WEKO3
アイテム
{"_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": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "1970-10-05", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "1", "bibliographicPageEnd": "64", "bibliographicPageStart": "37", "bibliographicVolumeNumber": "5", "bibliographic_titles": [{"bibliographic_title": "信州大学理学部紀要"}]}]}, "item_10_description_20": {"attribute_name": "抄録", "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^γexp(-R/R_0) and the latitude distribution has a form of (√3)/2cos^2λ.", "subitem_description_type": "Abstract"}]}, "item_10_description_30": {"attribute_name": "資源タイプ(コンテンツの種類)", "attribute_value_mlt": [{"subitem_description": "Article", "subitem_description_type": "Other"}]}, "item_10_description_31": {"attribute_name": "フォーマット:mimeタイプ", "attribute_value_mlt": [{"subitem_description": "application/pdf", "subitem_description_type": "Other"}]}, "item_10_description_5": {"attribute_name": "引用", "attribute_value_mlt": [{"subitem_description": "信州大学理学部紀要 5(1): 37-64(1970)", "subitem_description_type": "Other"}]}, "item_10_publisher_4": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "信州大学理学部"}]}, "item_10_select_64": {"attribute_name": "著者版フラグ", "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": "PISSN"}]}, "item_10_source_id_39": {"attribute_name": "NII ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0583-063X", "subitem_source_identifier_type": "PISSN"}]}, "item_10_source_id_40": {"attribute_name": "書誌レコードID", "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": "出版タイプ", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_970fb48d4fbd8a85", "subitem_version_type": "VoR"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "MORI, SATORU", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "37290", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "YASUE, SHIN-ICHI", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "37291", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "ファイル情報", "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": "言語", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "資源タイプ", "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": "タイトル", "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": ["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}
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 |
---|---|---|
![]() |
|
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× YASUE, SHIN-ICHI |
|||||
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 |