Volume 30 Issue 4
Jul.  2010
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Y. Miyashita. Observations of magnetic reconnection in the magnetotail associated with substorms[J]. Chinese Journal of Space Science, 2010, 30(4): 312-320. doi: 10.11728/cjss2010.04.312
Citation: Y. Miyashita. Observations of magnetic reconnection in the magnetotail associated with substorms[J]. Chinese Journal of Space Science, 2010, 30(4): 312-320. doi: 10.11728/cjss2010.04.312

Observations of magnetic reconnection in the magnetotail associated with substorms

doi: 10.11728/cjss2010.04.312 cstr: 32142.14.cjss2010.04.312
  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2010-07-15
  • Magnetic reconnection is one of the most important, dynamic phenomena in the magnetotail in terms of magnetic field line configuration change and energy release. It is believed to occur in the distant magnetotail mainly during southward interplanetary magnetic field periods and in the near-Earth magnetotail in association with substorms. In the present paper, we discuss several important issues concerning magnetic reconnection in the magnetotail associated with substorms, such as reconnection signatures, location, timing, spatial scale, and behavior, from the macroscopic, observational point of view.

     

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