showed HONO uptake coefficients in the 0.02 to 0.12 range as long as surface HCl concentrations significantly exceed HONO concentrations. ClNO was evolved qua ntitatively with HONO consumption.

29. HONO + HCl on H 2 SO 4 • nH 2 O(l). Fenter and Rossi [120] saw no reaction for acid wt. % > 65. They
measured γ = 2.0 ± 0.7 × 10 –3 for 60 wt. % acid saturated with HONO at 230 K. Zhang et al. [368] also measured the uptake of HCl after exposure to HONO, they observed HCl uptake with γ s between 0.01–0.02 over an acid wt. % range of 60.8–71.3 (T = 207.9–222.6 K). The reaction was also st udied by Longfellow et al. [242] using both HCl doped and HONO doped sulfuric acid aerosols. Their uptake measurements5-24 confirmed reaction at highe r acid wt. %, but by usi ng lower HONO partial pressures they measured smaller

γ s. The reverse reaction, ClNO hydrolys is, was also studied in a wetted wa ll flow reactor and in the aerosol flow reactor by Longfellow et al. [ 242] and in a Knudsen cell reactor by Fenter and Rossi [120]. Data show clear evidence of both surface and bulk kinetics for the forward reaction. Longfello w et al. [242] report k II values for the bulk reaction (in units of 10 4 M –1 s –1 ) for 50 wt. %: 81 at 250 K and 15 at 205 K; for 60 wt. %: 9.4 at 250 K, 6.9 at 230 K and 5.0 at 219 K; for 67 wt. %: 3.9 at 250 K; and for 70 wt. %: 5.8 at 269 K and 0.35 at 215 K. The reaction is clearly complex and w ill require a comprehensive model of both the surface and bulk processes to arrive at an appropriate parameterization for γ. 30. HONO + NaCl(s). Diffuse reflectan ce experiments by Vogt and Finlayson-Pitt [343] on room temperature NaCl(s) and Knudsen cell uptake experiments by Fenter and Rossi on room temperature NaCl(s) and frozen 0.1 M NaCl aqueous solutions, all failed to show HONO uptake. The latter results yield γ < 1 × 10 –4

. 31. HNO 3 + NaX(s)/KX(s). Vogt and Finlay son-Pitts [342,344] used diffuse in frared reflectance spectroscopy to characterize the process. There was absorption of HNO 3 , but no reaction was observed on completely dry NaCl(s); however, NaNO 3 forms in the presence of very low (well below the deliquescence point) levels of H 2 O(g). Using XPS spectroscopy to id entify surface products and a dry HNO 3 source, Laux et al. [230] (also see Vogt et al.) measured γ = (4 ±2) × 10 –4 at 298 K. Fenter et al. [118] measured the room temperature uptake of HNO 3 on solid powders of NaCl, NaBr, KCl, KBr, and NaNO 3, using Knudsen cell/mass spectrometry techniques. They saw similar uptake for all surfaces, including unreactive NaNO 3 , and recommend γ = (2.8 ±0.3) × 10 –2 for all salts. HCl or HBr was produced with ~100% yield from the halide surfaces. There is some concern about the effective surface area of the powders used by Fenter et al. (see Leu et al.[235]). Fenter et al. report new HNO 3 data to support their argument that “sticky” gases such as HNO 3 cannot penetrate below the top surface layer of the powders used in their experiment s. Leu et al. [235] used flow tube/mass spectrometry techniques to measure γ = (1.3 ±0.4) × 10 –2 at 296 K and γ > 8 × 10 –3 at 223 K, both in the presence of low levels of H 2 O(g). They determined that uptak e at 296 K was reactive, producing HCl but that at 223 K reaction was suppressed and uptake was largely ab sorptive. Beichert and FinlaysonPitts [46] measured γ = (1.4 ±0.6) × 10 –2 at 298 K with a Knudsen cell technique, and, using D 2 O, demonstrated that chemisorbed water, presumably retained on defect sites, was crucial for NaNO 3 formation. This suggests that low levels of defect-retained water are responsible for the small uptake values measured by Laux et al.

32. HO 2 NO 2 + HCl on H 2 SO 4 • nH 2 O(l). Zhang et al. [369] performed we tted-wall flow-reactor studies with HCl and HO 2 NO 2 partial pressures in the 10 –6 to 10 –7 Torr range. Using chemical ionization mass spectrometry (CIMS) to detect expected reaction products, no Cl 2 (using SF 4 – as an analyte ion) or HOCl (using F

– ) was detected over a temperature range of 200–225 K and an acid concentration range of 50–70 wt. % H 2 SO 4 . An upper limit for the reactive uptake coefficient for HO 2 NO 2 reacting with HCl of γ < 1 × 10 –4 was deduced.

33. NH 3 + H 2 SO 4 • nH 2 O. Robbins and Cadle [289], Huntzicker et al. [184], McMurry et al. [253], and Daumer et al. [97] all studied NH 3 uptake by sulfuric acid aerosols in near room temperature flow reactors (T = 281–300 K). Uptake coefficients varied between 0. 1 and 0.5. Rubel and Gentry [299] used levitated H 3 PO 4 acid droplets to show that heterogeneous reaction does control the initial NH 3 uptake on strong acid solutions. Both Rubel and Gentry and Däumer et al. also explored the effect of organic surface coatings.

34. CH 3 C(O)O 2 + H 2 O(l) and H 2 SO 4 • nH 2 O. Villalta et al. [339] used we tted-wall flow tube techniques to

measure γ = 4.3 (+ 2.4 /–1.5) × 10 –3 for water at 274 ± 3K. They also measured uptake for 34 wt % H 2 SO 4 at 246 K ( γ = (2.7 ± 1.5) × 10 –3 ), 51 wt % at 273 K ( γ = (0.9 ± 0.5) × 10 –3 ), and 71 wt % at 298 K ( γ = (1.4 ± 0.7) × 10 –3 ). They suggest that products subsequent to hydrolysis are HO 2 and CH 3 C(O)OH.

35. CH 3 C(O)O 2 NO 2 + HCl, Cl, ClO, and OClO on H 2 SO 4 • nH 2 O(l). Zhang and Leu [364] performed wetted wall flow reactor studies with Cl sp ecies partial pressures in the 10 –6 to 10 –7 Torr range and CH 3 C(O)O 2 NO 2 at 3 × 10 –6 Torr after equilibrating the acid surfaces ( 42, 51, and 69 wt. % at 202 and 224 K) with CH 3 C(O)O 2 NO 2 . Also uptake studies with 5 × 10 –7 Torr CH 3 C(O)O 2 NO 2 were performed after exposing the acid surface to the Cl speci es. No Cl species or CH 3 C(O)O 2 NO 2 uptake enhancements were observed under either condition and an upper limit for the reactive uptake coefficient of γ < 1 × 10 –4 of CH 3 C(O)O 2 NO 2 was deduced. No gas phase reaction products we re observed using CIMS after 42 wt. % H 2 SO 4 at 210 K was exposed to CH 3 C(O)O 2 NO 2 and each Cl species for 20 minutes.

36. Cl + H 2 SO 4 • nH 2 O(l). Measured reaction probability (Martin et al. [250]) varies between 3 × 10 –5 and 7 × 10 –4 as H 2 O and T co-vary. Reaction product is claimed to be HCl.5-25 37. Cl 2 +HBr + H 2 O(s). Hanson and Ravishankara [159] measured a reaction proba bility of > 0.2 on water ice near 200 K. BrCl was not detected, presumab ly due to rapid reaction with excess HBr.

38. Cl 2 and BrCl + KBr(s). Caloz et al. [64] measured γ > 0.1 for reactive uptake of Cl 2 and BrCl on KBr(s) in a room temperature Knudsen cell experiment.

39. Cl 2 and Br 2 + NaBr(aq) and NaI(aq). Hu et al. [181] measured large uptake coefficients for Cl 2 on dilute aqueous droplets of NaBr and NaI solutions and Br 2 on NaI solutions using a droplet train technique. Reaction was demonstrated to proceed through bot h a chemisorbed surface complex and normal bulk solution second-order kinetics. S econd-order bulk reaction rate cons tants near the diffusion limit and consistent with bulk-phase kinetic measur ements were obtained between 263 and 293 K.

40. ClO + H 2 O(s) and HNO 3 • nH 2 O(s). Proposed reaction (Leu [233]) is 2 ClO → Cl 2 + O 2; reactive uptake may depend on ClO surface coverage, which in turn may de pend on gas phase ClO concen trations. Kenner et al. [214] measured reaction pr obabilities of (8 ±2) × 10 –5 for ice at 183 K which is far lower than the limit of >1 × 10 –3 obtained by Leu [233]. Abbatt [3], using nearly the same low levels of ClO as Kenner et al., obtained γ < 1 × 10 –5 at 213 K. The difference may lie in the level of ClO or other adsorbable reactive species present. The lower value of Abbatt is probably closer to the expected reactivity under stratospheric conditions. Kenner et al. also measured a reaction probability limit of < (8 ±4) × 10 –5 for NAT at 183 K.

41. ClO + H 2 SO 4 • nH 2 O. Measured reaction probability (Martin et al. [250]) varies between 2 × 10 –5 and 2 × 10 –4 as H 2 O content is varied by changing wall temperature. Reaction product is claimed to be HCl, not Cl 2 . Abbatt [3] measured γ < 1 × 10 –5 for 60 and 70 wt % H 2 SO 4 at 213 K.

42. HCl + HNO 3 on H 2 SO 4 • m HNO 3 • nH 2 O(l). Two studies have noted HCl activation in concentrated ternary H 2 SO 4 /HNO 3 /H 2 O solutions or ice slurries. Luick et al. [246] saw only gas phase HCl in 64.6 wt. % H 2 SO 4 / 4.8 wt. % HNO 3 at 200 K, but saw a vapor phase Cl partitioning of 50% HC l and 50% ClNO/ClNO 2 for a 76.6/20.1 wt. % solution (an ice slurry) at 200 K. Cappa et al. [65] saw substantial yields of ClNO, ClNO 2 , and Cl 2 at 273 K for a range of solution compositions ; e.g. 32.6%, 9.8% and 44.4% respectively for a total HCl conversion of 86.9% in a 35% H 2 SO 4 /45% HNO 3 solution and 20.2%, 6.9%, 27.9% for a 60/25 wt. % solution. While no kinetic coefficients or detailed m echanisms are available, these studies do show the potential for HCl activation in strong H 2 SO 4 /HNO 3 /H 2 O solutions.

43. HOCl + HCl + H 2 O(s) and HNO 3 • 3H 2 O(s). Hanson and Ravishankara [158] and Abbatt and Molina [6] have investigated the HOCl + HCl reaction on water ice and NAT-like surfaces, a nd Chu et al. [76][72] studied the reaction on water ice. Product yield measurements support the identification of Cl 2 and H 2 O as the sole products. The measured yield of product Cl 2 is 0.87 ±0.20 and was stated to be similar on both surfaces according to Abbatt and Molina. Within the accuracy of the e xperiments, the reaction probability does not depend on the gas phase HCl and HOCl densities. Only Abbatt and Molina investigated at more than one temperature, th eir data indicates that γ increases at lower temperatures . A plot of data from the three studies does show a weak temperature trend, with γ increasing about a factor of two as the temperature drops from 202 to 188 K. However, the data are too sparse to assign a definitive temperature dependence. The average of all three studies yields γ = 0.26 ± 0.08 for data based on the geometrical area of the flow tube surfaces. Chu et al. [72] i ndicate that a porosity correction for their data would reduce their value bya factor of 3 to 4. The real uncertainty would appear to be dominated by systematic uncertainties in porosity corrections and a potential temperature dependence. Give n the fact that any porosity correction must reduce the value, a central value of 0.2 is adopted with an uncertainty factor of 2. The high reaction probabilities measured for water ice indicate that this reaction may pl ay a significant role in re lease of reactive chlorine from the HCl reservoir.
Two studies (Hanson and Ravisha nkara [158]; Abbatt and Molina [6]) have measured the reaction probability of HOCl + HCl on NAT surfaces. These data show γ increases as the ambient water pressure increases and then reaches a plat eau. At relatively high water pre ssure, the two studies averaged γ = 0.135 ± 0.049, with no porosity correction. The reaction pr obability on water poor NAT-like surfaces falls off dramatically (a factor of 10). A recommendation of 0.1 with an uncertainty factor of 2 is shown in Table 5-2. Carslaw and Peter [67] have published a model of this reaction and its dependence on HCl uptake.

44. HOCl + HCl + H 2 SO 4 • nH 2 O(l). This process has been studied in coated flow tubes over ~200–260 K by Zhang et al. [363], Hanson and Ravishankara [161], D onaldson et al. [107], and Hanson and Lovejoy [154]. Hanson and Lovejoy also made measurements in an aer osol flow tube from 251 to 276 K. A model of this and related sulfuric acid aerosol reactions tailored to stratospheric conditions has been published by Hanson et al. [168]. Zhang et al. held the water vapor partial pressure at 3.8 × 10 –4 Torr and showed γ increased by a5-26 factor of 50 as the temperature was lowered from 209 to 198 K, showing that the reaction rate is strongly dependent on water activity.
A detailed kinetic uptake model has been developed to fit the experimental data [313]. The formulation for γ is given as:


### 11 1

rxn H

OCl 

### γ α = + Γ

where 

# ( ) 1/2

_ 

### 4

rxn HOCl HOCl HOCl HOCl HCl 

### H RT D k

c Γ =

At the low temperatures of interest, α for HOCl was assumed to be unity consistent with the value for HCl measured at 240 K and below (Robinson et al. [294]). The individual formulations for H HOCl , D HOCl and k HOCl-HCl are given in Table A-4 in Shi et al. [313]. Reaction of HOCl with HCl is considered to be acid catalyzed. It is known that the reac tion rate for HOCl + HCl in pure wate r is low (Donaldson et al. [107]). Experimental data noted a bove indicated that the reaction rate of HOCl + HCl increases with acidicity of H 2 SO 4 solution. The data from the experimental studies noted above were fit to the model without bias. Using the same error analysis discussed in the note for N 2 O 5 uptake on sulfuric acid, a detailed kinetic model yields a 33.4% error (one sigma fit to the available data set, with σ m =33.3% and σ d =3.0%).
In the cold stratosphere where T<190 K, the reaction of ClONO 2 + HCl is so fast that HCl is depleted which slows down the reaction of HOCl + HCl. As shown in Table A-4 in Shi et al., the effect of HCl depletion on the HOCl reactive uptake coefficien t (due to reaction with ClONO 2 inside/on the surface of particles) is taken into account via the factor F HCl (also see the note on chlorine nitrate/hydrochloric acid reactive uptake on sulfuric acid surfaces).

45. HOCl + HBr on H 2 O(s). Chu and Chu [72] measured γ at 189 K to be in the range from 0.06 to 0.38 for HBr partial pressures ranging from 1.1 × 10 –7 to 6.6 × 10 –5 Torr. At 220 K they measured γ in the range from 0.01 to 0.07 for HBr partial pressures in the range from 7.2 × 10 –7 to 1.3 × 10 –5 Torr. These γ values were estimated assuming the area of the i ce surface to be equal to the geomet ric area of the cylindrical flow reactor; corrections for surface porosity effect s range from a factor of 3 to 10 lower.

46. HOCl + HBr on H 2 SO 4 • nH 2 O(l). Abbatt and Nowak [8] measured upt ake of HOCl in the presence of excess HBr on a 69.3 wt. % sulfuric acid solution in a wette d wall flow reactor at 228 K. A second order bulk reaction rate constant, k II , of 2 × 10 6 M –1 s –1 was derived; this is a factor of ~10 faster than HOBr + HCl under the same conditions. Since HOCl and HBr have si milar solubilities under stratospheric conditions, characterizing this reaction with a simple uptake coefficient is not appropriate. A full reaction/solubility/liquid phase diffusion model will require further data.

47. ClNO and ClNO 2 + NaCl(s). Using a Knudsen cell technique Be ichart and Finlayson-Pitts set upper limits of

γ < ~10 –5 for reactive uptake of ClNO and ClNO 2 on NaCl(s) powders at 298 K.

