Cassini / Huygens Program

Archive Plan

for Science Data

PD 699-068

JPL D-15976

Version 3

June 2004

![](media/image1.png){width="1.2354166666666666in"
height="0.4666666666666667in"}

**National Aeronautics and Space Administration**

**Jet Propulsion Laboratory**

**California Institute of Technology**

**Pasadena, California**

**Prepared By:**

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Diane Conner, Cassini Program Archive Engineer

**Approved By:**

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Susan Linick, Cassini Project Instrument Operations Manager

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Dennis Matson, Cassini Project Scientist

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Kathryn Weld, Cassini Project Science and Uplink Operations Manager

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Robert Mitchell, Cassini Program Manager

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Jean-Pierre Lebreton, Huygens Project Scientist

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Laverne Hall, Planetary Data System Project Manager

**Concurred by:**

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Reta Beebe, Planetary Data System Project Scientist

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Don Sawyer, National Space Science Data Center Manager

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Denis Bogan, Cassini Program Scientist

\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_\_

Mark Dahl, Cassini Program Executive

**Change Record for 699-068**

+------------+----------+------------------------------+-------------+
| **Revision | **Date** | **Changes**                  | **Sections  |
| No.**      |          |                              | Affected**  |
+============+==========+==============================+=============+
| Draft 1    | 7/15/98  | First version for review     | All         |
+------------+----------+------------------------------+-------------+
| Draft 2    | 8/1/98   | Minor updates,               | All         |
|            |          |                              |             |
|            |          | Appendix A \-- added         |             |
|            |          | definition of processing     |             |
|            |          |                              |             |
|            |          | Appendix C \-- added Archive |             |
|            |          | schedule                     |             |
+------------+----------+------------------------------+-------------+
| Draft 3    | 9/16/98  | Reorganization \-- Updated   | All         |
|            |          | signature page, replaced     |             |
|            |          | references to SO and DOI     |             |
|            |          | with the new "Instrument     |             |
|            |          | Operations Team", replaced   |             |
|            |          | references to MSO and        |             |
|            |          | Science Office with "Science |             |
|            |          | Operations Office"           |             |
|            |          |                              |             |
|            |          | Section 2, item 2 \-- states |             |
|            |          | that Cassini provides        |             |
|            |          | volumes to PDS CN who in     |             |
|            |          | turn provides copies to the  |             |
|            |          | relevant PDS DNs. It should  |             |
|            |          | be noted that this is still  |             |
|            |          | listed as a TBD              |             |
|            |          |                              |             |
|            |          | Incorporated PDS comments    |             |
+------------+----------+------------------------------+-------------+
| Draft 4    | 10/5/98  | Section 2, item 5 Added      | All         |
|            |          | cruise archive policy &      |             |
|            |          | included in delivery of      |             |
|            |          | cruise science in Archive    |             |
|            |          | schedule                     |             |
|            |          |                              |             |
|            |          | OTLs and MSOCs listed as     |             |
|            |          | archive contacts for each    |             |
|            |          | instrument                   |             |
+------------+----------+------------------------------+-------------+
| P          | 4/1/99   | Changed document title       | All         |
| reliminary |          |                              |             |
|            |          | Revised signature page       |             |
|            |          |                              |             |
|            |          | Changed instances of         |             |
|            |          | "Cassini Project" to         |             |
|            |          | "Cassini Program"            |             |
|            |          |                              |             |
|            |          | Updated applicable document  |             |
|            |          | listing                      |             |
+------------+----------+------------------------------+-------------+
| P          | 12/27/99 | Updated Signature page       | All         |
| reliminary |          |                              |             |
| V1         |          | Major changes to Roles and   |             |
|            |          | Responsibility section 2.0   |             |
|            |          |                              |             |
|            |          | Some changes to policy       |             |
|            |          | section 3.0                  |             |
|            |          |                              |             |
|            |          | Review and comment on To be  |             |
|            |          | Supplied list                |             |
|            |          |                              |             |
|            |          | Formatting changes           |             |
+------------+----------+------------------------------+-------------+
| P          | 4/1/00   | Incorporated updates         | All         |
| reliminary |          | throughout the document as   |             |
|            |          | requested by reviewers.      |             |
| V2         |          | Incorporated Huygens data in |             |
|            |          | the plan.                    |             |
|            |          |                              |             |
|            |          | Updated distribution list.   |             |
|            |          |                              |             |
|            |          | Updated archive policies.    |             |
+------------+----------+------------------------------+-------------+
| Initial    | 4/25/00  | Clarified PDS CN and PDS DN  | All         |
| Release,   |          | roles and responsibilities   |             |
| Version 0  |          | throughout document.         |             |
|            |          |                              |             |
| UNSIGNED   |          | Updated table 1.5.2 data     |             |
|            |          | product levels to reflect    |             |
|            |          | CODMAC and PDS definitions.  |             |
|            |          | (see unresolved list)        |             |
|            |          |                              |             |
|            |          | Clarified the project intent |             |
|            |          | to archive level 1A and      |             |
|            |          | level 1B data products in    |             |
|            |          | section 6.                   |             |
|            |          |                              |             |
|            |          | Reorganized dataset tables   |             |
|            |          | in appendices.               |             |
|            |          |                              |             |
|            |          | Added new issues to          |             |
|            |          | unresolved issues list.      |             |
|            |          |                              |             |
|            |          | Added High-Level Catalog     |             |
|            |          | documents to schedule.       |             |
+------------+----------+------------------------------+-------------+
| Initial    | 8/3/00   | Higher level product         | 6.4         |
| Release,   |          | archive.                     |             |
| Version 1  |          |                              |             |
+------------+----------+------------------------------+-------------+
| Version 2  | 8/12/02  | Clarified Policies           | All.        |
|            |          |                              |             |
| UNSIGNED   |          | Clarified Roles and          |             |
|            |          | Responsibilities             |             |
|            |          |                              |             |
|            |          | Updated products list        |             |
|            |          |                              |             |
|            |          | Updated archive contacts     |             |
|            |          |                              |             |
|            |          | Added Huygens archive        |             |
|            |          | contacts                     |             |
|            |          |                              |             |
|            |          | Added Huygens Products list  |             |
|            |          |                              |             |
|            |          | Added Mission and instrument |             |
|            |          | overview                     |             |
|            |          |                              |             |
|            |          | Moved CODMAC data level to   |             |
|            |          | NASA levels table to         |             |
|            |          | appendix.                    |             |
|            |          |                              |             |
|            |          | Removed data level           |             |
|            |          | references from document in  |             |
|            |          | lieu of descriptions of      |             |
|            |          | products.                    |             |
|            |          |                              |             |
|            |          | Added Peer Review and        |             |
|            |          | Validation Process           |             |
|            |          |                              |             |
|            |          | Clarified archive terms      |             |
|            |          |                              |             |
|            |          | Removed Data Flow that       |             |
|            |          | appeared to cause confusion. |             |
|            |          |                              |             |
|            |          | Added standard values for    |             |
|            |          | PDS High-Level Catalog files |             |
|            |          |                              |             |
|            |          | Added PDS label keyword      |             |
|            |          | requirements section.        |             |
|            |          |                              |             |
|            |          | Added coordinate system      |             |
|            |          | designations.                |             |
|            |          |                              |             |
|            |          | Clarified roles and          |             |
|            |          | responsibilities.            |             |
|            |          |                              |             |
|            |          | Added a detailed data        |             |
|            |          | delivery schedule.           |             |
+------------+----------+------------------------------+-------------+
| Version 3  | 6/04     | Incorporate many editorial   | All         |
|            |          | changes requested by         |             |
|            |          | reviewers of version 2:      |             |
|            |          |                              |             |
|            |          | Updated Mission overview to  |             |
|            |          | correct tense.               |             |
|            |          |                              |             |
|            |          | Updated Dist list and        |             |
|            |          | acronym list.                |             |
|            |          |                              |             |
|            |          | Updated Contacts list.       |             |
|            |          |                              |             |
|            |          | Updated Appendices.          |             |
|            |          |                              |             |
|            |          | Added Huygens Archive Plan   |             |
|            |          | to Appendix.                 |             |
|            |          |                              |             |
|            |          | Added Cassini data volume    |             |
|            |          | Section.                     |             |
|            |          |                              |             |
|            |          | Changed policy of when       |             |
|            |          | pipeline production should   |             |
|            |          | be ready.                    |             |
|            |          |                              |             |
|            |          | Added data distribution      |             |
|            |          | section.                     |             |
|            |          |                              |             |
|            |          | Added/Clarified definitions  |             |
|            |          | of terms.                    |             |
|            |          |                              |             |
|            |          | Updated Press Release        |             |
|            |          | products section.            |             |
|            |          |                              |             |
|            |          | Added Requirements section.  |             |
|            |          |                              |             |
|            |          | Eliminated reference to the  |             |
|            |          | MIFT. The SAWG will perform  |             |
|            |          | the production coordination  |             |
|            |          | function.                    |             |
|            |          |                              |             |
|            |          | Defined \"Cassini Program\"  |             |
|            |          | in scope.                    |             |
|            |          |                              |             |
|            |          | Merged sections 9 and 10.    |             |
+------------+----------+------------------------------+-------------+

TBDs

  ------------------------------------ ----------------------------------
  ITEM                                 Related section

  Standard keywords for labels and     9.2.2
  index files. (MASTER INDEX)          
  ------------------------------------ ----------------------------------

Distribution List

Achilleos, Nick MAG

Acton, Charles NAIF

Adams, Steven PDS CN

A\'Hearn, Mike PDS

Alanis, Rafael JPL/IMG

Anabtawi, Aseel RSS

Anderson, Theresa SE

Armstrong, Thomas FTECS

Arvidson, Ray PDS/GEO

Asmar, Sami RSS

Atkinson, Dave Huygens

Barbinis, Elias RSS

Beebe, Reta PDS/ATM

Blanc, Michel IDS

Bogan, Denis NASA

Bohlin, David NASA

Bolton, Scott SCI

Brown, Robert VIMS

Brown, Tyler PDS CN

Brun**,** Jean-Francis ACP

Bunker, Anne RADAR

Burton, Marcia CIRS

Cabane, Michel ACP

Callahan, Phil RADAR

Chin, Greg MSSO

Colombatti, Giacomo HASI

Conner, Diane IO

Cuzzi, Jeff IDS

Dougherty, Michele MAG

Dutta-Roy, Robin DWE

Edberg, Steve JPL

Elachi, Charles RADAR

Eliason, Eric USGS/IMG

Elson, Lee NAIF

Esposito, Larry UVIS

Flasar, Michael CIRS

Fletcher, Greg INMS

French, Dick RSS

Furman, Judy CAPS

Garcia, Patricia USGS/IMG

Gautier, Daniel IDS

Gell, David INMS

Goltz, Gene RSS

Gombosi, Tamas IDS

Gordon, Mitch PDS Rings

Gurnett, Don RPWS

Haberman, John GCMS

Hall, Laverne PDS

Hansen, Candy UVIS

Huber, Lyle PDS/ATM

Ivens, John VIMS

Jouchoux, Alain UVIS

Joy, Steve UCLA/PPI

Judd, David UVIS

Kazeminejad, Bobby Huygens

Kellock, Steve MAG

Kempf, Sascha CDA

Kirk, Randy USGS/IMG

Kliore, Arv RSS

Krimigis, Tom MIMI

Kunde, Virgil CIRS

Kurth, Bill RPWS

LaVoie, Sue JPL, Imaging

Lebreton**,** Jean-Pierre Huygens

Linick, Susan IO

Lorenz, Ralph Huygens

Lunine, Jonathan IDS

Maize, Earl Deputy PM

Matson, Dennis JPL

McCloskey, Rick VIMS

McFarlane, Lisa DISR

Mitchell, Don MIMI

Mitchell, Robert JPL

Nixon, Conor CIRS

Owen, Tobias IDS

Peterson, Joe ISS

Pieri, Leslie ISS

Porco, Carolyn ISS

Rappaport, Nicole RSS

Raulin, Francois IDS

Romani, Paul CIRS

Rye, Elizabeth JPL, Imaging

Sawyer, Don NSSDC

Sesplaukis, Tadas SE

Showalter, Mark PDS

Simpson, Richard PDS Radio Science

Slootweg, Peter MAG

Soderblom, Larry IDS

Southwood, David MAG

Spilker, Linda JPL

Srama, Ralf CDA

Stiles, Bryan RADAR

Strobel, Darrell IDS

Sykes, Mark SBN/DUST

Tingley, Jim CIRS

Waite, Hunter INMS

Walker, Ray UCLA/PPI

Wall, Steve RADAR

Weld, Kathryn JPL

West, Rich RADAR

Witasse, Olivier ESTEC

Young, David CAPS

Zarnecki, John SSP

Zinsmeyer, Charles CAPS

CEL (2)

1 Introduction [1](#introduction)

1.1 Purpose [1](#purpose)

1.2 Scope [1](#__RefHeading___Toc487861036)

1.3 Applicable Documents [1](#applicable-documents)

1.4 Document Change Control [2](#document-change-control)

2 Mission Overview [3](#mission-overview)

3 Science Instruments Overview [4](#science-instruments-overview)

3.1 Cassini Orbiter Science Instruments
[4](#cassini-orbiter-science-instruments)

3.2 Huygens Probe Science Instruments
[5](#huygens-probe-science-instruments)

4 Archive Terms Defined [6](#archive-terms-defined)

5 Cassini Data Volume Estimates [8](#cassini-data-volume-estimates)

5.1 Cassini Orbiter [8](#cassini-orbiter)

5.2 Huygens Probe [8](#huygens-probe)

6 Validation [9](#validation)

6.1 Project Design Peer Review [9](#__RefHeading___Toc487861048)

6.2 PDS Peer Review [9](#pds-peer-review)

6.3 Production Validation [10](#production-validation)

7 Delivery to PDS [10](#delivery-to-pds)

8 Distribution [10](#distribution)

9 Archive Policies, Guidelines and Requirements
[11](#archive-policies-guidelines-and-requirements)

9.1 Policies [11](#policies)

9.2 Guidelines [12](#__RefHeading___Toc487861055)

9.2.1 Designation of Coordinates [12](#designation-of-coordinates)

9.2.2 PDS Label and Index Keywords [13](#pds-label-and-index-keywords)

9.2.3 Standard Designation of Time [14](#standard-designation-of-time)

9.3 Requirements [15](#requirements)

9.3.1 Minimum Science Data Archive [15](#minimum-science-data-archive)

9.3.2 Documentation [16](#__RefHeading___Toc487861061)

9.3.3 Software [16](#__RefHeading___Toc487861062)

9.3.4 PDS High-Level Catalog Files [16](#__RefHeading___Toc487861063)

9.3.5 Filename and Directory name Maximum Lengths
[17](#filename-and-directory-name-maximum-lengths)

9.3.6 Volume Naming [17](#volume-naming)

10 Roles and Responsibilities [18](#__RefHeading___Toc487861066)

10.1 Principal Investigators (PIs), Team Leaders (TLs)
[18](#principal-investigators-pis-team-leaders-tls)

10.2 Interdisciplinary Scientists (IDSs)
[18](#interdisciplinary-scientists-idss)

10.3 Instrument Operations (IO) Program Archive Data Engineer
[18](#instrument-operations-io-program-archive-data-engineer)

