Journal
JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER
Volume 111, Issue 15, Pages 2139-2150Publisher
PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.jqsrt.2010.05.001
Keywords
Spectroscopic database; Molecular spectroscopy; Molecular absorption; Line parameters; High-temperature spectroscopy; HITEMP
Categories
Funding
- NASA [NAG5-13534]
- Planetary Atmospheres program [NNX10AB94G]
- Spectral Sciences, Inc.
- National Science Foundation [ATM-0803135]
- Russian Fund of Basic Research [06-05-39016-(1)GammaPhiEH_a, 09-05-93105-HPiHalephJI_a]
- NERC [NE/F01967X/1] Funding Source: UKRI
- STFC [ST/H008543/1] Funding Source: UKRI
- Natural Environment Research Council [NE/F01967X/1] Funding Source: researchfish
- Science and Technology Facilities Council [ST/H008543/1] Funding Source: researchfish
- NASA [NNX10AB94G, 136365] Funding Source: Federal RePORTER
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A new molecular spectroscopic database for high-temperature modeling of the spectra of molecules in the gas phase is described. This database, called HITEMP, is analogous to the HITRAN database but encompasses many more bands and transitions than HITRAN for the absorbers H2O, CO2, CO, NO, and OH. HITEMP provides users with a powerful tool for a great many applications: astrophysics, planetary and stellar atmospheres, industrial processes, surveillance, non-local thermodynamic equilibrium problems, and investigating molecular interactions, to name a few. The sources and implementation of the spectroscopic parameters incorporated into HITEMP are discussed. (C) 2010 Elsevier Ltd. All rights reserved.
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