Source: http://www.science.gov/topicpages/0-9/2011-07-01+false+nonflare.html
Timestamp: 2016-10-26 13:25:47
Document Index: 511720392

Matched Legal Cases: ['§ 65', '§ 63', '§ 104', '§ 106', '§ 406', '§ 26', '§ 1906']

2011-07-01 false nonflare: Topics by Science.gov
Sample records for 2011-07-01 false nonflare
40 CFR 63.986 - Nonflare control devices used for equipment leaks only.
... equipment leaks only. 63.986 Section 63.986 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY... leaks only. (a) Equipment and operating requirements. (1) Owners or operators using a nonflare control... test is not required for any nonflare control device used only to control emissions from...
... equipment leaks only. 65.146 Section 65.146 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY... Routing to a Fuel Gas System or a Process § 65.146 Nonflare control devices used for equipment leaks only... nonflare control device used only to control emissions from equipment leaks. (c) Monitoring...
... and Routing to a Fuel Gas System or a Process § 63.986 Nonflare control devices used for equipment... operated at all times when emissions are vented to them. (b) Performance test requirements. A...
40 CFR 63.985 - Nonflare control devices used to control emissions from storage vessels and low throughput...
... the reasonably expected maximum storage vessel filling or transfer loading rate. This documentation is... control emissions from storage vessels and low throughput transfer racks. 63.985 Section 63.985 Protection... transfer racks. (a) Nonflare control device equipment and operating requirements. The owner or...
Gary, D. E.; Linsky, J. L.
Results are presented of a search for nonflare microwave radiation from the coronae of nearby late-type dwarf stars comparable to the sun: single stars without evidence for either a large wind or circumstellar envelope. The observing program consisted of flux measurements of six stars over a 24-h period with the VLA in the C configuration at a wavelength of 6 cm with 50 MHz bandwidth. Positive detections at 6 cm were made for Chi 1 Ori (0.6 mJy) and the flare star UV Cet (1.55 mJy), and upper limits were obtained for the stars Pi 1 UMa, Xi Boo A, 70 Oph A and Epsilon Eri. It is suggested that Chi 1 Ori, and possibly UV Cet, represent the first detected members of a new class of radio sources which are driven by gyroresonance emission, i.e. cyclotron emission from nonrelativistic Maxwellian electrons.
"Hot" Non-flaring Plasmas in Active Region Cores Heated by Single Nanoflares
Barnes, Will Thomas; Cargill, Peter; Bradshaw, Stephen
We use hydrodynamic modeling tools, including a two-fluid development of the EBTEL code, to investigate the properties expected of "hot" (i.e. between 106.7 and 107.2 K) non-flaring plasmas due to nanoflare heating in active regions. Here we focus on single nanoflares and show that while simple models predict an emission measure distribution extending well above 10 MK that is consistent with cooling by thermal conduction, many other effects are likely to limit the existence and detectability of such plasmas. These include: differential heating between electrons and ions, ionization non-equilibrium and, for short nanoflares, the time taken for the coronal density to increase. The most useful temperature range to look for this plasma, often called the "smoking gun" of nanoflare heating, lies between 1 MK and 10 MK. Signatures of the actual heating may be detectable in some instances.
Temperature dependence of emission measure in solar X-ray plasmas. 1: Non-flaring active regions
X-ray and ultraviolet line emission from hot, optically thin material forming coronal active regions on the sun may be described in terms of an emission measure distribution function, Phi (T). A relationship is developed between line flux and Phi (T), a theory which assumes that the electron density is a single-valued function of temperature. The sources of error involved in deriving Phi (T) from a set of line fluxes are examined in some detail. These include errors in atomic data (collisional excitation rates, assessment of other mechanisms for populating excited states of transitions, element abundances, ion concentrations, oscillator strengths) and errors in observed line fluxes arising from poorly - known instrumental responses. Two previous analyses are discussed in which Phi (T) for a non-flaring active region is derived. A least squares method of Batstone uses X-ray data of low statistical significance, a fact which appears to influence the results considerably. Two methods for finding Phi (T) ab initio are developed. The coefficients are evaluated by least squares. These two methods should have application not only to active-region plasmas, but also to hot, flare-produced plasmas.
