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  1. F300 宇宙地球環境研究所
  2. F300b 紀要
  3. Proceedings of the Research Institute of Atmospherics, Nagoya University
  4. 18

PRELIMINARY OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 69.3 MHz

http://hdl.handle.net/2237/22176
http://hdl.handle.net/2237/22176
ecb2774d-4012-44ad-ab5f-3e6a3588f845
名前 / ファイル ライセンス アクション
proria_18_59.pdf proria_18_59.pdf (1.9 MB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2015-06-01
タイトル
タイトル PRELIMINARY OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 69.3 MHz
言語 en
著者 WATANABE, Takashi

× WATANABE, Takashi

WEKO 59129

en WATANABE, Takashi

Search repository
WASHIMI, Haruichi

× WASHIMI, Haruichi

WEKO 59130

en WASHIMI, Haruichi

Search repository
KAKINUMA, Takakiyo

× KAKINUMA, Takakiyo

WEKO 59131

en KAKINUMA, Takakiyo

Search repository
KOJIMA, Masayoshi

× KOJIMA, Masayoshi

WEKO 59132

en KOJIMA, Masayoshi

Search repository
MARUYAMA, Kazuo

× MARUYAMA, Kazuo

WEKO 59133

en MARUYAMA, Kazuo

Search repository
ISHIDA, Yoshio

× ISHIDA, Yoshio

WEKO 59134

en ISHIDA, Yoshio

Search repository
アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
抄録
内容記述 Observations of interplanetary scintillation of radio sources for studying the solar wind have been carried out at two stations, Toyokawa and Fujigane, since June, 1970. The aerial is a square array containing 256 half-wave dipoles. A phase-switching receiver and a recording system which assure the simultaneity of the records taken at the two stations are used. The observational data are analysed by the statistical method. The velocity enhancements of the solar wind which correspond to the Forbush decrease and the geomagnetic storm have been detected by the observation of 3C 48 about 3 days after the solar flare. There is a tendency for the scale of the diffraction pattern to increase with increasing velocity, as pointed out by Vitkevich and Vlasov. The average scale of the diffraction pattern is about 300 km and it appears that the scale of the pattern or the size of the density fluctuations in the solar wind increases with increasing solar activity.
言語 en
内容記述タイプ Abstract
出版者
言語 en
出版者 The Research Institute of Atmospherics, Nagoya University
言語
言語 eng
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ departmental bulletin paper
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
ISSN(print)
収録物識別子タイプ PISSN
収録物識別子 0077-264X
書誌情報 en : Proceedings of the Research Institute of Atmospherics, Nagoya University

巻 18, p. 59-71, 発行日 1971-03-30
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/22176
識別子タイプ HDL
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