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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Submitted on : Friday, February 3, 2012 - 5:41:45 PM
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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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