{"created":"2023-07-25T11:03:13.215067+00:00","id":6047,"links":{},"metadata":{"_buckets":{"deposit":"f20f2885-7178-4f2a-b71a-74069cc14890"},"_deposit":{"created_by":4,"id":"6047","owners":[4],"pid":{"revision_id":0,"type":"depid","value":"6047"},"status":"published"},"_oai":{"id":"oai:nipr.repo.nii.ac.jp:00006047","sets":["1259:1260:1264:773:781"]},"author_link":["9942"],"item_1_alternative_title_5":{"attribute_name":"論文名よみ","attribute_value_mlt":[{"subitem_alternative_title":"Implications of isotopic anomalies and presolar grains for the formation of the solar system"}]},"item_1_biblio_info_14":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2004-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"152","bibliographicPageStart":"132","bibliographicVolumeNumber":"17","bibliographic_titles":[{"bibliographic_title":"Antarctic meteorite research"}]}]},"item_1_creator_8":{"attribute_name":"著者名(英)","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Huss,  Gary R.","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_1_description_1":{"attribute_name":"ページ属性","attribute_value_mlt":[{"subitem_description":"P(論文)","subitem_description_type":"Other"}]},"item_1_description_12":{"attribute_name":"抄録(英)","attribute_value_mlt":[{"subitem_description":"Isotopic anomalies are widespread in primitive chondritic meteorites and most of them can be tied to specific presolar materials from the Sun's parent molecular cloud. The known types of presolar materials come from many stellar and interstellar sources and exhibit a wide range of thermal and chemical stability. Bulk compositions and the abundances and characteristics of presolar grains indicate that CI chondrites and CM2 matrices originated from unfractionated samples of the Sun's parent molecular cloud. In the least metamorphosed members of other chondrite classes, correlations between the abundances and characteristics of presolar grains and the bulk compositional properties of the host meteorites indicate that the chondrite classes arose through different degrees of partial evaporation of the dust inherited from the Sun's parent molecular cloud. Condensation from a gas of solar composition is effectively ruled out as the primary mechanism for the volatility-controlled fractionations among the chondrite classes.","subitem_description_type":"Other"}]},"item_1_identifier_registration":{"attribute_name":"ID登録","attribute_value_mlt":[{"subitem_identifier_reg_text":"10.15094/00006047","subitem_identifier_reg_type":"JaLC"}]},"item_1_publisher_22":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"National Institute of Polar Research"}]},"item_1_source_id_13":{"attribute_name":"雑誌書誌ID","attribute_value_mlt":[{"subitem_source_identifier":"AA11182426","subitem_source_identifier_type":"NCID"}]},"item_1_text_10":{"attribute_name":"著者所属(英)","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Department of Geological Sciences and Center for Meteorite Studies, Arizona State"}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2004-09-01"}],"displaytype":"detail","filename":"KJ00002352028.pdf","filesize":[{"value":"825.3 kB"}],"format":"application/pdf","licensetype":"license_6","mimetype":"application/pdf","url":{"label":"KJ00002352028","url":"https://nipr.repo.nii.ac.jp/record/6047/files/KJ00002352028.pdf"},"version_id":"eeef17b6-338d-4ae8-8455-2bc5d11a85ca"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"isotopic anomalies, presolar grains, chemical fractionations, chondritic","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":"Implications of isotopic anomalies and presolar grains for the formation of the solar system","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Implications of isotopic anomalies and presolar grains for the formation of the solar system"}]},"item_type_id":"1","owner":"4","path":["781"],"pubdate":{"attribute_name":"公開日","attribute_value":"2004-09-01"},"publish_date":"2004-09-01","publish_status":"0","recid":"6047","relation_version_is_last":true,"title":["Implications of isotopic anomalies and presolar grains for the formation of the solar system"],"weko_creator_id":"4","weko_shared_id":4},"updated":"2023-07-25T12:06:58.600081+00:00"}