{"created":"2023-06-20T14:52:26.278744+00:00","id":20577,"links":{},"metadata":{"_buckets":{"deposit":"adb9c776-f70e-403c-ba56-c66be321e823"},"_deposit":{"created_by":1,"id":"20577","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20577"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020577","sets":["1543:1778:1791","1887:1891"]},"author_link":["196339","196338","196337","196340"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006-03","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"235","bibliographicPageStart":"232","bibliographic_titles":[{"bibliographic_title":"第38回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 38th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Secular obliquity variations due to climate friction on Mars are calculated. Martian interior is considered to be a three-layered structure. A viscosity of each layer is treated as a parameter. The results give knowledge as follows. First, under an internal structure with a visco-elastic crust and/or a solid core, the effect of the climate friction becomes greater than that concluded by previous research. Second, under an internal structure with a heterogeneous mantle, the possibility of the great effect of the climate friction becomes stronger than that concluded by previous research.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063350062","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構宇宙科学研究本部"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"東京大学地震研究所 地球流動破壊部門"},{"subitem_text_value":"北海道大学 大学院理学研究科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Earthquake Research Institute, University of Tokyo Division of Earth Mechanics"},{"subitem_text_language":"en","subitem_text_value":"Hokkaido University Graduate School of Science"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"原田, 雄司"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"日置, 幸介"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Harada, Yuji","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Heki, Kosuke","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"火星","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星表面","subitem_subject_scheme":"Other"},{"subitem_subject":"気候摩擦","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星気象学","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星地質学","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星マントル","subitem_subject_scheme":"Other"},{"subitem_subject":"粘度","subitem_subject_scheme":"Other"},{"subitem_subject":"傾斜度","subitem_subject_scheme":"Other"},{"subitem_subject":"極域","subitem_subject_scheme":"Other"},{"subitem_subject":"極冠","subitem_subject_scheme":"Other"},{"subitem_subject":"曲げ剛性","subitem_subject_scheme":"Other"},{"subitem_subject":"Mars","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary surface","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"climate friction","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary meteorology","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary geology","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary mantle","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"viscosity","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"obliquity","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"polar region","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"polar cap","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"flexural rigidity","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":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"Secular obliquity variations due to climate friction on Mars: Re-examination in influence of Martian internal viscosity structure","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Secular obliquity variations due to climate friction on Mars: Re-examination in influence of Martian internal viscosity structure","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1791","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20577","relation_version_is_last":true,"title":["Secular obliquity variations due to climate friction on Mars: Re-examination in influence of Martian internal viscosity structure"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:48:17.854077+00:00"}