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Theoretical Calculation of Cosmic-Ray Solar Semi-Diurnal Variation -Nucleonic Component
http://hdl.handle.net/10091/10437
http://hdl.handle.net/10091/10437dd21eb2d-a575-4ac4-9f58-73ebd0bebcd9
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
Science05-01-06.pdf (1.2 MB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||||||
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| 公開日 | 2010-10-06 | |||||||||
| タイトル | ||||||||||
| タイトル | Theoretical Calculation of Cosmic-Ray Solar Semi-Diurnal Variation -Nucleonic Component | |||||||||
| 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 | |||||||||
| 著者 |
MORI, SATORU
× MORI, SATORU
× YASUE, SHIN-ICHI
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| 出版者 | ||||||||||
| 出版者 | 信州大学理学部 | |||||||||
| 引用 | ||||||||||
| 内容記述 | 信州大学理学部紀要 5(1): 37-64(1970) | |||||||||
| 書誌情報 |
信州大学理学部紀要 巻 5, 号 1, p. 37-64, 発行日 1970-10-05 |
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| 抄録 | ||||||||||
| 内容記述 | Theoretical calculations of the solar semi-diurnal variation expected at 41 stations for the nucleonic component have been made for two types of spectra, the power- and exponential-type. The latitude distribution of the semi-diurnal anisotropy has also been considered of both forms of the cosine- and the square of the cosine-function of the geographic latitude. Calculated results for four cases of the combination of these spectral and latitude dependences are compared. It is found that a difference in the results for the two types of the latitude distribution is appreciably large, particularly in the amplitude at high and very high latitude stations. A tendency is also shown in comparison of the results for the two types of spectral dependences that the calculated values with some higher cut-off rigidity in the power-type spectrum rather corresponds to the values with the rigidity giving the peak intensity in the exponential-type spectrum. Finally the expected relative amplitude and average deflection angle are tabulated for the case where the spectral form is of the exponential-type of R^γexp(-R/R_0) and the latitude distribution has a form of (√3)/2cos^2λ. | |||||||||
| 資源タイプ（コンテンツの種類） | ||||||||||
| ISSN | ||||||||||
| 収録物識別子タイプ | PISSN | |||||||||
| 収録物識別子 | 0583-063X | |||||||||
| 書誌レコードID | ||||||||||
| 収録物識別子タイプ | NCID | |||||||||
| 収録物識別子 | AA00697923 | |||||||||
| 出版タイプ | ||||||||||
| 出版タイプ | VoR | |||||||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||||||
