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  1. 040 理学部
  2. 0402 紀要
  3. 04021 Journal of the Faculty of Science, Shinshu University
  4. Vol. 05

Theoretical Calculation of Cosmic-Ray Solar Semi-Diurnal Variation -Nucleonic Component

http://hdl.handle.net/10091/10437
http://hdl.handle.net/10091/10437
dd21eb2d-a575-4ac4-9f58-73ebd0bebcd9
名前 / ファイル ライセンス アクション
Science05-01-06.pdf Science05-01-06.pdf (1.2 MB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2010-10-06
タイトル
言語 en
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

WEKO 37290

en MORI, SATORU

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YASUE, SHIN-ICHI

× YASUE, SHIN-ICHI

WEKO 37291

en YASUE, SHIN-ICHI

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出版者
出版者 信州大学理学部
引用
内容記述タイプ Other
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
抄録
内容記述タイプ Abstract
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)
内容記述タイプ Other
内容記述 Article
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
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