10.4 Spacecraft Operations & Navigation
[18](#spacecraft-operations-navigation)

10.5 Planetary Data System (PDS) [19](#planetary-data-system-pds)

10.6 National Space Science Data Center (NSSDC)
[19](#national-space-science-data-center-nssdc)

11 PDS Discipline Nodes Contacts [20](#pds-discipline-nodes-contacts)

12 Cassini Principal Investigators and Team Leaders (PIs/TLs) Archive
Contacts
[21](#cassini-principal-investigators-and-team-leaders-pistls-archive-contacts)

13 Cassini Interdisciplinary Scientists
[22](#cassini-interdisciplinary-scientists)

14 SPICE Archive Contact [22](#spice-archive-contact)

15 PDS Discipline Nodes Responsible for Archiving Data by Instrument
[23](#pds-discipline-nodes-responsible-for-archiving-data-by-instrument)

16 Data Product Levels [24](#data-product-levels)

17 Appendix A: Cassini Science and Ancillary Datasets to be Archived
with PDS by Instrument Teams [25](#__RefHeading___Toc487861079)

18 Appendix B: Archive Delivery Schedule
[32](#appendix-b-archive-delivery-schedule)

19 Appendix C: Acronyms [33](#appendix-c-acronyms)

20 Appendix D: Huygens Data Archive Generation, Validation and Transfer
Plan [35](#__RefHeading___Toc487861082)

# Introduction

## Purpose

This document describes the Cassini / Huygens Program plan for
generating, validating, and delivering data products to the Planetary
Data System (PDS). Included are the policies, guidelines and
requirements that will be followed by instrument teams in the generation
of PDS compliant archives. It provides a high-level description of
science and SPICE datasets, data size estimates, and a delivery schedule
that can be used by the PDS for planning purposes.

A high-level overview of the mission and instrumentation is included to
provide context to the archiving discussion.

[]{#__RefHeading___Toc487861036 .anchor}Scope

This document is applicable to all science and supplementary data
resulting from Cassini Program investigations. The Cassini Program
includes the Cassini (orbiter) and Huygens (probe), which are referred
to in this document collectively as \"Cassini.\" Although the content of
this document applies to both projects, additional details for Huygens
are provided in the Appendix D of this document.

Separate agreements, established through the Cassini Program Science
Group (PSG) and Huygens Science Working Team (HSWT), address data
sharing policies.

Each team\'s data delivery methods are described in team Software
Interface Specifications (SISs).

This document is subordinate to the Cassini Program Data Management Plan
and Science Management Plan.

## Applicable Documents 

The Cassini / Huygens Archive Plan for Science Data (APSD) is responsive
to the following program documents found on-line in the Master
Controlled Document Library at https://cassini.jpl.nasa.gov/mcdl

> a\) Cassini Operations System Functional Requirements Document,
> 699-500-3-GS/R
>
> b\) Cassini Program Science Management Plan (SMP), D-9178, PD 699-006,
> July 1999.
>
> c\) Cassini Program Data Management Plan (PDMP), D-12560, PD 699-061,
> Rev.B, April 1999.
>
> d\) Cassini/Planetary Data System Interface Requirements Document
> (MSO - PDS IRD), PD 699-108, Rev. B, 14 April 1998.
>
> e\) Huygens Data Archive Generation, Validation and Transfer Plan,
> HUY-RSSD-PL-001, DRAFT, June 2004.

The following PDS documentation, that is referred to in this document,
is available on-line from the PDS Website at <http://pds.jpl.nasa.gov/>
.

> f\) Planetary Data System, Data Preparation Workbook, February 17,
> 1995, Version 3.1, JPL D-7669, Part 1
>
> g\) Planetary Data System, Standards Reference, August 1, 2003,
> Version 3.6, JPL D-7669, Part 2
>
> h\) Planetary Science Data Dictionary Document, August 28, 2002, JPL
> D-7116, Rev. E

## Document Change Control 

The APSD is under change control once all parties sign it. All
signatories must approve each published revision. The Appendix A is a
living part of this document. It will be updated periodically and made
available as new products are identified.

# Mission Overview

The Cassini spacecraft is a combined Saturn orbiter and ESA Huygens
Titan atmospheric probe. The orbiter is a three-axis stabilized
spacecraft equipped with twelve instruments. The probe has six
instruments designed to study the atmosphere and surface of Titan.

Cassini was launched on 15 October 1997 using a Titan IV/Centaur launch
vehicle with Solid Rocket Motor Upgrade strap-ons and a Centaur upper
stage. A Venus-Venus-Earth-Jupiter Gravity Assist trajectory was used to
reach Saturn in 6.7 years. Science was limited during the cruise phases
due to restricted spacecraft and instrument flight software capabilities
and cost constraints. Cruise periods were used to check out instrument
operations and gather instrument calibration data. Magnetosphere and
Plasma Science data were collected nearly continuously beginning in
February 2000. Following the Jupiter flyby, the spacecraft was used to
search for gravitational waves using its Ka-band and X-band radio
equipment.

Science activities increased in intensity six months before arriving at
Saturn. On 11 June 2004, just prior to Saturn Orbit Insertion (SOI),
instruments observed the small outer moon Phoebe. During SOI on 1 July
2004 (GMT) the spacecraft will make its closest approach to the
planet\'s surface at an altitude of only 0.3 Saturn radii (18,000 km).
The approximately 90-minute SOI burn required to place Cassini in orbit
around Saturn will be executed earlier than its optimal point centered
around periapsis and instead will end near periapsis. This will allow
science observations to be taken during this unique opportunity to
gather data while passing through the ring plane.

The Huygens probe will be released from the orbiter on 24 December 2004,
(11 days after the second Titan flyby). Two days after the probe is
released the orbiter will perform an orbit deflection maneuver to place
itself on the proper trajectory for the next Titan encounter. At the
third Titan flyby, on 14 January 2005, the probe will descend through
the atmosphere of Titan and relay data to the orbiter for up to 2.5
hours during its descent to the surface. The orbiter will continue to
tour the Saturn system, which includes multiple close Titan flybys for
gravity assists and science acquisition. Targeted and non-targeted
flybys of selected icy satellites will be used to determine surface
compositions and geologic histories. Cassini\'s orbital inclination will
vary widely to facilitate investigations of the field, particle, and
wave environment at high latitudes, including the hypothesized source of
the unique Saturn kilometric radiation. High inclinations also permit
high-latitude Saturn radio occultations, viewing of Saturn\'s polar
regions, and more nearly vertical viewing of Saturn\'s rings. The
baseline mission is scheduled to end mid 2008, for a total mission
duration of 10.7 years.

# Science Instruments Overview

## Cassini Orbiter Science Instruments

The Cassini orbiter hosts twelve science instrument subsystems briefly
described in the table below. CAPS, CDA, and the MIMI LEMMS detector are
capable of some limited articulation independent of the spacecraft
pointing.

  -------- ------------------------- ------------------------------------
  CAPS     Cassini Plasma            in-situ study of plasma within and
           Spectrometer              near Saturn\'s magnetosphere.

  CDA      Cosmic Dust Analyzer      in-situ study of dust grains in the
                                     Saturn system.

  CIRS     Composite Infrared        spectral mapping to study
           Spectrometer              temperature and composition of
                                     surfaces, atmospheres, and rings
                                     within the Saturn system.

  ISS      Imaging Science Subsystem multispectral imaging of Saturn,
                                     Titan, rings, and icy satellites to
                                     observe their properties.

  INMS     Ion and Neutral Mass      in-situ study of compositions of
           Spectrometer              neutral and charged particles within
                                     the Saturn magnetosphere.

  MAG      Magnetometer              study Saturn\'s magnetic field and
                                     interactions with the solar wind.

  MIMI     Magnetospheric Imaging    global magnetospheric imaging and
           Instrument                in-situ measurements of Saturn\'s
                                     magnetosphere and solar wind
                                     interactions.

  RADAR    Radio Detection and       synthetic aperture RADAR (SAR)
           Ranging                   imaging, altimetry, and radiometry
                                     of Titan\'s surface.

  RPWS     Radio and Plasma Wave     study plasma waves, radio emissions,
           Science                   and dust in the Saturn system.

  RSS      Radio Science Subsystem   study atmospheres and ionospheres of
                                     Saturn and Titan, rings, and gravity
                                     fields of Saturn and its satellites.
                                     During cruise, RSS also made
                                     investigations into solar plasma and
                                     relativity, and searched for
                                     gravitational waves.

  UVIS     Ultraviolet Imaging       investigate the chemistry, aerosols,
           Spectrograph              clouds, and energy balance of the
                                     Titan and Saturn atmospheres;
                                     neutrals in the Saturn
                                     magnetosphere; the
                                     deuterium-to-hydrogen ratio for
                                     Titan and Saturn; icy satellite
                                     surface properties; and the
                                     structure and evolution of Saturn\'s
                                     rings.

  VIMS     Visible and Infrared      spectral mapping to study the
           Mapping Spectrometer      composition and structure of
                                     surfaces, atmospheres, and rings.
  -------- ------------------------- ------------------------------------

## Huygens Probe Science Instruments

There are six science instrument subsystems on the Huygens Probe. The
science instruments are listed below along with their measurement
objectives.

  ----------------------------------- -----------------------------------
  ACP Aerosol Collector and Pyrolyser collect aerosols for GCMS to
                                      analyze their chemical
                                      compositions.

  DISR Descent Imager / Spectral      multi-sensor optical instrument
  Radiometer                          capable of imaging and making
                                      spectral measurements over a wide
                                      range of the optical spectrum.

  DWE Doppler Wind Experiment         measures wind direction and
                                      velocity using Probe-Orbiter radio
                                      link.

  GCMS Gas Chromatograph Mass         identifies and quantifies the
  Spectrometer                        abundances of the various
                                      atmospheric constituents.

  HASI Huygens Atmospheric Structure  multi-sensor instrument, intended
  Instrument                          to measure the atmosphere\'s
                                      physical properties, including its
                                      electrical properties.

  SSP Surface Science Package         a suite of simple sensors for
                                      determining the physical properties
                                      of the surface at the impact site
                                      and for providing unique
                                      information on the composition of
                                      the surface material.
  ----------------------------------- -----------------------------------

# Archive Terms Defined

**Ancillary Data** -- Data that are needed to generate calibrated or
resampled data that may come from sources other than the science
instrument.

**Archive** -- An archive consists of one or more datasets along with
all the documentation and ancillary information needed to understand and
use the data. An archive is a logical construct independent of the
medium on which it is stored.

**Archive Medium** - A physical device for storing data such as CD or
DVD. For PDS archives, the medium must be approved by PDS as described
in the PDS Standards Reference.

**Archive System** -- The archive system comprises hardware, software,
procedures, interfaces, and personnel necessary to complete the
archiving of science and ancillary data with the PDS.

**Archive Volume, Archive Volume Set** -- A volume is a unit of medium
on which data products are stored; for example, one CD-ROM. An *archive
volume* is a volume containing all or part of an archive, that is, data
products plus documentation and ancillary files. When an archive spans
multiple volumes, they are called an *archive volume set*.

**Data Product** -- A labeled grouping of data resulting from a
scientific observation. A product label identifies, describes, and
defines the structure of the data. An example of a data product is a
planetary image, a spectrum table, or a time series table accompanied by
its PDS label.

**Dataset** -- An accumulation of data products together with supporting
documentation and ancillary files.

**Data Object** - A data object is that portion of a data product that
contains the actual data. It is described in a data object definition
within a PDS label; it is tangible, and can be physically accessed and
manipulated. For example the data object T142836.DAT could be described
in a PDS label using the following keywords. Additional keywords would
fill in the \"...\" lines.

> \^TABLE = \"T142836.DAT\"
>
> \...
>
> OBJECT = TABLE
>
> ROWS = 1028
>
> \...
>
> END_OBJECT = TABLE

**Metadata** - A label or file that describes one or more science data
objects or products.

**PDS** - Planetary Data System. The primary organization within NASA
responsible for the archive of planetary science data obtained from NASA
sponsored missions. The PDS consists of a Central Node located at JPL
and several Discipline Nodes located around the country.

**SAWG** - The Science Archive Working Group includes instrument teams,
PDS Nodes, and Project representatives. The group is chartered to
coordinate the archive system development and coordinate production.

**Science Data** -- All data acquired that are used to accomplish
primary science goals of the Cassini Orbiter and Huygens Probe science
teams.

**SIS** -- Software Interface Specification. Describes the volume
organization, data file structures, label contents, and operational
procedure for delivering data archives.

**Standard Data Product** -- A data product that has been defined that
is contractually required by the PI or TL as part of the investigation.
Standard data products are generated in a predefined way, using
well-understood procedures, and processed in \"pipeline\" fashion.

# Cassini Data Volume Estimates

## Cassini Orbiter

[Raw Science Downlinked Data Volume:]{.underline}

Full Mission Success:  95% of the data transmitted from the spacecraft
is received on the ground.

Calculations are rounded, and assume one 9-hour pass per day, and full
mission success as described above.

