An atmospheric model designed for integration into coupled models of magma ocean planets

Abstract : A 1D radiative-convective model of a thick (up to several hundreds of bars) H2O-CO2 atmosphere has been developped and coupled with a simple magma ocean interior model[1]. In this paper, we will focus on describing the atmospheric model. Preliminary results regarding observable parameters and the cooling rates of the magma ocean will also be discussed and compared with similar studies[2].
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https://hal.archives-ouvertes.fr/hal-00666266
Contributeur : Catherine Cardon <>
Soumis le : vendredi 3 février 2012 - 17:41:45
Dernière modification le : mercredi 19 septembre 2018 - 01:27:35

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Emmanuel Marcq, H. Massol, T. Lebrun, François Leblanc, Eric Chassefière. An atmospheric model designed for integration into coupled models of magma ocean planets. EPSC-DPS Joint Meeting 2011, Oct 2011, Nantes, France. 〈hal-00666266〉

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