volume 13, issue S335, P314-317 2017
DOI: 10.1017/s174392131700833x
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Tomoya Ogawa, Mitsue Den, Takashi Tanaka, Kazuyuki Yamashita

Abstract: AbstractWe perform simulations of the interplanetary coronal mass ejections relating to the magnetic storm on 17 March 2015. A hierarchical mesh structure is used, which is controlled by an adaptive mesh refinement technique, with fine-scale cells where it matters, the structure of the running shock waves of the coronal mass ejections and co-rotating interactive regions. The initial and the inner-boundary conditions are derived from another simulation, which uses a split dodecahedron grid. The resulting shock-…

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