Prospect for Multiple Time and Spatial Scale Simulation Research in Astrophysical Plasma Phenomena: Multiple Scale Simulation of Magnetic Reconnection Phenomena in the Solar Corona

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  • KUSANO Kanya
    Graduate School of Advanced Sciences of Matter, Hiroshima University

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  • 異なった時空間スケールが関与する多階層プラズマシミュレーション―現状からの展望―５．天体プラズマ現象における多階層シミュレーション研究の展望　　５．１　　太陽磁気リコネクション現象の多階層性とシミュレーション
  • 太陽磁気リコネクション現象の多階層性とシミュレーション
  • タイヨウ ジキ リコネクション ゲンショウ ノ タカイソウセイ ト シミュレーション

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Abstract

Although magnetic reconnection is believed to be a key process in solar flares, the flares' triggering mechanism remains a long-standing problem. In order to resolve this issue, the physical linkage between the magnetohydrodynamic (MHD) process in the macroscopic scale and the plasma kinetics in the microscopic scale has to be understood. Multiple-scale simulation, which can precisely describe the nonlinear process of the MHD equations as well as the complexity in the solar corona, will play a crucial role in this field of study.

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