48. ClONO 2 + H 2 O(s). Measurement of γ = 0.3 (+0.7, –0.1) (Hanson and Ravishankara [155]) significantly exceeds previous measurements of Molin a et al. [260], Tolbert et al. [333] , Leu [232] and M oore et al. [262] but agrees reasonably well with subsequent measurements by Chu et al. [76] and Zhang et al. [365] when geometrical surface areas are assumed for analysis. Pr evious measurements were probably complicated by NAT formation on the surface (Hanson and Ravishankara [158]; Chu et al. [76]). Lower levels of ClONO 2 (g) used by Hanson and Ravishanka ra [155] minimized this surface sa turation problem. Also, using lower ClONO 2 concentrations, Zhang et al. obtained a reaction probability of 0.08 ± 0.02 at 195 K, in fair agreement with the range of 0.03 to 0.13 measured by Chu et al. Subsequent Knudsen cell measurements at 180 and 200 K by Oppliger et al . [272] showed initial uptake γ s in the 0.2 to 0.4 range. Measured reaction products were HNO 3 and HOCl. All of the HNO 3 and much of the HOCl is retained on the surface under polar stratospheric conditions (Hanson and Ravi shankara [155,158]). Hanson [149] deposited ClONO 2 on H 2 18 O enriched ice and detected H 18 OCl showing the Cl–ONO 2 bond is broken at 191 K.
Data plots confirm a trend showing that at a high density of ClONO 2 , the product HNO 3 covers the ice surface preventing the further reaction of ClONO 2 with H 2 O molecules on the surface. Therefore, data obtained at high ClONO 2 densities (>10 14 molecules/cm 3 ) are excluded from furt her evaluation. An experiment (Berland et al. [53]) using a laser-induced thermal desorption technique yielded a much lower value of ClONO 2 reaction probability at 190 K (a bout 3 orders of magnitude lo wer) after extrapolating the5-27 results obtained at temperatures of 140 K and below. We also exclude this point in the averaging of data since the physical characteristics of ice surfaces at these very low temperatures may not be very representative of those found at stratospheric temperatures. Selected data show no temperature dependence between T=180 and 200 K and averaged γ o = 0.28 ± 0.25. Again, within the experimental accuracy, the Hanson and Ravishankara [158,160] and Chu et al. [76] data show that uptake measurements are nearly independent of ice substrate thickne ss. See Henson et al. [173,174] for discussion of a model which accounts for the effect of HNO 3 on the reaction ClONO 2 on water and nitric acid ice surfaces.
Zondlo et al. [374] report the formation of a supercooled H 2 O/HNO 3 liquid layer at 185 K as a reaction product, forming NAT or NAD only after decreasing the relative humidity below the ice frost point. This effect is similar to that resulting from the interaction of gaseous HNO 3 or N 2 O 5 with the ice surface. These authors measured γ = (3 ± 2) ×10 –3 at 185 K for the reaction of ClONO 2 with this supercooled liquid layer.

49. ClONO 2 + HNO 3 •nH 2 O(s). Hanson and Ravishankara [155] report a γ value of 0.006 at 201 K for the ClONO 2 reaction with the water on NAT (HNO 3 •nH 2 O). However, these authors present re-analyzed and additional data with γ ≈ 0.001 at 191 K in Hanson and Ravishanka ra [158,160]. Similar experiments (Moore et al. [262], Leu et al. [234]) report a larger value of 0. 02 ±0.01 which falls very rapidly as slight excesses of H 2 O above the 3/1 H 2 O/HNO 3 ratio for NAT are removed. They measure γ of less than 1×10 –6 for slightly water poor NAT surfaces. The inconsistency between Hanson and Ravishankara and the JPL group (Moore et al. [262]; Leu et al., [234]) has not been resolved. Abbatt and Molina [7] report γ values reaching 0.002 at 202 K and high RH. Hanson and Ravi shankara [158] reported that γ for this reaction increases by a factor of 4 as the surface temperature increases from 191 to 211 K. However, Knudsen cell measurements at 185 K by Barone et al. [30] reported γ = 0.004 at a relative humidity (RH) of 100%, rising to 0.007 near RH = 120%, indicating a possible mild negative temperature dependen ce when high RH values from this and other studies are compared. Excluding the JPL data, the other data obtained at high RH (~90%) were averaged, assuming no temperature dependence, to yield γ = 0.0043 ±0.0021. The strong dependence on RH and the possible temperature dependence suggest that sy stematic error probably exceeds the cal culated statistical error. Within the experimental accuracy, the data of Hanson and Ravishankara [158, 160] show that measured uptake coefficients are independent of ice substrate thickness. Barone et al. re port very similar uptake coefficients for nitric acid dihydrate (NAD) as for NAT as a function of RH at 202 K. See Henson et al. [173,174] for discussion of a model which accounts for the effect of HNO 3 on the reaction of ClONO 2 on water and nitric acid ice surfaces.

50. ClONO 2 + H 2 SO 4 •nH 2 O(l). Results from wetted-wall flow tube (Hanson and Ravishankara [165]) Knudsen cell reactor (Manion et al. [249]), aerosol flow tube (Han son and Lovejoy [153]), and droplet train uptake (Robinson et al. [293]) experiments supplement older wetted-wall flow tube (Hanson and Ravishankara, [157]) and Knudsen cell measurements (Rossi et al. [298]), (Tolbert et al [332]). Although earlier Knudsen cell measurements probably suffered from surface satura tion, more recent results compare well with those from other techniques. Saturation free results, ava ilable over a temperature range of 200–265 K and a H 2 SO 4 concentration range of 39 to 75 wt. %, were fit to a phenomenological model developed by Robinson et al. [293]. Measured γ values depend strongly on H 2 SO 4 concentration and vary modestly with temperature, with a trend to somewhat higher values for the 210–220 K temperature range. The temperature-dependent uptake model takes into account the temperature and compositi on dependence of the effective Henry's Law constant, liquid phase diffusion coefficient, and the liquid phase hy drolysis rate constant. The hydrolysis reaction was treated by modeling two reaction channels, a direct hydrolysis process dominating reaction at low H 2 SO 4 concentrations with a reaction rate proportional to wate r activity and a proton-cataly zed reaction with a rate proportional to H + activity, which dominates at higher acid concentrations.
The data fit to the original Robinson et al. model have been supplemented by additional wetted-wall flow tube and aerosol flow tube data from Hanson [150] and aer osol flow tube data from Ball et al. [28]. A revised kinetic model (Shi et al. [313]) incorporating these data has been developed that is based on the earlier work of Robinson et al. [293].In this model, γ is calculated using the expression

2 

### 11 1

H O b 

### γ α = + Γ

where, 

# ( ) 2 2

2 1/2 

### 4 ClONO H O b ClONO hydr 

### H RT D k

c Γ =5-28 The detailed parameterizations for H ClONO 2 , D ClONO 2 , and k hydr are given in the Appendix in Shi et al. [313] As was the case for N 2 O 5 hydrolysis k hydr is seen to have a direct and an aci d catalyzed channel. Using the same error analysis approach as in the note on N 2 O 5 uptake, the model error is about 32.4% (one sigma), with

σ m =32.2% and σ d =4.0%. In the calculation of the chlorine activation (Cl 2 production) rate under stratos pheric conditions, one needs to take into account the competition between the reactions of ClONO 2 + H 2 O and ClONO 2 + HCl. The presence of HCl will depress the reaction probability of ClONO 2 with H 2 O (see note 49).

51. ClONO 2 + H 2 SO 4 • H 2 O(s) and H 2 SO 4 • 4H 2 O(s). Measurements by Hanson and Ravishankara [162] and Zhang et al. [363] demonstrate that the reaction probability on the tetrah ydrate is a strong function of both temperature and relative humidity, both of which affect the level of adsorbed H 2 O. Both groups covered the temperature range of 192–205 K. The reaction is slow est at higher temperatures and lower relative humidities. Zhang et al. [363] have parame terized their data in the form of log γ = a 1 + a 2 log x + a 3 log 2 x; for 195 K and x = water partial pressure in Torr: a 1 = 10.12, a 2 = 5.75 and a 3 = 0.62; for a water partial pressure of 3.4 × 10 –4 Torr and x = T(K) between 182 and 206: a 1 = 318.67, a 2 =–3.13 and a 3 = 0.0076. Zhang et al.[367] have also measured a low value of γ ∼ 2 × 10 –4 on sulfuric acid monohydrate at 195 K.

52. ClONO 2 + HCl + H 2 O(s). Reaction probabilities of 0.27 (+0.73, –0.13) (Leu [232]) and 0.05 to 0.1 (Molina et al. [260]) were reported at 195 and 185 K, re spectively. Abbatt and Molina [7] and Hanson and Ravishankara [157] report th at a portion of the reaction may be due to HOCl + HCl → Cl 2 + H 2 O, with HOCl formed from ClONO 2 + H 2 O(s) → HOCl + HNO 3 (s). Hanson and Ravishankara [155] saw no enhancement of the ClONO 2 reaction probability when H 2 O(s) is doped with HCl. Their preferred value at 192 K is γ = 0.3, but this is consistent with γ = 1. Chu et al. [76] also report a value of 0.27 (±0.19) at 188 K, assuming no correction for porosity, but suggest the true value is 0.10 (±0.08). Using a Knudsen cell technique and looking at initial uptake, Opplig er et al. [272] measured γ = 0.7 at 180 K and 0.2 at 200 K with HCl in excess. Eliminating the Molina et al. points, which were taken at much higher ClONO 2 concentrations than the others, plots of the remaini ng data show no obvious bias when plotted as a function of reactant concentration or temperature (180–200 K). Their average value γ = 0.26 ±0.06. The Oppliger et al. data were presented for two HCl concentrations, differing by a factor of three. All points from both HCl concentrations were included since all the data were generally cons istent with previous measurements, although the higher HCl concentrations did tend to produce modestly higher uptake coefficients. Until a fuller model is available, a single temperature independent value with a m oderate uncertainty due to surface porosity seems appropriate.

53. ClONO 2 + HCl + HNO 3 •3H 2 O. Measurements by Hanson and Ravish ankara [155,158], Leu and co-workers in Moore et al. [262] and Leu et al. [234], and Abbatt and Molina [7] all report high γ values (>0.1) on NAT for temperatures between 192 and 202 K. Hanson and Ravishankara indicate th at reaction probabilities on NAD are similar to those on NAT. The most recent NAT studies (Abbatt and Molina [7]) show a strong falloff with relative humidity from γ > 0.2 at 90% RH to 0.002 at 20% RH, indicating the necessity of sufficient water to solvate reactants. Within the limited measurements, data plots show no indication that the reaction probability of ClONO 2 + HCl depends on HCl and ClONO 2 gas phase concentrations or temperature between 191 and 202 K. Averaged data yield is γ = 0.23 ±0.10. Carslaw and Peter [67] have published a model of this reaction and its dependence on HCl uptake.

54. ClONO 2 + HCl + H 2 SO 4 •nH 2 O(l). Early work by Tolbert et al. [332] and Hanson and Ravishankara [157] indicated that the presence of HCl ha d little effect on the reaction of ClONO 2 with concentrated sulfuric acid (>65 wt.% H 2 SO 4 ). Subsequent realization that HCl would be more soluble, and therefore a more potent reactant, in the colder, mo re dilute sulfuric acid aerosols character istic of the polar stratosphere led to additional investigations by Hanson and Ravishankara [165], Zhang et al. [363], Elrod et al. [113] and Hanson [150]. All these measurements show a strong dependence of reactivity on HCl solubility, which in turn depends on water activity. The solubility of HCl in a wide range of sulfuric acid solutions has been experimentally determined by a range of techniques th at agree well with current thermodynamic models. See Robinson et al. [294] fo r a review. Hanson and Lovejoy [153] measured a reacto-diffusive length, 

### A , of only 0.009±0.005 μ m for 60 wt.% H 2 SO 4 in an aerosol flow reactor. (See Ha nson et al. [168] fo r a definition of 

### A .) This is a factor of four lower than the value for the hydrolysis reaction of ClONO 2 showing the significant enhancement of ClONO 2 uptake due to HCl.5-29 The ClONO 2 + HCl reaction on sulfuric acid has been modeled in Shi et al. [313] using the same phenomenological model for ClONO 2 hydrolysis driven uptake by sulfuric acid. Since the effect of HCl on the ClONO 2 uptake is to increase the ClONO 2 pseudo-first-order reaction rate, the model of ClONO 2 uptake (see note on ClONO 2 uptake on sulfuric acid ) should include the pseudo first order reaction rate, k HCl . The formulation of k HCl is found in the Appendix in Shi et al. [313].. It is likely that the ClONO 2 reaction with HCl, like the ClONO 2 hydrolysis reaction, is acid catalyzed via protonated HClONO 2 + , where Cl + is activated as in the case of HOCl + HCl. For the ClONO 2 + HCl reaction, there is al so a surface reaction (Hanson [150]). Hanson proposed that Γ s is linearly proportional to water activity; however, the calculated value of γ o at 250 K and 60 wt% H 2 SO 4 using his formulation is 0.02 (here γ o ~ Γ s ), which is contradictory to his aerosol flow reactor result, which yielded γ o =0.0079 (here γ o ~ Γ b ) (Hanson and Lovejoy [153]). In the model presented in the Shi et al. appendix, it is assumed that that Γ s is linearly proportional to Henry’s law constant of ClONO 2 , rather than the water activity . The temperature dependence of Γ s is determined, based on two measured values of Γ s at 203 K (Hanson, [150]) and 250 K (Hanson and Lovejoy, [153]). The model yields a value of γ o ~0.011 (here γ o ~ Γ s ), which is close to the measured value.
In the stratosphere, when the reaction rate of ClONO 2 with HCl exceeds the flux of HCl to the particle surface, HCl is depleted. This, in turn , will depress the rate of both the ClONO 2 and HOCl + HCl reactions, and increase the ClONO 2 hydrolysis rate. Shi et al. [313] have proposed a model in which this effect is taken into account by including a factor F HCl (see Table A–3 in Shi et al.). The formulation of F HCl is based on scaling HCl reaction and accommodation fluxes. This flux correction is not exact (i.e. it does not rigorously calculate the HCl surface or bulk concentration) but provides a good approximation to the expected reduction in HCl + ClONO 2 /HOCl reactivity and, just as importantly, the effective increase in ClONO 2 + H 2 O reactivity when p ClONO 2 > p HCl . This is particularly relevant during cold Cl activation events when HCl can be removed almost completely (i.e., see Jaegle et al. [194]).
Using the same error analysis approach as in the note on N 2 O 5 uptake by sulfuric acid, the error of using the model in the Appendix is about 40.0% (one sigma), with σ m =39.8% and σ d =4.0%

55. ClONO 2 +HCl + H 2 SO 4 • H 2 O(s) and H 2 SO 4 • 4H 2 O(s). This reaction has been studied by Hanson and Ravishankara [162] and Zhang et al. [363]. The reaction probability is strongly dependent on the thermodynamic state of the SAT surface, which is cont rolled by the temperature and the water vapor partial pressure. At a water vapor pressure of 5.6 × 10 –4 Torr the measured γ drops by over two orders of magnitude as the SAT surface temperature rises from 195 to 206 K. The results from the two groups are in qualitative agreement, but sample different H 2 O and HCl partial pressures. Zhang et al. have parameterized their data as a function of water partial pressure (at 195 K) and temp erature (both at an HCl partial pressure of 4 to 8 × 10 –7 Torr) in the form log γ = a 1 + a 2 log x + a 3 (log x) 2 . For H 2 O partial pressure, a 1 = 5.25, a 2 = 1.91, and a 3 = 0.0; for T(K), a 1 = 175.74, a 2 = –1.59, and a 3 = 0.0035. Care must be taken in extrapolating either data set to lower HCl concentrations. Zhang et al. [367] measured no enhancement of ClONO 2 uptake on sulfuric acid monohydrate at 195 K with (2–8) × 10 –7 Torr of HCl present, implying γ < 1 × 10 –4

. 56. ClONO 2 + HCl + Al 2 O 3 (s). Molina et al. [259] used flow tube techniques to measure γ = 0.020 ±0.005 on

α− alumina at 195–230 K with stratospheric (5 ppmV) water vapor levels. Measured γ was independent of T and was affected very little by 5 ppbv HNO 3 vapor. The same γ was measured for a Pyrex surface, indicating the absorbed water and not the inorganic substrate hosted the reaction.

