Applications of a new set of methane line parameters to the modeling of Titan's spectrum in the 1.58 μm window

Planetary and Space Science

Volumn 61, Issue 1, 2012, Pages 85-98

  De Bergh, Catherine ^a   Courtin, Régis ^a   Bézard, Bruno ^a   Coustenis, Athéna ^a   Lellouch, Emmanuel ^a   Hirtzig, Mathieu ^a,b   Rannou, Pascal ^c   Drossart, Pierre ^a   Campargue, Alain ^d   Kassi, Samir ^d   Wang, Le ^d   Boudon, Vincent ^e   Nikitin, Andrei ^f   Tyuterev, Vladimir ^c  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b LABORATOIRE DE MÉTÉOROLOGIE DYNAMIQUE   (France)

^c UNIVERSITÉ DE REIMS CHAMPAGNE ARDENNE   (France)

^d LIPHY   (France)

^e UNIVERSITÉ DE BOURGOGNE   (France)

^f V E ZUEV INSTITUTE OF ATMOSPHERIC OPTICS   (Russian Federation)

Author keywords

Atmosphere; Infrared; Methane; Spectroscopy; Titan

Indexed keywords

AEROSOL MODELS; BAND MODEL; CASSINI; DATA SETS; HIGH RESOLUTION; HIGH SPECTRAL RESOLUTION; HUYGENS; IN-SITU; LINE PARAMETERS; LINE SHAPE; METHANE ABSORPTION; MOLE FRACTION; PHASE ANGLES; SYNTHETIC SPECTRA; TEMPERATURE-PRESSURE CONDITIONS; TITAN; TITAN'S ATMOSPHERE;

EARTH ATMOSPHERE; INFRARED RADIATION; SPECTRAL RESOLUTION; SPECTROSCOPY;

METHANE;

EID: 84856225230     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.pss.2011.05.003     Document Type: Conference Paper

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