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Aspects of Multi-Dimensional Modelling of Substellar Atmospheres

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arxiv 1012.3013 v1 pith:HHDT73W2 submitted 2010-12-14 astro-ph.SR astro-ph.EPcs.CEphysics.ao-phphysics.flu-dyn

Aspects of Multi-Dimensional Modelling of Substellar Atmospheres

Ch. Helling (SUPA , St Andrews , UK) , E. Pedretti (SUPA , S. Berdyugina (Kiepenheuer Institut , Freiburg , D) , A.A. Vidotto (SUPA
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B. Beeck (University Goettingen E. Baron (University of Oklahoma Norman US) A.P. Showman (University of Arizona Tucson US) E. Agol (University of Washington Seattle D. Homeier (University Goettingen
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classification astro-ph.SR astro-ph.EPcs.CEphysics.ao-phphysics.flu-dyn
keywords atmospheresmodellingcs16observationssubstellaranticipatedargumentsarising
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Theoretical arguments and observations suggest that the atmospheres of Brown Dwarfs and planets are very dynamic on chemical and on physical time scales. The modelling of such substellar atmospheres has, hence, been much more demanding than initially anticipated. This Splinter (http://star-www.st-and.ac.uk/~ch80/CS16/MultiDSplinter_CS16.html) has combined new developments in atmosphere modelling, with novel observational techniques, and new challenges arising from planetary and space weather observations.

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