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Solar wind dependence of the electron flux variation at geostationary orbit observed by ETS-V
https://doi.org/10.15094/00006340
https://doi.org/10.15094/00006340775663c6-d65f-470a-b8a7-8f5b34bdc226
名前 / ファイル | ライセンス | アクション |
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KJ00000048080 (921.5 kB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 2001-09-01 | |||||
タイトル | ||||||
タイトル | Solar wind dependence of the electron flux variation at geostationary orbit observed by ETS-V | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15094/00006340 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Yokoyama,N.
× Yokoyama,N.× Goka,T.× Matsumoto,H.× Koga,K.× Koshiishi, H.× Kimoto, Y. |
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著者所属(英) | ||||||
en | ||||||
National Space Development Agency of Japan/National Space Development Agency of Japan/National Space Development Agency of Japan/National Space Development Agency of Japan/National Space Development Agency of Japan/National Space Development Agency of Japan | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | In this study we have examined the relationship between the energetic electron flux at geostationary orbit and the solar wind speed. We have compared the electron flux ( >0.4MeV) observed by the Engineering Test Satellite V (ETS-V) with solar wind speed measurements in the OMNI data set obtained from the National Space Science Data Center (NSSDC). The tendency has been observed for the logarithm of the electron flux to be proportional to the solar wind speed at solar minimum, but scattered at solar maximum. We have found that during the main and recovery phases of magnetic storms occurring at solar minimum, the logarithm of the electron flux is roughly proportional to the solar wind speed. At solar maximum, however, there is no apparent correlation between both these parameters. Moreover, in quiet periods there is also no observable correlation at both solar minimum and maximum. The dependence of the electron flux at geostationary orbit on the solar wind speed is related to recurrent storms caused by high-speed solar wind streams. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11397422 | |||||
書誌情報 |
Advances in polar upper atmosphere research 巻 15, p. 193-200, 発行日 2001-09 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |