Can Solar Wind Decompressive Discontinuities Suppress Magnetospheric Electromagnetic Ion Cyclotron Waves Associated With Fresh Proton Injections?

被引:14
|
作者
Liu, Nigang [1 ,2 ,3 ]
Su, Zhenpeng [1 ,2 ]
Gao, Zhonglei [4 ,5 ]
Zheng, Huinan [1 ,2 ]
Wang, Yuming [1 ,2 ]
Wang, Shui [1 ,2 ]
机构
[1] Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei, Peoples R China
[2] Univ Sci & Technol China, CAS Ctr Excellence Comparat Planetol, Hefei, Peoples R China
[3] Univ Sci & Technol China, Anhui Mengcheng Geophys Natl Observat & Res Stn, Mengcheng, Peoples R China
[4] Harbin Inst Technol, Inst Space Sci & Appl Technol, Shenzhen, Peoples R China
[5] Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha, Peoples R China
基金
中国国家自然科学基金; 中国博士后科学基金;
关键词
EMIC waves</AUTHOR_KEYWORD>; solar wind discontinuity</AUTHOR_KEYWORD>; storm; substorm injection</AUTHOR_KEYWORD>; wave generation</AUTHOR_KEYWORD>; adiabatic deceleration</AUTHOR_KEYWORD>; inner magnetosphere</AUTHOR_KEYWORD>; VAN ALLEN PROBES; PITCH-ANGLE DISTRIBUTIONS; EMIC WAVES; DYNAMIC PRESSURE; RING CURRENT; ENERGETIC PARTICLE; LOW-FREQUENCY; TANGENTIAL DISCONTINUITIES; ROTATIONAL DISCONTINUITIES; MAGNETIC PULSATIONS;
D O I
10.1029/2020GL090296
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Electromagnetic ion cyclotron (EMIC) waves play an important role in the energy transfer among particles of different energies and species in the magnetosphere, whose drivers have been commonly recognized as solar wind compressions and storm/substorm proton injections. However, how the solar wind decompressions related to frequently occurring discontinuities compete with the proton injections in the evolution of EMIC waves has been rarely investigated. Here we present a complete end-to-end observation by Wind, THEMIS, and Van Allen Probes missions during the main phase of the 23 February 2014 storm of a succession of solar wind rotational discontinuities decompressing the magnetosphere within 200 s, adiabatically decelerating the freshly injected >10 keV protons, and thus suppressing the EMIC waves in the inner magnetosphere. Our results highlight the importance of solar wind conditions for the evolution of inner magnetospheric EMIC waves from a new perspective.
引用
收藏
页数:13
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