**Prime Mission (1643 days):**

X-Band, 30% passes to 70-m antenna (4Gbit/pass) total 2060 Gbits

X-Band, 70% passes to 34-m antenna (1Gbit/pass) total 1045 Gbits

**Extended Mission (730 days):**

X-Band, 30% passes to 70-m antenna (4Gbit/pass) total 915 Gbits

X-Band, 70% passes to 34-m antenna (1Gbit/pass) total 465 Gbits

[Dataset Volume Estimates:]{.underline}

**Prime Mission:**

Cassini Capability in Science Phase Prime Mission (Jan 2004 -- Jul 2008)

> 3 Tbits of raw telemetry data based upon prime mission downlink
> capability

    From Cassini Data Archive Plan:  (26.1 Tbits + 2.1 Tbits RSS**)**
**= 28.2** **Tbits** total

    TLM Expansion factor = 26/3 = 8.6

**Extended Mission:**

Cassini Capability in Science Phase Extended Mission (Jul 2008 -- July
2010)

    If that data were reduced as before (same expansion factor):

1.3 Tb raw telemetry data based upon extended mission downlink
capability

(1.3 \* 8.6) = 11.6 Tbits + 1.1 Tbits RSS = **12.7** **Tbits**

Grand total for the primary and extended missions : **40.9 Tbits**

Recommend PDS size their system to accept, at a minimum, **41**
**Tbits** of data from the Cassini prime and extended missions.

## Huygens Probe

The raw data volume for Huygens is approximately 173.1 Mbits. The
reduced data volume has not been calculated.

# Validation

This section describes the validation process for Cassini Orbiter
datasets. Huygens probe dataset validation is described in appendix D.

There are pre-production and production validation activities.
Pre-production validation includes a project design peer review,
followed by a PDS peer review. Production validation for science
usability is best achieved through science data analysis using the
archive products. Production validation for format includes built in
quality control to ensure archives comply with the Software Interface
Specification (SIS).

## Project Design Peer Review

The project design peer review provided an assessment of instrument
archive designs and allowed instruments to proceed with production
software design. Ray Walker, the PDS PPI Node Manager, chaired the
review. Other members included representatives from instrument teams,
science teams, and PDS. Requests for action were gathered and responded
to.

The review board was asked to evaluate designs to determine if:

1\. List of data products identified for archive was complete.

2\. Calibration methods are understood.

> 3\. Mission consistent attributes are used in data labels. For
> example: time, latitude, longitude, coordinate systems, and reference
> frames.

4\. Data labels provide the information necessary to narrow searches on
data products.

5\. Validation process is described and specifically assigns
responsibilities. 

6\. Delivery mechanism is understood.

7\. Liens are identified with resolution plans.

## PDS Peer Review

The PDS Discipline Node (DN) assigned to an instrument team coordinates
and leads a peer review of a sample volume. Members of the PSG will be
asked to participate in peer reviews as well as members of the science
community outside the PSG. The peer review is used to ensure the archive
contains all the components needed to perform science analysis, and is
prepared as documented in the Software Interface Specification (SIS).
The PDS DN documents all liens and their closures.

Success Criteria:

1.  All liens are resolved and the SIS is updated as necessary and
    signed.

2.  The supporting documentation is comprehensive and complete to
    support science analysis.

3.  Calibration and other data processing algorithms are provided in a
    way that ensures data access and algorithms can be implemented in
    future programming languages and computing environments.

4.  If calibrated data are not provided, sample calibrated data must be
    provided for users to verify correct implementation of algorithm(s).

## Production Validation

Each team in coordination with the PDS DN will develop the validation
process used during production of datasets and document their validation
plan in their SIS. Production validation for science usability through
data use is encouraged. PDS will provide teams with tools as needed for
validating products for PDS compliance. The PDS DN will hold peer
reviews as necessary.

# Delivery to PDS

Cassini orbiter archive datasets will be provided to PDS by the
instrument teams either electronically or on physical media as
negotiated between individual instrument teams, the program archive data
engineer and the PDS. The agreed to delivery method and volume
organization will be documented in Software Interface Specifications
(SISs). The delivery schedule for all level 1A & level 1B (CODMAC 2 & 3)
is defined in appendix B of this document.

Please refer to appendix D for the Huygens PDS transfer plan.

# Distribution

PDS archives will be accessible to the public on-line. The PDS on-line
system will provide search filters, such as time range or target name,
so that a user can retrieve data that meet specific search criteria. Map
coordinate based searches will be supported as appropriate for
higher-level products. Data will be made available via electronic
transfer or on physical media. The NSSDC will be responsible for
replication and distribution of large volumes of data on appropriate
physical media.

# Archive Policies, Guidelines and Requirements

Archive policies, guidelines and requirements have been developed to
ensure data products meet PDS standards and support collaborative
studies among Cassini Orbiter and Huygens Probe data.

## Policies

1)  Cassini is committed to archiving data products as summarized in
    Section 9.3.1 of this document.

2)  Instrument teams will produce archives that adhere to the PDS
    standards version specified in their SISs.

3)  Each instrument team will be assigned to one primary PDS science
    discipline node to design and deliver its archives. Primary nodes
    should ensure the requirements of the secondary PDS science
    discipline node are met.

4)  Data distribution will be done by PIs, TLs, or IDSs through their
    science team interfaces or the PDS after archives are released.

5)  Cassini orbiter production pipelines will be complete and validated
    by March 2005, unless specifically approved otherwise by the
    project.

6)  SPICE files that are used in the processing of archive products may
    be included on archive volumes, but are not required if they are the
    standard products produced and delivered to the program database. If
    SPICE files are used in processing that are not delivered to the
    program database then those files must be included on instrument
    archive volumes.

7)  

8)  Although not required, higher-level products developed by PIs, TLs,
    and IDSs may be archived with the PDS, if resources are available to
    do so. Cassini recognizes those higher-level products are valuable
    and should be preserved, however funding restrictions may preclude
    the complete archiving of these products.

9)  Cassini will provide a regular forum for discussing archive progress
    and issues with the PDS, PIs, and TLs.

[]{#__RefHeading___Toc487861055 .anchor}Guidelines

### Designation of Coordinates 

A global reference system for a given body consists of several elements.
These may include a) a cartographic coordinate system, b) a specified
reference surface and its dimensions, and c) orientation information for
the coordinate system.

The International Astronomical Union (IAU) and International Association
of Geodesy (IAG) sponsor a "Working Group on Cartographic Coordinates
and Rotational Elements of the Planets and Satellites" which sets
standards in this area. The latest version of their recommendations is
available as Seidelmann, et al., Celestial Mechanics and Dynamical
Astronomy, 82, pp. 83-110, 2002.

For all planetary bodies, the IAU allows two possible types of
coordinate systems, planetocentric and planetographic, (ibid, pp.
100-101). In both systems, the origin is the center of mass of the body
in question. The rotational pole of the body which lies on the north
side of the invariable plane of the solar system (the ecliptic) will be
called north, and northern latitudes will be designated as positive.

The planetocentric coordinate system is a right-hand spherical
coordinate system in which latitude is defined as the angle between a
vector passing through the origin of the spherical coordinate system and
the equator, and longitude is the angle between the vector and the plane
of the prime meridian measured in an eastern direction. Although this
system is consistent with right hand coordinates commonly used to
formulate physical problems, historical astronomers used a system in
which longitude increased with time.

The Cassini Mission will continue the tradition established through
historic telescopic observations. A planetographic system will be used.
The longitude in such a system is specified so that the longitude of the
central meridian, as observed from a fixed direction in inertial space,
will increase with time, and range from 0º to 360º. This results in
longitudes being measured positively to the west when the body's
rotation is prograde, and to the east when the body's rotation is
retrograde. Jupiter, Saturn and all satellites rotate in the prograde
sense; therefore, all longitudes will be West Longitude.

According to the IAU, a planetographic system requires a reference
surface and the latitude is specified for a point on the reference
surface as the angle between the equatorial plane and the normal to the
reference surface at that point. Either a sphere or rotational ellipsoid
is used. The WG notes that some bodies (e.g., Io, Mimas, Enceladus, and
Miranda) could be well represented by a triaxial ellipsoid, but in
practice a sphere will be used due to computational difficulties.
Likewise for computational convenience a sphere is often used for
irregularly shaped bodies.

The IAU has not defined East Longitude for the Giant Planets and
traditionally either planetographic (based on the local normal) or
planetocentric (a spherical coordinate system) latitude has been used
with West Longitude. Thus, For Jupiter and Saturn, depending on the
observational goals, either a spherical or an ellipsoidal reference
surface with given equatorial and polar radii will be used and indexes
will include both centric and graphic latitudes.

In order to specify the orientation of a planetary body at a given
instant, the WG provides recommended equations which specify the
position of the body's celestial pole (in right ascension and
declination at the epoch J2000.0), and the orientation on its axis, by
W, the angle along the equator to the east between the prime meridian
and the equator's intersection with the celestial equator.

The prime meridian itself can be specified in several ways. Where
possible it is specified by defining the longitude of the center of some
small surface feature near the body's equator. If a body is tidally
locked to its parent body, the prime meridian is usually that longitude
passing through the average sub-planetary (parent body) point. If a body
has no fixed surface features, the equation for W is chosen so as to
define an arbitrary prime meridian.

The reference radius (for a spherical reference surface) or reference
equatorial and polar radii (for an ellipsoidal reference surface) will
be included in the labels of data from remote sensing instruments. The
reference radius should be included in MAPS labels where range is
expressed in radii. Currently recommended (mean) radii and reference
ellipsoidal radii, and definitions for orientation are available in the
latest NAIF CASSINI PCK file. These are initially the IAU/IAG WG
recommended values but may be updated as the mission progresses. The
location of the prime meridian for each body is defined by the equation
for the value of W, unless fixed surface features have been identified
in the past. For such bodies a named crater and its defined longitude
are specified in the IAU/IAG WG report (Table 2, footnotes).

Ring coordinates are given in terms of radius from Saturn's center of
mass in kilometers and longitude measured in degrees from 0 to 360 in
the celestial reference frame at J2000.0 (the ICRF). Radii are measured
from the center of the planet along the nominal ring plane. The inertial
longitude of a ring feature is measured relative to the ring prime
meridian (different from Saturn's prime meridian) where the ring prime
meridian passes through the ascending node of the Saturn\'s invariable
plane (equivalent to the equatorial plane in this case) on the celestial
equator at J2000.0. Longitudes are measured in the direction of orbital
motion along the Saturn\'s invariable plane to the ring\'s ascending

node, and thence along the ring plane.

### PDS Label and Index Keywords

PDS labels and index files provide searchable keys and describe
characteristics of the products. Index files are used to populate the
PDS search catalog. PDS requested keywords for index files are detailed
in TBD. If it is not possible for Cassini to provide values for keywords
due to funding limitations, then the keywords will be included with NULL
values.

### Standard Designation of Time 

There should be a consistent representation of time used in filenames,
directory names, labels, and index files.

The time of data acquisition (written to memory or telemetry stream)
should be expressed as spacecraft UTC (coordinated universal time) or
Earth UTC for Radio Science data. Other representations of time may also
be included in labels and index files. In the case of in-situ instrument
data, if the instrument samples are filtered (digital, analog, or both)
or averaged, the magnitude of the filters/average delays (may be
telemetry rate dependent) should be described in the dataset
documentation. Raw data that are sampled synchronously with the
spacecraft clock should also contain the spacecraft clock value (SCLK).
SCLK values are irrelevant if the instrument sampling is asynchronous,
(as is the case for MAG), or nonexistent (as is the case for RSS).

If data files are in binary format, and the overhead of including a
21-byte time tag increases the file storage requirements beyond reason
(doubles the size), then an 8-byte binary floating-point representation
of the Ephemeris Time (Barycentric Dynamical Time) consistent with the
output of the SPICE Toolkit UTC2ET function is an acceptable
alternative. These values can be converted back to the ASCII format by
using the SPICE Toolkit function ET2UTC with the appropriate string
format specification.

Format descriptions:

The Cassini UTC system format formation rule is:
YYYY-DDDThh:mm:ss\[.fff\]

Spacecraft clock count (SCLK) format is NNNNNNNNNN.NNN

## Requirements

### Minimum Science Data Archive

Cassini is committed to archiving full resolution uncalibrated data
products, calibration files, algorithms for applying calibration, and
sample calibrated data. See Appendix A of this document for the list of
orbiter products and Appendix D for the list of probe products planned
for archive.

Below is a summary of the science data archive requirement specified in
Cassini Operations System Functional Requirements Document,
699-500-3-GS/R.

Instrument teams shall produce validated PDS compliant science data
archives that contain:

-   Uncalibrated full resolution data

-   Calibration files

-   Algorithms for applying calibration and any other data processing
    which is critical to use the data.

-   Sample calibrated data files for future users to verify their
    application of calibration algorithms.

-   Metadata as specified by PDS Standards.

-   Documentation that describes the instrument and dataset and
    anomalies that affect the archive data products.

-   A searchable index that provides access to data products (at a
    minimum, this implies access through a simple set of keys, such as
    data source identification, data product type, time, geometry, or
    target).

Note: The Instrument Operations (IO) team generates data products for
VIMS, ISS, RS, and RADAR Facility Instruments. IO produces data products
according to TL-approved Software Interface Specifications (SISs) and
Operational Interface Agreements (OIAs). TLs are encouraged to negotiate
with IO to use PDS formats for these products. TLs are responsible for
archive volume generation and validation. TLs will be required to
reformat products to PDS standards if IO creates products that are not
PDS compliant.

#### Raw Telemetry Data

There is no plan to archive raw telemetry data with PDS other than what
is required for Radio Science. Cassini Mission Science and Support
Operations (MSSO) Office has a requirement to store raw telemetry data
that includes engineering, science and housekeeping packets in the form
of raw telemetry frames through End-of-Mission + 1 year.

