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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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Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Monday, November 19, 2018 - 1:25:27 PM
Last modification on : Friday, December 3, 2021 - 11:42:50 AM


  • HAL Id : insu-01916874, version 1


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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