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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. 8

OBSERVATIONS OF SOLAR RADIO EMISSION AT 9.4 Gc/s BY 16-ELEMENT INTERFEROMETER

http://hdl.handle.net/2237/21714
http://hdl.handle.net/2237/21714
bf4a55f9-28c1-4024-9577-043271af8fce
名前 / ファイル ライセンス アクション
proria_8_51.pdf proria_8_51.pdf (992.2 kB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2015-04-24
タイトル
タイトル OBSERVATIONS OF SOLAR RADIO EMISSION AT 9.4 Gc/s BY 16-ELEMENT INTERFEROMETER
言語 en
著者 TANAKA, HARUO

× TANAKA, HARUO

WEKO 57435

en TANAKA, HARUO

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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 16-element interferometer for use at 9.4 Gc/s was completed in the early summer of 1960. Maximum resolving power is 2.2'. Observations for more than 5 hours are being conducted every day. The most remarkable feature is the capability of taking 2 series of drift curves for both brightness and circular polarization. Bipolar nature of the source of polarization over the bipolar sunspot has now become clear. Size of a radio spot at this frequency seems to be not much larger than the area of optical sunspot in contrast with more diffused feature observed at lower frequencies. The size does not change appreciably during its travel across the solar disk. Some centers of polarization were found to shift during the 2nd phase of the em wave burst, probably due to the change of emission mechanism.
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 8, p. 51-56, 発行日 1961-06-15
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/21714
識別子タイプ HDL
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