Microwave diagnostics of magnetic field strengths in solar flaring loops

著录项

• 来源
  《中国科学》 |2021年第1期|P.169-178|共10页
• 作者

  ZHU Rui; TAN BaoLin; SU YingNa; TIAN Hui; XU Yu; CHEN XingYao; SONG YongLiang; TAN GuangYu;

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• 作者单位

  School of Earth and Space Sciences Peking University Beijing 100871 China;

  Key Laboratory of Solar Activity National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 ChinaSchool of Astronomy and Space Science University of Chinese Academy of Sciences Beijing 100049 China;

  Key Laboratory of Dark Matter and Space Astronomy Purple Mountain Observatory Chinese Academy of Sciences Nanjing 210008 ChinaSchool of Astronomy and Space Science University of Science and Technology of China Hefei 230026 China;

  School of Earth and Space Sciences Peking University Beijing 100871 ChinaKey Laboratory of Solar Activity National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China;

  School of Astronomy and Space Science Nanjing University Nanjing 210023 China;

  Key Laboratory of Solar Activity National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China;

  Key Laboratory of Solar Activity National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China;

  School of Earth and Space Sciences Peking University Beijing 100871 China;

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• 原文格式 PDF
• 正文语种 chi
• 中图分类 太阳系;
• 关键词

  solar magnetic field; solar flare; microwave observation; gyrosynchrotron emission;