#### Higher Level Science Data Products

PI and TL teams and Interdisciplinary Scientists (IDSs) generate
higher-level science products. Although not contractually required, it
is expected that higher-level data products developed by PIs, TLs, and
IDSs in the course of doing their data analysis will be archived with
the PDS. Cassini recognizes that higher-level products are valuable and
should be preserved; therefore, a joint effort between Cassini and PDS
will be made to facilitate the generation of such products in PDS
compliant formats, thereby minimizing any additional effort that might
occur in accomplishing this objective.

#### Public Release Data Products

Public released products will be generated in accordance with
Cassini/JPL/NASA policies and procedures for public information and
press releases. All press release products will be archived with the PDS
by the data producers.

#### SPICE Data Products and Toolkit

The Instrument Operations Team is responsible for generating the archive
of SPICE datasets. Final versions of SPICE (SPK, PCK, IK, FK, CK, EK,
SCLK, and LSK) files will be archived by the PDS NAIF node in big-endian
IEEE binary and text formats, as appropriate, with accompanying
documentation. The SPICE toolkit will always be available on line from
the NAIF node of the PDS, for all platforms supported by NAIF, including
MAC, PC/Windows, PC/Linux, and Sun/Solaris. Copies of each toolkit
version are delivered to the NSSDC.

### Documentation

Documentation relevant to understanding the archive will be delivered to
PDS. At a minimum documentation should include:

a)  Software Interface Specifications (SISs) that define the format and
    content of data files and volume organization.

b)  Calibration and data processing algorithms necessary to use the
    data.

c)  Instrument catalog file that describes the instrument capabilities
    and operations (INST.CAT).

d)  Dataset description files (DATASET.CAT).

e)  References to publications that are relevant to the data (REF.CAT).

f)  Listing of personnel involved in the dataset generation (PERS.CAT).

### Software

It is expected that standard data products delivered by the PI or TL
will be in a format that is accessible by other users. If the products
cannot be accessed using commonly available software tools, then the
products should be accompanied by software, source code, and
documentation or detailed algorithms that allow a user to access the
data.

### PDS High-Level Catalog Files

PDS high-level catalog files will be included in the CATALOG directory
of archive volumes, as defined in JPL D-7669, Planetary Data System
Standards Reference. High-level catalog files include Mission,
Instrument Host, Instrument, Dataset, Reference, and Personnel catalog
files.

IO provided a draft version of the Mission, Instrument Host, and Mission
Reference files to PDS for catalog ingestion at SOI-1 year. Updates to
these files will be provided at least every two years if new information
is available. Final versions will be provided no later than two months
prior to end of mission.

Archive producers will provide Instrument, Dataset, Personnel, and
Reference catalog files with their archive submissions. The Cassini
Archive Coordinator will generate team specific reference files with
input from science teams.

The Cassini Project Archive Coordinator will maintain the mission
reference catalog file that includes references found in the MISSION.CAT
file.

Keyword Values defined for the mission that should be used in PDS
objects include:

**MISSION_NAME** = \"CASSINI-HUYGENS\"

**INSTRUMENT_HOST_ID** = \"CO\"

**INSTRUMENT_HOST_NAME** = \"CASSINI ORBITER\"

**MISSION_ALIAS_NAME** = \"CASSINI\"

**INSTRUMENT_HOST_ID** = \"HP\"

**INSTRUMENT_HOST_NAME** = \"HUYGENS PROBE\"

**MISSION_ALIAS_NAME** = \"HUYGENS\"

Keyword values for INSTRUMENT_ID and INSTRUMENT_NAME are as follows:

  ------------------- --------------- ----------------------------------------------------
  **INSTRUMENT_ID**                   **INSTRUMENT_NAME**

  CAPS                                CASSINI PLASMA SPECTROMETER

  CDA                                 COSMIC DUST ANALYZER

  CIRS                                COMPOSITE INFRARED SPECTROMETER

  INMS                                ION AND NEUTRAL MASS SPECTROMETER

  ISSNA                               IMAGING SCIENCE SUBSYSTEM NARROW ANGLE

  ISSWA                               IMAGING SCIENCE SUBSYSTEM WIDE ANGLE

  MAG                                 MAGNETOMETER

  MIMI                                MAGNETOSPHERIC IMAGING INSTRUMENT

  RADAR                               RADAR

  RPWS                                RADIO AND PLASMA WAVE SCIENCE

  RSS                                 RADIO SCIENCE SUBSYSTEM

  UVIS                                ULTRAVIOLET IMAGIN SPECTROGRAPH

  VIMS                                VISUAL AND INFRARED MAPPING SPECTROMETER

  ACP                 AEROSOL         
                      COLLECTOR       
                      PYROLYSER       

  DISR                DESCENT IMAGER  
                      / SPECTRAL      
                      RADIOMETER      

  DWE                 DOPPLER WIND    
                      EXPERIMENT      

  GCMS                GAS             
                      CHROMATOGRAPH   
                      MASS            
                      SPECTROMETER    

  HASI                HUYGENS         
                      ATMOSPHERIC     
                      STRUCTURE       
                      INSTRUMENT      

  SSP                 SURFACE SCIENCE 
                      PACKAGE         
  ------------------- --------------- ----------------------------------------------------

### Filename and Directory name Maximum Lengths

Filenames will adhere to ISO 9660 level 2 specifications that allow the
total filename length of 31 characters.

### Volume Naming

The following is a constant that shall be used across the Cassini
mission.

VOLUME_SERIES_NAME = \"MISSION TO SATURN\"

Volume IDs can contain up to 11 characters and shall use the following
convention:

COIIII_NNNN, for orbiter data.

HPIIII_NNNN, for probe data.

Where :

> CO = Cassini Orbiter
>
> HP = Huygens Probe
>
> IIII = Instrument acronyms up to 4 characters in length (CAPS, CDA,
> CIRS, INMS, ISS, MAG, MIMI, RADR, RPWS, RSS, UVIS, VIMS, ACP, DISR,
> DWE, GCMS, HASI, SSP)
>
> NNNN = volume number

# Roles and Responsibilities

g)  
h)  
i)  
j)  

## 

## 

## 

## 

  ------------------ -- ----------------------------------------------------
                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        

                        
  ------------------ -- ----------------------------------------------------

# 

# Principal Investigators (PIs), Team Leaders (TLs)

The following responsibilities apply:

a)  Works directly with assigned PDS Discipline Nodes to define dataset
    content and format. (Discipline Nodes have expertise in archiving
    specific types of data and will help define file formats, keywords
    and standard values for keywords in metadata such as a dataset
    description file and data product label files.)

b)  Provides PDS with datasets that include data products (includes
    labels), other metadata that include Instrument, Dataset, Reference,
    and Personnel high-level catalog files, and ancillary data necessary
    to understand the data.

c)  Provides PDS with archive science datasets that are validated for
    science content and PDS format compliance with documentation,
    calibration and other data processing algorithms that ensure data
    access. (The list of these datasets can be found in Appendix A)

d)  Participates in Science Archive Working Group (SAWG) Meetings.

e)  Participates in peer reviews.

f)  Reports archive status to Instrument Operations (IO) by providing
    metadata that details submissions to PDS.

## Interdisciplinary Scientists (IDSs) 

a)  Archives any significant new science data products and associated
    metadata and supplementary products created from the investigation.
    These will likely be higher-level products and few in number. IDSs
    will inform the Cassini Archive Coordinator of archive plans.

b)  Participates in peer reviews.

## Instrument Operations (IO) Program Archive Data Engineer

a)  Coordinates archive dataset design and production schedule.

b)  Maintains the Archive Plan for Science Data (699-068).

c)  Participates in peer reviews.

d)  Acts as agent between PDS, Project and PI and TL when necessary to
    resolve PDS format and delivery issues.

e)  Leads the Science Archive Working Group (SAWG) Meetings.

f)  Receives metadata describing archive submissions from instruments.

g)  Tracks and reports archive status to program weekly.

h)  Produces and validates SPICE data product archive as specified in
    Appendix A.

i)  Produces Mission, Instrument Host, and reference catalog files and
    provide to PDS.

## Spacecraft Operations & Navigation

Generate and validate certain SPICE data products as specified in
Appendix A. Assist IO in identifying the files that should be included
in the SPICE archive.

## Planetary Data System (PDS) 

[Central Node (CN):]{.underline}

a)  Coordinates the definition and production of the archives and
    ensures they are compatible with PDS standards.

b)  Maintains a database of all PDS holdings, which will be updated
    after Cassini archive volumes have completed the peer review
    process.

c)  Makes archive volumes available to the science community.

d)  Provides archive volume validation tools, consultation, and review
    of validation reports.

e)  Provides PDS training and instruction to archive volume producers.

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f)  Participates in Science Archive Working Group (SAWG) Meetings.

g)  Provides copies of archive volumes to the NSSDC.

[Lead Node(LN)]{.underline}

a)  Coordinates interactions between instrument teams and specific
    discipline nodes.

b)  Monitors the development of Cassini data base of PDS holdings and
    ensures its completion by the DNs.

c)  Ensures consistency across nodes with regard to data formats,
    labels, indexes, documentation, and calibration practices.

d)  Participates in peer reviews, monitors progress, and works with
    participants as needed to resolve issues.

e)  Designs PDS Master index. Validates that SIS\'s provide data to
    populate.

[Primary Science Discipline Nodes (DN):]{.underline}

a)  Works with archive producers to define archive format and content.

b)  Leads peer reviews.

c)  Maintain archive of released Cassini products for access by the
    science community.

d)  Provides additional archive volume validation tools as needed.

e)  Participates in Science Archive Working Group (SAWG) Meetings.

f)  Produces physical volumes, if negotiated with team to do so.

## National Space Science Data Center (NSSDC) 

NSSDC ensures the long-term preservation of data. The NSSDC is also be
responsible for filling large delivery orders to the science community,
and making data available to foreign investigators, educators, and the
general public.

# PDS Discipline Nodes Contacts

+-----------------------------+---------+-------------------+---------+
| PDS Node                    | Contact | Email             | Phone   |
|                             |         |                   | Number  |
+=============================+=========+===================+=========+
| Central Node (CN)           | Steven  | Steven.A          | \(818\) |
|                             | Adams   | dams@jpl.nasa.gov | 3       |
| JPL, Pasadena, CA           |         |                   | 54-2624 |
+-----------------------------+---------+-------------------+---------+
| Atmospheres Node (ATM)      | Lyle    | Lhuber@NMSU.edu   | \(505\) |
|                             | Huber   |                   | 6       |
| New Mexico State            |         | Rbeebe@nmsu.edu   | 46-1862 |
| University, Las Cruces, NM  | Reta    |                   |         |
|                             | Beebe   |                   | \(505\) |
|                             |         |                   | 6       |
|                             |         |                   | 46-1938 |
+-----------------------------+---------+-------------------+---------+
| Geosciences Node (GEO)      | Ray     | arvidson          | \(314\) |
|                             | A       | @wunder.wustl.edu | 9       |
| Washington University, St.  | rvidson |                   | 35-5609 |
| Louis, MO                   |         |                   |         |
+-----------------------------+---------+-------------------+---------+
| USGS Imaging Subnode        | Lisa    | lgaddis@usgs.gov  | \(928\) |
| (IMG/USGS)                  | Gaddis  |                   | 5       |
|                             |         | pgarcia@usgs.gov  | 56-7053 |
| Flagstaff, AZ               | Patty   |                   |         |
|                             | Garcia  |                   | \(928\) |
|                             |         |                   | 5       |
|                             |         |                   | 56-7246 |
+-----------------------------+---------+-------------------+---------+
| JPL Imaging Subnode         | Sue     | Susan.K.La        | \(818\) |
| (IMG/JPL)                   | Lavoie  | Voie@jpl.nasa.gov | 3       |
|                             |         |                   | 54-5677 |
| JPL, Pasadena, CA           | Rafael  | Rafael.Al         |         |
|                             | Alanis  | anis@jpl.nasa.gov | \(818\) |
|                             |         |                   | 3       |
|                             |         |                   | 54-8959 |
+-----------------------------+---------+-------------------+---------+
| Planetary Plasma            | Ray     | rwal              | \(310\) |
| Interactions Node (PPI)     | Walker  | ker@igpp.ucla.edu | 8       |
|                             |         |                   | 25-7685 |
| University of California,   | Steve   | s                 |         |
| Los Angeles, CA             | Joy     | joy@igpp.ucla.edu | \(310\) |
|                             |         |                   | 8       |
|                             |         |                   | 25-3506 |
+-----------------------------+---------+-------------------+---------+
| Rings Node (RINGS)          | Mark    | showalter@ring    | \(650\) |
|                             | Sh      | side.arc.nasa.gov | 6       |
| Ames Research Center,       | owalter |                   | 04-3382 |
| Moffet Field, CA            |         | mgordon@          |         |
|                             | Mitch   | mail.arc.nasa.gov | \(650\) |
|                             | Gordon  |                   | 6       |
|                             |         |                   | 04-2529 |
+-----------------------------+---------+-------------------+---------+
| Small Bodies Node (SBN),    | Mark    | syk               | \(520\) |
| Dust Subnode                | Sykes   | es@as.arizona.edu | 6       |
|                             |         |                   | 21-5381 |
| University of Arizona,      |         |                   |         |
|                             |         |                   |         |
| Tucson, AZ                  |         |                   |         |
+-----------------------------+---------+-------------------+---------+
| Navigation and Ancillary    | Lee     | Lee.E             | \(818\) |
| Information Facility (NAIF) | Elson   | lson@jpl.nasa.gov | 3       |
|                             |         |                   | 54-4223 |
| JPL, Pasadena, CA           |         |                   |         |
+-----------------------------+---------+-------------------+---------+
| Radio Science Subnode (RS)  | Dick    | rsimpson@mage     | \(650\) |
| \*                          | Simpson | llan.stanford.edu | 7       |
|                             |         |                   | 23-3525 |
| Stanford University,        |         |                   |         |
| Stanford, CA                |         |                   |         |
+-----------------------------+---------+-------------------+---------+

