Statistical distribution of EMIC wave spectra: Observations from Van Allen Probes

被引:86
作者
Zhang, X. -J. [1 ,2 ]
Li, W. [1 ,3 ]
Thorne, R. M. [1 ]
Angelopoulos, V. [2 ]
Bortnik, J. [1 ]
Kletzing, C. A. [4 ]
Kurth, W. S. [4 ]
Hospodarsky, G. B. [4 ]
机构
[1] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA 90095 USA
[2] Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA 90095 USA
[3] Boston Univ, Ctr Space Phys, Boston, MA 02215 USA
[4] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
基金
美国国家科学基金会;
关键词
ION-CYCLOTRON WAVES; RELATIVISTIC ELECTRON-PRECIPITATION; 1-2 MAGNETIC PULSATIONS; EQUATORIAL MAGNETOSPHERE; SCATTERING; LOCATION; EVENT; O+;
D O I
10.1002/2016GL071158
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
It has been known that electromagnetic ion cyclotron (EMIC) waves can precipitate ultrarelativistic electrons through cyclotron resonant scattering. However, the overall effectiveness of this mechanism has yet to be quantified, because it is difficult to obtain the global distribution of EMIC waves that usually exhibit limited spatial presence. We construct a statistical distribution of EMIC wave frequency spectra and their intensities based on Van Allen Probes measurements from September 2012 to December 2015. Our results show that as the ratio of plasma frequency over electron gyrofrequency increases, EMIC wave power becomes progressively dominated by the helium band. There is a pronounced dawn-dusk asymmetry in the wave amplitude and the frequency spectrum. The frequency spectrum does not follow the commonly used single-peak Gaussian function. Incorporating these realistic EMIC wave frequency spectra into radiation belt models is expected to improve the quantification of EMIC wave scattering effects in ultrarelativistic electron dynamics.
引用
收藏
页码:12348 / 12355
页数:8
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