57. ClONO 2 + MX(s). Finlayson-Pitts and co-workers have shown that ClONO 2 reacts with crystalline NaCl (Finlayson-Pitts et al. [122]) and Na Br (Berko et al. [52]) to produce Cl 2 and BrCl, respectively. Timonen et al. [329] have measured the reaction rate for ClONO 2 with dry and slightly wet (water vapor pressure 5 × 10

–
5 to 3 × 10 –4 Torr) NaCl at temperatures of 225 and 296 K. Reaction probabilities were analyzed as

γ = 4–7 × 10 –3 and were independent of temperature and water vapor pressure within experimental error. The Cl 2 yield on dry NaCl was 1.0 ±0.2. Caloz et al. [64] used a room temperature Knudsen cell technique to

measure γ = 0.23 ±0.06 for NaCl(s) and γ = 0.35 ±0.06 for KBr(s). They argue that the surface corrections imposed by Timonen et al. were too large. Caloz et al. measured quantitative yields of Cl 2 and BrCl products.

58. ClONO 2 +HBr + H 2 O(s) and HNO 3 • nH 2 O(s). This reaction was studied by Hanson and Ravishankara [159] on water ice and NAT near 200 K. A diffusion-limited reac tion probability of >0.3 was observed. Allanic et al. [17] measured γ = 0.56 ± 0.11 at 200 K on water ice, observing Cl 2 and Br 2 to be formed in yields of 100% and 66 to 80%, respectively, in the range 180 to 200 K.

59. ClONO 2 + HF + H 2 O(s) and HNO 3 • nH 2 O(s). Hanson and Ravishankara [159] were not able to observe this reaction on water ice and NAT surfaces near 200 K.5-30 60. CF x Cl (4-x) (x=0–3) and CF 2 Br 2 + Al 2 O 3 (s). Robinson et al. [291] reported dissociative uptake of CF 2 Cl 2 and CF 2 Br 2 on α -alumina surfaces at 210 and 315 K. Reaction probabilities of about 1 × 10 –3 at 210 K were measured by monitoring the amounts of surface species bonded to the Al 2 O 3 substrate. A re-analysis (Robinson et al. [292]) lowered this value by about a factor of 50. Moderate surface dosage with water vapor did not quench the reaction. In addition, Dai et al. [95] and Robinson et al. [290] studied dissociative chemisorption of CF 3 Cl, CF 2 Cl 2 , CFCl 3, and CCl 4 on dehydroxylated γ -alumina powders. The obtained reactive uptake probabilities ranging from 0.4 × 10 –5 for CFCl 3 to 1.0 × 10 –5 for CFCl 3 over a temperature range of 120 to 300 K. HCl and halomethyl radicals were observed as desorption products. Loss of these products may point to somewhat higher γ s, since they were measured by integrating halogen bound to Al 2 O 3 substrates.

61. BrO + H 2 O(s) and H 2 SO 4 • nH 2 O(l) and NaCl(aq). Abbatt [3] used a coated flow tube technique to measure heterogeneous uptake on water ice, 60 and 70 wt % H 2 SO 4 at 213 K, and 23 wt % aqueous NaCl at 253 K. He obtained γ (ice) = (1.0 ± 0.4) × 10 –3

, γ (60 wt % H 2 SO 4 ) = (7 ± 2) × 10 – 4

, γ (70 wt % H 2 SO 4 ) = (5 ± 2) × 10 – 4 and γ (23 wt % NaCl) < 3 × 10 –3 . He observed product Br 2 , indicating BrO self-reaction on both water ice and sulfuric acid solutions. Since reaction rate will depend on BrO concentrations, no recommendation is made for an atmospheric rate.
62. HOBr + HCl(s). Abbatt [1] measured γ = 0.25 (+0.10/–0.05) for this reaction on ice at 228 K. The BrCl product was observed by mass spectrometry. No da ta on NAT surfaces are currently available.

For the sulfuric acid reac tion, Abbatt [2] measured γ s of ~ 0.1 to 0.2 for [HCl] > 1 × 10 12 cm –3 over 68.8 wt. % H 2 SO 4 at 228 K; yielding an estimated k II HCl+HOBr = 1.4 × 10 5 M –1 s –1 with a factor of 2 uncertainty. Hanson and Ravishankara [166] also measured γ = 0.2 [+0.2, – 0.1] for 60 wt. % H 2 SO 4 at 210 K. However, both of these measurements were base d on significant underestimati on of the solubility of HOBr in the relevant sulfuric acid solutions. More recent measurements by Waschewsky and Abbatt [347] indicate that H for HOBr vari es slightly with acidity between 60 to 70 wt.% H 2 SO 4 and more strongly with temperature between 208 and 238 K. (For 59.7 wt.% H 2 SO 4 , H (M atm –1 ) = 1.2×10 6 at 208 K and and 2.2×10 5 at 228 K.) The HOBr + HCl second order liquid phase rate constant, k II HCl+HOBr , varies between 2×10 5 and 3×10 8 (M –1 s –1 ) between 213 and 238 K over the same composition range (60–70 wt.% H 2 SO 4 ). Such a strong dependence on acid composition for the reaction rate of HOBr + HCl and the very small acid composition dependence for HOBr solubility in H 2 SO 4 solution might be partially due to the formation of H 2 OBr + in the acidic solution as discussed in their paper. Ho wever, this acid catalyzed reaction, i.e. H 2 OBr + + HCl, alone does not completely account for measured reacti on rates over the acid co mposition range studied.
Using the Henry’s Law data for HOB r reported by Waschewsky and A bbatt [347], the limiting reagent will vary depending on atmospheric temperature (H 2 SO 4 wt.%) and the concentrations of HOBr and HCl. For stratospheric conditions where [HOB r] is 10 pptv and [HCl] 1ppbv, they predict dissolved HOBr will be in excess above 204 K and HCl in excess below 204 K for a H 2 O vapor partial pressure of 3×10 –7 atm. From their coated wall flow reactor uptak e measurements, Waschewsky and A bbatt [347] derived expressions for k II HCl+HOBr and predicted uptake coefficients. For temperature between 204 and 218 K where HOBr is likely to be in excess, they calcu lated HCl uptake coefficients, γ HCl , which range between 7×10 –5 and 9×10 –5 . For temperatures in the 202–198 K range, where dissolved HCl is likely to be excess, the calculated uptake coefficients for HOBr, γ HOBr , of

∼ 1×10 –2 . Clearly, the HOBr + HCl reaction will be difficult to parameterize in a simple manner. Potential inconsistencies in their k II HCl+HOBr values, as discussed by Waschewsky and Abbatt, indicate that further measurements will be requi red before this reaction can be definitively modeled.

63. HOBr + HBr + H 2 O(s) and H 2 SO 4 • nH 2 O. Abbatt [1] measured γ = 0.12 ± (0.03) on ice at 228 K. The Br 2 product was observed by mass spectrometry. Abbatt [2] measured γ = 0.25 for [HBr] = 1 × 10 12 cm –3 over 68.8 wt % H 2 SO 4 at 228 K; yielding an estimated k II > 5 × 10 4 M –1 s –1

. 64. BrONO 2 + H 2 O(s). Hanson and Ravishankara [160] investigated these reactions in an ice-coated flow reactor at 200 (± 10) K. The reaction of BrONO 2 with H 2 O(s) proceeded at a rate i ndistinguishable from the gas phase diffusion limit, implying that the reaction probability may be as high as one; the product BrNO(g) was observed. Allanic et al [16] used a Knudsen cell reactor to measure BrONO 2 uptake between 190–200 K. Values of initial γ s in the 0.2–0.3 range were observed. An average γ = 0.26 ± 0.05 was obtained from all of the appropriate data from both experiments.

65. BrONO 2 + H 2 SO 4 •nH 2 O(l). Hanson and co-workers used both coat ed flow tube and aerosol flow tube techniques to show that the reaction of BrONO 2 with 45–70 wt. % H 2 SO 4 is extremely facile at temperatures5-31 from 210 to 298 K. Hanson and Ravishankara [166] measured γ s of 0.5 (+0.5, –0.25) (45 wt. % H 2 SO 4 , 210 K, 0.4 (+0.6, –0.2) (60 wt. %, 210 K) , and 0.3 (+0.7, –0.1) (70 wt. %, 220 K) in a coated-wall flow tube experiment. Hanson et al. [167] measured γ ~ 0.8 (20 to 40% error) for submicron aerosols at temperatures between 249 and 298 K and H 2 SO 4 concentrations of 45 to 70 wt. %; they did observe a sharp fall off in γ for H 2 SO 4 concentrations between 73 and 83 wt. %. Hanson ha s analyzed these combined data sets, the data indicated that γ is a function of sulfuric acid concentration, but independent of temperature. He has fit an empirical expression for γ for BrONO 2 + H 2 O of: γ = exp(a+b*wt.)+c [Hanson, priv. comm.]. The data have been fitted to the formulation 1/ γ =1/ α +1/ γ rxn , yielding α =0.805, and a=29.24, b=–0.396, c=0.114. Additional unpublished measurements using both techniques at highe r temperatures performed by Hanson [priv. comm.] also fit this functional form. Using the same approach as detailed in the note for N 2 O 5 uptake on sulfuric acid, the error for BrONO 2 + H 2 O is 27.3% (one sigma), with σ m =26.6% and σ d =6.3%.

66. CF 3 OH + H 2 O + H 2 O(l) and H 2 SO 4 • nH 2 O(l). Lovejoy et al. [245] used both wetted-wall and aerosol flow tube techniques to measure reactive uptake of CF 3 OH on water at 274 K and 39–60 wt % H 2 SO 4 at various temperatures between 206 and 250 K. γ ’s showed a strong dependence on water activity. Aerosol uptake studies yielded reacto-di ffusive lengths of > 0.4 μm for 40 wt % H 2 SO 4 and 1.0 μm for 50 wt % H 2 SO 4 , both at 250 K. Recommended γ ’s were estimated by averaging bul k uptake measurements at similar H 2 SO 4 concentrations and ignoring temperature effects on water activity.

67. SO 2 + H 2 O 2 , O 3 , HONO, NO 2 , HNO 3 on H 2 SO 4 • nH 2 O(l). Rattigan et al. [282] us ed a bubble train reactor to measure the uptake of SO 2 in the presence of solvated oxidants at 293 K. For H 2 O 2 the second order rate constant at 1 wt. % H 2 SO 4 agreed well with previous bulk kinetics measurements and with previous droplet train/flow reactor measurements. Meas urements at 20, 40, and 60 wt. % H 2 SO 4 are the first reported for concentrated acid. Reaction rate data were fit to a two term (acid catalyzed and water catalyzed) bulk second order rate expression, which, in the limit of high acid activity ( a H + = α H+ [H + ], where α H+ is the H + activity coefficient) reduces to: k II H 2 O 2 = 8.3 × 10 4 ( α H 2 O / a H + ), where α H 2 O is the water activity coefficient. Both α H+ and α H 2 O can be obtained from the sulfuric acid thermodynamic model of Carslaw et al. [66]. The high a H + approximation for k II H 2 O 2 should be accurate to a factor of two between 40 and 70 wt %.
Uptake of SO 2 in the presence of solvated O 3 was measured for 1–70 wt. % acid; the Henry’s law expression for O 3 was determined in separate experiments. Meas ured second order rates agree reasonably well with previous results measured below 18 wt. %. A three term fit for reaction with SO 2 (aq), HSO 3 – , and SO 4 = was fit to the data: k ii O 3 = 6.6 × 10 3 [SO 2 (aq)] + 3.2 × 10 5 [HSO 3 – ] + 1 × 10 9 [SO 4 = ]. This expression should be accurate to a factor of two between 20 and 70 wt. %.

The HONO reaction was studied by adding nitrosyl sulfuric acid to 20, 40, 60, and 70 wt. % acid. Measured second order rate constants were m oderately consistent with previous measurements below 10 wt. %. A k ii HONO = 142[H + ] was fit to the full data set; it should be accurate to a factor of two for acid concentrations between 10 and 70 wt. %.

No enhanced SO 2 uptake was observed with added gas phase NO, NO 2 , or with 20 wt. % HNO 3 added to 50–60 wt. % sulfuric acid.

68. SO 3 on H 2 SO 4 • nH 2 O(l). Jayne et al. [199] measured the uptake coefficient in a wetted wall-flow reactor at 300 K over a composition range of 78–92 H 2 SO 4 wt. %. The measured γ was indistinguishable from 1.0. Higher water concentrations and lower temperatures probably tend to increase γ, so a value near 1.0 probably holds for all atmospheric conditions.5-32 

### 5.14 Soot Surface Uptake Coefficients

Table 5-3. Soot Surface Uptake Coefficients.

Gaseous Species Uptake Coefficient ( γ ) Notes SO 2 See Note 1, 2 NH 3 0, See Note 1, 3 O 3 See Note 1, 4 HNO 3 See Note 1, 5 N 2 O 5 See Note 1, 6 NO 2 See Note 1, 7 NO 3 See Note 1, 8 HO 2 See Note 1, 9 HO 2 NO 2 See Note 1, 10 H 2 O See Note 1, 11



### 5.15 Notes to Table 5-3

1. See also the sections on soot under “Surface Types” and “Parameter Defin itions” for a description of some of the factors affecting the uptake and reaction of gases on soot surfaces. In most cases, the available reactive surface area rather than the geometri c areas have been used in obtaini ng the uptake coefficients; in those cases where the geometric area was used but a higher available surface area was involved in the measured uptake, the uptake coefficient is given as an upper limit. Most data are available at room temperature or there are very limited data at lower temperatures characteristic of the upper troposphere.

2. SO 2 + soot. γ < 3 × 10 –3 measured using Degussa FW2 carbon black by Rogaski et al. [295]. This is an upper limit since it is based on the geometric surface area. Ko ehler et al. [226] measur ed an average value of (2 ± 1) × 10 –3 over the first 10–30 s on n-hexane soot at –100 ° C (the initial uptake may be larger), but indicate that taking into account surface roughness would reduce this value. A number of studies [25,77,78,90,226,238,295] suggest that uptake is primarily due to physi sorption on the surface; oxidation occurs in the presence of water, oxidants and metals.

3. NH 3 + soot. Chughtai et al. [77] and Muenter and Koehler [267] measured the uptake of NH 3 on soot. Based on Muenter and Koehler [267] where cond itions are closest to atmospheric, NH 3 is not taken up by soot particles at temperatures above 173 K.

4. O 3 + soot. Many studies report a rapid, initial loss of O 3 followed by a slower loss that also occurs on aged soot or soot pre-exposed to ozone [81, 87,104,115,117,187,210,244,295,316,319,323]. Initial, rapid O 3 loss may be most applicable for soot as it comes out of aircraft exhaust, with γ init ~ 10 –3 from most studies using both carbon black and organic combus tion soots [115,117,187,295,323]. The s econd stage of the reaction is probably more applicable to soot dispersed in air; γ aged ~ 10 –4 –10 –6 using both carbon black and organic combustion soots [115,117,187,210,244,278,323], but in the range of 10 –4 to 10 –5 based on organic combustion soot data alone [187,244]. A few studies ha ve been carried out at temperatures below room temperature [81,187,210,244]; given the wide ranges measured even at room temperature, these values generally fall in the same range. Il ’in et al. [187] report a temperatur e dependence for the initial uptake on fresh soot of γ fresh = 1.9 × 10 –3 (exp–780/T) and for aged soots, γ aged = 1.8 × 10 –4 (exp–1000/T). Both physisorption and reaction of ozone with the surface appear to take pl ace. The studies of Fendel et al. [115] suggest that lower particle growth in size below 40 ppb O 3 is due to less than a monolayer of O 3 on the surface. Stephens et al. [ 323] proposed a Langmuir-type re versible adsorption of O 3 , followed by a slower reaction with the surface. Pöschl et al. [278] proposed a similar sc heme for uptake of ozone on sparkgenerated graphite soot coated with benzo[ a ]pyrene. Initial reversible physisorption occurred with γ ~ 10 –3

, and “apparent reaction probabilities” for O 3 with BaP on soot of γ ~ 10 –5 –10 –6 were reported. The presence of water inhibited the reaction, which was postulated to be due to competitive adsorption between water and ozone on the surface; this is in contrast to the report of Chughtai et al. [82] in wh ich the rate of ozone loss increased with RH. Pöschl et al. [278] report Langmuir adsorption equilib rium constants for O 3 and H 2 O, and a second order surface reaction rate constant for the O 3 -BaP reaction of (2.6 ± 0.8) × 10 –17 cm –2 s –1 . Three possible paths have been proposed: (1) chemisorption of O 3 ; (2) catalytic decomposition of O 3 : 2O 3 → 3O 2 ; (3) surface oxidation and formation of gas-phase carbon oxides. The studies of Fendel et al. [116] suggest that lower particle growth in size below 40 ppb O 3 is due to less than a monolayer of O 3 . Studies of Smith et5-33 al. [319] and Smith and Chught ai [316] suggest that catal ytic decomposition occurs to some extent over the entire reaction sequence. CO 2 and H 2 O are the major gas phase and surf ace oxidized functional groups on the surface such as carboxylic acids ar e observed [82-84,104,115,210,252,316-318,323].

