Plasma and Fusion Research
Volume 8, 2406132 (2013)
Regular Articles
- Kobe University, 1-1 Rokkodai-cho, Nada-ku, Kobe 657-8501, Japan
- 1)
- National Institute for Fusion Science, 322-6 Oroshi-cho, Toki 509-5292, Japan
- 2)
- Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai 599-8531, Japan
- 3)
- Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara 252-5210, Japan
Abstract
A parallelized two-dimensional full particle-in-cell (PIC) simulations with an adaptive mesh refinement (AMR) technique for the interaction of solar wind with kinetic scale magnetosphere around a magnetic sail are conducted. For multi-scale simulations, the newly developed AMR-PIC code has a method to modify the grid size and time step interval of computational domain in the midst of the simulations temporally and locally. In the simulation results under the typical working condition introducing the AMR technique, it is shown that the direction of interplanetary magnetic field depend strongly on the magnetospheric configuration including electron dynamics and Alfven bow shock structure. Although more validation studies are needed, the AMR-PIC code shows the worth of development for multi-scale simulations.
Keywords
kinetic scale magnetosphere, particle-in-cell, adaptive mesh refinement, solar wind, space plasma
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This paper may be cited as follows:
Masaharu MATSUMOTO, Hideyuki USUI, Masanori NUNAMI, Masao NAKAMURA and Iku SHINOHARA, Plasma Fusion Res. 8, 2406132 (2013).