The impact of atmospheric circulation on the chemistry of the hot Jupiter HD 209458b

Astronomy and Astrophysics

Volumn 548, Issue , 2012, Pages

  Agundez M ^a,b   Venot, O ^a,b   Iro, N ^c   Selsis, F ^a,b   Hersant, F ^a,b   Hebrard E ^a,b   Dobrijevic, M ^a,b  

^a UNIVERSITÉ DE BORDEAUX   (France)

^b CNRS   (France)

^c KEELE UNIVERSITY   (United Kingdom)

Author keywords

Astrochemistry; Planets and satellites: atmospheres; Planets and satellites: individual: HD 209458b

Indexed keywords

ASTROCHEMISTRY; ATMOSPHERIC CIRCULATION; ATMOSPHERIC CONSTITUENTS; CHEMICAL COMPOSITIONS; CHEMICAL EQUILIBRIUMS; CHEMICAL NETWORKS; CIRCULATION MODELS; DEEP LAYER; DYNAMICAL MODEL; EQUATORIAL SUPERROTATION; JUPITERS; LONGITUDINAL VARIATIONS; MOLECULAR ABUNDANCES; PLANETS AND SATELLITES: ATMOSPHERES; PLANETS AND SATELLITES: INDIVIDUAL: HD 209458B; PRESSURE LEVEL; QUENCHING EFFECT; ROTATION RATE; SOLID BODIES; SUBSTANTIAL VARIATIONS; TEMPERATURE CONTRAST; TEMPERATURE STRUCTURE; TIME-SCALES; TRANSITION LAYERS; TRANSMISSION SPECTRUMS; TWO-REGIME; VERTICAL MIXING; ZONAL WIND;

ATMOSPHERIC STRUCTURE; CLIMATOLOGY; DIGITAL TELEVISION; MIXING; PLANETS; SATELLITES;

THREE DIMENSIONAL;

EID: 84870010326     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220365     Document Type: Article

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