Modeling the interaction of solar wind with a dipole magnetic field with Shenguang II intense lasers

K. Zhang, J. Y. Zhong, J. Q. Wang, X. X. Pei, H. G. Wei, D. W. Yuan, Z. W. Yang, C. Wang, F. Li, B. Han, C. L. Yin, G. Q. Liao, Y. Fang, S. Yang, X. H. Yuan, Y. Sakawa, T. Morita, Z. R. Cao, S. E. Jiang, Y. K. DingY. Kuramitsu, G. Y. Liang, F. L. Wang, Y. T. Li, J. Q. Zhu, J. Zhang, G. Zhao

研究成果: Contribution to journalArticle査読

8 被引用数 (Scopus)

抄録

The interaction of solar wind with a dipole magnetic field is modeled in a laboratory setting with a small cylindrical permanent magnet and magnetized plasma driven by intense lasers. The result shows a potential application in the understanding of Earth's magnetosphere near the pole region. Some significant features are observed in our experiments, such as magnetic reconnection and repulsion, which agree well with magnetohydrodynamics (MHD) simulation results.

本文言語英語
ページ(範囲)32-37
ページ数6
ジャーナルHigh Energy Density Physics
17
DOI
出版ステータス出版済み - 12 1 2015
外部発表はい

All Science Journal Classification (ASJC) codes

  • 放射線
  • 核物理学および高エネルギー物理学

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