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On the solar activity dependence of midnight equatorial plasma bubbles during June solstice periods

K.K.Ajith S.Tulasi Ram GuoZhu Li M.Yamamoto K.Hozumi C.Y.Yatini P.Supnithi

地球与行星物理(英文)2021,Vol.5Issue(5):378-386,9.
地球与行星物理(英文)2021,Vol.5Issue(5):378-386,9.DOI:10.26464/epp2021039

On the solar activity dependence of midnight equatorial plasma bubbles during June solstice periods

On the solar activity dependence of midnight equatorial plasma bubbles during June solstice periods

K.K.Ajith 1S.Tulasi Ram 2GuoZhu Li 1M.Yamamoto 3K.Hozumi 4C.Y.Yatini 5P.Supnithi6

作者信息

  • 1. Key Laboratory of Earth and Planetary Physics,Institute of Geology and Geophysics,Chinese Academy of Sciences,Beijing 100029,China
  • 2. Indian Institute of Geomagnetism,Mumbai,India
  • 3. Beijing National Observatory of Space Environment,Institute of Geology and Geophysics,Chinese Academy of Sciences,Beijing 100029,China
  • 4. College of Earth and Planetary Sciences,University of Chinese Academy of Sciences,Beijing 100049,China
  • 5. Research Institute for Sustainable Humanosphere,Kyoto University,Uji,Japan
  • 6. National Institute of Information and Communications Technology,Tokyo,Japan
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摘要

关键词

equatorial plasma bubbles/equatorial ionosphere/ionospheric instabilities and irregularities

Key words

equatorial plasma bubbles/equatorial ionosphere/ionospheric instabilities and irregularities

引用本文复制引用

K.K.Ajith,S.Tulasi Ram,GuoZhu Li,M.Yamamoto,K.Hozumi,C.Y.Yatini,P.Supnithi..On the solar activity dependence of midnight equatorial plasma bubbles during June solstice periods[J].地球与行星物理(英文),2021,5(5):378-386,9.

基金项目

This work was partly supported by the National Natural Science Foundation of China(42020104002)and by a Postdoctoral Fellow-ship at the Institute of Geology and Geophysics,Chinese Academy of Sciences(IGGCAS).K.Hozumi was partially supported by JSPS KAKENHI Grant Number 20H00197.The EAR data can be obtained from http://www.rish.kyoto-u.ac.jp/ear/index-e.html.The CPN and KTB ionosonde data are available under SEALION network at ht-tps://aer-nc-web.nict.go.jp/sealion/.The CINDI-IVM data are provided through the auspices of the CINDI team at the Uni-versity of Texas at Dallas,supported by NASA grant NAS5-01068(https://cdaweb.gsfc.nasa.gov/index.html/).The F10.7 cm solar flux is obtained from https://omniweb.gsfc.nasa.gov/form/dx1.html. (42020104002)

地球与行星物理(英文)

OACSCDEI

2096-3955

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