\* through September 2004

# Cassini Principal Investigators and Team Leaders (PIs/TLs) Archive Contacts

+-------------+-----------+-------------------+----------+-----------+
| **I         | **I       | **Email**         | **Phone  | **PI or   |
| nstrument** | nstrument |                   | Number** | TL**      |
|             | Team      |                   |          |           |
|             | Archive   |                   |          |           |
|             | R         |                   |          |           |
|             | epresenta |                   |          |           |
|             | tive(s)** |                   |          |           |
+=============+===========+===================+==========+===========+
| CAPS        | Charles   | CZ                | \(210\)  | David     |
|             | Zinsmeyer | insmeyer@swri.edu | 522-5018 | Young, PI |
| Cassini     |           |                   |          |           |
| Plasma      | Judy      | jfurman@swri.edu  | \(210\)  |           |
| S           | Furman    |                   | 522-6040 |           |
| pectrometer |           |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+
| CDA         | Sascha    | Sascha.Ke         | 49 6221  | Ralf      |
|             | Kempf     | mpf@mpi-hd.mpg.de | 51 6247  | Srama, PI |
| Cosmic Dust |           |                   |          |           |
| Analyzer    |           |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+
| CIRS        | Conor     | nixon@cirs        | \(301\)  | Michael   |
|             | Nixon     | rss.gsfc.nasa.gov | 286-6757 | Flasar,   |
| Composite   |           |                   |          | PI        |
| Infrared    | Jim       | James.S.Ting      | \(301\)  |           |
| S           | Tingley   | ley@gsfc.nasa.gov | 286-4980 |           |
| pectrometer |           |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+
| INMS        | Greg      | gfletch@umich.edu | \(734\)  | Hunter    |
|             | Fletcher  |                   | 763-8182 | Waite, TL |
| Ion and     |           | gellda@umich.edu  |          |           |
| Neutral     | Dave Gell |                   | \(734\)  |           |
| Mass        |           |                   | 763-6221 |           |
| S           |           |                   |          |           |
| pectrometer |           |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+
| ISS         | Leslie    | L                 | \(830\)  | Carolyn   |
|             | Pieri     | eslie@ciclops.org | 693-8955 | Porco, TL |
| Imaging     |           |                   |          |           |
| Science     | Ben       | kn                | \(720\)  |           |
| Subsystem   | Knowles   | owles@ciclops.org | 974-5852 |           |
|             |           |                   |          |           |
|             | Josh      | josh@ ciclops.org | \(720\)  |           |
|             | Riley     |                   | 974-5856 |           |
+-------------+-----------+-------------------+----------+-----------+
| MAG         | Nick      | n.achille         | 44 207   | Michele   |
|             | Achilleos | os@imperial.ac.uk | 594 7759 | D         |
| M           |           |                   |          | ougherty, |
| agnetometer | Steve     | s.kello           | 44 207   | PI        |
|             | Kellock   | ck@imperial.ac.uk | 594 7760 |           |
+-------------+-----------+-------------------+----------+-----------+
| MIMI        | Don       | Don.Mi            | \(240\)  | Tom       |
|             | Mitchell  | tchell@jhuapl.edu | 228-5981 | Krimigis, |
| Mag         |           |                   |          | PI        |
| netospheric | Thomas    | Ar                | \(785\)  |           |
| Imaging     | Armstrong | mstrong@FTECS.com | 840-0800 |           |
| Instrument  |           |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+
| RADAR       | Bryan     | Bryan.St          | \(818\)  | Charles   |
|             | Stiles    | iles@jpl.nasa.gov | 354-5329 | Elachi,   |
|             |           |                   |          | TL        |
|             | Rich West | Richard.D.        | \(818\)  |           |
|             |           | West@jpl.nasa.gov | 354-6025 |           |
|             | Randy     |                   |          |           |
|             | Kirk      | rkirk@usgs.gov    | \(520\)  |           |
|             |           |                   | 556-7020 |           |
+-------------+-----------+-------------------+----------+-----------+
| RPWS        | Bill      | willia            | \(319\)  | Don       |
|             | Kurth     | m-kurth@uiowa.edu | 335-1926 | Gurnett,  |
| Radio and   |           |                   |          | PI        |
| Plasma Wave |           |                   |          |           |
| S           |           |                   |          |           |
| pectrometer |           |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+
| RSS         | Op        | Elias.Barb        | \(818\)  | Arv       |
|             | erations: | inis@jpl.nasa.gov | 393-0661 | Kliore,   |
| Radio       |           |                   |          | TL        |
| Science     | Elias     | Gene.G            | \(818\)  |           |
| Subsystem   | Barbinis  | oltz@jpl.nasa.gov | 393-1142 |           |
|             |           |                   |          |           |
|             | Gene      | rfre              | \(781\)  |           |
|             | Goltz     | nch@wellesley.edu | 283-3747 |           |
|             |           |                   |          |           |
|             | Science:  |                   |          |           |
|             |           |                   |          |           |
|             | Dick      |                   |          |           |
|             | French    |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+
| UVIS        | David     | David.Judd@       | \(303\)  | Larry     |
|             | Judd      | lasp.colorado.edu | 492-8582 | Esposito, |
| Ultraviolet |           |                   |          | PI        |
| Imaging     |           |                   |          |           |
| S           |           |                   |          |           |
| pectrograph |           |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+
| VIMS        | Rick      | rick              | \(520\)  | Robert    |
|             | McCloskey | m@lpl.arizona.edu | 626-3255 | Brown, TL |
| Visual and  |           |                   |          |           |
| Infrared    | John      | jiven             | \(520\)  |           |
| Mapping     | Ivens     | s@lpl.arizona.edu | 621-7301 |           |
| S           |           |                   |          |           |
| pectrometer |           |                   |          |           |
+-------------+-----------+-------------------+----------+-----------+

##  {#section-5 .unnumbered}

# Cassini Interdisciplinary Scientists 

  ------------------------------------------------------------------------------------
  **Discipline**           **Name**         **Email**                  **Phone
                                                                       Number**
  ------------------------ ---------------- -------------------------- ---------------
  Solar Wind               Darrell F.       strobel@jhu.edu            \(410\)
                           Strobel                                     516-7829

  Atmospheres              Tobias C. Owen   owen@ifa.hawaii.edu        \(808\)
                                                                       956-8007

  Magnetospheres/Plasma    Michel Blanc     blanc@obs-mip.fr           33 561 33 2948
  Physics                                                              

  Rings                    Jeffrey N. Cuzzi jcuzzi@mail.arc.nasa.gov   650
                                                                       604-6343/5524

  Magnetospheres/Plasma    Tamas I. Gombosi tamas@umich.edu            \(734\)
  Physics                                                              764-7222

  Satellites               Laurence A.      lsoderblom@usgs.gov        \(928\)
                           Soderblom                                   556-7018
  ------------------------------------------------------------------------------------

# SPICE Archive Contact

+-----------+----------------------------+-----------------------------+
| **        | **Team**                   | **Archive Representative**  |
| Dataset** |                            |                             |
+===========+============================+=============================+
| SPICE     | SAUL/IO                    | Diane Conner                |
|           |                            |                             |
|           | Science and Uplink Office  | Diane.Conner@jpl.nasa.gov   |
|           | / Instrument Operations    |                             |
|           | Element                    | \(818\) 354-8586            |
+-----------+----------------------------+-----------------------------+

# PDS Discipline Nodes Responsible for Archiving Data by Instrument

Instrument teams submit archives to the primary nodes for distribution
within the PDS and to NSSDC.

+--------------+----------------+-------------------------------------+
| **           | **Primary      | **Secondary Node**                  |
| Instrument** | Node**         |                                     |
+==============+================+=====================================+
| CAPS         | PPI            | N/A                                 |
+--------------+----------------+-------------------------------------+
| CDA          | Small Bodies   | Rings, PPI                          |
+--------------+----------------+-------------------------------------+
| CIRS         | Atmospheres    | Rings                               |
+--------------+----------------+-------------------------------------+
| INMS         | PPI            | Atmospheres                         |
+--------------+----------------+-------------------------------------+
| ISS          | Imaging / JPL  | Rings, Geosciences, Atmospheres     |
+--------------+----------------+-------------------------------------+
| MAG          | PPI            | N/A                                 |
+--------------+----------------+-------------------------------------+
| MIMI         | PPI            | Atmospheres                         |
+--------------+----------------+-------------------------------------+
| RADAR        | Imaging/ USGS  | Geosciences, Rings                  |
+--------------+----------------+-------------------------------------+
| RPWS         | PPI            | N/A                                 |
+--------------+----------------+-------------------------------------+
| RSS          | Radio Science  | All                                 |
|              | subnode        |                                     |
+--------------+----------------+-------------------------------------+
| UVIS         | Atmospheres    | Rings                               |
+--------------+----------------+-------------------------------------+
| VIMS         | Imaging / JPL  | Rings, Atmospheres                  |
+--------------+----------------+-------------------------------------+
| SPICE        | NAIF           |                                     |
+--------------+----------------+-------------------------------------+
| Huygens      | Atmospheres    | Geosciences                         |
|              |                |                                     |
| ACP          |                |                                     |
|              |                |                                     |
| DISR         |                |                                     |
|              |                |                                     |
| DWE          |                |                                     |
|              |                |                                     |
| GCMS         |                |                                     |
|              |                |                                     |
| HASI         |                |                                     |
|              |                |                                     |
| SSP          |                |                                     |
+--------------+----------------+-------------------------------------+

# Data Product Levels

There is no official reference for the NASA product level descriptions.
The source for the NASA product level descriptions found below was taken
from a Mars project archive plan. CODMAC descriptions were taken from
the \"Issues and Recommendations Associated with Distributed Computation
and Data Management Systems for Space Sciences\", Committee on Data
Management and Computation Space Science Board Commission on Physical
Sciences, Mathematics, and Resources National Research Council,
PB88-1884466, 1986.

+----------+----------------------------------------+------------------+
| **NASA   | **Product Description**                | **CODMAC         |
| Levels** |                                        | Equivalent**     |
+----------+----------------------------------------+------------------+
| Raw      | Telemetry data stream as received at   | Level 1 -- Raw   |
|          | the ground station, with science and   | Data             |
|          | engineering data embedded.             |                  |
+----------+----------------------------------------+------------------+
| Level 0  | Instrument science data (e.g., raw     | Level 2 --       |
|          | voltages, counts) at full resolution,  | Edited Data      |
|          | time ordered, with duplicates and      |                  |
|          | transmission errors removed.           |                  |
+----------+----------------------------------------+------------------+
| Level 1A | Level 0 data that have been located in | Level 3 --       |
|          | space and may have been **reversibly** | Calibrated       |
|          | transformed (e.g., calibrated,         |                  |
|          | rearranged) in a reversible manner and |                  |
|          | packaged with needed ancillary and     |                  |
|          | auxiliary data (e.g., radiances with   |                  |
|          | the calibration equations applied). No |                  |
|          | resampling.                            |                  |
+----------+----------------------------------------+------------------+
| Level 1B | **Irreversibly** transformed (e.g.,    | Level 3 --       |
|          | resampled, remapped, calibrated)       | Calibrated       |
|          | values of the instrument measurements  |                  |
|          | (e.g., radiances magnetic field        | Level 4 --       |
|          | strength).                             | Resampled data   |
+----------+----------------------------------------+------------------+
| Higher   | Geophysical parameters mapped into     | Level 5 --       |
| levels   | uniform space time grids.              | Derived data     |
+----------+----------------------------------------+------------------+
|          |                                        | Level 6 --       |
|          |                                        |                  |
|          |                                        | Ancillary Data   |
+----------+----------------------------------------+------------------+

+-------------------+--------------------------------------------------+
| **CODMAC          | **CODMAC Description**                           |
| Equivalent**      |                                                  |
+-------------------+--------------------------------------------------+
| Level 1 -- Raw    | Telemetry data with data embedded.               |
| Data              |                                                  |
+-------------------+--------------------------------------------------+
| Level 2 -- Edited | Corrected for telemetry errors and split or      |
| Data              | decommutated into a dataset for a given          |
|                   | instrument. Sometimes called Experimental Data   |
|                   | Record. Data are also tagged with time and       |
|                   | location of acquisition.                         |
+-------------------+--------------------------------------------------+
| Level 3 --        | Edited data that are still in units produced by  |
| Calibrated        | instrument, but that have been corrected so that |
|                   | values are expressed in or are proportional to   |
|                   | some physical unit such as radiance. No          |
|                   | resampling, so edited data can be reconstructed. |
+-------------------+--------------------------------------------------+
| Level 4 --        | Data that have been resampled in the time or     |
| Resampled data    | space domains in such a way that the original    |
|                   | edited data cannot be reconstructed. Could be    |
|                   | calibrated in addition to being resampled.       |
+-------------------+--------------------------------------------------+
| Level 5 --        | Derived results, as maps, reports, graphics,     |
| Derived data      | etc. NASA Levels 2 through 5.                    |
+-------------------+--------------------------------------------------+
| Level 6 --        | Non-science data needed to generate calibrated   |
|                   | or resampled datasets. Consists of instrument    |
| Ancillary Data    | gains, offsets; pointing information for scan    |
|                   | platforms, etc                                   |
+-------------------+--------------------------------------------------+

Appendix A: Cassini Science and Ancillary Datasets to be archived with
PDS by Instrument Teams

The Appendix A will be periodically updated to add or modify products as
needed then posted for electronic access on the Cassini archive web
site.

