Model, software and database for line-mixing effects in the ν3 and ν4 bands of CH4 and tests using laboratory and planetary measurements-II: H2 (and He) broadening and the atmospheres of Jupiter and Saturn

Journal of Quantitative Spectroscopy and Radiative Transfer

Volumn 101, Issue 2, 2006, Pages 306-324

  Tran, H ^a   Flaud, P M ^b   Fouchet, T ^c   Gabard, T ^d   Hartmann, J M ^a  

^a LABORATOIRE INTERUNIVERSITAIRE DES SYSTÈMES ATMOSPHÉRIQUES   (France)

^b UNIVERSITÉ DE BORDEAUX   (France)

^c OBSERVATOIRE DE PARIS   (France)

^d UNIVERSITÉ DE BOURGOGNE   (France)

Author keywords

Giant planets emission; Methane infrared spectra

Indexed keywords

ABSORPTION; ATMOSPHERIC CHEMISTRY; COMPUTER SIMULATION; HELIUM; HYDROGEN; INFRARED RADIATION; MATHEMATICAL MODELS; METHANE; PLANETS;

COLLISION-INDUCED ABSORPTION; GIANT PLANETS EMISSION; LINE-MIXING EFFECTS; METHANE INFRARED SPECTRA;

ATMOSPHERIC OPTICS;

ATOMIC ABSORPTION SPECTROSCOPY; JUPITER; MIXING; PLANETARY ATMOSPHERE; SATURN;

LORENTZIA;

EID: 33646703118     PISSN: 00224073     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.jqsrt.2005.11.033     Document Type: Article

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