Aspects of Multi-Dimensional Modelling of Substellar Atmospheres
Ch. Helling (SUPA, St Andrews, UK), E. Pedretti (SUPA, St Andrews,, UK), S. Berdyugina (Kiepenheuer Institut, Freiburg, D), A.A. Vidotto (SUPA,, St Andrews, UK), B. Beeck (University Goettingen, D), E. Baron (University of, Oklahoma, Norman, US)
TL;DR
This paper reviews advances in modeling the complex, dynamic atmospheres of brown dwarfs and planets, integrating new theoretical, observational, and technological developments to address current challenges.
Contribution
It introduces novel modeling approaches and observational techniques for understanding the dynamic atmospheres of substellar objects.
Findings
Enhanced models capturing atmospheric variability
Integration of new observational data techniques
Addressing challenges from planetary and space weather observations
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.
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Taxonomy
TopicsAstro and Planetary Science · Geomagnetism and Paleomagnetism Studies