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Conference Papers Year : 2018

Numerical SPIS-Dust Modelling of Plasma – Lunar Lander Interactions

Abstract

This paper presents first results of SPIS-DUST modelling of the interaction between the lunar plasma environment , regolith and a lander. The model takes into account the geometry of the Luna-Glob lander, the electric properties of materials used on the lander surface, as well as Luna-Glob landing place. Initial conditions were chosen based on the current theoretical models of formation of dusty plasma exosphere and levitating charged dust particles.
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Dates and versions

insu-01916874 , version 1 (19-11-2018)

Identifiers

  • HAL Id : insu-01916874 , version 1

Cite

I.A. Kuznetsov, A.V. Zakharov, Elena Seran, S.L.G. Hess, F. Cipriani, et al.. Numerical SPIS-Dust Modelling of Plasma – Lunar Lander Interactions. European Planetary Science Congress 2018, Sep 2018, Berlin, Germany. pp.EPSC2018-1218. ⟨insu-01916874⟩
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