{"created":"2021-03-01T06:15:10.219330+00:00","id":12261,"links":{},"metadata":{"_buckets":{"deposit":"47cb7709-d0bd-4689-b5d8-f00bf6f03e0b"},"_deposit":{"id":"12261","owners":[],"pid":{"revision_id":0,"type":"depid","value":"12261"},"status":"published"},"_oai":{"id":"oai:soar-ir.repo.nii.ac.jp:00012261"},"item_10_biblio_info_6":{"attribute_name":"\u66f8\u8a8c\u60c5\u5831","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1970-10-05","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1","bibliographicPageEnd":"64","bibliographicPageStart":"37","bibliographicVolumeNumber":"5","bibliographic_titles":[{"bibliographic_title":"\u4fe1\u5dde\u5927\u5b66\u7406\u5b66\u90e8\u7d00\u8981"}]}]},"item_10_description_20":{"attribute_name":"\u6284\u9332","attribute_value_mlt":[{"subitem_description":"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^\u03b3exp(-R/R_0) and the latitude distribution has a form of (\u221a3)/2cos^2\u03bb.","subitem_description_type":"Abstract"}]},"item_10_description_30":{"attribute_name":"\u8cc7\u6e90\u30bf\u30a4\u30d7\uff08\u30b3\u30f3\u30c6\u30f3\u30c4\u306e\u7a2e\u985e\uff09","attribute_value_mlt":[{"subitem_description":"Article","subitem_description_type":"Other"}]},"item_10_description_5":{"attribute_name":"\u5f15\u7528","attribute_value_mlt":[{"subitem_description":"\u4fe1\u5dde\u5927\u5b66\u7406\u5b66\u90e8\u7d00\u8981 5(1): 37-64(1970)","subitem_description_type":"Other"}]},"item_10_publisher_4":{"attribute_name":"\u51fa\u7248\u8005","attribute_value_mlt":[{"subitem_publisher":"\u4fe1\u5dde\u5927\u5b66\u7406\u5b66\u90e8"}]},"item_10_source_id_35":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0583-063X","subitem_source_identifier_type":"ISSN"}]},"item_10_source_id_40":{"attribute_name":"\u66f8\u8a8c\u30ec\u30b3\u30fc\u30c9ID","attribute_value_mlt":[{"subitem_source_identifier":"AA00697923","subitem_source_identifier_type":"NCID"}]},"item_creator":{"attribute_name":"\u8457\u8005","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"MORI,  SATORU"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"YASUE,  SHIN-ICHI"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"\u30d5\u30a1\u30a4\u30eb\u60c5\u5831","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2015-09-28"}],"displaytype":"detail","filename":"Science05-01-06.pdf","filesize":[{"value":"1.2 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"Science05-01-06.pdf","url":"https://soar-ir.repo.nii.ac.jp/record/12261/files/Science05-01-06.pdf"},"version_id":"1066f01b-9d8a-430b-8295-793d59f4a1de"}]},"item_language":{"attribute_name":"\u8a00\u8a9e","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"\u8cc7\u6e90\u30bf\u30a4\u30d7","attribute_value_mlt":[{"resourcetype":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Theoretical Calculation of Cosmic-Ray Solar Semi-Diurnal Variation -Nucleonic Component","item_titles":{"attribute_name":"\u30bf\u30a4\u30c8\u30eb","attribute_value_mlt":[{"subitem_title":"Theoretical Calculation of Cosmic-Ray Solar Semi-Diurnal Variation -Nucleonic Component"}]},"item_type_id":"10","owner":"1","path":["1169/1171/1172/1214"],"pubdate":{"attribute_name":"\u516c\u958b\u65e5","attribute_value":"2010-10-06"},"publish_date":"2010-10-06","publish_status":"0","recid":"12261","relation_version_is_last":true,"title":["Theoretical Calculation of Cosmic-Ray Solar Semi-Diurnal Variation -Nucleonic Component"],"weko_creator_id":"1","weko_shared_id":null},"updated":"2021-03-01T11:31:14.556008+00:00"}