Relativistic electron microbursts and variations in trapped MeV electron fluxes during the 8-9 October 2012 storm: SAMPEX and Van Allen Probes observations

被引:15
|
作者
Kurita, Satoshi [1 ]
Miyoshi, Yoshizumi [1 ]
Blake, J. Bernard [2 ]
Reeves, Geoffery D. [3 ]
Kletzing, Craig A. [4 ]
机构
[1] Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi 4648601, Japan
[2] Aerosp Corp, Dept Space Sci, El Segundo, CA 90245 USA
[3] Los Alamos Natl Lab, Space Sci & Applicat Grp, Los Alamos, NM USA
[4] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
基金
日本学术振兴会;
关键词
OUTER RADIATION BELT; GEOMAGNETIC STORMS; GEM STORMS; ACCELERATION; PRECIPITATION; CHORUS; LOSSES; WAVES; SOLAR;
D O I
10.1002/2016GL068260
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
It has been suggested that whistler mode chorus is responsible for both acceleration of MeV electrons and relativistic electron microbursts through resonant wave-particle interactions. Relativistic electron microbursts have been considered as an important loss mechanism of radiation belt electrons. Here we report on the observations of relativistic electron microbursts and flux variations of trapped MeV electrons during the 8-9 October 2012 storm, using the SAMPEX and Van Allen Probes satellites. Observations by the satellites show that relativistic electron microbursts correlate well with the rapid enhancement of trapped MeV electron fluxes by chorus wave-particle interactions, indicating that acceleration by chorus is much more efficient than losses by microbursts during the storm. It is also revealed that the strong chorus wave activity without relativistic electron microbursts does not lead to significant flux variations of relativistic electrons. Thus, effective acceleration of relativistic electrons is caused by chorus that can cause relativistic electron microbursts.
引用
收藏
页码:3017 / 3025
页数:9
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