Relativistic Electron Microbursts as High Energy Tail of Pulsating Aurora Electrons
書誌事項
- タイトル別名
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- Relativistic Electron Microbursts as High‐Energy Tail of Pulsating Aurora Electrons
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説明
In this study, by simulating the wave‐particle interactions, we show that subrelativistic/relativistic electron microbursts form the high‐energy tail of pulsating aurora (PsA). Whistler‐mode chorus waves that propagate along the magnetic field lines at high latitudes cause precipitation bursts of electrons with a wide energy range from a few kiloelectron volts (PsA) to several megaelectron volts (relativistic microbursts). The rising tone elements of chorus waves cause individual microbursts of subrelativistic/relativistic electrons and the internal modulation of PsA with a frequency of a few hertz. The chorus bursts for a few seconds cause the microburst trains of subrelativistic/relativistic electrons and the main pulsations of PsA. Our simulation studies demonstrate that both PsA and relativistic electron microbursts originate simultaneously from pitch angle scattering by chorus wave‐particle interactions along the field line.
収録刊行物
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- Geophysical Research Letters
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Geophysical Research Letters 47 (21), e90360-, 2020-11-16
American Geophysical Union (AGU)
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詳細情報 詳細情報について
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- CRID
- 1051130853452063488
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- NII論文ID
- 120006898199
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- ISSN
- 00948276
- 19448007
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- HANDLE
- 2433/258959
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- 本文言語コード
- en
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- 資料種別
- journal article
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- データソース種別
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