globalchange  > 气候减缓与适应
DOI: 10.1002/2017JA024676
Scopus记录号: 2-s2.0-85041222391
论文题名:
The Effect of Hot Protons on Magnetosonic Waves Inside and Outside the Plasmapause: New Observations and Theoretic Results
作者: Liu B.; Li L.; Yu J.; Cao J.
刊名: Journal of Geophysical Research: Space Physics
ISSN: 21699380
出版年: 2018
卷: 123, 期:1
起始页码: 653
结束页码: 664
语种: 英语
英文关键词: damping of magnetosonic waves ; growth of magnetosonic waves ; magnetosonic waves ; magnetospheric hot protons ; wave-particle interactions
英文摘要: Based on the wave and proton observations by Van Allen Probes A and B, we examined the effects of hot protons (0.01–50 keV) on fast magnetosonic (MS) waves inside and outside the Earth's plasmasphere. In the low-density plasma trough outside the plasmapause, the gyroresonance interactions between hot protons and MS waves not only cause the MS wave growth at some frequencies but also lead to the damping of MS waves at other frequencies, which depends on the proton phase space density gradient and the ambient plasma density. The gyroresonance of the observed hot protons cannot excite MS waves near the lower hybrid resonance frequency and even causes the MS wave damping. Thus, the frequencies of the observed MS waves outside the plasmapause are usually lower than the lower hybrid resonance frequency. In the high-density plasmasphere, the observed hot protons merely lead to the weak gyrodamping of MS waves. The persistent existence of lower band MS waves indicates that the weak gyrodamping effect of hot protons on MS waves is ignorable in the high-density plasmasphere. ©2018. American Geophysical Union. All Rights Reserved.
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/114806
Appears in Collections:气候减缓与适应

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作者单位: School of Space and Environment, Beihang University, Beijing, China

Recommended Citation:
Liu B.,Li L.,Yu J.,et al. The Effect of Hot Protons on Magnetosonic Waves Inside and Outside the Plasmapause: New Observations and Theoretic Results[J]. Journal of Geophysical Research: Space Physics,2018-01-01,123(1)
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