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Identification of optical auroras caused by mantle precipitation with the aid of particle observations from DMSP satellites

HAN Desheng YANG Huigen

极地科学进展(英文版)2018,Vol.29Issue(4):233-242,10.
极地科学进展(英文版)2018,Vol.29Issue(4):233-242,10.DOI:10.13679/j.advps.2018.4.00233

Identification of optical auroras caused by mantle precipitation with the aid of particle observations from DMSP satellites

Identification of optical auroras caused by mantle precipitation with the aid of particle observations from DMSP satellites

HAN Desheng 1YANG Huigen2

作者信息

  • 1. State Key Laboratory of Marine Geology, School of Ocean and Earth Science, Tongji University, Shanghai 20092, China
  • 2. SOA Key Laboratory for Polar Science, Polar Research Institute of China, Shanghai 200136, China
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摘要

关键词

mantle aurora/plasma mantle/dayside aurora/high-latitude aurora

Key words

mantle aurora/plasma mantle/dayside aurora/high-latitude aurora

引用本文复制引用

HAN Desheng,YANG Huigen..Identification of optical auroras caused by mantle precipitation with the aid of particle observations from DMSP satellites[J].极地科学进展(英文版),2018,29(4):233-242,10.

基金项目

This work was supported by the National Natural Science Foundation of China (NSFC) (Grants nos. 41831072, 41774174, 41431072, 41474146, and 41674169). (NSFC)

极地科学进展(英文版)

OACSCDCSTPCD

1674-9928

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