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第9次南極地域観測越冬隊宇宙線部門報告 : 宇宙線中性子連続観測(日本南極地域観測隊の報告)
https://doi.org/10.15094/00007638
https://doi.org/10.15094/00007638e350b01d-89b9-4659-bd2e-9b48aa4da325
名前 / ファイル | ライセンス | アクション |
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KJ00002476638 (3.6 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1971-12-01 | |||||
タイトル | ||||||
タイトル | 第9次南極地域観測越冬隊宇宙線部門報告 : 宇宙線中性子連続観測(日本南極地域観測隊の報告) | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Report of Cosmic-Ray Neutron Observation in the 9th Japanese Antarctic Research Expedition 1968-1969 (Reports of the Japanese Antarctic Research Expedition) | |||||
言語 | ||||||
言語 | jpn | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15094/00007638 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
論文名よみ | ||||||
その他のタイトル | ダイ9ジ ナンキョク チイキ カンソク エットウタイ ウチュウセン ブモン ホウコク ウチュウセン チュウセイシ レンゾク カンソク ニホン ナンキョク チイキ カンソクタイ ノ ホウコク | |||||
著者名(日) |
須田, 友重
× 須田, 友重× 小玉, 正弘 |
|||||
著者名(英) |
SUDA, Tomoshige
× SUDA, Tomoshige× KODAMA, Masahiro |
|||||
著者所属(日) | ||||||
気象研究所 | ||||||
著者所属(日) | ||||||
理化学研究所 | ||||||
著者所属(英) | ||||||
en | ||||||
Meteorological Research Institute | ||||||
著者所属(英) | ||||||
en | ||||||
The Institute of Physical and Chemical Research | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | From February 1968 to January 1969, cosmic ray nucleonic component was observed at Syowa Station, Antarctica (69°00'S, 39°35'E), using a duplicate set of 5-NM-64 super neutron monitor with a multiplicity meter. Almost complete observations were achieved except the lack of 4 consecutive days for one monitor. The mean multiplicity of the monitor is 1.42 ± 0.03 and is in agreement with the value of the standard 6-NM-64 monitor obtained by HATTON, et al. The mean life time of neutrons in the pile is found to be 547 ± ^<123>_<85>μs which is a little longer than that in the 6-NM-64 monitor. These results come from the pile which was constructed as a single pile consisting of 10-NM-64 neutron counters. The annual change of neutron intensity covers 9.0% in range, showing the maximum in April and the minimum in November, with larger disturbance in the later half year than in the former half. The multiplicity dependence of the barometric pressure effect and Forbush decreases are surveyed briefly. Using the data from three large Forbush decreases, the relation between the multiplicity events and their corresponding primary rigidities is discussed by comparing the latitude dependence of the amount of decrease. Descriptions and data of the solar cosmic ray event of November 18, 1968 are also given. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN00181831 | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00857289 | |||||
書誌情報 |
南極資料 巻 42, p. 1-15, 発行日 1971-12 |
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国際十進分類法 | ||||||
主題Scheme | UDC | |||||
主題 | 551.510.535/.537 | |||||
出版者 | ||||||
出版者 | 国立極地研究所 |