Multiple-Satellite Observation of Magnetic Dip Event During the Substorm on 10 October 2013
- Harbin Institute of Technology Shenzhen Graduate School, Shenzhen (China); Univ. of Science and Technology of China, Hefei (China); Univ. of Texas at Dallas, Richardson, TX (United States)
- Univ. of Texas at Dallas, Richardson, TX (United States)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Peking Univ., Beijing (China)
- Harbin Institute of Technology Shenzhen Graduate School, Shenzhen (China)
Here, we present a multiple-satellite observation of the magnetic dip event during the substorm on 10 October 2013. The observation illustrates the temporal and spatial evolution of the magnetic dip and gives a compelling evidence that ring current ions induce the magnetic dip by enhanced plasma beta. The dip moves with the energetic ions in a comparable drift velocity and affects the dynamics of relativistic electrons in the radiation belt. In addition, the magnetic dip provides a favorable condition for the electromagnetic ion cyclotron (EMIC) wave generation based on the linear theory analysis. The calculated proton diffusion coefficients show that the observed EMIC wave can lead to the pitch angle scattering losses of the ring current ions, which in turn partially relax the magnetic dip in the observations. This study enriches our understanding of magnetic dip evolution and demonstrates the important role of the magnetic dip for the coupling of radiation belt and ring current.
- Research Organization:
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- National Aeronautics and Space Administration (NASA); USDOE
- Grant/Contract Number:
- AC52-06NA25396
- OSTI ID:
- 1415429
- Report Number(s):
- LA-UR-17-30359; TRN: US1800822
- Journal Information:
- Geophysical Research Letters, Vol. 44, Issue 18; ISSN 0094-8276
- Publisher:
- American Geophysical UnionCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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