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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. 12

OBSERVATIONS OF RADIO SOURCES AT 9.4 GC/S WITH MASER AND HIGH-RESOLUTION INTERFEROMETER

http://hdl.handle.net/2237/21875
http://hdl.handle.net/2237/21875
b2d09632-0df0-4c22-8ada-60fc6a4ae8d5
名前 / ファイル ライセンス アクション
proria_12_35.pdf proria_12_35.pdf (1.9 MB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2015-05-12
タイトル
タイトル OBSERVATIONS OF RADIO SOURCES AT 9.4 GC/S WITH MASER AND HIGH-RESOLUTION INTERFEROMETER
言語 en
著者 TANAKA, Haruo

× TANAKA, Haruo

WEKO 58045

en TANAKA, Haruo

Search repository
KAKINUMA, Takakiyo

× KAKINUMA, Takakiyo

WEKO 58046

en KAKINUMA, Takakiyo

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YAMASHITA, Takashi

× YAMASHITA, Takashi

WEKO 58047

en YAMASHITA, Takashi

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UCHIDA, Hidenari

× UCHIDA, Hidenari

WEKO 58048

en UCHIDA, Hidenari

Search repository
INABA, Humio

× INABA, Humio

WEKO 58049

en INABA, Humio

Search repository
TSURU, Hiroshi

× TSURU, Hiroshi

WEKO 58050

en TSURU, Hiroshi

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TAKAHASHI, Kenichi

× TAKAHASHI, Kenichi

WEKO 58051

en TAKAHASHI, Kenichi

Search repository
YOSHIKAWA, Syogo

× YOSHIKAWA, Syogo

WEKO 58052

en YOSHIKAWA, Syogo

Search repository
HOZUMI, Hidekichi

× HOZUMI, Hidekichi

WEKO 58053

en HOZUMI, Hidekichi

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HAYASHI, Hiromi

× HAYASHI, Hiromi

WEKO 58054

en HAYASHI, Hiromi

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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 The observations at 9.4 Ge/s of Cygnus A, Taurus A, Orion Nebula and Omega Nebula have been made with the 2. 2' fan beam of the 16-element interferometer and the maser amplifier. Cygnus A has also been observed with the 0.7' fan beam of the compound interferometer. The maser amplifier for radio astronomical observations has been developed, with special emphasis on the high stable performance and the convenience of adjustment and handling in the field installations. The voltage-gain band-width product is about 100 Mc/s, the noise temperature is 40 K and the gain instability is 0.1 db up to 30 minutes and 0.2 db up to 2 hours. The brightness distributions, sizes and flux densities of the radio sources have been compared with the results of the earlier observations. Flux densities of the sources have been derived from that of the sun, comparing the areas under the drift-curves of the sources with that of the sun. The results of flux density measurements show that our scale of flux density at 9.4 Gc/s of the solar observations is nearly equal to the average scale of the galactic or extragalactic observations.
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 12, p. 35-48, 発行日 1965-03-25
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/21875
識別子タイプ HDL
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