<table>
<colgroup>
<col style="width: 2%" />
<col style="width: 12%" />
<col style="width: 19%" />
<col style="width: 7%" />
<col style="width: 5%" />
<col style="width: 6%" />
<col style="width: 6%" />
<col style="width: 6%" />
<col style="width: 6%" />
<col style="width: 7%" />
<col style="width: 20%" />
</colgroup>
<thead>
<tr class="header">
<th> </th>
<th><strong>Standard_data_product_id</strong></th>
<th><strong>Science Data Product Description</strong></th>
<th><strong>Product Specification ID (SIS)</strong></th>
<th><strong>CODMAC Level</strong></th>
<th><strong>PDS Format IMG, etc..</strong></th>
<th><strong>Prime PDS Node interface</strong></th>
<th><strong>Producer</strong></th>
<th><strong>Supplier to PDS</strong></th>
<th><strong>Estimated Data Set Size</strong></th>
<th><strong>Data Set ID</strong></th>
</tr>
</thead>
<tbody>
<tr class="odd">
<td>1</td>
<td>CAPS_ACT</td>
<td>Actuator Data Files</td>
<td>IO-AR-017</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>132MB/Year = 528 MB</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>2</td>
<td>CAPS_ELS</td>
<td>Electron sensor data</td>
<td>IO-AR-017</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>9.3GB/Year = 37.1 GB</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>3</td>
<td>CAPS_ANC</td>
<td>Ancillary information</td>
<td>IO-AR-017</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>138MB/Year = 550 MB</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>4</td>
<td>CAPS_IBS</td>
<td>Ion Beam sensor data</td>
<td>IO-AR-017</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>32GB/Year =</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>5</td>
<td>CAPS_IMS_EVN</td>
<td>IMS event data</td>
<td>IO-AR-017</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>??</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>6</td>
<td>CAPS_IMS_LOG</td>
<td>Ion Mass logicals</td>
<td>IO-AR-017</td>
<td>27</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>4.2GB/Year = 16.7 GB</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>7</td>
<td>CAPS_IMS_SNG</td>
<td>Ion Mass singles</td>
<td>IO-AR-017</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>5GB/Year= 20 GB</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>8</td>
<td>CAPS_IMS_ION</td>
<td>Ion Mass Ion data</td>
<td>IO-AR-017</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>137GB/Year= 548 GB</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>9</td>
<td>CAPS_IMS_TOF</td>
<td>Ion Mass Time of Flight data</td>
<td>IO-AR-017</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>J. Furman</td>
<td>J. Furman</td>
<td>485MB/Year = 2 GB</td>
<td>CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>10</td>
<td>CDA_PNT</td>
<td>J2000 Pointing vector of instrument as a function of time when CDA
is on</td>
<td>IO-AR-012</td>
<td>3</td>
<td>table</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>4 GB</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="odd">
<td>11</td>
<td>CDA_CAL_AREA</td>
<td>The sensitive area of the CDA impact detector (IID) and chemical
analyser (CAT) is tabulated as a function of the incident angle with
respect to the instrument axis.</td>
<td>IO-AR-012</td>
<td>3</td>
<td>table</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>10 KB</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="even">
<td>12</td>
<td>CDA_STAT</td>
<td>Cassini mission and CDA configuration, tests and other events.
Records are triggered by change in status affecting the sensitivity of
the different CDA instruments and mission events that may affect the
interpretation of the data.</td>
<td>IO-AR-012</td>
<td>3</td>
<td>table</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>300 MB</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="odd">
<td>13</td>
<td>CDA_DA_IMP</td>
<td>Detector responses and derived quantities from the Cassini dust
detector as well as spacecraft geometry information for reliable
impacts.</td>
<td>IO-AR-012</td>
<td>3</td>
<td>table</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>10 GB</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="even">
<td>14</td>
<td>CDA_MS_PEAKS</td>
<td>Time-of-flight mass spectra peaks for individual impact events.</td>
<td>IO-AR-012</td>
<td>3</td>
<td>table</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>1 GB</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="odd">
<td>15</td>
<td>CDA_MS_SPECTRA</td>
<td>Time-of-flight mass spectra for individual impacts, identified by
their unique identifier number xxxxxx</td>
<td>IO-AR-012</td>
<td>3</td>
<td>table</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>1 GB</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="even">
<td>16</td>
<td>CDA_CAL_SET</td>
<td>Table of voltages corresponding to voltage level codes and Coulomb
threshold settings.</td>
<td>IO-AR-012</td>
<td>3</td>
<td>tables</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>20 KB</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="odd">
<td>17</td>
<td>CDA_DA_CTR</td>
<td>CDA impact counter time history file.</td>
<td>IO-AR-012</td>
<td>6</td>
<td>table</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>1 GB</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="even">
<td>18</td>
<td>CDA_HRD</td>
<td>HRD data and ancillary files - HRD takes data only during Saturn
ring plane crossings</td>
<td>IO-AR-012</td>
<td>3</td>
<td>table</td>
<td>SBN</td>
<td>S. Kempf</td>
<td>S. Kempf</td>
<td>TBD</td>
<td>CO-D-CDA-3/4/5-DUST-V1.0</td>
</tr>
<tr class="odd">
<td>19</td>
<td>CIRS_IHSK</td>
<td>Resampled (interpolated) housekeeping data</td>
<td>IO-AR-002, IO-AR-003</td>
<td>3</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>3.5 MB/mon=<br />
168 MB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="even">
<td>20</td>
<td>CIRS_GEO</td>
<td>spacecraft orientation w.r.t. target, sun</td>
<td>IO-AR-002, IO-AR-003</td>
<td>2</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>41 MB/mon = 2.0 GB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="odd">
<td>21</td>
<td>CIRS_HSK</td>
<td>Housekeeping Data</td>
<td>IO-AR-002, IO-AR-003</td>
<td>2</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>18.5 MB/mon = 890 MB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="even">
<td>22</td>
<td>CIRS_IFGM</td>
<td>uncompressed, raw interferogram data</td>
<td>IO-AR-002, IO-AR-003</td>
<td>2</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>682 MB/mon= 32.7 GB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="odd">
<td>23</td>
<td>CIRS_OBS</td>
<td>observation parameters</td>
<td>IO-AR-002, IO-AR-003</td>
<td>2</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>1 MB/mon = 48 MB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="even">
<td>24</td>
<td>CIRS_POI</td>
<td>pointing information for detectors on target</td>
<td>IO-AR-002, IO-AR-003</td>
<td>2</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>236 MB/mon=11.3 GB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="odd">
<td>25</td>
<td>CIRS_RIN</td>
<td>pointing information for detectors on rings</td>
<td>IO-AR-002, IO-AR-003</td>
<td>2</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>200 MB/mon= 9.6 GB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="even">
<td>26</td>
<td>CIRS_AIFM</td>
<td>averaged reference interferograms (deep space, warm shutter)</td>
<td>IO-AR-002, IO-AR-003</td>
<td>4</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>42.5 MB/mon =<br />
2.0 GB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="odd">
<td>27</td>
<td>CIRS_ISPM</td>
<td>Calibrated individual spectra</td>
<td>IO-AR-002, IO-AR-003</td>
<td>4</td>
<td>table</td>
<td>Atmos</td>
<td>CIRS</td>
<td>CIRS PI</td>
<td>500 MB/mon = 24 GB</td>
<td>CO-S-CIRS-2/4-TSDR-V1.0</td>
</tr>
<tr class="even">
<td>28</td>
<td>INMS_SCI</td>
<td>Science data, counts/sec</td>
<td>IO-AR-016</td>
<td>2</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>1600 MB</td>
<td>CO-EJS-INMS-2-SCI-U-V1.0</td>
</tr>
<tr class="odd">
<td>29</td>
<td>INMS_HKG</td>
<td>Housekeeping in engineering units</td>
<td>IO-AR-016</td>
<td>2</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>90 MB</td>
<td>CO-EJS-INMS-2-HKG-U-V1.0</td>
</tr>
<tr class="even">
<td>30</td>
<td>INMS_OSI</td>
<td>Operations tables</td>
<td>IO-AR-016</td>
<td>2</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>10 MB</td>
<td>CO-EJS-INMS-2-OSI-U-V1.0</td>
</tr>
<tr class="odd">
<td>31</td>
<td>INMS_EVT</td>
<td>Event times</td>
<td>IO-AR-016</td>
<td>2</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>TBD</td>
<td>CO-EJS-INMS-2-EVT-U-V1.0</td>
</tr>
<tr class="even">
<td>32</td>
<td>INMS_SMD</td>
<td>Science memory dump</td>
<td>IO-AR-016</td>
<td>2</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>TBD</td>
<td>CO-EJS-INMS-2-SMD-U-V1.0</td>
</tr>
<tr class="odd">
<td>33</td>
<td>INMS_HMD</td>
<td>Housekeeping memory dump</td>
<td>IO-AR-016</td>
<td>2</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>TBD</td>
<td>CO-EJS-INMS-2-HMD-U-V1.0</td>
</tr>
<tr class="even">
<td>34</td>
<td>INMS_CNT</td>
<td>Science data, spectra with ancillary data</td>
<td>IO-AR-016</td>
<td>3</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>TBD</td>
<td>CO-EJS-INMS-3-CNT-C-V1.0</td>
</tr>
<tr class="odd">
<td>35</td>
<td>INMS_SPC</td>
<td>Science data, species</td>
<td>IO-AR-016</td>
<td>5</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>TBD</td>
<td>CO-EJS-INMS-5-SPC-C-V1.0</td>
</tr>
<tr class="even">
<td>36</td>
<td>INMS_MSS</td>
<td>Science data, mass spectra</td>
<td>IO-AR-016</td>
<td>5</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>TBD</td>
<td>CO-EJS-INMS-5-MSS-C-V1.0</td>
</tr>
<tr class="odd">
<td>37</td>
<td>INMS_TTN</td>
<td>Science data, titan atmospheric profiles</td>
<td>IO-AR-016</td>
<td>5</td>
<td>table</td>
<td>PPI</td>
<td>INMS</td>
<td>INMS</td>
<td>TBD</td>
<td>CO-EJS-INMS-5-TTN-C-V1.0</td>
</tr>
<tr class="even">
<td>38</td>
<td>ISS_EDR</td>
<td>Raw, uncalibrated images</td>
<td>DOIS-002, IO-AR-005</td>
<td>2</td>
<td>IMG</td>
<td>Imaging (JPL)</td>
<td>IO/MIPL</td>
<td>ISS TL</td>
<td>650 GB</td>
<td>CO-S-ISSNA/ISSWA-2-EDR-V1.0,<br />
CO-J-ISSNA/ISSWA-2-EDR-V1.0</td>
</tr>
<tr class="odd">
<td>39</td>
<td>ISS_CAL</td>
<td>Calibration files, sample calibrated images</td>
<td>IO-AR-005</td>
<td>3</td>
<td>IMG, algorithms, software</td>
<td>Imaging (JPL)</td>
<td>ISS/CICLOPS</td>
<td>ISS TL</td>
<td>TBD</td>
<td>CO-X-ISSNA/ISSWA-2-CAL-V1.0</td>
</tr>
<tr class="even">
<td>40</td>
<td>MAG_FGM</td>
<td>L1A fluxgate magnetometer data (duplicates removed, gaps filled,
idiosyncrasies of onboard data processing unit fixed, data separated
into files by type) 75 GB (combined size of FGM, VHM, SHM, CON, ANA,
ERR, CMD, CHATT, CHUSR data)</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td>75 GB (combined size of FGM, VHM, SHM, CON, ANA, ERR, CMD, CHATT,
CHUSR data)</td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="odd">
<td>41</td>
<td>MAG_VHM</td>
<td>L1A vector helium magnetometer data</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td> </td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="even">
<td>42</td>
<td>MAG_SHM</td>
<td>L1A scalar helium magnetometer data</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td> </td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="odd">
<td>43</td>
<td>MAG_CON</td>
<td>L1A configuration image data</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td> </td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="even">
<td>44</td>
<td>MAG_ANA</td>
<td>L1A analog housekeeping data</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td> </td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="odd">
<td>45</td>
<td>MAG_ERR</td>
<td>L1A error counter data</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td> </td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="even">
<td>46</td>
<td>MAG_CMD</td>
<td>L1A command validation data</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td> </td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="odd">
<td>47</td>
<td>MAG_CHATT</td>
<td>L1A Cassini attitude data</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td> </td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="even">
<td>48</td>
<td>MAG_CHUSR</td>
<td>L1A engineering data from a user-selected set of channels</td>
<td>IO-AR-020</td>
<td>2</td>
<td>Time series binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td> </td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="odd">
<td>49</td>
<td>MAG_CAL</td>
<td>Calibration files</td>
<td>IO-AR-020</td>
<td>2</td>
<td>binary TABLE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td>500 MB</td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="even">
<td>50</td>
<td>MAG_SW</td>
<td>software to convert L1A to L1B</td>
<td>IO-AR-020</td>
<td>6</td>
<td>TEXT, binary FILE</td>
<td>PPI</td>
<td>MAG</td>
<td>MAG PI</td>
<td>500 MB</td>
<td>CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0</td>
</tr>
<tr class="odd">
<td>51</td>
<td>MAPS_KEY_PARAMETERS</td>
<td>MAPS instruments key parameters dataset - may contain plots and
model data</td>
<td>IO-AR-004</td>
<td>4</td>
<td>ascii</td>
<td>PPI</td>
<td>MAPS Instrument teams</td>
<td>Univ of Michigan</td>
<td>28 GB</td>
<td><p>CO-V/E/J/S/SS-RPWS-4-SUMM-KEY60S-V1.0</p>
<p>CO-V/E/J/S/SS-MAG-4-SUMM-KEY60S-V1.0</p>
<p>CO-V/E/J/S/SS-MIMI-4-SUMM-KEY-5MIN-V1.0</p>
<p>CO-V/E/J/S/SS-CAPS-5-DDR-KEY-5MIN-V1.0</p>
<p>CO-S-INMS-5-DDR-KEY-5MIN-V1.0</p></td>
</tr>
<tr class="even">
<td>52</td>
<td>MIMI_CHEMS_PHA</td>
<td>CHEMS Pulse Height Analysis data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td>450 MB / Day Maximum = 722 GB</td>
<td>CO-E/J/S-MIMI-2-CHEMS-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>53</td>
<td>MIMI_CHEMS_ACC</td>
<td>CHEMS accumulation rate data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td>7 MB / Day Maximum = 12 GB</td>
<td>CO-E/J/S-MIMI-2-CHEMS-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>54</td>
<td>MIMI_CHEMS_SCI</td>
<td>CHEMS science rate data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td> </td>
<td>CO-E/J/S-MIMI-2-CHEMS-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>55</td>
<td>MIMI_INCA_PHA</td>
<td>INCA Pulse Height Analysis data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td>300 MB / Day Maximum = 482 GB</td>
<td>CO-E/J/S-MIMI-2-INCA-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>56</td>
<td>MIMI_INCA_RAT</td>
<td>INCA accumulation rate data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td>4 MB / Day Maximum = 6.5 GB</td>
<td>CO-E/J/S-MIMI-2-INCA-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>57</td>
<td>MIMI_INCA_IMG</td>
<td>INCA image data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td>110 MB / Day Maximum = 177 GB</td>
<td>CO-E/J/S-MIMI-2-INCA-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>58</td>
<td>MIMI_LEMMS_PHA</td>
<td>LEMMS Pulse Height Analysis data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td>30 MB / Day Maximum = 49 GB</td>
<td>CO-E/J/S-MIMI-2-LEMMS-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>59</td>
<td>MIMI_LEMMS_ACC</td>
<td>LEMMS accumulation rate data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td>35 MB / Day Maximum = 57 GB</td>
<td>CO-E/J/S-MIMI-2-LEMMS-UNCALIBRATED-V1.0</td>
</tr>
<tr class="even">
<td>60</td>
<td>MIMI_LEMMS_FRT</td>
<td>LEMMS fine accumulation rate data</td>
<td>IO-AR-006</td>
<td>2</td>
<td>ASCII</td>
<td>PPI</td>
<td>MIMI</td>
<td>MIMI PI</td>
<td> </td>
<td>CO-E/J/S-MIMI-2-LEMMS-UNCALIBRATED-V1.0</td>
</tr>
<tr class="odd">
<td>61</td>
<td>RADAR_SBDR</td>