5. HNO 3 + soot. Studies of the uptake of HNO 3 on soot have been carried out over a range of nitric acid pressures [70,92,103,220,244,295,297,304,305]. Measured values of γ at room temperature are typically in the range 10 –1 –10 –5 , with smaller uptake coefficients measured at longer reaction times. S aatthoff et al. [304] report an upper limit of 3 × 10 –7 as a time-averaged value over two days. At lower concentrations characteristic of the atmosphere, uptake appears to be primarily due to physisorption while at higher concentrations, > 2 × 10 12 molecule cm –3 , a surface reaction occurs. At 220 K, γ ~ 0.1 with irreversible uptake attributed to reaction with surface groups [70]. Reaction of HNO 3 at concentrations from (1–9) × 10 12 molecule cm –3 with “grey” soot from a rich flame using he xane has been reported [305] to generate HONO as the major gaseous product with initial and steady-state reaction probabilities of γ o = 4.6 × 10 –3 and

γ ss = 5.2 × 10 –4 respectively; reaction with “black” soot fro m a lean flame gave NO as the major gaseous product, with initial and steady- state reaction probabilities of γ o = 2.0 × 10 –2 and γ ss = 4.6 × 10 –3 respectively (based on geometric surface area of sample holder). The NO was hypothesized to result from secondary reactions of an initial HONO product.

6. N 2 O 5 + soot. Brouwer et al. [58], Longfellow et al. [244] and Saathoff et al. [304]studied the uptake of N 2 O 5 at room temperature on a ground charcoal (carbon black) sample, on propane soot and on spark-generated graphite soot, respectively. Brouwer et al. and Longf ellow et al. report uptake coefficients based on the geometric sample surface area, and therefore give upper limits. An upper limit of γ < 0.02 can be derived based on the larger value of 0.016 reported by Longfellow et al. As discussed below, much smaller values are reported by Saathoff et al.: 4 × 10 –5 under dry conditions and 2 × 10 –4 at 50% RH. Three possible reactions may occur: (1) Decomposition of N 2 O 5 on the surface to generate NO 2 + NO 3 ; (2) reaction of N 2 O 5 with the soot; (3) hydrolysis of N 2 O 5 with water on the surface to generate HNO 3 . The studies of Longfellow et al. support the decomposition reaction, with yields of NO 2 within experimental error of 100%; the generation of NO 3 on the surface followed by its decomposition to NO 2 , may contribute to the observed production of NO 2 . The studies of Brouwer et al. suggest that a redox reaction with the soot surface to generate NO occurs in parallel with hydrolysis of N 2 O 5 to generate HNO 3 . Saathoff et al. propose two independent, parallel reactions: (1) hydrolysis generating HNO 3 , N 2 O 5 + soot → 2 HNO 3 with γ = (4 ± 2) × 10 –5 under dry conditions (< 10 ppm H 2 O) which increases to (2 ± 1) × 10 –4 at 50% RH. (2) decomposition to NO and NO 2 : N 2 O 5 + soot → NO + NO 2 + products, with γ = (4 ± 2) × 10 –6 under dry conditions.

7. NO 2 + soot. A fast initial uptake of NO 2 is observed on fresh soots [13,14,21,77,80,85,86,134,205,220,243,295,321,325,326] with the initial uptake coefficient in studies involving both carbon blacks and organic combustion soots in the range of γ init ≅ 10 –1 to 10 –4 . For longer reaction times on carbon black soots, γ aged ~ 10 –4 based on studies by Kalberer et al. [206] and Ammann et al. [21,22]. However, Kleffmann et al. [223] report a lower uptake coefficient of ~ 10 –7 on carbon black over the first 5 minutes of reaction and and Saathoff et al. [304] report an upper limit of < 4 × 10 –8 averaged over 5 days under dry conditions (< 10 ppm H 2 O) on spark-generated graphite. On organic combustion soots, γ aged has been reported to be in the range of ~ 10 –4 –10 –6 [13,22,23,243,321][305]. All studies were done at room temperature except those of Longfello w et al. [243] which we re carried out at 262 K. The surface deactivates on continued exposure to NO 2 , suggesting a maximum amount of HONO that can be formed per cm 2 of soot area or mg of soot; this has been reported to be in the range of 10 16 to 10 18 HONO per mg of soot [23,134,204,205,223,321]. However, reactiv ation on heating of the surface, exposure to water vapor and/or with time after the exposure is stopped has been observed [134,243,321,325,326]. A small portion (~10- 20%) of the NO 2 taken up appears to be chemisorbed to the surface [13,23,80,204,205,220,223,321,325,326]. In frared studies [13,220,318] s how that surface C–ONO, C–N– NO 2 , and C–NO 2 groups are formed. The remainder of NO 2 reacted appears as gaseous HONO and NO; Salgado and Rossi [305] report HONO as the major product for hexane soot from a flame at near stoichiometric ratio but NO as the major product for s oot from an extremely lean flame. In addition, N 2 O, CO, and CO 2 have been observed as products at higher temperatures [34,35]. At lower NO 2 concentrations, the HONO yield can approach 100%; production of NO ma y be due to the bimolecular reaction of HONO on the surface at higher concentrations to give NO + NO 2 + H 2 O. The HONO yield at 262 K appears to be smaller than at room temperature [243]. Formation of HONO is due to reaction with a reduced surface site and not to NO 2 surface-catalyzed hydrolysis. The formation of HONO from the reaction of NO 2 with unspecified semi-volatile organics in5-34 diesel exhaust has been reported [ 143] and proposed to be a much larger source of HONO than the reaction with the soot itself.

8. NO 3 + soot. Saathoff et al. [304] report an upper limit of γ < 3 × 10 –4 on dry soot (< 10 ppm H 2 O) and < 10 –3 at 50% RH based on measurements of NO 3 and N 2 O 5 . 9. HO 2 + soot. Saathoff et al. [304] report an upper limit of γ < 10 –2 on dry soot (<10 ppm H 2 O) based on the decay of HO 2 NO 2 (in equilibrium with HO 2 and NO 2 ) in the presence and absence of soot.

10. HO 2 NO 2 + soot. Saathoff et al. [304] report an upper limit of γ < 10 –5 on dry soot (<10 ppm H 2 O) based on the decay of HO 2 NO 2 in the presence and absence of soot.

11. H 2 O + soot. Alcala–Jornod et al. [14] report an upper limit to th e initial uptake coefficient of γ < 2 × 10 –3

, consistent with the earlier measurements of Rogaski et al. [295]. The uptake is most likely a reversible physisorption [14,277] although based on water uptake isotherms, Chughtai et al. [77,79,84,87] propose that at low relative humidities (< 25%) chemisorption occu rs. While prior exposure of Degussa FW-2 to NO 2 and SO 2 was not found to increase the uptake coefficient for water, treatment with HNO 3 increased the measured uptake coefficient by a factor of 28 and with H 2 SO 4 by a factor of 68 [295]. Water adsorption isotherms on soot have been measured in a number of studies, e.g. [77,79,82,84,87] and the amount of water taken up found to increase with the air/fuel ratio used to generate the soot, with the sulfur content, with aging and oxidation of the surface (e.g. by O 3 ) and with the presence of metals [77,79,82,84,87,350].5-35 

### 5.16 Henry’s Law Constants for Pure Water

Table 5-4. Henry’s Law Co nstants for Pure Water.

Substance Temperature Range, K H (298 K) a A B C Uncertainty Range b Note

O 2 273–348 1.27×10 –3 –161.6 8160 22.39 A 1 O 3 273–333 1.03×10 –2 –14.08 2830 C 2 HO 2 298 1000 D 3 H 2 O 2 278–303 7.73×10 4 –13.27 7310 C 4 N 2 273–348 6.52×10 –4 –177.1 8640 24.71 A 5 NH 3 273–348 60.2 –9.84 4160 C 6 NO 273–358 1.92×10 –3 –157.1 7950 21.298 B 7 NO 2 298 1×10 –2 E 8 N 2 O 273–313 2.42×10 –2 –148.1 8610 20.266 A 9 CO 278–323 9.81×10 –4 –178.0 8750 24.875 A 10 CO 2 273–353 3.38×10 –2 –145.1 8350 19.960 A 11 CH 4 273–328 1.41×10 –3 –194.7 9750 27.274 A 12 C 2 H 6 273–323 1.88×10 –3 –240.2 12420 33.744 A 13 C 3 H 8 273–348 1.51×10 –3 –281.1 14510 39.652 A 14 n–C 4 H 10 273–348 1.24×10 –3 –269.9 14330 37.734 A 15 CH 3 CH(CH 3 )CH 3 278–318 9.18×10 –4 –360.6 18020 51.444 B 16 C 2 H 4 288–348 5.96×10 –3 –154.6 8540 21.202 B 17 C 2 H 2 273–343 4.14×10 –2 –145.8 7880 20.384 B 18 CH 3 OH 273–298 220 –12.08 5210 C 19 CH 3 CH 2 OH 273–298 200 –16.98 6630 C 20 n–C 3 H 5 OH 273–298 130 –20.16 7470 D 21 iso–C 3 H 5 OH 273–298 130 –20.15 7450 D 21 n–C 4 H 9 OH 273–298 127 –19.34 7210 D 21 iso–C 4 H 9 OH 298 102 D 21 sec–C 4 H 9 OH 273–298 110 –19.65 7260 D 21 tert–C 4 H 9 OH 273–298 70 –23.63 8310 D 21 CH 3 OOH 277–293 300 –11.99 5280 D 22 HOCH 2 OOH 278–293 1.7×10 6 –18.79 9870 E 23 HCHO 288–318 3.23×10 3 –15.73 7100 D H * 24 CH 3 CHO 273–313 12.9 –17.19 5890 D H * 25 C 2 H 5 CHO 273–313 10.0 –12.20 4330 E 26 C 3 H 7 CHO 283–318 9.6 –18.59 6220 E 27 CH 3 COCH 3 273–311 28.1 –13.62 5050 D 28 C 2 H 5 COCH 3 273–298 18 –16.40 5740 D 29 HC(O)OH 275–308 8.9×10 3 –11.40 6100 D 30 CH 3 C(O)OH 275–308 4.1×10 3 –12.50 6200 D 31 CH 3 CN 273–303 52.8 –9.35 3970 C 32 CH 3 NO 2 293–323 34.6 –9.92 4010 D 33 C 2 H 5 NO 2 293–323 21.7 –11.80 4430 D 33 C 3 H 7 NO 2 293–323 13.1 –13.22 4710 D 33 CH 3 CH(NO 2 )CH 3 293–323 8.42 –13.02 4520 D 33 CH 3 ONO 2 273–298 2.0 –15.20 4740 D 34 C 2 H 5 ONO 2 273–298 1.59 –17.50 5360 D 34 1–C 3 H 7 ONO 2 273–298 1.10 –18.31 5490 D 34 2–C 3 H 7 ONO 2 273–298 0.791 –18.20 5360 D 34 1–C 4 H 9 ONO 2 273–298 1.01 –19.40 5790 D 34 2–C 4 H 9 ONO 2 273–298 0.648 –18.59 5410 D 34 CH 3 C(O)O 2 NO 2 274–297 2.8 –18.15 5730 D 35 O 2 NOC 2 H 4 ONO 2 293 640 D 36 HOC 2 H 4 ONO 2 293 3.99×10 4 D 36 HOCH 2 CH(ONO 2 )CH 3 293 7.3×10 3 D 36 CH 3 CH(OH)CH 2 ONO 2 293 6.7×10 3 D 36 CH 3 CH(ONO 2 )CH 2 ONO 2 293 175 D 36 CH 3 C(O)CH 2 ONO 2 293 1.01×10 3 D 36 Cl 2 283–383 9.29×10 –2 –134.4 7590 18.702 B 37 Cl 2 O 273–293 17 –3.23 1810 D 385-36 Substance Temperature Range, K H (298 K) a A B C Uncertainty Range b Note

ClO 2 383–333 1.01 –11.65 3470 B 39 HOCl 660 –13.2 5880 D 40 Br 2 273–308 0.725 –15.05 4390 B 41 BrCl 279–299 0.98 –18.9 5630 C 42 278–383 1.36 –39.72 4250 4.525 SO 2 278–298 –9.53 2930 B 43

H 2 S 273–323 0.102 –145.2 8120 20.296 C 44 CS 2 274–305 0.062 –17.05 4250 D 45 COS 273–288 2.02×10 –2 –15.68 3510 D 46 CH 3 SH 298–368 0.39 –12.42 3420 E 47 C 2 H 5 SH 298–368 0.28 –13.82 3740 E 48 CH 3 SCH 3 272–305 0.54 –12.19 3460 E 49 CH 3 S(O)CH 3 298 9.9×10 4 E 50

a. ln H = A + B/T +C ln(T) [M atm –1 ]

b. Uncertainty Classes: A—Better than 10% B—10% to 50% C—50% to 100% D—Factor of 2 to factor of 10 E—Factor of 10 to factor of 100 F—Greater than a factor of 100



### 5.17 Notes to Table 5-4

Many of the data sets required various transformations to convert them to the units (mol L –1 atm –1 ) and form (solubility instead of volatility) used in this Table. The transformations often involve either the mass or molar density of water, which in all cases was taken from [231].

1. O 2 . The recommendation was taken from the studies of Be nson [51] and Rettich [285] . The data show clear curvature in a plot of ln (K h ) v. 1/T. A two parameter fit gives A = –13.26 and B = 1950 K for the temperature range 273–285 K.

2. O 3 . The recommendation of Rischbieter [288] was accepted and refitted.

3. HO 2 . The recommendation was based on a calculation by Schwartz [307]. Thermodynamic values were updated to those in our Thermodynamic tables.

4. H 2 O 2 . The data of Lind and Kok [239,240], Hwang and Dasgupta [186], Yoshizumi et al. [361], and O’Sullivan et al. [273] are all in good agreement. The recommendation is fro m a two-parameter fit to all the results.

5. N 2 . The recommendation of Battino [34] was accepted a nd refitted to three-parameter equations. A two parameter fit gives A = 12.81 and B = 1625 K for the temperature range 273–293 K.

6. NH 3 . Based on the recommendation by Edwards et al. [111], refit to a two-parameter equation. Over the temperature range 273–348 K, there appears to be little curvature in the data. Th e more recent work of Dasgupta and Dong [96] are in quite good agreement with this recommendation, whereas the results of Hales and Drewes [144] are somewhat higher and those of Shi and Davidovits [312] (an uptake study) are significantly lower. The Hales and Drewes paper also included studies of the effect of dissolved CO 2 on the solubility of NH 3 . The solubility of NH 3 in solutions containing a wide variety of ions is discussed by Clegg and Brimblecombe [89].
7. NO. Three-parameter refit from the recommendation of Battino [32]. Two-parameter fit gives A = –12.27 and B = 1790 K for the temperature range 273–293 K.

