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Poster De Conférence Année : 2011

Simulation study of Solar Wind interaction with Mercury's magnetosphere

Résumé

The interaction of the Hermean magnetosphere and the Solar Wind is investigated using a 3-dimensional parallel multi-species hybrid model. In the simulation, it is assumed that Mercury is at its Aphelion and the IMF orientation is the orientation reported by MESSENGER during its first flyby. The principal regions of this interaction are reproduced by the hybrid model and the electromagnetic field spatial variations are described as well. This model represents a strong tool to study Mercury's plasma environment.
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Dates et versions

hal-02860535 , version 1 (08-06-2020)

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  • HAL Id : hal-02860535 , version 1

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Emilie Richer, Ronan Modolo, Gérard Chanteur, Sebastien Hess, Marco Mancini, et al.. Simulation study of Solar Wind interaction with Mercury's magnetosphere. EPSC-DPS Joint Meeting 2011, Oct 2011, Nantes, France. 6, pp.EPSC-DPS2011-760, 2011. ⟨hal-02860535⟩
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