Citation:
ZhongLei Gao, ZhenPeng Su, FuLiang Xiao, HuiNan Zheng, YuMing Wang, Shui Wang, H. E. Spence, G. D. Reeves, D. N. Baker, J. B. Blake, H. O. Funsten,
2018: Exohiss wave enhancement following substorm electron injection in the dayside magnetosphere, Earth and Planetary Physics, 2, 359-370.
http://doi.org/10.26464/epp2018033
2018, 2(5): 359-370. doi: 10.26464/epp2018033
Exohiss wave enhancement following substorm electron injection in the dayside magnetosphere
| 1. | School of Physics and Electronic Sciences, Changsha University of Science and Technology, Changsha 410004, China |
| 2. | CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China |
| 3. | Collaborative Innovation Center of Astronautical Science and Technology, University of Science and Technology of China, Hefei 230026, China |
| 4. | Mengcheng National Geophysical Observatory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China |
| 5. | Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, New Hampshire, USA |
| 6. | Space Science and Applications Group, Los Alamos National Laboratory, Los Alamos, New Mexico, USA |
| 7. | Space Sciences Division, New Mexico Consortium, Los Alamos, New Mexico, USA |
| 8. | Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Colorado, USA |
| 9. | The Aerospace Corporation, Los Angeles, California, USA |
| 10. | ISR Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA |
Exohiss is a low-frequency structureless whistler-mode emission potentially contributing to the precipitation loss of radiation belt electrons outside the plasmasphere. Exohiss is usually considered the plasmaspheric hiss leaked out of the dayside plasmapause. However, the evolution of exohiss after the leakage has not been fully understood. Here we report the prompt enhancements of exohiss waves following substorm injections observed by Van Allen Probes. Within several minutes, the energetic electron fluxes around 100 keV were enhanced by up to 5 times, accompanied by an up to 10-time increase of the exohiss wave power. These substorm-injected electrons are shown to produce a new peak of linear growth rate in the exohiss band (< 0.1fce). The corresponding path-integrated growth rate of wave power within 10° latitude of the magnetic equatorial plane can reach 13.4, approximately explaining the observed enhancement of exohiss waves. These observations and simulations suggest that the substorm-injected energetic electrons could amplify the preexisting exohiss waves.
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