8. NO 2 . From analysis of studies of reactive dissolution of NO 2 by Schwartz and White [309].

9. N 2 O. Three-parameter refit to the recommendation of Battino [31]. Two parameter fit gives A = 13.40 and B = 2880 K for the temperature range 273–293 K.5-37 10. CO. The recommendation is based on smoothed data fro m Rettich et al. [284] and refit to three-parameter equation. A two parameter fit gives A = –12.72 and B = 1720 K for the temperature range 273–293 K.

11. CO 2 . Refit to three- parameter equation from the recommendation of Wilhelm et al. [352]. Two parameter fit gives A = 12.49 and B = 2710 K for the temperature range 273–293 K.

12. CH 4 . The recommendation is a three-parameter fit to the smoothed recommendation of Battino [41]. There is very good agreement with the more recent data of Be n-Naim and Battino [50]. A two parameter fit gives A = –13.45 and B = 2040 K for the temperature range 273–293 K.

13. C 2 H 6 . The recommendation is a three-parameter fit to the smoothed recommendation of Battino [33]. There is very good agreement with the more recent data of Ben-Naim and Battino [50]. Two parameter fit gives A = –15.95 and B = 2875 K for the temperature range 273–293 K.

14. C 3 H 8 . The recommendation is from a three-parameter fit to the smoothed recommendation of [40]. There is very good agreement with the more recent data of Be n-Naim and Battino [50]. A two parameter fit gives A = 17.52 and B = 3275 K for the temperature range 273–293 K.

15. n-C 4 H 10 . The recommendation is from a three-parameter fit to the smoothed recommendation of Battino [39]. There is very good agreement with th e more recent data of Ben-Naim and Battino [50]. A two parameter fit gives A = –19.28 and B = 3740 K for the temperature range 273–288 K.

16. CH 3 CH(CH 3 )CH 3 . The recommendation is from a three-parameter fit to the smoothed recommendation of Battino [38]. A two parameter fit gives A = 18.22 and B = 3340 K for the temperature range 278–293 K.

17. C 2 H 4 . The recommendation is from a three-parameter fit to the smoothed recommendation of Wilhelm [352]. A two parameter fit gives A = –12.40 and B = 2170 K for the temperature range 288–313 K.

18. C 2 H 2 . The recommendation is from a three-parameter fit to the smoothed recommendation of Wilhelm [352]. The recommendation of Yaws et al. [360] generates id entical results. A two parameter fit gives A = –10.12 and B = 2065 K for the temperature range 273–298 K.

19. CH 3 OH. The recommendation is based on the two data points of Snider and Dawson [320]. The 298 K result of Butler et al. [62] and a calculation based on the NBS Thermodynamic tables, [345], are in very good agreement. The 298 K result of Altschuh et al. [20] is about 40% lower.

20. C 2 H 5 OH. The recommendation is based on the two data points of Snider and Dawson [320]. The 298 K results of [62] and [296], and a calculation based on the NBS Thermodynamic tables, [345], are in very good agreement. The 298 K result of Altschuh [20] is about 50% lower.

21. All of the recommendations for the C3–C4 alcohol s are based on two data points each from Snider and Dawson [320]. Room temperature data from other studies ([61],[62], and [20]) typically support these results.

22. CH 3 OOH. The data of Lind and Kok [239,240] and O’Sullivan et al. [273] are in excellent agreement and were fit to a two-parameter expression.

23. HOCH 2 OOH. The results of O’Sullivan [273] and Staffelback and Kok [322] are very close and were fit to obtain the recommended values. The results of Zhou and Lee [371] are much lower and were not included.
24. HCHO. The recommended value is the apparent Henr y’s law constant and includes a contribution due to hydrolysis H *= H(1 + K hyd

). Data from Betterton and Hoffmann [54] and Zhou and Mopper [372] are in substantial agreement and were fit to a two-parame ter expression. Betterton and Hoffmann have calculated K

H

= 2.5 M atm –1 at 298 K for the physical solubility.

25. CH 3 CHO. The recommended value is the apparent Henry’ s law constant and includes a contribution due to hydrolysis H *= H(1 + K hyd

). The results of Snider and Dawson [320], Benkelberg et al. [49], and Betterton and Hoffmann [54] are in excellent agreement and have been fit to a two-parameter expression for the recommendation. The results of Zhou and Mopper [372] curve off at higher temperatures and were not included in the fit. (Note the similar situation for acetone.) Betterton and Hoffmann have calculated K

H

= 4.8 M atm –1 at 298 K for the physical solubility.

26. C 2 H 5 CHO. Results of Zhou and Mopper [372] and Snider and Dawson [320] agree only to within about a factor of two. The two points from the former were weighted by 3 and combined with the five points of the latter to generate the recommendation.

27. C 3 H 7 CHO. The only results are from Zhou and Mopper [372], which have been fit to a two-parameter expression.5-38 28. CH 3 COCH 3 . The recommendation is from a fit to the data of Snider and Dawson [320] and Benkelberg et al. [49]. Room temperature data points of Hoff et al. [176], Burnett [61] and Vitenberg et al. [340] are in very good agreement. Results of Zhou and Mopper [372] are somewhat higher, particularly at room temperature and above. The situation is similar for acetaldehyde.

29. C 2 H 5 COCH 3 . The recommendation is from the two points of Snider and Dawson [320]. The room temperature points of Vitenberg et al. [340] and Rohrschneider [296] are in good agreement. The higher temperature data of Zhou and Mopper [372] are somewhat higher and the those of Friant and Suffet [128] are lower than the recommendation.
30. HC(O)OH. The results of Johnson et al. [203] are accep ted. The 298 K result of Khan et al. [219] are about 75% lower. Bob, did you consider the results of Servant et al. (quoted in 97-4)?

31. CH 3 C(O)OH. The results of Johnson et al. [203] are accepted. A value calculated from the NBS Thermodynamic tables [345] is about a factor of two higher. Bob, did you consider the results of Servant et al. (quoted in 97-4)?

32. CH 3 CN. The values reported by Benkelberg [49], Snider and Dawson [320], Hamm et al. [146] are all in good agreement and have been fit to a two-parameter expression for the recommendation. The Hamm et al. paper includes a measurement with artificial seawater at 293 K.
33. Nitroalkanes (CH 3 NO 2 , C 2 H 5 NO 2 , C 3 H 7 NO 2 , and CH 3 CH(NO 2 )CH 3 ). The recommended values are all taken from the work of Benes and Dohnal [47]. For nitromethane, the 298 K value from Rohrschneider [296] is about 30% higher.
34. Alkyl nitrates (CH 3 ONO 2 , C 2 H 5 ONO 2 , 1-C 3 H 7 ONO 2 , 2-C 3 H 7 ONO 2 , 1-C 4 H 9 ONO 2 , 2-C 4 H 9 ONO 2 ). The recommended values are all taken from the work of Ka mes and Schurath [208]. The results of Luke et al. [247] are in very good agreement for 1-butyl and 2- butyl nitrates, but the values reported by Hauff [170] for 1- and 2-propyl and butyl n itrates by head-space chroma tography are significantly (

∼ 50%) lower.

35. CH 3 C(O)O 2 NO 2 . The results of Kames and Schurath [208] and Frenzel et al. [127] are close, but somewhat higher (~60%) than the single temperature point of Holdren et al. [178]. The recommendation is a fit to the data of Kames and Schurath, and Fren zel et al. Frenzel et al., Kames and Schurath, and Holdren et al. also measured hydrolysis rate constants and Kames and Schurath measured solubility in artificial sea water.
36. Bifunctional alkyl nitrates. The recommended values (at 293 K) are taken from the work of Kames and Schurath [207].

37. Cl 2 . Three-parameter refit to the recommendation of Battino [36]. Two parameter fit gives A = 9.38 and B = 2090 K for the temperature range 283–313 K.

38. Cl 2 O. Fit to recommendation of Wilhelm et al. [351]. Data appear somewhat uncertain.

39. ClO 2 . Two-parameter fit to the recommendation of Battino [35].
40. HOCl. Huthwelker et al. [185] analyzed the limited data for pure water from Blatchley et al. [55] and Holzwarth et al. [179] along with the more extensive data for uptake by sulfuric acid from Hanson and Ravishankara [164], along with thermodynamic informa tion, and obtained a consistent expression for the solubility of HOCl.

41. Br 2 . The results of Kelley and Tartar [213] and Jenki ns and King [202] agree well below about 313 K, and with the 298 K point of Hill et al. [175]. Recommendation based on a two-pa rameter fit to all data at and below 308 K.
42. BrCl. The recommendation is from the work of Barlett and Margerum [29].

43. SO 2 . Two- and three-parameter fits to the recommendation of Battino [37]. The earlier recommendation of Edwards et al. [111] is slightly lower.

44. H 2 S. In the recommendation of Fogg [125], two expressions were given, representing the results above and below 283 K. The predicted values from these expressions were calculated, with the points at 283 K averaged, converted to the desired units, and then fit with the two- and three-parameter expressions. These are the recommended values. More r ecent results of Rinker and Sandall [ 287] and Munder et al. [268] are slightly lower; in these studies, the physical solubility of H 2 S was determined through measurements involving aqueous solutions of glycols or amines, neutra lized with HCl. The reported values of De Bruyn et al. [101] are significantly (~30%) lower. The earlier recommendation of Edwards et al. [111] is very close to5-39 the recommendation of Fogg [125] as is the recommendation of Yaws et al. [360]. The room temperature point calculated from the NBS Thermodynamic tables Wagman et al. [345] is also slightly lower. The work of De Bruyn et al. [101] covered also a wide range of NaCl and (NH 4 ) 2 SO 4 concentration and of pH.

45. CS 2 . The recommendation is from a fit to data of E lliott [112], who also present data in 0.5 mol L –1 NaCl. The results of De Bruyn et al. [101] are significantly (50%) lower. The work of DeBruyn et al. covered also a wide range of NaCl and (NH 4 ) 2 SO 4 concentration and of pH.
46. COS. The reviews by Wilhelm et al. [352] and Yaws et al. [360] result in identical results over the low temperature range (<303 K) and are combined to genera te the recommendation. The results of De Bruyn et al. [101] are somewhat (~25%) lower at the lower temperature range. The work of De Bruyn et al. covered also a wide range of NaCl and (NH 4 ) 2 SO 4 concentration and of pH.

47. CH 3 SH. The recommendation is based on the data of Przyjazny et al. [279]. Results of De Bruyn et al. [101] are about half the recommended value at 298 K. Simila r low values were observed for other compounds in the work of De Bruyn et al. The work of De Bruy n et al. covered a wide range of pH and NaCl and (NH 4 ) 2 SO 4 concentrations.

48. C 2 H 5 SH. The recommendation is based on the data of Przyjazny et al. [279]. The results of Vitenberg [340] are slightly lower than the extrapolated value at 293 K.

49. CH 3 SCH 3 . The recommendation is based on the values of Dacey et al. [93]. The singl e temperature point of Wong and Wang [357] and the higher temperature results of Przyjazny et al. [279] are in good agreement. The results of De Bruyn et al. [101] are about 30% lower. The studies of Dacey et al. [93] and Wong and Wang [357] were also carried out with seawater. The work of De Bruyn et al. [101] covered also a wide range of NaCl and (NH 4 ) 2 SO 4 concentration and of pH.

50. CH 3 S(O)CH 3 . The recommendation is from Watts and Brimblecombe [349], cited by Allen et al. [19].5-40 

### 5.18 Henry’s Law Constants for Acids

Table 5-5. Henry’s Law Constants for Acids T(K) Wt. % H 2 SO 4 H or H* (M/atm) Notes O 3 in H 2 SO 4 • nH 2 O(l) 293 1–70 Ln(H o /H) = (4.08 ± 0.2) × 10 –3 × wt H o = 0.012 M atm –1 wt is the H 2 SO 4 wt. % 1

NO 2 in H 2 SO 4• nH 2 O(l) 203–343 39–68 See Note 2 HONO in H 2 SO 4 • nH 2 O(l) 248–298 >60 ln H*= a 1 + a 2 wt + a 3 wt 2 + (b 1 + b 2 wt)/T

a 1 = 26.1 ± 9.4, a 2 = –1.095 ± 0.21, a 3 = 0.00732 ± 0.00121 b 1 = –5792 ± 1610, b 2 = 181.3 ± 24 3

HNO 3 in H 2 SO 4 • nH 2 O(l)

∼ 195–300 0–80 See Note 4 HNO 3 and HCl in H 2 SO 4 • nHNO 3 • mH 2 O(l) ∼ 195–300 0–80 See Note 4

HO 2 NO 2 in H 2 SO 4 • nH 2 O(l) 201–230 50–75 ln H = 3.69–mH 2 SO 4 × (–0.25 + 65/T) – 8400 × (1/T o– 1/T) mH 2 SO 4 is the molality of the H 2 SO 4 solution, T o = 298.15 K 5

CH 2 O in H 2 SO 4 • mHNO 3 • nH 2 O(l) 240–300 10–85 also 8–40 wt. % HNO 3 See Note 6

CH 3 OH in H 2 SO 4 • nH 2 O(l) 197–223 See Note 7 CH 3 C(O)CH 3 in H 2 SO 4 • nH 2 O(l) 198–298 10–80 ln H* = a 1 +a 2 wt+a 3 wt 2 + (b 1 +b 2 wt+b 3 wt 2 )/T wt is the H 2 SO 4 wt. %,

a 1 = –21.438 ± 4.31, a 2 = –0.32163 ± 0.207, a 3 = 0.0072935 ± 0.00235 b 1 = 7292 ± 1220, b 2 = 33.524 ± 53.42, b 3 = –0.975 ± 0.571 8

CH 3 C(O)O 2 NO 2 in H 2 O(l), H 2 SO 4• nH 2 O(l) 199–295 0–75 ln H * = 1.07–mH 2 SO 4 × (0.69 – 152/T) – 5810 × (1/T o –1/T), mH 2 SO 4 = molality of the H 2 SO 4 solution T o = 298.15 K 9

CF 2 O in H 2 SO 4 • nH 2 O(l) 215–230 60 < 5 10 CF 3 OH in H 2 SO 4 • nH 2 O(l) 250 40 50 > 240 210 11

HOCl in H 2 SO 4 • nH 2 O(l) 200–300 46–80 H HOCl = 1.91×10 –6 × exp(5862.4/T) × exp(–S HOCl M H2SO4 ) M atm –1 where: S HOCl = 0.0776+59.18/T M –1 , M H2SO4 = H 2 SO 4 molar conc 12

ClONO 2 in H 2 SO 4 • nH 2 O(l) 200–265 40–75 H ClONO2 = 1.6 ×10 –6 × exp(4710/T) × exp(–S HOCl M H2SO4 ) M atm –1 where: S ClONO2 = 0.306 + 24.0/T M –1 , M H2SO4 = H 2 SO 4 molar conc. 13

HBr in H 2 SO 4 • nH 2 O • H 2 O(l) and H 2 SO 4 • nHNO 3 • mH 2 O(l) 200–240 40–72 ln H* = a 1 + (b 1 +b 2 wt)/T

a 1 = –11.695 ± 0.537, b 1 = 11,101 ± 163, b 2 = –90.7 ± 1.2 14

SO 2 in H 2 O (l), H 2 SO 4 • nH 2 O(l) 193–242 0–97 ln H* = a 1 +a 2 wt+a 3 wt 2 + (b 1 +b 2 wt+b 3 wt 2 )/T, where: wt is the H 2 SO 4 wt. %,

a 1 = –10.778 ± 2.07, a 2 = –0.11541 ± 0.0827, a 3 = 0.0012506 ± 0.000811 b 1 = 3310 ± 578, b 2 = 30.581 ± 22.2, b 3 = –0.35469 ± 0.209 15



### 5.19 Notes to Table 5-5

1. O 3 in H 2 SO 4 • nH 2 O(l)—Bubble train uptake measurements where pe rformed by Rattigan et al. [282] at 293 K for 1–70 wt. % H 2 SO 4 . Recommended expression is a Setchenow coefficient formulation where H o = 0.012 M atm –1 is the 293 K value of H for pure water fom Wilhelm et al. [351]. In the measurement, account was taken of the loss of O 3 due to reaction with H +

. 2. NO 2 in H 2 SO 4 • nH 2 O(l)—Langenberg et al. [229] present novel capillary gas chromatography measurements for 39, 59, and 68 wt. % H 2 SO 4 over the temperature range of 203 to 243 K. However, NO 2 solubility must be derived from chromatographic waveforms which are contorted by much higher N 2 O 4 solubility. The resulting values for H NO2 are in the 1 to 10 2 range, but show inconsistent trends with temperature and concentration, indicating possibly large systematic error.

