Water vapor map of Mars near summer solstice using ground-based infrared spectroscopy

Astronomy and Astrophysics

Volumn 520, Issue 3, 2010, Pages

  Encrenaz, T ^a   Greathouse, T K ^b   Bezard B ^a   Fouchet, T ^a   Lefevre F ^c   Montmessin, F ^c   Bitner, M ^d   Kruger, A ^e   Richter, M J ^e   Lacy, J H ^f   Forget, F ^g   Atreya, S K ^h  

^a CNRS   (France)

^b SwRI   (United States)

^c INSTITUT PIERRE SIMON LAPLACE   (France)

^d STScI   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f The University of Texas at Austin   (United States)

^g LABORATOIRE DE MÉTÉOROLOGIE DYNAMIQUE   (France)

^h UNIVERSITY OF MICHIGAN   (United States)

Author keywords

Planets and satellites: atmospheres; Planets and satellites: individual: Mars; Planets and satellites: surfaces; Techniques: spectroscopic

Indexed keywords

ATMOSPHERIC SPECIES; CLIMATE MODEL; CONTINUUM FLUX; DYNAMICAL EFFECTS; ECHELLE SPECTROGRAPH; GLOBAL CLIMATE MODEL; GLOBAL DISTRIBUTION; GROUND BASED; INFRARED TELESCOPES; LONGITUDINAL VARIATIONS; MIDLATITUDES; MODEL PREDICTION; NORTHERN LATITUDES; PLANETS AND SATELLITES: ATMOSPHERES; PLANETS AND SATELLITES: INDIVIDUAL: MARS; PLANETS AND SATELLITES: SURFACES; SPATIAL MAPPING; SPATIAL RESOLUTION; SUMMER SOLSTICE; SURFACE TEMPERATURES; TECHNIQUES: SPECTROSCOPIC; TRANSIENT PHENOMENON; WATER VAPOR MIXING RATIO;

CLIMATE MODELS; FORECASTING; INFRARED SPECTROSCOPY; NASA; PLANETS; TELESCOPES; WATER VAPOR;

SATELLITES;

EID: 77957194181     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913905     Document Type: Article

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