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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. 7(1-2)

太陽電波の観測と二三の考察

http://hdl.handle.net/2237/21745
65edc220-7aeb-4e30-8ae6-227d93f0c8a2
名前 / ファイル ライセンス アクション
bulria_7_1-2_66.pdf bulria_7_1-2_66.pdf (5.1 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 太陽電波の観測と二三の考察
その他のタイトル
その他のタイトル DATA ON SOLAR RADIO EMISSION WITH SOME NOTES
著者 柿沼, 隆清

× 柿沼, 隆清

WEKO 57553

柿沼, 隆清

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高柳, 利男

× 高柳, 利男

WEKO 57554

高柳, 利男

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太陽電波研究室一同

× 太陽電波研究室一同

WEKO 57555

太陽電波研究室一同

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Kakinuma, Takakiyo

× Kakinuma, Takakiyo

WEKO 57556

Kakinuma, Takakiyo

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Takayanagi, Toshio

× Takayanagi, Toshio

WEKO 57557

Takayanagi, Toshio

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other members of Radio Astronomy Section

× other members of Radio Astronomy Section

WEKO 57558

other members of Radio Astronomy Section

Search repository
抄録
内容記述 The results of observations by 3750 and 9400 Mc/s radiometers are tabulated. The daily flux density at both frequencies has a correlation coefficient of 0.95, and the S-component at 9400 Mc/s is 0.8 times as large as that at 3750 Mc/s. The sense of polarization at both frequencies is similar. The percentage polarization referring to the S-component of an isolated radio spot occasionally exceeds 30 percent at 9400 Mc/s, which is much larger than that at 3750 Mc/s. Some bursts show yet a remarkable structure of frequency spectrum at these super-high-frequencies. The observations with an 8-element interferometer have been made for five hours every day for locating sources of outstanding occurrences. A burst occasionally occurs in an emissive region where no intense radiation is usually observed.
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 7, 号 1-2, p. 66-99, 発行日 1957-05-25
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/21745
識別子タイプ HDL
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