3. HONO in H 2 SO 4• nH 2 O(l)

— Becker et al. [42] measured HONO partial pressue, P HONO , over bulk solutions in a temperature range of 248–298 K and a H 2 SO 4 concentration range of 0–67 wt. %. Longfellow et al. [242] measured P HONO in a wetted wall flow reactor over a temperature range of 218–295 K and an acid concentration range of 60–83 wt. %. Agreement between these two data sets is excellent. H* decreases from5-41 0 wt. % to 53 wt. % due to physical solubility, then increases above 53 wt. % due to pr otonation and/or association with H 2 SO 4 to make nitrosyl sulfuric acid. Becker et al. parameterize their data as a function of sulfuric acid wt. % and temperature. However, the Beck er et al. parameterization is not able to fit the combined sets of Becker et al. [42] and Longfellow et al. [242] data, particularly at the lower temperatures and higher wt. % most relevant to the stratosphere. Th erefore, the recommended functional form was used to fit the data for >60 wt. %. This function fits both sets of data very well It is important to note that this function is only valid for H 2 SO 4 concentrations near 60 wt% and above. The parameterization in Becker et al. [42] should be used to calculate H for H 2 SO 4 concentrations <60 wt %. (Not e that the units for H are mol/kgbar in Becker et al. [42]. The density parameterization of Myhre et al. [269] was used to convert to M/atm units.)

4. HNO 3 and HCl in H 2 SO 4 • nH 2 O(l) and H 2 SO 4 • nHNO 3 • mH 2 O(l)—Effective Henry’'s law coefficients, H *

, for HNO 3 , and HCl in binary H 2 SO 4 /H 2 O and ternary H 2 SO 4 /HNO 3 /H 2 O solutions over the temperature range 195 to 300 K are required to model the composition and heterogeneous chemistry of stratospheric and upper tropospheric aerosols. Solubility data can be obtained from analysis of heterogeneous upt ake experiments with the liquid phase diffusion coe fficient estimated from acid solution viscosity (Williams and Long [355]) Solubilities can also be obtained from equilibrium or from vapor pressure data.
Experimental solubility data for HNO 3 is provided by Van Doren et al. [338], Reihs et al. [283] and Zhang et al. [370]. Data for HCl solubility is provided by Watson et al. [348] , Hanson and Ravish ankara [158,161], Zhang et al. [370], Williams and Go lden [353], Abbatt [2], Elrod et al.[113] and Robins on et al. [294].

These studies all show that trace species solubility in H 2 SO 4 /H 2 O and H 2 SO 4 /HNO 3 /H 2 O solutions is a strong function of water activity, which, in turn, depends on both temperature and acid concentrations. Prediction of HNO 3 and HCl H * values for atmospheric compositions requi res a sophisticated model. Comprehensive thermodynamic models of acid solutions for a range of atmospheric conditions have been published by Carslaw et al. [66], Tabazadeh et al . [324] and Luo et al. [248] and reviewed by Carslaw and Peter [68]. These models do an excellent job of reproducing the available experimental data, even for ternary H 2 SO 4 /HNO 3 /H 2 O solutions (Elrod et al. [113]). These models and the Carslaw review should be consulted for plots/predictions of H * for HNO 3 and HCl in strong acid solutions over the atmospheric temperature range. The most widely used model of Carslaw et al. [66] was revised in Massucci et al. [251].

5. HO 2 NO 2 in H 2 SO 4 • nH 2 O(l)—Zhang et al. [369] perfo rmed wetted wall flow reactor studies using CIMS to detect HO 2 NO 2 uptake over a temperature range of 201–230 K and an acid concentration range of 52.9–74 wt. % H 2 SO 4 . HD l 1/2 values where determined for 52.9, 58.3/59.1, 66.4 and 73.8/74 wt. %, with 5 to 15 data points per temperature or temperature pair. All upt ake appeared to be reversible with the variation in H strongly temperature dependent, but only moderately dependent on H 2 SO 4 wt. %. D l values were calculated from a cubic cell model to derive H. Uncer tainties in measured H values were estimated by authors to be 25% for H <1 × 10 6 M atm –1 and 50% for H >1 × 10 6 M atm –1 . These data were parameterized by Leu and Zhang [236] in the Setchenow coefficient form adopted by Huthwelker for HOCl [185], and their formulation is recommended.

6. CH 2 O in H 2 SO 4 • mHNO 3 • nH 2 O(l)—The recommended Henry’s Law relationship is: 

# ( )

+ 2 2 HO 3 H 

### H H 1+K a K a

∗ 

### = +

where: H = 3.4 × 10 –5 exp –[(–0.0456 + 55.5/T) (0.46 m H 2 SO 4 + 0.13 m HNO 3 )] M atm –1 , T is the temperature in K, and m H 2 SO 4 and m HNO 3 are the respective acid molalities; K 2 = exp (4020/T–5.83) M –1

, K 3 = 0.56 exp [8.84–(T–260/T)] M –1 , and a H 2 O and a H+ are the water and H + activities which are obtained from a thermodynamic model of the solution, e.g. Carslaw et al. [66] Valid for 10–85 wt. % H 2 SO 4 , 8–40 wt % HNO 3 , T = 240–300 K. Knudsen cell studies by Tolbert et al . [330] and Iraci and Tolbert [192] a nd droplet train/flow reactor studies by Jayne et al. [200] all yield data showing that CH 2 O is strongly absorbed by sulfuric acid solutions, and Jayne et al. also provide data for ternary acid solutions. The Jayne et al. [200] studies included H 2 SO 4 concentrations from 10 to 85 wt. % and HNO 3 concentration between 8 and 40 wt. % with temperature variations from 241 to 300 K. These data were parame terized with three terms, representing physical CH 2 O solubility, reversible hydrolysis to CH 2 (OH) 2 , important in more dilute solutions, and reversible formation of CH 3 O + , dominant at high acidities. The Jayne et al. [ 200] parameterization is recommended above. The H* data from Iraci and Tolbert [192] cover 49 to 95 wt. % H 2 SO 4 and a temperature range of 197 to 214.5 K and are in fair agreement with extrapolation of H* expr ession from Jayne et al. [200] for concentrations below5-42 ~75 wt. %. However, the Iraci and Tolbert data are taken on such thin acid films that initial uptake slopes are difficult to determine accurately and the data scatter is large. While the Iraci and Tolbert data do indicate significantly larger H* values for H 2 SO 4 concentrations above 75 wt. %, the data do not compel a reformulation of the Jayne et al. parameterization.

7. CH 3 OH in H 2 SO 4 • nH 2 O(l)—H* data from Kane and Leu [211], taken over 40–85 wt. % H 2 SO 4 and from 210–235 K, indicate soluble uptake below 65 wt. % and predominately reactive uptake to form methanesulfonic acid and dimethysulfate above 65 wt. %. Uptake decreased slightly with temperature below 65 wt. % and increases slightly with temperature above. Data yield H*k 1/2 at high acid concentrations. Weakly temperature dependent γ s of ~0.15 were measured for 65, 75, and 80 wt. %. However, Knudsen cell studies by Iraci et al. [190] at 45, 61 and 72 wt. % over a 197–223 K temperature range show only well behaved reversible uptake. They argue that low vapor pressures explain the lack of CH 3 OH recovery for the short observation times used by Kane and Leu. They also cite three olde r literature studies on the reaction of methanol and ethanol at room temperature in sulfuric acid which report reaction rate constants much lower than those deduced by Kane and Leu [190]. Iraci et al . present the following parameterization of their data plus data for water:
log H* = A + 1000B/T
where A = 7.00 + log M H2O , B = 0.000619 m 2 + 0.00544 m + 2.267, M H2O is the molarity of water in the solution (mol L –1 ) and m is the molality of the H 2 SO 4 (moles H 2 SO 4 per kg H 2 O).
Note that this parameterization is based only on the Iraci et al. data. A reanalysis of the Kane and Leu [211] results to provide additional data in the 40–72 wt. % range, and H * values for higher wt. % should be undertaken to validate and extend the Iraci et al. data.

8. CH 3 C(O)CH 3 in H 2 SO 4 • nH 2 O(l)—Duncan et al. [109,110] used IR spectra of thin sulfuric acid films to establish that acetone is absorbed as the protonated species. Above 70 wt. % protonated acetone undergoes a self-condensation/dehydrati on reaction to form protonated mesityl oxi de, which, in turn, reacts with an additional protonated acetone to form tr imethyl benzene. Duncan et al. [ 110] measured reversible uptake and derived Henry’s law constants for 70 wt. % H 2 SO 4 at 180, 187 and 195 K and a value at 201 K for 76 wt. %. Kane et al. [212] measured uptake in a wetted wall flow reactor and deri ved H* parameters for 40, 50, 65, and 75 wt. % over a much wider temperature range than Duncan et al. [110]. Their data diverge above 80 wt. % which they attribute to reactive uptake a la Duncan et al. [109,110]. Klassen et al. [221] provide Knudsen cell uptake derived data for 48.7 to 78.3 H 2 SO 4 wt % between 210 and 240 K that are generally consistent with that of Kane et al. [212]. Im amura and Akiyoshi [188] report wetted wall flow reactor H* measurements at 230 K for 50 and 60 wt. %, 250 K for 60, 69 and 76 wt. %, and 270 K for 76 and 79 wt. %; their data diverges a factor of 2 to 4 from that of Kane et al. [212] and Klassen et al. [221].
Equally weighted data sets from Kane et al. [212] and Kl assen et al. [221] were combined and fit to generate the recommended parameterization. Two points for the solubility of acetone in water at 298 K and 273 K (Benkelberg et al. [48]) were included to improve the extrapolation to low wt. % solutions.
The data points from Imamura and Akiyos hi [188] were not incl uded because they were inconsistent with the other data and have a very different temperature dependence. The few data points from Duncan et al. [109,110] are also inconsistent with the other data and were not included in the parameterization.

9. CH 3 C(O)O 2 NO 2 in H 2 O and H 2 SO 4 • nH 2 O(l)—Zhang and Leu [364] perform ed wetted wall flow reactor studies using CIMS to detect CH 3 C(O)O 2 NO 2 uptake over a temperature range of 199 to 226 K. Uptake studies were performed at 46, 54, 59, and 72 wt. % H 2 SO 4 to yield H * D l 1/2 values. D l values were calculated from a cubic cell model to derive H*. Leu and Zha ng [236] fit their data from Zhang and Leu [364], including water data from Kames and Schurath [208] and Kames et al. [209], using the Setchenow coefficient form adopted by Huthwelker for HOCl [185]. This formulation is recommended for both water and sulfuric acid solutions.

10. CF 2 O in H 2 SO 4 • nH 2 O(l)—Hanson and Ravishankara [156] calculate an upper limit for H of CF 2 O based on assumed solubility limit resulting in lack of measurable uptake into 60 wt% H 2 SO 4 . 11. CF 3 OH in H 2 SO 4 • nH 2 O(l)—Lovejoy et al. [245] determined react o-diffusive lengths of > 0.4 μm and 1.0 μm for CF 3 OH uptake at 250 K on 40 and 50 wt % H 2 SO 4 aerosols, respectively. This leads to H * estimates of >240 and 210 M atm –1 , respectively.5-43 12. HOCl in H 2 SO 4 • nH 2 O(l)—Recommendation is from the model of Shi et al. [313] which is based on wetted wall flow tube data from Hanson a nd Ravishankara [162] and Hanson and Lovejoy [154], and uptake by stirred and static solutions by Donaldson et al. [107]. This model incorporates newer, higher temperature data and replaces earlier recommended formula tion by Huthwelker et al. [185].

13. ClONO 2 in H 2 SO 4 • nH 2 O(l)—Recommendation is from the model of Shi et al. [313] who used a measurement of the hydrolysis reaction’s reacto-diffu sive length by Ha nson and Lovejoy [153] on 60 wt. % H 2 SO 4 at 250 K to derive the hydrolysis rate constant, k hyd , and constrain H ClONO2 at 250 K. Shi et al. fit the Hk 1/2 dependence of the ClONO 2 uptake coefficients for a variety of ClONO 2 hydrolysis and ClONO 2 + HCl data to derive a parameterization for H as a function of wt. % and T.

14. HBr in H 2 SO 4 • mHNO 3 • nH 2 O(l)—Experimental data for HBr solubility is provided by Williams et al.[354], Abbatt [2], Abbatt and Nowak [8], Kleffman et al. [222], and Behr et al. [45]. Data from timedependent uptake measurements and from vapor pressure measurements is in good agreement after correcting for the fact that for some of the vapor pr essure measurements the HB r concentration in solution was high enough to increase the acidity and thereby decrease the HBr solub ility. By comparing pairs of data points with different HBr concentra tions (from the same experiment), an average correction factor was obtained. The correction factor was us ed to correct the vapor pressure da ta of Williams et al. [354], Abbatt and Nowak [8] and Kleffmann et al. to zero effective HBr concentration. (T his is different than the approach taken in Kleffmann et al . of using a “corrected” H 2 SO 4 wt. %. However, the resulting parameterization is very similar to the one in Kleffma nn et al. [222].) The time-dependent upt ake data of Williams et al. [354] and Abbatt [2], and the molecular beam uptake data of Behr et al. [45] did not require correction. All of the experimental data have been fit to obtain th e recommended parameterization as a function of H 2 SO 4 wt. % and temperature.
Agreement between this parameterization and the updated activity coefficient model of Massucci et al. [251] (and http://www.hpc1.uea.ac.uk/~e770/aim.html) is good for > 60 wt. %, but not very good at lower H 2 SO 4 wt. %, particularly at low temperatures. Ther efore, this parameterization is recommended for calculating HBr Henry’s law solubilities.
The only data for HBr solubilities in ternary solutions is from Kleffmann et al. [222]. The data do not agree well with the updated activity coefficient in Massucci et al. [222] or with the older activity coefficient model in Luo et al. [248]. Until further information becomes available, the recommendation is to use the parameterization for ternary solutions given in Kleffmann et al. [222].

15. SO 2 in H 2 SO 4 • nH 2 O(l)—Room temperature vapor pressure measurements reviewed by Hayduk et al. [171] and bubble train reactor uptake measurements by Rattigan et al. [282] for 0–70 wt. % H 2 SO 4 agree very well. Langenberg et al. [229]] used a novel capillary gas ch romatography technique to deduce H* values for 41–83 wt. % H 2 SO 4 over a temperature range of 193–242 K. The recommended parameterization is a fair fit to the Rattigan et al. and Langenberg et al. data sets and allows reasonable extrapolation over the full range of atmospheric temperatures. Note that the Langenberg et al. [229] data is in mol/kg-bar units and was converted to mole/l units using the density parameterization of Myhre et al. [269].5-44 

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### A-1 

## APPENDIX A. THERMODYNAMIC PARAMETERS

Table of Contents

APPENDIX A. THERMODY NAMIC PARA METERS ..........................................................................................A -1 A.1 Gas-phase entropy and enthalpy values...................................................................................... ............A-1 A.1 References ................................................................................................................. .............................A-8



### Tables

Table A-1. Gas-phase entropy and enthalpy values fo r selected species at 298.15 K and 100 kPa. .........................A-1



### A.1 Gas-phase entropy and enthalpy values

Table A-1 lists selected entropy and enthalpy of formation values at 298 K for a number of atmospheric species. As much as possible, the values were taken from primary evaluations, that is, evaluations that develop a recommended value from the original studies. Otherwise, the values were selected from the original literature, which is referenced in the table. Often, the enthalpy of form ation and the entropy values are taken from different sources, usually due to a more recent value fo r the enthalpy of formation. The c ited error limits are from the original references and therefore reflect often widely varying criteria. Some enthalpy values were corrected slightly to reflect the value of a reference compound selected for this table; th ese are indicated. Values that are calculated or estimated are also indicated in the table.