<td>Short Burst Data Record. Time ordered tabular data records including
engineering telemetry, spacecraft geometry, calibrated science data
(radiometry, scatterometry, and altimetry) and associated meta data.
Also includes time-ordered SAR metadata.</td>
<td>DORA-001<br />
DORA-002</td>
<td>3</td>
<td>table</td>
<td><a href="#RANGE!_ftn1">Imaging</a></td>
<td>IO/RADAR</td>
<td>Radar TL</td>
<td>1100 MB</td>
<td>CO-V/E/J/S-RADAR-3-SBDR-V1.0</td>
</tr>
<tr class="even">
<td>62</td>
<td>RADAR_LBDR</td>
<td>Same as RADAR_SBDR with addition of sample radar echo data for each
burst.</td>
<td>DORA-001<br />
DORA-002</td>
<td>3</td>
<td>table</td>
<td><a href="#RANGE!_ftn1">Imaging</a></td>
<td>IO/RADAR</td>
<td>Radar TL</td>
<td>44000 MB</td>
<td>CO-V/E/J/S-RADAR-3-LBDR-V1.0</td>
</tr>
<tr class="odd">
<td>63</td>
<td>RADAR_ABDR</td>
<td>Same as RADAR_SBDR with addition of altimeter profile vector (range
compressed echo data) for each burst.</td>
<td>DORA-001<br />
DORA-002</td>
<td>3</td>
<td>table</td>
<td><a href="#RANGE!_ftn1">Imaging</a></td>
<td>IO/RADAR</td>
<td>Radar TL</td>
<td>4800 MB</td>
<td>CO-SSA-3-ABDR-V1.0</td>
</tr>
<tr class="even">
<td>64</td>
<td>RADAR_BIDR</td>
<td>Basic Image Data Record. SAR data correlated, resampled to oblique
cylindrical grid (different projection for each swath), looks summed.
Includes latitude, longitude, incidence angle, and beam mask
back-planes.</td>
<td>DORA-002<br />
DORA-003</td>
<td>5</td>
<td>IMG</td>
<td>Imaging</td>
<td>IO/RADAR</td>
<td>Radar TL</td>
<td>5600 MB</td>
<td>CO-SSA-RADAR-5-BIDR-V1.0</td>
</tr>
<tr class="odd">
<td>65</td>
<td>RADAR_PRDR</td>
<td>Calibrated &amp; gridded radiometer data</td>
<td>IO-AR-012<br />
IO-AR-018</td>
<td>5</td>
<td>IMG</td>
<td>Imaging</td>
<td>USGS</td>
<td>Radar TL</td>
<td>300 MB</td>
<td>CO-SSA-RADAR-5-PRDR-V1.0</td>
</tr>
<tr class="even">
<td>66</td>
<td>RADAR_PSDR</td>
<td>Calibrated &amp; gridded scatterometer data</td>
<td>IO-AR-012<br />
IO-AR-018</td>
<td>5</td>
<td>IMG</td>
<td>Imaging</td>
<td>USGS</td>
<td>Radar TL</td>
<td>300 MB</td>
<td>CO-SSA-RADAR-5-PSDR-V1.0</td>
</tr>
<tr class="odd">
<td>67</td>
<td>RADAR_GRDR</td>
<td>Mosaicked radiometer data</td>
<td><p>IO-AR-012</p>
<p>IO-AR-018</p></td>
<td>5</td>
<td>IMG</td>
<td>Imaging</td>
<td>USGS</td>
<td>Radar TL</td>
<td>100 MB</td>
<td>CO-SSA-RADAR-5-GRDR-V1.0</td>
</tr>
<tr class="even">
<td>68</td>
<td>RADAR_MIDR</td>
<td>Mosaicked SAR image data</td>
<td>IO-AR-012<br />
IO-AR-018</td>
<td>5</td>
<td>IMG</td>
<td>Imaging</td>
<td>USGS</td>
<td>Radar TL</td>
<td>6500 MB</td>
<td>CO-SSA-RADAR-5-MIDR-V1.0</td>
</tr>
<tr class="odd">
<td>69</td>
<td>RADAR_RIDR</td>
<td>Multilook SAR "cubes"</td>
<td>IO-AR-012<br />
IO-AR-018</td>
<td>5</td>
<td>IMG</td>
<td>Imaging</td>
<td>USGS</td>
<td>Radar TL</td>
<td>50 MB</td>
<td>CO-SSA-RADAR-5-RIDR-V1.0</td>
</tr>
<tr class="even">
<td>70</td>
<td>RADAR_DTM</td>
<td>Digital Topographic Models (DTMs)</td>
<td>IO-AR-012<br />
IO-AR-018</td>
<td>5</td>
<td>IMG</td>
<td>Imaging</td>
<td>USGS</td>
<td>Radar TL</td>
<td>10 MB</td>
<td>CO-SSA-RADAR-5-DTM-V1.0</td>
</tr>
<tr class="odd">
<td>71</td>
<td>RPWS_KEY_PARAMETERS</td>
<td>spectral information as a function of time</td>
<td>IO-AR-019</td>
<td>4</td>
<td>ascii</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>4 GB</td>
<td>CO-V/E/J/S/SS-RPWS-4-SUMM-KEY60S-V1.0</td>
</tr>
<tr class="even">
<td>72</td>
<td>RPWS_ANCIL</td>
<td>Description of RPWS IEBs</td>
<td>IO-AR-019</td>
<td>6</td>
<td>ascii</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>&lt;1 MB</td>
<td>CO-V/E/J/S/SS-RPWS-4-SUMM-KEY60S-V1.0,<br />
CO-V/E/J/S/SS-RPWS-2-REFDR-ALL-V1.0,<br />
CO-V/E/J/S/SS-RPWS-3-RDR-LRFULL-V1.0,<br />
CO-V/E/J/S/SS-RPWS-2-REFDR-WBRFULL-V1.0,<br />
CO-V/E/J/S/SS-RPWS-2-REFDR-WFRFULL-V1.0</td>
</tr>
<tr class="odd">
<td>73</td>
<td>RPWS_RAW_COMPLETE</td>
<td>Raw telemetry data, edited</td>
<td>IO-AR-019</td>
<td>2</td>
<td>BINARY</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>65 GB</td>
<td>CO-V/E/J/S/SS-RPWS-2-REFDR-ALL-V1.0</td>
</tr>
<tr class="even">
<td>74</td>
<td>RPWS_WIDEBAND_FULL</td>
<td>Wideband Full Resolution Uncalibrated</td>
<td>IO-AR-019</td>
<td>2</td>
<td>Time Series</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>10 GB</td>
<td>CO-V/E/J/S/SS-RPWS-2-REFDR-WBRFULL-V1.0</td>
</tr>
<tr class="odd">
<td>75</td>
<td>RPWS_WAVEFORM_FULL</td>
<td>Waveform Full Resolution Uncalibrated</td>
<td>IO-AR-019</td>
<td>2</td>
<td>Time Series</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>10 GB</td>
<td>C0-V/E/J/S/SS-RPWS-2-REFDR-WFRFULL-V1.0</td>
</tr>
<tr class="even">
<td>76</td>
<td>RPWS_LOW_RATE_FULL</td>
<td>Low Rate Full Resolution Calibrated</td>
<td>IO-AR-019</td>
<td>3</td>
<td>Time Series</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>65 GB</td>
<td>CO-V/E/J/S/SS-RPWS-3-RDR-LRFULL-V1.0</td>
</tr>
<tr class="odd">
<td>77</td>
<td>RPWS_LOW_RATE_BROWSE</td>
<td>Low Rate Browse</td>
<td>IO-AR-019</td>
<td>3</td>
<td>PNG</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>6.5 GB</td>
<td>CO-V/E/J/S/SS-RPWS-3-RDR-LRFULL-V1.0</td>
</tr>
<tr class="even">
<td>78</td>
<td>RPWS_WIDEBAND_BROWSE</td>
<td>Wideband Browse</td>
<td>IO-AR-019</td>
<td>2</td>
<td>PNG</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>1 GB</td>
<td>CO-V/E/J/S/SS-RPWS-2-REFDR-WBRFULL-V1.0</td>
</tr>
<tr class="odd">
<td>79</td>
<td>RPWS_WAVEFORM_BROWSE</td>
<td>Waveform Browse</td>
<td>IO-AR-019</td>
<td>2</td>
<td>PNG</td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>1 GB</td>
<td>C0-V/E/J/S/SS-RPWS-2-REFDR-WFRFULL-V1.0</td>
</tr>
<tr class="even">
<td>80</td>
<td>RPWS_SP</td>
<td>Special Data Sets</td>
<td>IO-AR-019</td>
<td>4+</td>
<td></td>
<td>PPI</td>
<td>RPWS</td>
<td>RPWS</td>
<td>1 GB</td>
<td>C0-V/E/J/S/SS-RPWS-4-SP-V1.0</td>
</tr>
<tr class="odd">
<td>81</td>
<td>RSS_ATMOS_OCCULT</td>
<td>complex signal amplitude A(f,r,lambda,t) for frequency f at ring
plane (model-independent quantity)radius r, longitude lambda, and time t
(direct ray) (model-independent quantity)Fresnel scale Fr(f,r,lambda,t)
(model-independent quantity)range to ring intercept pt of center of beam
R(t) (model-independent quantity)transverse and radial velocity
components of direct ray (model-independent quantity)normal and slant
path optical depth tau(f,r,lambda,t) at multiple resolutions (derived
quantities)Spectrograms of scattered signal as function of time (derived
quantities)</td>
<td>IO-AR-022</td>
<td>5</td>
<td></td>
<td>RS Subnode</td>
<td>Radio Science Team (RST)</td>
<td>RST</td>
<td>N/A</td>
<td>CO-X-RSS-5-EXP-V1.0</td>
</tr>
<tr class="even">
<td>82</td>
<td>RSS_GRAV_FIELDS</td>
<td>frequency residuals vs time (model-independent quantity)<br />
<br />
covariance matrix (derived)<br />
<br />
reconstructed trajectory vs time (derived)</td>
<td>IO-AR-022</td>
<td>5</td>
<td></td>
<td>RS Subnode</td>
<td>Radio Science Team (RST)</td>
<td>RST</td>
<td>N/A</td>
<td>CO-X-RSS-5-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>83</td>
<td>RSS_RING_OCCULT</td>
<td>complex signal amplitude A(f,r,lambda,t) for frequency f at ring
plane radius r, longitude lambda, and time t (direct
ray)(model-independent quantity)Fresnel scale
Fr(f,r,lambda,t)(model-independent quantity)range to ring intercept pt
of center of beam R(t)(model-independent quantity)transverse and radial
velocity components of direct ray(model-independent quantity)normal and
slant path optical depth tau(f,r,lambda,t) at multiple resolutions
(derived quantities)Spectrograms of scattered signal as function of
time(derived quantities)</td>
<td>IO-AR-022</td>
<td>5</td>
<td></td>
<td>RS Subnode</td>
<td>Radio Science Team (RST)</td>
<td>RST</td>
<td>N/A</td>
<td>CO-X-RSS-5-EXP-V1.0</td>
</tr>
<tr class="even">
<td>84</td>
<td>RSS_SC_GWE</td>
<td>sky frequency at 1 sec interval (90% level of completeness) for each
observed frequency [1GB ascii file for 40 days of obs]</td>
<td>IO-AR-022</td>
<td>5</td>
<td></td>
<td>RS Subnode</td>
<td>Radio Science Team (RST)</td>
<td>RST</td>
<td>N/A</td>
<td>CO-X-RSS-5-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>85</td>
<td>RSS_ODF</td>
<td>Closed-loop Orbit Data File (ODF); Doppler, range, and ramps</td>
<td>DSN-001<br />
IO-AR-021</td>
<td>4</td>
<td>Binary</td>
<td>RS Subnode</td>
<td>RMDCT</td>
<td>RST</td>
<td>2 GB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="even">
<td>86</td>
<td>RSS_EOP</td>
<td>EOP – Earth Orientation Parameters File</td>
<td>DSN-004<br />
IO-AR-021</td>
<td>6</td>
<td>ASCII</td>
<td>RS Subnode</td>
<td>TSAC</td>
<td>RST</td>
<td>250 MB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>87</td>
<td>RSS_MCF</td>
<td>MCF - Media Calibration Files</td>
<td>DSN-005<br />
IO-AR-021</td>
<td>6</td>
<td>ASCII</td>
<td>RS Subnode</td>
<td>TSAC</td>
<td>RST</td>
<td>2 MB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="even">
<td>88</td>
<td>RSS_PDD</td>
<td>[Advanced Media Calibration System] Path Delay Data (PDD)</td>
<td>DSN-005<br />
IO-AR-021</td>
<td>6</td>
<td>ASCII</td>
<td>RS Subnode</td>
<td>IO-RS</td>
<td>RST</td>
<td>1 GB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>89</td>
<td>RSS_ATDF</td>
<td>Closed-loop Archival Tracking Data File (ATDF); Doppler, range, and
ramps</td>
<td>DSN-023<br />
IO-AR-021</td>
<td>2</td>
<td>Binary</td>
<td>RS Subnode</td>
<td>Radio Metric Data Conditioning Team (RMDCT)</td>
<td>RST</td>
<td>10 GB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="even">
<td>90</td>
<td>RSS_TDAF</td>
<td>Closed Tracking Data Archival File (TDAF); up-link and downlink
carrier and range phase</td>
<td>DSN-025<br />
IO-AR-021</td>
<td>1 ,2,3,4</td>
<td>Binary</td>
<td>RS Subnode</td>
<td>Tracking Data Delivery Subsystem (TDDS)</td>
<td>RST</td>
<td>3 GB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>91</td>
<td>RSS_RSR</td>
<td>Open-loop Radio Science Data (ODS), from RSR; digitized signal</td>
<td><p>DSN-026</p>
<p>IO-AR-021</p></td>
<td>1</td>
<td>Binary</td>
<td>RS Subnode</td>
<td>IO-RS *</td>
<td>RST</td>
<td>200 GB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="even">
<td>92</td>
<td>RSS_MON</td>
<td>Mission Monitor Data</td>
<td>DSN-027<br />
IO-AR-021</td>
<td>6</td>
<td>ASCII</td>
<td>RS Subnode</td>
<td>IO-RS</td>
<td>RST</td>
<td>13 GB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>93</td>
<td>RSS_HGA_CAL</td>
<td>High Gain Antenna (HGA) Boresight Alignment reports</td>
<td>IO-AR-021</td>
<td>6</td>
<td>ASCII</td>
<td>RS Subnode</td>
<td>IO-RS</td>
<td>RST</td>
<td>N/A</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="even">
<td>94</td>
<td>RSS_HGA_PAT</td>
<td>High Gain Antenna (HGA) Pattern reports</td>
<td>IO-AR-021</td>
<td>6</td>
<td>ASCII</td>
<td>RS Subnode</td>
<td>IO-RS</td>
<td>RST</td>
<td>N/A</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>95</td>
<td>RSS_USO_CAL</td>
<td>Ultrastable Oscillator Characterization reports</td>
<td>IO-AR-021</td>
<td>6</td>
<td>ASCII</td>
<td>RS Subnode</td>
<td>IO-RS</td>
<td>RST</td>
<td>N/A</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="even">
<td>96</td>
<td>RSS_CK</td>
<td>C-Kernel</td>
<td><p>NAV-005</p>
<p>IO-AR-021</p></td>
<td>6</td>
<td>Binary</td>
<td>RS Subnode</td>
<td>SCO</td>
<td>RST</td>
<td>1 GB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>97</td>
<td>RSS_SPK</td>
<td>SP-Kernel; spacecraft and planetary ephemeredes</td>
<td><p>NAV-009</p>
<p>IO-AR-021</p></td>
<td>6</td>
<td>Binary</td>
<td>RS Subnode</td>
<td>SCO</td>
<td>RST</td>
<td>400 MB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="even">
<td>98</td>
<td>RSS_TLM</td>
<td>RFS/RFIS engineering telemetry</td>
<td><p>TLM-007</p>
<p>IO-AR-021</p></td>
<td>6</td>
<td>ASCII</td>
<td>RS Subnode</td>
<td>IO-RS</td>
<td>RST</td>
<td>31 GB</td>
<td>CO-X-RSS-1-EXP-V1.0</td>
</tr>
<tr class="odd">
<td>99</td>
<td>UVIS_1WAV</td>
<td>Image at one wavelength</td>
<td>IO-AR-023<br />
IO-AR-024</td>
<td>2</td>
<td>Image</td>
<td>Atmos</td>
<td>UVIS</td>
<td>UVIS PI</td>
<td>34 MB</td>
<td>CO-S-UVIS-2-WAV-V1.0</td>
</tr>
<tr class="even">
<td>100</td>
<td>UVIS_QUBE</td>
<td>Spatial and spectral qubes</td>
<td>IO-AR-023<br />
IO-AR-024</td>
<td>2</td>
<td>Qube</td>
<td>Atmos</td>
<td>UVIS</td>
<td>UVIS PI</td>
<td>34 GB</td>
<td>CO-S-UVIS-2-CUBE-V1.0</td>
</tr>
<tr class="odd">
<td>101</td>
<td>UVIS_SPEC</td>
<td>Spectra</td>
<td>IO-AR-023<br />
IO-AR-024</td>
<td>2</td>
<td>Spectrum</td>
<td>Atmos</td>
<td>UVIS</td>
<td>UVIS PI</td>
<td>136 MB</td>
<td>CO-S-UVIS-2-SPEC-V1.0</td>
</tr>
<tr class="even">
<td>102</td>
<td>UVIS_SSB</td>
<td>Solar and Stellar brightness time history</td>
<td>IO-AR-023<br />
IO-AR-024</td>
<td>2</td>
<td>Time Series</td>
<td>Atmos</td>
<td>UVIS</td>
<td>UVIS PI</td>
<td>2 MB</td>
<td>CO-S-UVIS-2-SSB-V1.0</td>
</tr>
<tr class="odd">
<td>103</td>
<td>UVIS_CAL</td>
<td>Calibration files, algorithms and calibrated data examples</td>
<td>IO-AR-023<br />
IO-AR-024</td>
<td>6</td>
<td>Qube, algorithms, etc..</td>
<td>Atmos</td>
<td> </td>
<td>UVIS</td>
<td>2 GB</td>
<td>CO-S-UVIS-2-CAL-V1.0</td>
</tr>
<tr class="even">
<td>104</td>
<td>VIMS_EDR</td>
<td>Image cube of visible bands</td>
<td>DOVI-002, IO-AR-009</td>
<td>3</td>
<td>PDS Spectral Cube</td>
<td>Imaging (JPL)</td>
<td>IO/MIPS</td>
<td>VIMS Team</td>
<td>125 GB</td>
<td>CO-S-VIMS-3-QUBE-V1.0<br />
CO-J/JSA-VIMS-3-QUBE-V1.0<br />
CO-X-VIMS-3-QUBE-V1.0</td>
</tr>
<tr class="odd">
<td>105</td>
<td>SPICE_HUYSPK</td>
<td>Spacecraft, Planet, satellite, and rock ephemeredes</td>
<td>NAV-009</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>NAVT &amp; ISS</td>
<td>Instrument Ops</td>
<td>5 GB in ascii</td>
<td>HP-SSA-SPICE-6-V1.0</td>
</tr>
<tr class="even">
<td>106</td>
<td>SPICE_SPK</td>
<td>Spacecraft, Planet, satellite, and rock ephemeredes</td>
<td>NAV-009</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>NAVT &amp; ISS</td>
<td>Instrument Ops</td>
<td>5 GB in ascii</td>
<td>CO-S/J/E/V-SPICE-6-V1.0</td>
</tr>
<tr class="odd">
<td>107</td>
<td>SPICE_PCK</td>
<td>Planetary Constants and basic models</td>
<td>NAV-010</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>MP</td>
<td>Instrument Ops</td>
<td>2 MB</td>
<td>CO-S/J/E/V-SPICE-6-V1.0</td>
</tr>
<tr class="even">
<td>108</td>
<td>SPICE_IK</td>
<td>Instrument description and frame definitions</td>
<td>DOI-002</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>NAIF</td>
<td>Instrument Ops</td>
<td>2 MB</td>
<td>CO-S/J/E/V-SPICE-6-V1.0</td>
</tr>
<tr class="odd">
<td>109</td>
<td>SPICE_CK</td>
<td>Pointing</td>
<td>MSAS-005</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>SCO/AACS</td>
<td>Instrument Ops</td>
<td>3.3 MB/Day = 6 GB in ascii</td>
<td>CO-S/J/E/V-SPICE-6-V1.0</td>
</tr>
<tr class="even">
<td>110</td>
<td>SPICE_EK</td>
<td>Events</td>
<td>DOI-001</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>Instrument Ops</td>
<td>Instrument Ops</td>
<td>500 MB</td>
<td>CO-S/J/E/V-SPICE-6-V1.0</td>
</tr>
<tr class="odd">
<td>111</td>
<td>SPICE_LSK</td>
<td>Leapseconds</td>
<td>MSAS-019</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>IO/NAIF</td>
<td>Instrument Ops</td>
<td>5 KB</td>
<td>CO-S/J/E/V-SPICE-6-V1.0</td>
</tr>
<tr class="even">
<td>112</td>
<td>SPICE_SCLK</td>
<td>spacecraft clock offset</td>
<td>MSAS-017</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>SCO</td>
<td>Instrument Ops</td>
<td>3 MB</td>
<td>CO-S/J/E/V-SPICE-6-V1.0</td>
</tr>
<tr class="odd">
<td>113</td>
<td>SPICE_FK</td>
<td>Frames</td>
<td>DOI-035</td>
<td>6</td>
<td>SPICE</td>
<td>NAIF</td>
<td>Instrument Ops</td>
<td>Instrument Ops</td>
<td>500 MB</td>
<td>CO-S/J/E/V-SPICE-6-V1.0</td>
</tr>
</tbody>
</table>

