Abstract: SHOTS: Comparison of numerical approaches for the solar wind interaction with Mercury’s magnetosphere within the BepiColombo simulation group (AGU Fall Meeting 2018)

SHOTS: Comparison of numerical approaches for the solar wind interaction with Mercury’s magnetosphere within the BepiColombo simulation group

Sae Aizawa^1,2, Willi Exner³, Léa Sophie Griton⁴, Shahab Fatemi⁵, Manabu Yagi⁶, Jorge Amaya⁷, Lucas Liuzzo⁸, Hideyuki Usui⁹, Go Murakami¹⁰, Daniel Heyner¹¹ and Satoki Oki⁹, (1)LPP, Ecole Polytechnique, Sorbonne Université, CNRS, Jussieu, Paris, France, (2)Tohoku University, Sendai, Japan, (3)Technical University of Braunschweig, Institute for Geophysics and extraterrestrial Physics, Braunschweig, Germany, (4)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, Meudon, France, (5)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, (6)RIKEN, R-CCS, Kobe, Japan, (7)Katholieke Universiteit Leuven, Department of Mathematics, Leuven, Belgium, (8)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (9)Kobe University, Kobe, Japan, (10)ISAS-JAXA, Sagamihara, Japan, (11)TU Braunschweig, Institute of Geophysics and Extraterrestrial Physics, Braunschweig, Germany

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