Responses of relativistic electron fluxes in the outer radiation belt to geomagnetic storms
Abstract
Geomagnetic storms can either increase or decrease relativistic electron fluxes in the outer radiation belt. A statistical survey of 84 isolated storms demonstrates that geomagnetic storms preferentially decrease relativistic electron fluxes at higher energies, while flux enhancements are more common at lower energies. In about 87% of the storms, 0.3–2.5 MeV electron fluxes show an increase, whereas 2.5–14 MeV electron fluxes increase in only 35% of the storms. Superposed epoch analyses suggest that such “energy‐dependent” responses of electrons preferably occur during conditions of high solar wind density which is favorable to generate magnetospheric electromagnetic ion cyclotron (EMIC) waves, and these events are associated with relatively weaker chorus activities. We have examined one of the cases where observed EMIC waves can resonate effectively with >2.5 MeV electrons and scatter them into the atmosphere. The correlation study further illustrates that electron flux dropouts during storm main phases do not correlate well with the flux buildup during storm recovery phases. We suggest that a combination of efficient EMIC‐induced scattering and weaker chorus‐driven acceleration provides a viable candidate for the energy‐dependent responses of outer radiation belt relativistic electrons to geomagnetic storms. These results are of great interest to both understanding of the radiation belt dynamics and applications in space weather.
Document Details
- Document Type
- Pub Defense Publication
- Publication Date
- Nov 01, 2015
- Source ID
- 10.1002/2015ja021440
Entities
People
- Binbin Ni
- G. K. Parks
- Jinxing Li
- Lun Xie
- Lunjin Chen
- Ruilong Guo
- S. Y. Fu
- Wen Li
- Ying Xiong
- Z. Y. Pu
Organizations
- Air Force Office of Scientific Research
- National Natural Science Foundation of China
- Peking University
- University of California, Los Angeles
- University of Texas at Dallas
- Wuhan University