Table A-1. Gas-phase entropy and enthalpy values for selected species at 298.15 K and 100 kPa.

SPECIES ∆ H f (298 K) kJ mol –1 ∆ H f (298 K) kcal mol –1 S(298 K) J K –1 mol –1 S(298 K) cal K –1 mol –1 Reference a, b, c

H 217.998 ± 0.006 52.103 ± .001 114.717 ± 0.002 27.418 ± .0.001 [28] H 2 0.00 0.00 130.680 ± 0.003 31.233 ± 0.001 [28] O( 3 P) 249.18 ± 0.10 59.56 ± 0.02 161.059 ± 0.003 38.194 ± 0.001 [28] O( 1 D) 438.05 ± 0.1 104.70 ± 0.03 [70] O 2 0.00 0.00 205.152 ± 0.005 49.033 ± 0.001 [28] O 2 ( 1 ∆ g ) 94.29 ± 0.01 22.54 ± 0.01 [36] O 2 ( 1 Σ g + ) 156.96 ± 0.01 37.51 ± 0.01 [36] O 3 141.8 ± 2 33.9 ± 0.5 239.01 57.12 [33] OH 37.20 ± 0.38 8.89 ± 0.09 183.74 43.91 [33,87] HO 2 13.8 ± 3.3 3.3 ± 0.8 229.1 54.76 [35,58] H 2 O –241.826 ± 0.040 –57.798 ± 0.010 188.835 ± 0.010 45.133 ± .002 [28] H 2 O 2 –135.88 ± 0.22 –32.48 ± 0.05 234.52 56.05 [33] N( 4 S) 472.68 ± 0.40 112.973 ± 0.10 153.301 ± 0.003 36.640 ± 0.001 [28] N 2 0.00 0.00 191.609 ± 0.004 45.796 ± 0.001 [28] NH 357 ± 1 85.3 ± 0.3 181.25 ± 0.04 43.32 ± 0.01 [4] NH 2 186 ± 1 44.5 ± 0.3 194.71 ± 0.05 46.54 ± 0.01 [4] NH 3 –45.94 ± 0.35 –10.98 ± 0.08 192.77 ± 0.05 46.07 ± 0.01 [28] NH 2 OH –40.2 ± 9.2 –9.6 ± 2.2 236.18 56.45 [5] NH 2 NO 2 –26 ± 10 –6.2 ± 3 268.54 64.18 [33] NO 91.29 ± 0.17 21.82 ± 0.04 210.76 50.37 [5,22] N 2 O 81.6 ± 0.5 19.50 ± 0.12 220.01 52.58 [33] NO 2 34.19 ± 0.5 8.17 ± 0.1 240.17 57.40 [33] NO 3 73.7 ± 1.4 17.6 ± 0.3 258.4 ± 1.0 61.76 ± 0.24 [1,29] N 2 O 3 86.6 ± 1 20.7 ± 0.3 314.74 75.22 [33] N 2 O 4 11.1 ± 1 2.65 ± 0.25 340.45 81.37 [33] N 2 O 5 13.3 ± 1.5 3.18 ± 0.36 355.7 ± 7 85.01 ± 2 [33] HNO 107.1 ± 2.5 25.6 ± 0.6 [5]

### A-2 SPECIES ∆ H f (298 K) kJ mol –1 ∆ H f (298 K) kcal mol –1 S(298 K) J K –1 mol –1 S(298 K) cal K –1 mol –1 Reference a, b, c

HONO –78.45 ± 0.8 –18.75 ± 0.2 254.07 60.72 [33] HONO 2 –133.9 ± 0.6 –32.0 ± 0.1 266.88 63.78 [33] HO 2 NO –23.8 –5.7 274 65.6 [61], calc. HO 2 NO 2 –53.1 ± 2.5 –12.7 ± 0.6 294 ± 3 70.3 ± 0.7 [84] C 716.68 ± 0.45 171.29 ± 0.11 158.100 ± 0.001 37.787 ± 0.001 [28] CH 597.37 ± 1.3 142.77 ± 0.3 183.04 43.75 [33] CH 2 ( 3 B 1 ) 390.4 ± 0.8 93.31 ± 0.2 194.90 46.58 [88] CH 2 ( 1 A 1 ) 428.0 ± 0.8 102.3 ± 0.2 [39] CH 3 146.65 ± 0.29 35.05 ± 0.07 193.96 46.36 [33,88] CH 4 –74.48 ± 0.41 –17.80 ± 0.10 186.38 44.55 [31,82] CN 440 ± 5 105 ± 1 202.64 48.43 [33] HCN 132 ± 4 31.5 ± 1 201.82 48.24 [33] C 2 N 2 309.1 ± 0.8 73.9 ± 0.2 242.20 57.89 [33] CH 2 NH 2 149 ± 8 35.6 ± 2 [62], corr. CH 3 NH 2 –23.4 ± 1.0 –5.6 ± 0.3 242.89 58.05 [31,79] CH 2 NO 157 ± 4 37.5 ± 1 [96], calc. NH 2 CO –15.1 ± 4 –3.6 ± 1 [96], calc. NCO 151 ± 14 36 ± 3 232.38 55.54 [75], corr., [33] HNCO –104 ± 12 – 24.8 ± 2.8 237.97 ± 0.8 56.9 ± 0.2 [97], corr.,[102] CO –110.53 ± 0.17 –26.42 ± 0.04 197.660 ± 0.004 47.242 ± 0.001 [28] CO 2 –393.51 ± 0.13 –94.05 ± 0.03 213.785 ± 0.010 51.096 ± 0.002 [28] HCO 44.15 ± 0.43 10.55 ± 0.10 224.34 53.62 [8], corr., [33] CH 2 O –108.7 ± 0.05 –25.98 ± 0.01 218.76 52.28 [33] HCOO 127 30 244.7 58.5 [106], calc. C(O)OH –193 –45 251.6 60.1 [106] HC(O)OH –378.8 ± 0.5 –90.54 ± 0.1 248.87 59.48 [33,106] CH 3 O 17.15 ± 3.8 4.1 ± 0.9 232.86 55.655 [11,33] CH 3 O 2 9.0 ± 5.1 2.15 ± 1.2 [46] CH 2 OH –11.5 ± 1.3 –2.75 ± 0.31 244.170 ± 0.018 58.358 ± 0.004 [41] CH 3 OH –201.0 ± 0.6 –48.04 ± 0.14 239.865 57.329 [33] CH 3 OOH –139.0 ± 8.1 –33.2 ± 1.9 [46] CH 2 NO 2 147.3 35.2 272.48 65.12 [31] CH 3 NO 2 –74.3 ± 0.6 –17.8 ± 0.2 275.2 65.8 [31,79] CH 3 ONO –64.0 –15.3 284.3 67.95 [98] CH 3 ONO 2 –122.2 ± 4.3 –29.2 ± 1.1 301.9 72.15 [79,98] C 2 H 565.3 ± 2.9 135.1 ± 0.7 209.73 50.13 [11,33] C 2 H 2 227.4 ± 0.8 54.35 ± 0.2 200.93 48.02 [33] C 2 H 2 OH 121 ± 11 28.9 ± 2.6 [32] C 2 H 3 299 ± 5 71.5 ± .1 [99] C 2 H 4 52.4 ± 0.5 12.52 ± 0.12 219.316 52.418 [33] C 2 H 5 120.9 ± 1.7 28.9 ± 0.4 250.52 59.88 [11,33] C 2 H 6 –83.85 ± 0.29 –20.04 ± 0.07 229.162 54.771 [33,82] CH 2 CN 252.6 ± 4 60.4 ± 1.0 [52] CH 3 CN 74.04 ± 0.37 17.70 ± 0.09 245.12 ± 0.8 58.59 ± 0.2 [2,102] CH 2 CO –49.58 ± 0.88 –11.85 ± 0.21 [88] CH 3 CO –10.0 ± 1.2 –2.4 ± 0.3 [11] CH 2 CHO 10.5 ± 9.2 2.5 ± 2.2 [11] CH 3 CHO –166.1 ± 0.5 39.7 ± 0.1 263.95 63.09 [31,79] CH 3 CH 2 O –15.5 ± 3.3 –3.7 ± 0.8 [11] (CHO) 2 –212 ± 0.8 –50.7 ± 0.2 [30]

### A-3 SPECIES ∆ H f (298 K) kJ mol –1 ∆ H f (298 K) kcal mol –1 S(298 K) J K –1 mol –1 S(298 K) cal K –1 mol –1 Reference a, b, c

C 2 H 5 O –17.2 –4.1 [62] C 2 H 5 O 2 –27.4 ± 9.9 –6.6 ± 2.4 [46] C 2 H 5 OOH –175.4 ± 12.9 –41.9 ± 3.1 [46] CH 2 CH 2 OH –31 ± 7 –7.5 ± 1.7 [32] CH 3 CHOH –63.7 ± 4 –15.2 ± 1 [62] C 2 H 5 OH –234.8 ± 0.5 –56.12 ± 0.12 281.622 67.309 [33] CH 3 COO –190 –45 284.9 68.1 [106], calc. CH 2 C(O)OH –243 58 238.4 57.0 [106] CH 3 C(O)O –192.5 –46.0 [63], calc. CH 3 C(O)OH –432.8 ± 0.5 –103.4 ± 0.1 332.67 79.51 [18,79] CH 3 C(O)O 2 –154.4 –36.9 [63], calc. CH 3 C(O)O 2 NO 2 –240.1 –57.4 [63], calc. HOCH 2 COOH –583 ± 10 –139 ± 3 318.6 ± 5.0 76.1 ± 1.2 [30] CH 3 OCH 2 –13.0 ± 4 –3.1 ± 1 [62], corr. CH 3 OCH 3 –184.1 ± 0.5 –44.0 ± 0.1 267.34 63.90 [31,79] CH 2 (OH)CH 2 OH –392.2 ± 4.0 93.7 ± 1.0 303.81 72.61 [31,79] CH 3 OOCH 3 –125.5 ± 5.0 –30.0 ± 1.2 [30] (HOCO) 2 –731.8 ± 2.0 –174.9 ± 0.5 320.6 ± 5.0 76.6 ± 1.2 [30] C 3 H 5 166.1 ± 4.3 39.7 ± 1.0 248 ± 15 59.3 ± 3.6 [94] C 3 H 6 20.0 ± 0.7 4.78 ± 0.2 266.6 63.72 [17,79] n–C 3 H 7 100 ± 2 24 ± 0.5 [99] i–C 3 H 7 86.6 ± 2.0 20.7 ± 0.5 281 ± 5 67.2 ± 1.2 [95] i–C 3 H 7 O 2 –65.4 ± 11.3 –15.6 ± 2.7 [46] C 3 H 8 –104.68 ± 0.50 –25.02 ± 0.12 270.20 64.58 [16,82] C 2 H 5 CHO –185.6 ± 0.8 44.4 ± 0.2 304.51 [31,79] CH 3 COCH 3 –217.1 ± 0.7 51.9 ± 0.2 295.46 70.62 [31,79] n-C 4 H 10 -125.65 ± 0.67 -30.03 ± 0.16 309.91 74.07 [31,82] (CH 3 COO) 2 –500 ± 10 –120 ± 3 390.7 ± 6.0 93.4 ± 1.4 [30] F 79.38 ± 0.30 18.94 ± 0.07 158.751 ± 0.004 37.942 ± 0.001 [28] F 2 0.00 0.00 202.791 ± 0.005 48.468 ± 0.001 [28] HF –273.30 ± 0.70 –65.32 ± 0.17 173.799 ± 0.003 41.539 ± 0.001 [28] HOF –98.3 ± 4.2 –23.5 ± 1.0 226.77 ± 0.21 54.20 ± 0.05 [22] FO 109 ± 10 26 ± 3 216.40 ± 0.3 51.72 ± 0.07 [21] FOF 24.5 ± 2 5.86 ± 0.5 247.46 ± 0.4 59.14 ± 0.1 [21] OFO 380 ± 20 90.8 ± 5 251 ± 1 60.0 ± 0.3 [21], calc. FOO 25.4 ± 2 6.07 ± 0.5 259.5 ± 0.2 62.02 ± 0.05 [21] FOOF 19.2 ± 2.0 4.59 ± 0.5 277.2 ± 0.2 66.25 ± 0.05 [21] FONO 67 16 [6], est FNO –65.7 –15.70 248.0 59.27 [98] FNO 2 –79 –19.0 277.1 66.24 [98] FONO 2 10 ± 2 2.5 ± 0.5 290 70 [22], est. CF 244.1 ± 10 58.3 ± 2.4 213.03 ± 0.04 50.92 ± 0.01 [22,33] CHF 143.1 ± 12 34.2 ± 3.0 234.87 56.14 [33,83] CF 2 –184 ± 8 –44.0 ± 2 240.83 ± 0.04 57.56 ± 0.01 [22,83] CF 3 –465.7 ± 2.1 –111.3 ± 0.5 264.56 63.23 [33,89] CF 4 –933.20 ± 0.75 –223.04 ± 0.18 261.454 62.49 [28] CHF 3 –692.9 ± 2.1 –165.6 ± 0.5 259.67 62.06 [33,89] CHF 2 –239 ± 4 –57.1 ± 1.0 258.50 61.78 [81] CH 2 F 2 –452.7 ± 0.8 –108.2 ± 0.2 246.59 58.94 [85] CH 2 F –32 ± 8 –7.6 ± 2 236.52 56.53 [81]

### A-4 SPECIES ∆ H f (298 K) kJ mol –1 ∆ H f (298 K) kcal mol –1 S(298 K) J K –1 mol –1 S(298 K) cal K –1 mol –1 Reference a, b, c

