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DOI10.1029/2019GL086040
Comprehensive Observations of Substorm-Enhanced Plasmaspheric Hiss Generation; Propagation; and Dissipation
Liu N.; Su Z.; Gao Z.; Zheng H.; Wang Y.; Wang S.; Miyoshi Y.; Shinohara I.; Kasahara Y.; Tsuchiya F.; Kumamoto A.; Matsuda S.; Shoji M.; Mitani T.; Takashima T.; Kazama Y.; Wang B.-J.; Wang S.-Y.; Jun C.-W.; Chang T.-F.; Tam S.W.Y.; Kasahara S.; Yokota S.; Keika K.; Hori T.; Matsuoka A.
发表日期2020
ISSN 0094-8276
卷号47期号:2
英文摘要Plasmaspheric hiss is an important whistler-mode emission shaping the Van Allen radiation belt environment. How the plasmaspheric hiss waves are generated, propagate, and dissipate remains under intense debate. With the five spacecraft of Van Allen Probes, Exploration of energization and Radiation in Geospace (Arase), and Geostationary Operational Environmental Satellites missions at widely spaced locations, we present here the first comprehensive observations of hiss waves growing from the substorm-injected electron instability, spreading within the plasmasphere, and dissipating over a large spatial scale. During substorms, hot electrons were injected energy-dispersively into the plasmasphere near the dawnside and, probably through a combination of linear and nonlinear cyclotron resonances, generated whistler-mode waves with globally drifting frequencies. These waves were able to propagate from the dawnside to the noonside, with the frequency-drifting feature retained. Approximately 5 hr of magnetic local time away from the source region in the dayside sector, the wave power was dissipated to (Formula presented.) of its original level. ©2020. American Geophysical Union. All Rights Reserved.
英文关键词Geostationary satellites; Hot electrons; Ionizing radiation; Radiation belts; Wave power; Wave propagation; Geostationary operational environmental satellites; Large spatial scale; Magnetic local time; Plasmasphere; plasmaspheric hiss; Van allen radiation belts; Wave dissipation; Wave generation; Atmospherics; energy dissipation; geostationary satellite; observational method; plasma; probe; radiation balance; satellite mission; spacecraft; storm; wave generation; wave propagation
语种英语
来源期刊Geophysical Research Letters
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/170813
作者单位CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China; CAS Center for Excellence in Comparative Planetology, University of Science and Technology of China, Hefei, China; Mengcheng National Geophysical Observatory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China; Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, China; School of Physics and Electronic Sciences, Changsha University of Science and Technology, Changsha, China; Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan; Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Kanagawa, Japan; Graduate School of Natural Science and Technology, Kanazawa University, Kanazawa, Japan; Graduate School of Science, Tohoku University, Sendai, Japan; Academia Sinica Institute of Astronomy and Astrophysics, Taipei, Taiw...
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Liu N.,Su Z.,Gao Z.,et al. Comprehensive Observations of Substorm-Enhanced Plasmaspheric Hiss Generation; Propagation; and Dissipation[J],2020,47(2).
APA Liu N..,Su Z..,Gao Z..,Zheng H..,Wang Y..,...&Matsuoka A..(2020).Comprehensive Observations of Substorm-Enhanced Plasmaspheric Hiss Generation; Propagation; and Dissipation.Geophysical Research Letters,47(2).
MLA Liu N.,et al."Comprehensive Observations of Substorm-Enhanced Plasmaspheric Hiss Generation; Propagation; and Dissipation".Geophysical Research Letters 47.2(2020).
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