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第4次南極地域観測隊宇宙線部門船上観測報告(超高層物理部門)(<特集>南極シンポジウム)
https://doi.org/10.15094/00007052
https://doi.org/10.15094/000070527253274b-aa4a-4642-aed5-953548d11b27
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
KJ00002406716 (1.6 MB)
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| Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 公開日 | 1961-01-01 | |||||||||||||
| タイトル | ||||||||||||||
| タイトル | 第4次南極地域観測隊宇宙線部門船上観測報告(超高層物理部門)(<特集>南極シンポジウム) | |||||||||||||
| タイトル | ||||||||||||||
| タイトル | REPORT ON RESULTS OF COSMIC-RAY OBSERVATIONS ON M/S "SOYA" DURING THE PERIOD FROM NOVEMBER, 1959 TO APRIL, 1960 (UPPER ATMOSPHERE PHYSICS) (<Special Publication>Antarctic Symposium in Tokyo, 1960) | |||||||||||||
| 言語 | en | |||||||||||||
| 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 | 10.15094/00007052 | |||||||||||||
| 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4ジ ナンキョク チイキ カンソクタイ ウチュウセン ブモン センジョウ カンソク ホウコク | |||||||||||||
| 著者名(日) |
福島, 紳
× 福島, 紳
× 中村, 強
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| 著者名(英) |
FUKUSHIMA, Shin
× FUKUSHIMA, Shin
× NAKAMURA, Tsuyoshi
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| 著者所属(日) | ||||||||||||||
| 理化学研究所:第3次南極地域観測隊:第4次南極地域観測隊越冬隊 | ||||||||||||||
| 著者所属(日) | ||||||||||||||
| 東京天文台:第4次南極地域観測隊 | ||||||||||||||
| 抄録(英) | ||||||||||||||
| 内容記述タイプ | Other | |||||||||||||
| 内容記述 | The third latitude survey in cosmic-ray neutrons has been carried out along the same ship-route and by using the same apparatus as in the preceeding two surveys. Although the observation room was the same as that in the second survey, one additional room was constructed over our room. Thus, as observational conditions in the three latitude surveys are different from one another, the obtained results could not be compared in absolute intensity but in relative. The periods during which each survey was performed are represented with the corresponding sunspot relative numbers in Fig. 1, where a full curve shows the 12 months running average of monthly mean values in sunspot numbers. Fig. 2 shows 12 hour mean values for each latitude curve in the southern hemisphere. It is seen from the figure that the slope of latitude curve becomes gentle at the second survey and then almost recovers at the third. To explain such changes in primary cosmic-rays by terms of changes in solar activity represented by sunspot numbers as shown in Fig. 1, we suppose a hysteresis effect of solar activity upon cosmic-rays. In other words, changes in cosmic-rays do not immediately follow that in solar activity but about half a year later. | |||||||||||||
| 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 11, p. 885-893, 発行日 1961-01 |
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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 | |||||||||||||
