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Theoretical arguments and observations suggest that the atmospheres of BrownDwarfs and planets are very dynamic on chemical and on physical time scales.The modelling of such substellar atmospheres has, hence, been much moredemanding than initially anticipated. This Splinter(http://star-www.st-and.ac.uk/~ch80/CS16/MultiDSplinter_CS16.html) has combinednew developments in atmosphere modelling, with novel observational techniques,and new challenges arising from planetary and space weather observations.

Aspects of Multi-Dimensional Modelling of Substellar Atmospheres