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  1. F300 宇宙地球環境研究所
  2. F300b 紀要
  3. 空電研究所報告
  4. 8(1-2)

IGYにおけるマイクロ派太陽電波の観測

http://hdl.handle.net/2237/21755
c603fbee-30bc-4022-9356-3d945c86b398
名前 / ファイル ライセンス アクション
bulria_8_1-2_67.pdf bulria_8_1-2_67.pdf (1.2 MB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2015-04-28
タイトル
タイトル IGYにおけるマイクロ派太陽電波の観測
その他のタイトル
その他のタイトル OBSERVATIONS OF SOLAR RADIO EMISSION AT MICROWAVE FREQUENCIES FOR IGY
著者 田中, 春夫

× 田中, 春夫

WEKO 57600

田中, 春夫

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柿沼, 隆清

× 柿沼, 隆清

WEKO 57601

柿沼, 隆清

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神藤, 英彦

× 神藤, 英彦

WEKO 57602

神藤, 英彦

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高柳, 利男

× 高柳, 利男

WEKO 57603

高柳, 利男

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鳥居, 近吉

× 鳥居, 近吉

WEKO 57604

鳥居, 近吉

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TANAKA, Haruo

× TANAKA, Haruo

WEKO 57605

TANAKA, Haruo

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KAKINUMA, Takakiyo

× KAKINUMA, Takakiyo

WEKO 57606

KAKINUMA, Takakiyo

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抄録
内容記述 Outline of the equipment used for solar radio observations at Toyokawa station which are in operation since the begining of IGY is described together with the method of tabulation. Percentage variation of the S-component versus frequency is calculated for the first half-year period of IGY, which shows a peak near 4000 Mc/s. Left-hand polarization of S-component prevails in this period at frequencies below 3750 Mc/s and there are many cases where the sense of polarization reverses between 3750 and 9400 Mc/s. Experiment has been made for detecting linear polarization at a frequency of 3750 ± 5 Mc/s, but we have yet no data to show the existence of linear polarization for both S-component and outstanding occurrences.
内容記述タイプ Abstract
出版者
出版者 名古屋大学空電研究所
言語
言語 jpn
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ departmental bulletin paper
ISSN(print)
収録物識別子タイプ ISSN
収録物識別子 0465-7756
書誌情報 空電研究所報告

巻 8, 号 1-2, p. 67-73, 発行日 1958-03-20
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/21755
識別子タイプ HDL
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