WEKO3
アイテム
{"_buckets": {"deposit": "b30b48ab-bfa2-419a-8cfb-293374fcf56d"}, "_deposit": {"created_by": 1, "id": "20331", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "20331"}, "status": "published"}, "_oai": {"id": "oai:jaxa.repo.nii.ac.jp:00020331", "sets": ["1786", "1891"]}, "author_link": ["194096", "194093", "194095", "194092", "194094"], "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": "Europa, the second Galilean satellites is an interesting object because subsurface ocean is thought to exist. The existence of the ocean has been proposed by researches such as the observation of induced magnetic field and the analysis of topography. However, these are not direct ones nor precise ones. In this report we propose a method for directing the subsurface ocean by using high energy cosmic neutrinos. We performed the simulation on detectability of interaction between the neutrinos and icy shell of Europa and recognized that the number of radiations caused by neutrinos depended on the thickness of the icy layer of Europa. We think that this method will be able to determine the thickness of ice and detect the subsurface ocean directly and accurately.", "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: AA0065116021", "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_35": {"attribute_name": "JAXAカテゴリ", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ: シンポジウム・研究会"}]}, "item_5_text_36": {"attribute_name": "JAXAカテゴリ2", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ2: IS"}]}, "item_5_text_42": {"attribute_name": "シンポジウム区分", "attribute_value_mlt": [{"subitem_text_value": "シンポジウム区分: 023"}]}, "item_5_text_43": {"attribute_name": "DSpaceコレクション番号", "attribute_value_mlt": [{"subitem_text_value": "DSpaceコレクション番号: 7"}]}, "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"}, {"subitem_text_value": "東京大学地震研究所"}, {"subitem_text_value": "東京大学地震研究所高エネルギー素粒子地球物理学研究センター"}]}, "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"}, {"subitem_text_language": "en", "subitem_text_value": "Earthquake Research Institute, University of Tokyo"}, {"subitem_text_language": "en", "subitem_text_value": "Center for High Energy Geophysics Research, Earthquake Research Institute, 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": "栗田, 敬"}], "nameIdentifiers": [{"nameIdentifier": "194092", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "田中, 宏幸"}], "nameIdentifiers": [{"nameIdentifier": "194093", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Daigo, Shoji", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "194094", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Kurita, Kei", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "194095", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Tanaka, Hiroyuki K. M.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "194096", "nameIdentifierScheme": "WEKO"}]}]}, "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": "A new method for detecting the subsurface ocean of Europa by using high energy neutrinos", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "A new method for detecting the subsurface ocean of Europa by using high energy neutrinos", "subitem_title_language": "en"}]}, "item_type_id": "5", "owner": "1", "path": ["1786", "1891"], "permalink_uri": "https://jaxa.repo.nii.ac.jp/records/20331", "pubdate": {"attribute_name": "公開日", "attribute_value": "2015-03-26"}, "publish_date": "2015-03-26", "publish_status": "0", "recid": "20331", "relation": {}, "relation_version_is_last": true, "title": ["A new method for detecting the subsurface ocean of Europa by using high energy neutrinos"], "weko_shared_id": -1}
A new method for detecting the subsurface ocean of Europa by using high energy neutrinos
https://jaxa.repo.nii.ac.jp/records/20331
https://jaxa.repo.nii.ac.jp/records/2033197a8fc38-5f8a-4b74-9283-3d1208b87bb6
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | A new method for detecting the subsurface ocean of Europa by using high energy neutrinos | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
栗田, 敬
× 栗田, 敬× 田中, 宏幸× Daigo, Shoji× Kurita, Kei× Tanaka, Hiroyuki K. M. |
|||||
著者所属 | ||||||
東京大学地震研究所 | ||||||
著者所属 | ||||||
東京大学地震研究所 | ||||||
著者所属 | ||||||
東京大学地震研究所高エネルギー素粒子地球物理学研究センター | ||||||
著者所属(英) | ||||||
en | ||||||
Earthquake Research Institute, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Earthquake Research Institute, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Center for High Energy Geophysics Research, Earthquake Research Institute, University of Tokyo | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | |||||
書誌情報 |
第43回月・惑星シンポジウム en : Proceedings of the 43th ISAS Lunar and Planetary Symposium 巻 43, 発行日 2010-08 |
|||||
会議概要(会議名, 開催地, 会期, 主催者等) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 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 | |||||
会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 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 | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Europa, the second Galilean satellites is an interesting object because subsurface ocean is thought to exist. The existence of the ocean has been proposed by researches such as the observation of induced magnetic field and the analysis of topography. However, these are not direct ones nor precise ones. In this report we propose a method for directing the subsurface ocean by using high energy cosmic neutrinos. We performed the simulation on detectability of interaction between the neutrinos and icy shell of Europa and recognized that the number of radiations caused by neutrinos depended on the thickness of the icy layer of Europa. We think that this method will be able to determine the thickness of ice and detect the subsurface ocean directly and accurately. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA12268968 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0065116021 |