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Mars mantle: forward modelling. Inputs: mineralogy, crust thickness and average density, core radius and mass, temperature profile, pressure gradient. Outputs: variation with depth of the density, seismic potential, and electrical conductivity. paper submitted for publication at JGR
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Mars mantle: forward modelling • Inputs: mineralogy, crust thickness and average density, core radius and mass, temperature profile, pressure gradient. • Outputs: variation with depth of the density, seismic potential, and electrical conductivity. • paper submitted for publication at JGR • see poster Network activity: MINT Working Group contribution
Mars mantle: inverse modelling • Inputs: global geodetic parameters, variation with depth of the seismic potential and electrical conductivity, crust thickness and core radius. • Outputs: mineralogy, crust average density, core mass, temperature profile, pressure gradient. • Paper in preparation • see poster Network activity : MINT Working Group contribution
Mars conductive structure from network magnetic data • Determination of the electromagnetic impedance Z(w) by means of space-time frequency filters*. • MCMC algorithms for Z(w) inversion Network activity: CETP, LPCE, UMLV, GGKI Sopron The hungarian PhD student got killed in a car crash by the end of october 2003.
Mars ionized environment: forward modelling • Hybrid 3-D forward modelling of the Mars ionized environment from the solar wind down to 500 kilometers above the Mars surface (R. Modolo thesis, G. Chanteur supervisor). • To be coupled with a ionospheric model, at present under development. • Paper in preparation (hybrid model) • see poster The model is a tool to be used in frame of the Post-Doc activities Network activity: Working group on Mars ionized environment studies
Post-Doc position • Use both MGS magnetic recordings and the Mars environment model to get information on the magnetic external sources in the Mars ionized environment. • Few candidates, no Post-Doc for the time being