Ishikawa, Shin-nosuke; Glesener, Lindsay; Christe, Steven; Ishibashi, Kazunori; Brooks, David H.; Williams, David R.; Shimojo, Masumi; Sako, Nobuharu; Krucker, Säm
We present new constraints on the high-temperature emission measure of a non-flaring solar active region using observations from the recently flown Focusing Optics X-ray Solar Imager (FOXSI) sounding rocket payload. FOXSI has performed the first focused hard X-ray (HXR) observation of the Sun in its first successful flight on 2012 November 2. Focusing optics, combined with small strip detectors, enable high-sensitivity observations with respect to previous indirect imagers. This capability, along with the sensitivity of the HXR regime to high-temperature emission, offers the potential to better characterize high-temperature plasma in the corona as predicted by nanoflare heating models. We present a joint analysis of the differential emission measure (DEM) of active region 11602 using coordinated observations by FOXSI, Hinode/XRT, and Hinode/EIS. The Hinode-derived DEM predicts significant emission measure between 1 MK and 3 MK, with a peak in the DEM predicted at 2.0-2.5 MK. The combined XRT and EIS DEM also shows emission from a smaller population of plasma above 8 MK. This is contradicted by FOXSI observations that significantly constrain emission above 8 MK. This suggests that the Hinode DEM analysis has larger uncertainties at higher temperatures and that > 8 MK plasma above an emission measure of 3 × 1044 cm-3 is excluded in this active region.
A new approach for deriving the solar irradiance from non-flaring solar upper atmosphere plasmas at 2 x 10^4<-T<-2 x 10^7 K
Colgan, James P; Abdallaf, Jr., Joseph; Fontes, Christopher J; Sherrill, Manolo E; Feldmn, U; Landi, E; Brown, C M; Seely, J F; Doschek, G A; Dammasch, I E
We propose a new approach for deriving the solar irradiance in the X-ray to VUV range due to the emission by solar upper atmosphere plasmas at 2 x 10{sup 4} {le} T {le} 2 x 10{sup 7} K. Our approach is based on new understanding of the properties of the solar upper atmosphere; specifically, the discovery that the majority of emission from the non-flaring solar upper transition region and corona in the temperature range 3 x 10{sup 5} {le} T {le} 3 x 10{sup 6} K arises from isothermal plasmas that have four distinct temperatures: 0.35, 0.9, 1.4 and 3 x 10{sup 6} K. In the lower transition region (2 x 10{sup 4} {le} T {le} 2 x 10{sup 5} K) of coronal holes, quiet regions or active regions, although multithermal and variable in brightness, the shape of emission measure vs. temperature curves is almost constant. Flaring plasmas are for most part isothermal, although their emission measure and temperature continuously change. In this paper we review these recent results and propose a set of simple spectrometers for recording the solar spectrum in several narrow bands. The solar emission measure, average plasma temperature, and composition can be derived using the measured line fluxes. By combining the emission measure and other plasma properties with the output of a suite of atomic physics codes, which are also described here, the solar irradiance in the temperature range 2 x 10{sup 4} {le} T {le} 2 x 10{sup 7} K can be calculated.
... 33 Navigation and Navigable Waters 1 2011-07-01 2011-07-01 false Communications. 104.245 Section... MARITIME SECURITY: VESSELS Vessel Security Requirements § 104.245 Communications. (a) The Vessel Security... board the vessel. (b) Communications systems and procedures must allow effective and...
33 CFR 106.240 - Communications.
... 33 Navigation and Navigable Waters 1 2011-07-01 2011-07-01 false Communications. 106.240 Section... Requirements § 106.240 Communications. (a) The Facility Security Officer (FSO) must have a means to effectively notify OCS facility personnel of changes in security conditions at the OCS facility. (b)...
36 CFR 406.160 - Communications.
... 36 Parks, Forests, and Public Property 3 2011-07-01 2011-07-01 false Communications. 406.160... COMMISSION § 406.160 Communications. (a) The agency shall take appropriate steps to ensure effective communication with applicants, participants, personnel of other Federal entities, and members of the public....
... 33 Navigation and Navigable Waters 1 2011-07-01 2011-07-01 false Communications. 26.07 Section 26.07 Navigation and Navigable Waters COAST GUARD, DEPARTMENT OF HOMELAND SECURITY GENERAL VESSEL BRIDGE-TO-BRIDGE RADIOTELEPHONE REGULATIONS § 26.07 Communications. No person may use the services of,...
32 CFR 1906.160 - Communications.
... 32 National Defense 6 2011-07-01 2011-07-01 false Communications. 1906.160 Section 1906.160 National Defense Other Regulations Relating to National Defense CENTRAL INTELLIGENCE AGENCY ENFORCEMENT OF... § 1906.160 Communications. (a) The Agency shall take appropriate steps to ensure effective...