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首页|期刊导航|地球与行星物理(英文)|Plasma depletions lasting into daytime during the recovery phase of a geomagnetic storm in May 2017:Analysis and simulation of GPS total electron content observations

Plasma depletions lasting into daytime during the recovery phase of a geomagnetic storm in May 2017:Analysis and simulation of GPS total electron content observations

Yuichi Otsuka Atsuki Shinbori Takuya Sori Takuya Tsugawa Michi Nishioka Joseph D.Huba

地球与行星物理(英文)2021,Vol.5Issue(5):427-434,8.
地球与行星物理(英文)2021,Vol.5Issue(5):427-434,8.DOI:10.26464/epp2021046

Plasma depletions lasting into daytime during the recovery phase of a geomagnetic storm in May 2017:Analysis and simulation of GPS total electron content observations

Plasma depletions lasting into daytime during the recovery phase of a geomagnetic storm in May 2017:Analysis and simulation of GPS total electron content observations

Yuichi Otsuka 1Atsuki Shinbori 1Takuya Sori 1Takuya Tsugawa 2Michi Nishioka 2Joseph D.Huba3

作者信息

  • 1. Institute for Space-Earth Environmental Research,Nagoya University,Nagoya,Japan
  • 2. National Institute of Information and Communications Technology,Tokyo,Japan
  • 3. Syntek Technologies,Fairfax,VA,USA
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摘要

关键词

plasma bubble/GPS/ionosphere/ionospheric irregularity/SAMI2

Key words

plasma bubble/GPS/ionosphere/ionospheric irregularity/SAMI2

引用本文复制引用

Yuichi Otsuka,Atsuki Shinbori,Takuya Sori,Takuya Tsugawa,Michi Nishioka,Joseph D.Huba..Plasma depletions lasting into daytime during the recovery phase of a geomagnetic storm in May 2017:Analysis and simulation of GPS total electron content observations[J].地球与行星物理(英文),2021,5(5):427-434,8.

基金项目

The GPS data in Japan were provided by The Geospatial Informa-tion Authority of Japan.The GPS-TEC data are archived by the Na-tional Institute of Information and Communications Technology,Japan.The SYM-H index was obtained from the GSFC/SPDF OMNI-Web(https://omniweb.gsfc.nasa.gov).IMF data were provided by NASA's CDAWeb(https://cdaweb.sci.gsfc.nasa.gov/index/.html).The Kp index was provided by the WDC for Geomagnetism,Kyoto(http://wdc.kugi.kyoto-u.ac.jp/wdc/Sec3.html).This work was sup-ported by the Japan Society for the Promotion of Science,KAKENHI Grants,16H06286 and 20H00197.This research was sup-ported by NASA(NNH17ZDA001N07)and NSF(AGS-1931415)grants(JDH). (https://omniweb.gsfc.nasa.gov)

地球与行星物理(英文)

OACSCDEI

2096-3955

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