{"created":"2023-06-20T15:02:16.222704+00:00","id":31357,"links":{},"metadata":{"_buckets":{"deposit":"de86ecb5-f08a-401f-ac3c-a43c7928be6d"},"_deposit":{"created_by":1,"id":"31357","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"31357"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00031357","sets":["1887:1890","1896:1898:1899:1903"]},"author_link":["404092"],"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1982-07","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"8","bibliographicPageStart":"1","bibliographicVolumeNumber":"600","bibliographic_titles":[{},{"bibliographic_title":"The Institute of Space and Astronautical Science report","bibliographic_titleLang":"en"}]}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"The origin of shift of spectral lines that are emitted from stars is generally assumed to be due to either of the following causes or combination of them : (1) Doppler effect, (2) plasma shift, (3) Einstein's general-relativistic redshift. Of these, (1) and (2) are discussed in detail. In connection with the Doppler effect, the reason of the fact that Hubble's constant can take a variety of values is explained. There are cases in which Doppler effect is negligible and plasma shift dominates. As an example, the shifts of spectral lines emitted from the symbiotic Cl Cygni in quiescent state and tabulated in the literature (reporting the spectroscopic observation done during the period between July 1980 and October 1980) are ascribed to plasma shifts alone.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0034911000","subitem_description_type":"Other"}]},"item_9_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙科学研究所"}]},"item_9_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science"}]},"item_9_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0285-6808","subitem_source_identifier_type":"ISSN"}]},"item_9_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA10632072","subitem_source_identifier_type":"NCID"}]},"item_9_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Emeritus Professor of the University of Tokyo."}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"MURAKAWA, Kiyoshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2020-01-23"}],"displaytype":"detail","filename":"SA0034911.pdf","filesize":[{"value":"480.7 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0034911.pdf","url":"https://jaxa.repo.nii.ac.jp/record/31357/files/SA0034911.pdf"},"version_id":"122914ff-cf89-449f-8d68-4864aa50bafb"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"cosmology","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"plasma shift","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Cl Cygni","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"Shifts of Spectral Lines emitted from Stars","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Shifts of Spectral Lines emitted from Stars","subitem_title_language":"en"}]},"item_type_id":"9","owner":"1","path":["1890","1903"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"31357","relation_version_is_last":true,"title":["Shifts of Spectral Lines emitted from Stars"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T01:02:16.877034+00:00"}