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Laboratory and theoretical work applied to planetary atmospheres

Published online by Cambridge University Press:  27 October 2016

Athena Coustenis
Athena Coustenis*
Affiliation:
Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (LESIA), Observatoire de Paris, PSL-Research Univ., CNRS, Univ. Paris 06, Sorbonne Univ., Univ. Paris-Diderot, Sorbonne Paris-Cité, 5, place Jules Janssen, 92195 Meudon Cedex, France email: athena.coustenis@obspm.fr
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Abstract

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We look at applications of recent work in theoretical and experimental spectroscopy for the analysis of IR data concerning giant planets, Titan and possibly exoplanets.

Keywords

planets and satellites: formationmethods: data analysistechniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , pp. 325 - 326
Copyright
Copyright © International Astronomical Union 2016 

References

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Coustenis, A. 2014, in: Spohn, T., Breuer, D., & Johnson, T. V. (eds.), “Titan”, in Encyclopedia of the Solar System, Third Edition (Elsevier), p. 831 CrossRefGoogle Scholar
Coustenis, A., et al. 2015, Icarus, in pressGoogle Scholar
Nixon, A., et al. 2012, ApJ 749 article id. 159 CrossRefGoogle Scholar