An atmospheric model designed for integration into coupled models of magma ocean planets
Year: 2011
Type: conference-paper
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].
Source: HAL
Authors: Marcq, Emmanuel, Massol, Hélène, Lebrun, T., Leblanc, François, Chassefière, Eric
Language: English
Topic: Astro and Planetary Science
Subfield: Space and Planetary Science
Field: Earth and Planetary Sciences
Domain: Physical Sciences
SDG: Climate action
Open Access status: green
OpenAlex ID: W2203090124