{"_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", "sets": []}, "author_link": ["37290", "37291"], "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_31": {"attribute_name": "\u30d5\u30a9\u30fc\u30de\u30c3\u30c8\uff1amime\u30bf\u30a4\u30d7", "attribute_value_mlt": [{"subitem_description": "application/pdf", "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_select_64": {"attribute_name": "\u8457\u8005\u7248\u30d5\u30e9\u30b0", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "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_39": {"attribute_name": "NII 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_10_text_66": {"attribute_name": "sortkey", "attribute_value_mlt": [{"subitem_text_value": "06"}]}, "item_1627890569677": {"attribute_name": "\u51fa\u7248\u30bf\u30a4\u30d7", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_970fb48d4fbd8a85", "subitem_version_type": "VoR"}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "MORI,  SATORU"}], "nameIdentifiers": [{"nameIdentifier": "37290", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "YASUE,  SHIN-ICHI"}], "nameIdentifiers": [{"nameIdentifier": "37291", "nameIdentifierScheme": "WEKO"}]}]}, "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", "download_preview_message": "", "file_order": 0, "filename": "Science05-01-06.pdf", "filesize": [{"value": "1.2 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 1200000.0, "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", "subitem_title_language": "en"}]}, "item_type_id": "10", "owner": "1", "path": ["1169/1171/1172/1214"], "permalink_uri": "http://hdl.handle.net/10091/10437", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2010-10-06"}, "publish_date": "2010-10-06", "publish_status": "0", "recid": "12261", "relation": {}, "relation_version_is_last": true, "title": ["Theoretical Calculation of Cosmic-Ray Solar Semi-Diurnal Variation -Nucleonic Component"], "weko_shared_id": -1}