{"created":"2023-06-20T14:52:12.632551+00:00","id":20337,"links":{},"metadata":{"_buckets":{"deposit":"f865740d-daf6-4e68-9f7b-af5dbacb758b"},"_deposit":{"created_by":1,"id":"20337","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20337"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020337","sets":["1543:1778:1786","1887:1891"]},"author_link":["194137","194139","194138"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-08","bibliographicIssueDateType":"Issued"},"bibliographicVolumeNumber":"43","bibliographic_titles":[{"bibliographic_title":"第43回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 43th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_14":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）","attribute_value_mlt":[{"subitem_description":"第43回月・惑星シンポジウム (2010年8月4-6日. 宇宙航空研究開発機構宇宙科学研究所), 相模原市, 神奈川県","subitem_description_type":"Other"}]},"item_5_description_15":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）（英）","attribute_value_mlt":[{"subitem_description":"43rd  ISAS Lunar and Planetary Symposium (August 4-6,  2010. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Using High Resolution Imaging Science Experiment (HiRISE) images, we observe two significant gullies. First, we newly find gullies whose shapes are very strange, which we call \"dune gully\". Second, 10 dune gullies are observed which these are now active and growing. Previous work didn't show that dune gullies are universal on the surface of Mars. We map dune gullies' distribution in the mid-to-high-latitude area (60 deg S to 45 deg S, -30 deg E to 45 deg E) and find that dune gullies are not unique for Russell Crater. We also consider that what the source of active dune gullies is. Our results are that the source is the debris flow which contains liquid water, and these two facts imply that water cycle over wide area may occur.","subitem_description_type":"Other"}]},"item_5_description_18":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"形態: カラー図版あり","subitem_description_type":"Other"}]},"item_5_description_19":{"attribute_name":"内容記述（英）","attribute_value_mlt":[{"subitem_description":"Physical characteristics: Original contains color illustrations","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0065116027","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所 (JAXA)(ISAS)"}]},"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_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA12268968","subitem_source_identifier_type":"NCID"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"東京大学総合研究博物館"},{"subitem_text_value":"東京大学総合研究博物館"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Univerisity Museum, University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"Univerisity Museum, University of Tokyo"}]},"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":"宮本, 英昭"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Maeda, S.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Miyamoto, Hideaki","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"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":"Gullies over sand dune; Water-related formation and their distribution of mid-to-high-latitude of southern hemisphere on Mars","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Gullies over sand dune; Water-related formation and their distribution of mid-to-high-latitude of southern hemisphere on Mars","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1786","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20337","relation_version_is_last":true,"title":["Gullies over sand dune; Water-related formation and their distribution of mid-to-high-latitude of southern hemisphere on Mars"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:51:40.946506+00:00"}