Study of Europa’s crust via a Stefan model with convection

Maria M. Cerimele, Daniela Mansutti and Francesca Pistella

Mathematics and Computers in Simulation (MATCOM), 2008, vol. 79, issue 3, 258-268

Abstract: We present results of a numerical simulation of the thermal convection in the subsurface mushy ice layer of Europa, one of the Jupiter’s moons. Beside fluid dynamics and heat transfer within such a layer, heat conduction in the solid crustal surface and heat exchange between the two phases – mushy ice and solid crust – are included in our model in order to follow also the evolution of the phase front.

Keywords: Mush; Solid; Phasetransition; Rayleigh–Benard convection; Numerical simulation (search for similar items in EconPapers)
Date: 2008
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Persistent link: https://EconPapers.repec.org/RePEc:eee:matcom:v:79:y:2008:i:3:p:258-268

DOI: 10.1016/j.matcom.2007.11.011

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