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

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

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..540m&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.540

Computer Science

Scientific paper

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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