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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
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