The Evolution of a Pitch-Angle "Bite-Out" Scattering Signature Caused by EMIC Wave Activity: A Case Study

被引:24
作者
Bingley, L. [1 ]
Angelopoulos, V [1 ]
Sibeck, D. [2 ]
Zhang, X. [1 ]
Halford, A. [3 ]
机构
[1] Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA 90095 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
[3] Aerosp Corp, Chantilly, VA USA
关键词
ION-CYCLOTRON WAVES; VAN ALLEN PROBES; RELATIVISTIC ELECTRON-PRECIPITATION; RADIATION BELT ELECTRONS; GEOMAGNETIC STORMS; DISTRIBUTIONS; ACCELERATION; PARTICLE; EVENT;
D O I
10.1029/2018JA026292
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Electromagnetic ion cyclotron (EMIC) waves are understood to be one of the dominant drivers of relativistic electron loss from Earth's radiation belts. Theory predicts that the associated gyroresonant wave-particle interaction results in a distinct energy-dependent "bite-out" signature in the normalized flux distribution of electrons as they are scattered into the loss cone. We identify such signatures along with the responsible EMIC waves captured in situ by the Van Allen Probes on 15-16 February 2017. Using the cold plasma approximation, we predict the pitch-angle cutoffs for the scattering signature for the captured EMIC wave and find it in good agreement with the observed electron bite-out scattering signature. Employing the close conjunction between the Van Allen Probes and THEMIS during this time, we explore the temporal and spatial evolution of the scattering signature, as well as the surrounding wave activity, and find that the scattering signature formed during continued wave activity over a period less than a day. These results are consistent with wave-particle interaction theory and support the hypothesis that EMIC waves are an important mechanism for rapid relativistic electron loss from the radiation belts.
引用
收藏
页码:5042 / 5055
页数:14
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