Volume 41 Issue 6
Nov.  2021
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Article Navigation >  Chinese Journal of Space Science  > 2021  >  41(6): 869-880
TI Shuo, SHEN Chao, CHEN Tao, JI Yong, HE Han, XU Ronglan, HUANG Ya. Influence of Continuous Magnetic Activities on the Evolution of the Plasmasphere[J]. Chinese Journal of Space Science, 2021, 41(6): 869-880. doi: 10.11728/cjss2021.06.869
Citation: TI Shuo, SHEN Chao, CHEN Tao, JI Yong, HE Han, XU Ronglan, HUANG Ya. Influence of Continuous Magnetic Activities on the Evolution of the Plasmasphere[J]. Chinese Journal of Space Science, 2021, 41(6): 869-880. doi: 10.11728/cjss2021.06.869
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Influence of Continuous Magnetic Activities on the Evolution of the Plasmasphere

doi: 10.11728/cjss2021.06.869 cstr: 32142.14.cjss2021.06.869

  • 1. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190;

  • 2. University of Chinese Academy of Sciences, Beijing 100049;

  • 3. School of Science, Harbin Institute of Technology, Shenzhen 518005;

  • 4. Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012

  • Received Date: 2020-09-25
  • Rev Recd Date: 2021-08-31
  • Publish Date: 2021-11-15
    Abstract
  • In this paper, the evolution of the plasmasphere's morning side viewing was analyzed under a series of magnetic activities using the extreme ultraviolet logarithmic data observed by the Chang'E-3 extreme ultraviolet camera on 21 February 2014. Based on the phase space distribution of the protons, the evolution of the plasmasphere on the magnetic equatorial plane was simulated when a series of magnetic storm events occurred from 18 to 22 February 2014. Through observation and simulation, it is found that the actual filling speed of the plasmasphere is greater than the filling speed of the plasmasphere during the simulation. It is presumed that the plume structure between the dusk side and the sun side has an affect on the position of the plasmapause on the sun side from side view. In simulation, the overall response of the plasmasphere to the magnetic storm is within 3 hours, but large magnetic storm has a long-term impact on the plasmasphere, which can reach 1~2 days. Continuous magnetic storm events have a significant impact on the plasmasphere, there is a superimposed effect. Refilling of the plasmasphere takes longer than erosion.

     

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