##   {#section-6 .unnumbered}

# Appendix B: Archive Delivery Schedule 

The below delivery schedule applies to data products identified in the
Appendix A that are classified as CODMAC levels 4 and below. Higher
level products are archived with the PDS on a best efforts basis on a
schedule developed by the producing team.

  ------------------------ ----------------------- -----------------------
  Data Collection Interval                         Delivery to the PDS
                                                   Required by the First
                                                   Day of:

  From First Day of:       Through Last Day of:    

  Oct 1997                 Jun 2004                Jul 2005

  Jul 2004                 Sep 2004                Jul 2005

  Oct 2004                 Dec 2004                Oct 2005

  Jan 2005                 Mar 2005                Jan 2006

  Apr 2005                 Jun 2005                Apr 2006

  Jul 2005                 Sep 2005                Jul 2006

  Oct 2005                 Dec 2005                Oct 2006

  Jan 2006                 Mar 2006                Jan 2007

  Apr 2006                 Jun 2006                Apr 2007

  Jul 2006                 Sep 2006                Jul 2007

  Oct 2006                 Dec 2006                Oct 2007

  Jan 2007                 Mar 2007                Jan 2008

  Apr 2007                 Jun 2007                Apr 2008

  Jul 2007                 Sep 2007                Jul 2008

  Oct 2007                 Jul 2008                Sep 2008
  ------------------------ ----------------------- -----------------------

# Appendix C: Acronyms

  ---------- ------------------------------------------------------------
  ACP        Aerosol Collector and Pyrolyser

  APSD       Archive Plan for Science Data (formerly known as the Archive
             Policy and Data Transfer Plan, APDTP)

  ASCII      American Standard Code for Information Interchange

  ATM        Atmospheres

  CAPS       Cassini Plasma Spectrometer

  CD         Compact Disc

  CDA        Cosmic Dust Analyzer

  CD-ROM     Compact Disc -- Read Only Memory

  CEL        Cassini Electronic Library

  CIRS       Composite Infrared Spectrometer

  CK         SPICE spacecraft orientation data

  CN         Central Node

  CO         Cassini Orbiter

  CODMAC     Committee on Data Management and Computation

  Co-I       Co-Investigator

  DISR       Descent Imager / Spectral Radiometer

  DN         Discipline Node

  DVD        Digital Versatile Disc the next generation of optical disc
             storage technology

  DWE        Doppler Wind Experiment

  EK         SPICE events information

  ESA        European Space Agency

  FK         SPICE Frames Kernel

  GCMS       Gas Chromatograph Mass Spectrometer

  GMT        Greenwich mean time

  GWE        Gravity Wave Experiment

  HASI       Huygens Atmospheric Structure Instrument

  HP         Huygens Probe

  HSWT       Huygens Science Working Team

  IAG        International Association of Geodesy

  IAU        International Astronomical Union

  IAU        International Astronomical Union

  IDS        Interdisciplinary Scientist

  IEEE       Institute of Electrical and Electronics Engineers

  IK         SPICE instrument Kernel

  INMS       Ion and Neutral Mass Spectrometer

  IO         Instrument Operations Team

  IRD        Interface Requirements Document

  ISS        Imaging Science Subsystem

  JPL        Jet Propulsion Laboratory

  LEMMS      Low Energy Magnetospheric Measurement  System

  LSK        SPICE leapseconds data

  MAG        Magnetometer

  MAPS       Magnetosphere and Plasma Science

  Mb         Megabits

  MIMI       Magnetospheric Imaging Instrument

  MIPS       Multimission Image Processing System

  MSSO       Mission Science and Support Operations

  NAIF       Navigation and Ancillary Information Facility

  NASA       National Aeronautics and Space Administration

  NSSDC      National Space Science Data Center

  OIA        Operational Interface Agreement

  OTL        Operations Team Leader

  PCK        SPICE Planetary Constants Kernel

  PDMP       Project Data Management Plan

  PDS        Planetary Data System

  PI         Principal Investigator

  PPI        Planetary Plasma Interactions

  PSG        Program Science Group

  RPIF       Regional Planetary Image Facility

  RPWS       Radio and Plasma Wave Spectrometer

  RSS        Radio Science Subsystem

  SAUL       Science and Uplink Office

  SAWG       Science Archive Working Group

  SCLK       SPICE spacecraft clock coefficients

  SCLK       Spacecraft Clock

  SIS        Software Interface Specification

  SMP        Science Management Plan

  SOI        Saturn Orbit Insertion

  SPICE      Spacecraft, Planet, Instrument, C-matrix, Events (NAIF PDS
             Node)

  SPK        SPICE Spacecraft and Planetary Kernel ephemeredes

  SSP        Surface Science Package

  TBD        To Be Determined

  Tbits      TerraBytesTerrabits

  TL         Team Leader

  UTC        Coordinated Universal Time

  UVIS       Ultraviolet Imaging Spectrograph

  VIMS       Visual and Infrared Mapping Spectrometer

  WG         Working Group

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             

             
  ---------- ------------------------------------------------------------

# Appendix D: Huygens Data Archive Generation, Validation and Transfer Plan