Aspects of Multi-Dimensional Modelling of Substellar Atmospheres
Solar and Stellar Astrophysics
2010-12-15 v1 Earth and Planetary Astrophysics
Computational Engineering, Finance, and Science
Atmospheric and Oceanic Physics
Fluid Dynamics
Abstract
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.
Keywords
Cite
@article{arxiv.1012.3013,
title = {Aspects of Multi-Dimensional Modelling of Substellar Atmospheres},
author = {Ch. Helling and E. Pedretti and S. Berdyugina and A. A. Vidotto and B. Beeck and E. Baron and A. P. Showman and E. Agol and D. Homeier},
journal= {arXiv preprint arXiv:1012.3013},
year = {2010}
}
Comments
12 pages, 5 figures, summery of Cool Stars 16 Splinter 'Multi-Dimensional Modelling of Substellar Atmospheres'