CH 3 F –238 ± 8 –56.8 ± 2 222.78 53.246 [85], H est. FCO –161.2 ± 8.1 –38.5 ± 2.0 [44] CHFO –383 ± 7 –91.6 ± 1.7 246.82 58.99 [91],calc., [33] CF 2 O –607.9 ± 7.1 –145.3 ± 1.7 258.97 61.89 [91],calc., [33] CF 3 O –624 ± 8 –149 ± 2 [91], calc. CF 2 O 2 –427 ± 6 –102 ± 1.5 [48], calc. CF 3 O 2 -612.5 ± 15.4 146 ± 4 [56] CF 3 OH –911 ± 8 –218 ± 2 [91] CF 3 OOCF 3 –1434 ± 11 –343 ± 3 [91] CF 3 OF –724 ± 8 –173 ± 2 [91] CH 2 CH 2 F 59.4 ± 8 –14.2 ± 2 279.7 66.86 [66],[25], calc. CH 3 CHF –70.3 ± 8 –16.8 ± 2 274.0 65.48 [66], [26], calc. CH 3 CH 2 F –277.4 ± 4.2 –66.3 ± 1 265.1 63.4 [59], est. [33] CH 2 FCH 2 F –432 ± 25 –103.2 ± 6 [42] CH 2 FCHF 235.5 56.28 293.3 70.11 [27] CH 2 FCHF 2 –665 ± 4 –158.9 ± 1 [51], corr. CHF 2 CHF 2 –860 ± 24 –205.6 ± 5.7 320.3 76.6 [64], corr. [31] CH 2 CF 3 –517.1 ± 5 –123.6 ± 1.2 306.8 73.32 [25,104] CH 3 CF 3 –745.6 ± 1.7 –178.2 ± 0.4 287.3 68.67 [23] CHF 2 CH 2 –277 –66.3 297.8 71.17 [25], calc. CH 3 CF 2 –302.5 ± 8.4 –72.3 ± 2 290.3 69.39 [80], [26], S calc CH 3 CHF 2 –500.1 ± 6.3 –119.7 ± 1.5 282.4 67.50 [23] CHFCF 3 –697 –166.5 326.2 77.97 [27], H corr. CH 2 FCF 3 –896 ± 8 –214.1 ± 2 316.2 75.58 [23], H est. CF 2 CF 3 –891 ± 5 –213 ± 1.3 [105] CHF 2 CF 3 –1105 ± 5 –264 ± 1.1 333.7 79.76 [23] C 2 F 6 –1344.3 ± 3.4 –321.3 ± 0.8 331.8 79.30 [23,89] Cl 121.301 ± 0.008 28.992 ± 0.002 165.190 ± 0.004 39.481 ± 0.001 [28] Cl 2 0.00 0.00 223.081 ± 0.010 53.318 ± 0.002 [28] HCl –92.31 ± 0.10 –22.06 ± 0.02 186.902 ± 0.005 44.671 ± 0.001 [28] ClO 101.63v0.1 24.29 ± 0.03 225.07 ± 0.5 53.79 ± 0.12 [22] ClOO 98.0v4 23.4 ± 1 269.32 ± 0.5 64.37 ± 0.1 [22] OClO 94.6v1.2 22.6 ± 0.3 256.84 ± 0.1 61.39 ± 0.03 [22,72] ClO 3 194 ± 12 46 ± 3 270.75 ± 0.5 64.71 ± 0.1 [22] ClClO 90 ± 30 22 ± 7 278.8 ± 2.0 66.6 ± 0.5 [22] ClOCl 81.3 ± 1.8 19.4 ± 0.4 [34] ClOOCl 127.6 ± 2.9 30.5 ± 0.7 301.0 ± 5.0 71.9 ± 1.2 [22,72] ClClO 2 154.2 36.9 294 ± 2 70.3 ± 0.5 [55],calc., [22] ClOClO 175.5 41.9 309 ± 2 73.9 ± 0.5 [55],calc., [22] Cl 2 O 3 150 ± 6 35.8 ± 1.5 390 ± 20 94 ± 5 [14] HOCl –74.8 ± 1.2 –17.9 ± 0.3 236.50 ± 0.42 56.52 ± 0.10 [22,34] ClNO 52.7 ± 0.5 12.6 ± 0.1 261.58 62.52 [33] ClNO 2 12.5 ± 1.0 3.0 ± 0.3 272.23 65.06 [33] cis–ClONO –64.4 ± 6.3 15.4 ± 1.5 [54], calc. trans–ClONO 75.3 ± 6.3 18.0 ± 1.5 [54], calc. ClO 2 NO 102 24.3 316 75.5 [61], calc. ClONO 2 22.9 ± 2.0 5.5 ± 0.5 302.38 72.27 [3] FCl –55.70 ± 0.31 13.31 ± 0.07 217.94 52.09 [33] CHCl 326 ± 8 78.0 ± 2.0 234.88 56.85 [33,83] CCl 2 230 ± 8 55.0 ± 2.0 265.03 63.34 [33,83]

### A-5 SPECIES ∆ H f (298 K) kJ mol –1 ∆ H f (298 K) kcal mol –1 S(298 K) J K –1 mol –1 S(298 K) cal K –1 mol –1 Reference a, b, c

CCl 3 71.1 ± 2.5 17.0 ± 0.6 303.24 72.47 [37] CCl 3 OH –293 ± 20 –70.0 ± 5 [90], calc. CCl 3 O –43.5 ± 20 –10.4 ± 5 [90], calc CCl 3 O 2 –20.9 ± 8.9 –5.0 ± 2.1 [46] CCl 4 –95.6 ± 2.5 –22.8 ± 0.6 309.90 74.069 [38,85][60] CHCl 3 –102.9 ± 2.5 –24.6 ± 0.6 295.51 70.63 [60,85] CHCl 2 89.0 ± 3.0 21.3 ± 0.7 280 ± 7 66.9 ± 2 [92] CHCl 2 O 2 –17 ± 7 –4 ! 2 [92] CH 2 Cl 117.3 ± 3.1 28.0 ± 0.7 271 ± 7 64.5 ± 2 [92] CH 2 ClO 2 –4v11 –1 ± 3 [92] CH 2 Cl 2 –95.1 ± 2.5 –22.8 ± 0.6 270.31 64.606 [60,85] CH 3 Cl –81.9 ± 0.6 –19.6 ± 0.2 227.15 54.290 [60,85] ClCO –24.9 ± 4.2 –5.9 ± 1.0 266.0 63.6 [22,57] CHClO –164 ± 20 –38 ± 5 259.07 61.92 [33], H est, CCl 2 O –220.9 –52.8 283.8 67.82 [98] CHFCl –61 ± 10 –14.5 ± 2.4 [100] CH 2 FCl –264 ± 8 –63.2 ± 2 264.3 63.17 [24,100], H est. CFCl 31v13 7.4 ± 3.2 259.032 61.91 [33,83] CFCl 2 –89.1 ± 10.0 –21.3 ± 2.4 [100] CFCl 3 –285.3 –68.2 309.9 74.06 [24], corr. CF 2 Cl 2 –494.1 –118.1 300.7 71.87 [24], corr. CF 3 Cl –709.2 ± 2.9 –169.5 ± 0.7 285.2 68.16 [24,89] CHFCl 2 –285 ± 9 –68.1 ± 2.1 293.0 70.04 [24], H est. CHF 2 Cl –484.8 –115.6 280.8 67.11 [24], H est. CF 2 Cl –279 ± 8 –66.7 ± 2 [68] CFClO –429 ± 20 –103 ± 5 276.70 66.13 [33] CH 2 ClCOOH –427.6 ± 1.0 –102.2 ± 0.2 325.9 ± 5.0 77.9 ± 1.2 [30] C 2 H 3 Cl 22 ± 3 5.3 ± 0.7 [60] CH 3 CHFCl –313.4 ± 2.6 –74.9 ± 0.6 [47] CH 2 CF 2 Cl –318 –75.9 322.08 76.98 [77] CH 3 CF 2 Cl –536.2 ± 5.2 –128.2 ± 1.2 307.1 73.41 [47,77] C 2 Cl 4 –18.8 ± 4 –4.5 ± 1 341.03 81.51 [33,38] 1,1–C 2 H 2 Cl 2 2.4 ± 2.0 0.6 ± 0.5 [60] Z

–1,2–C 2 H 2 Cl 2 –3 ± 2 –0.7 ± 0.5 [60] E

–1,2–C 2 H 2 Cl 2 –0.5 ± 2.0 –0.1 ± 0.5 [60] C 2 HCl 3 –19.1 ± 3.0 –.6 ± 0.7 325.20 77.72 [31,78] CH 2 CCl 3 71.5 ± 8 17.1 ± 2 [86] 1,1,1–C 2 H 3 Cl 3 –144.6 ± 2.0 –34.6 ± 0.5 320.03 76.488 [15,47,60] 1,1,2–C 2 H 3 Cl 3 –148.0 ± 4.0 –35.4 ± 0.9 [60] 1,1,1,2–C 2 H 2 Cl 4 –152.3 ± 2.4 –36.4 ± 0.6 [60] 1,1,2,2–C 2 H 2 Cl 4 –156.7 ± 3.5 –37.5 ± 0.8 [60] C 2 HCl 5 –155.9 ± 4.3 –37.3 ± 1.0 [60] CH 3 CCl 2 42.5 ± 1.7 10.2 ± 0.4 288 ± 5 68.8 ± 1.1 [92] CH 3 CCl 2 O 2 –69.7 ± 4 –16.7 ± 1 [45], corr. CH 3 CHCl 2 –130.6 ± 3.0 –31.2 ± 0.7 305.05 72.908 [15,47] CH 2 CH 2 Cl 93.0 ± 2.4 22.2 ± 0.6 271 ± 7 64.8 ± 2 [93] CH 3 CHCl 76.5 ± 1.6 18.2 ± 0.4 279 ± 6 66.7 ± 1.4 [92] CH 3 CH 2 Cl –112.1 ± 0.7 –26.8 ± 0.2 275.78 65.913 [15,60] C 2 Cl 6 –142 ± 4 –34.0 ± 1 398.62 95.27 [33,38]
Br 111.870 ± 12 26.74 ± 0.03 175.018 ± 0.004 41.830 

### ± 0.001 [28]

### A-6 SPECIES ∆ H f (298 K) kJ mol –1 ∆ H f (298 K) kcal mol –1 S(298 K) J K –1 mol –1 S(298 K) cal K –1 mol –1 Reference a, b, c

Br 2 (g) 30.91 ± 0.11 7.39 ± 0.03 245.468 ± 0.005 58.668 

### ± 0.001 [28]

HBr –36.29 ± 0.16 –8.67 ± 0.04 198.700 ± 0.004 47.490 

### ± 0.001 [28]
Br 2 O 106.2 ± 2.5 25.4 ± 0.6 [34] HOBr –60.5 ± 1.1 –14.5 ± 0.3 [34] BrO 126.2 ± 1.7 30.2 ± 0.4 232.97 ± 0.1 55.681 

### ± 0.023 [19,103]
OBrO 163.9 ± 4.4 39.2 ± 1.1 271 ± 2 64.8 

### ± 0.5 [19,43], est.
BrOO 108 ± 40 26 ± 10 289 ± 3 69.1 

### ± 0.7 [19]
BrO 3 221 ± 50 53 ± 12 285 ± 2 68.1 

### ± 0.5 [19], est.
BrOBr 107.6 ± 3.5 25.7 ± 0.8 290.8 ± 2 69.50 

### ± 0.48 [19]
BrBrO 168 ± 20 40 ± 5 313 ± 2 74.8 

### ± 0.5 [19], est.
BrNO 82.17 ± 0.8 19.64 ± 0.2 273.66 ± 0.8 65.41 

### ± 0.2 [102]
Z

–BrONO 71.9 17.19 [53], calc. E

–BrONO 88.3 21.1 [53], calc. BrNO 2 45.2 10.8 [53], calc. BrONO 2 42.3 ± 6.3 10.1 ± 1.5 [76] BrF –58.9 ± 1.0 –14.08 ± 0.3 228.985 54.729 [33] BrCl 14.79 ± 0.16 3.53 ± 0.04 240.046 57.372 [33] CH 2 Br 169 ± 4 40.4 ± 1.0 [100] CHBr 3 23.8 ± 4.5 5.7 ± 1.1 330.67 79.03 [13]calc.,[33] CHBr 2 188.9 45.0 ± 2.2 [100] CBr 3 235 ± 25 56 ± 6 334.57 80.0 [33] CH 2 Br 2 –11.1 ± 5.0 –2.7 ± 1.2 294 70.23 [13], calc. CH 3 Br –37.7 ± 1.5 –9.02 ± 0.36 245.85 ± 0.25 58.76 

### ± 0.06 [49] CH 2 CH 2 Br 135.6 ± 6.7 32.4 ± 1.6 [10] CH 3 CHBr 127 ± 4 30.4 ± 1 [67] corr. CH 3 CH 2 Br –61.5 ± 1.0 –14.7 ± 0.3 287.3 ± 0.4 68.66 

### ± 0.09 [47,50] CH 3 CBr 2 140.2 ± 5.4 33.5 ± 1.3 [69] CH 3 CBr 2 H 26.7 ± 1.9 6.4 ± 0.5 [47] CF 3 Br –641.4 ± 2.3 –153.3 ± 0.5 [89] CBr 4 83.9 ± 3.4 20.0 ± 0.8 358.06 85.6 [13,33] CH 2 BrCOOH –383.5 ± 3.1 –91.7 ± 0.7 337.0 ± 5.0 80.5 ± 1.2 [30]
I 106.76 ± 0.04 25.52 ± 0.01 180.787 ± 0.004 43.209 

### ± 0.001 [28]

I 2 62.42 ± 0.08 14.92 ± 0.02 260.687 ± 0.005 62.306 

### ± 0.001 [28]

HI 26.50 ± 0.10 6.33 ± 0.03 206.590 ± 0.004 49.376 

### ± 0.001 [28]
HOI –69.6 ± 5.4 –16.6 ± 1.3 255.0 ± 0.1 60.95 

### ± 0.03 [12,34]
IO 115.9 ± 5.0 27.7 ± 1.2 239.6 ± 0.1 57.27 

### ± 0.03 [9,34] OIO 77 ± 15 18 ± 4 279.9 66.9 [65], calc. IOO 96.6 ± 15 23 ± 4 308.4 73.7 [65], calc. IO 3 242 ± 50 58 ± 12 293 ± 4 70.0 

### ± 1.0 [20], est. IOI 92.4 ± 15 22.1 ± 4 306.5 73.3 [65] IIO 134.1 ± 15 32.1 ± 4 317.8 76.0 [65] IOOI 156.8 ± 15 37.5 ± 4 337.0 80.5 [65], calc. IIOO 103.0 ± 15 24.6v4 339.9 81.2 [65], calc. IOIO 124.2 ± 15 29.7 ± 4 349.7 83.6 [65], calc. OIIO 224.0 ± 15 53.5 ± 4 356.3 85.2 [65], calc. INO 121 ± 4 29.0 ± 1 282.8 ± 4 67.6 

### ± 1 [101]

### A-7 SPECIES ∆ H f (298 K) kJ mol –1 ∆ H f (298 K) kcal mol –1 S(298 K) J K –1 mol –1 S(298 K) cal K –1 mol –1 Reference a, b, c

INO 2 60.2 ± 4 14.4 ± 1 294 ± 6 70.3 

### ± 1.5 [101] ICl 17.506 ± 0.105 4.184 ± 0.025 427.567 102.191 [22] IBr 40.88 ± 0.08 9.77 ± 0.02 258.95 61.89 [22] CH 3 I 13.76 ± 0.12 3.29 ± 0.03 253.70 ± 0.25 60.635 

### ± 0.06 [49]

CH 2 I 2 118.4 ± 0.1 28.30 ± 0.03 309.41 ± 1.34 73.95 

### ± 0.32 [49] CF 3 I –586.2 ± 2.1 –140.1 ± 0.5 307.78 73.56 [33,89] CH 3 CH 2 I –7.5 ± 0.9 –1.79 ± 0.2 295.52 ± 0.42 70.63 

### ± 0.10 [47,50]
S 277.17 ± 0.15 66.25 ± 0.04 167.829 ± 0.006 40.112 

### ± 0.002 [28]
S 2 128.6 ± 0.3 30.74 ± .07 228.167 ± 0.010 54.533 

### ± 0.003 [28] HS 142.80 ± 2.85 34.13 ± 0.68 195.55 46.74 [74], corr., [33]
H 2 S –20.6 ± 0.5 –4.92 ± 0.12 205.81 ± 0.05 49.19 

### ± 0.01 [28] SO 4.78 ± 0.25 1.14 ± 0.06 221.94 53.04 [33] SO 2 –296.81 ± 0.20 –70.94 ± 0.05 248.223 ± 0.050 59.327 

### ± 0.012 [28] SO 3 –395.9 ± 0.7 –94.62 ± 0.17 256.541 61.315 [33] HSO –6.1 ± 2.9 –1.5 ± 0.7 [7] H 2 SO 4 –733 ± 2 –175.2 ± 0.5 299.282 71.530 [33] CS 279.775 ± 0.75 66.87 ± 0.18 210.55 50.32 [33] CS 2 116.7 ± 1.0 27.9 ± 0.2 237.882 56.855 [33] CS 2 OH 110.5 ± 4.6 26.4 ± 1.1 321 ± 20 77 

### ± 5 [71] CH 3 S 125.0 ± 1.8 29.87 ± 0.44 [73], corr. CH 3 SH –22.9 ± 0.7 –5.47 ± 0.17 255.14 60.98 [31,79] CH 2 SCH 3 136.8 ± 5.9 32.7 ± 1.4 [40] CH 3 SCH 3 –37.4 ± 0.6 –8.94 ± 0.2 285.96 68.35 [31,79] CH 3 SSCH 3 –24.7 ± 1.0 –5.9 ± 0.3 336.80 80.50 [31,79] OCS –141.7 ± 2 –33.9 ± 0.5 231.644 55.36 [33] Notes: a. Error limits are estimates fro m the original references. b. If two references are given for a substance, the firs t refers to the enthalpy value while the second to the entropy. c. The terms “calc” and “est” indicate that the value is calculated or estimated. The term “corr” indicates that an enthalpy value has been adjusted to reflect the value chos en in this table for a reference substance.

### A-8 References

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