WEKO3
アイテム
{"_buckets": {"deposit": "0be98a14-7f2f-493f-8be1-94fed92bbc5c"}, "_deposit": {"created_by": 3, "id": "9379", "owners": [3], "pid": {"revision_id": 0, "type": "depid", "value": "9379"}, "status": "published"}, "_oai": {"id": "oai:ynu.repo.nii.ac.jp:00009379", "sets": ["496"]}, "author_link": ["34733", "714", "34731"], "item_2_biblio_info_8": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2018-04", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "5", "bibliographicPageStart": "1", "bibliographicVolumeNumber": "32", "bibliographic_titles": [{"bibliographic_title": "Biological Sciences in Space"}]}]}, "item_2_description_5": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "We propose radiation shielding using Martian magnetic anomalies to protect human crews on the Martian surface. We have simulated the trajectories of energetic protons using the Buneman-Boris method to measure how magnetic anomalies affect the impact rate on the Martian surface. Protons from the west can be completely eliminated, while those from the east are concentrated on the area between the magnetic poles. This would mean crews would need to concern themselves about radiation from the vertex and east only. A Martian magnetic anomaly can therefore be used to realize continuous and efficient radiation shielding.", "subitem_description_type": "Abstract"}]}, "item_2_publisher_35": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "Japanese Society for Biological Sciences in Space "}]}, "item_2_relation_13": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type": "isIdenticalTo", "subitem_relation_type_id": {"subitem_relation_type_id_text": "info:doi/10.2187/bss.32.1", "subitem_relation_type_select": "DOI"}}]}, "item_2_rights_14": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "© 2018 by Japanese Society for Biological Sciences in Space"}]}, "item_2_source_id_9": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "09149201", "subitem_source_identifier_type": "ISSN"}]}, "item_2_text_4": {"attribute_name": "著者所属", "attribute_value_mlt": [{"subitem_text_value": "Department of Systems Integration, Yokohama National University"}, {"subitem_text_value": "Division of Systems Research, Yokohama National University"}, {"subitem_text_value": "Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency"}]}, "item_2_version_type_18": {"attribute_name": "著者版フラグ", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_970fb48d4fbd8a85", "subitem_version_type": "VoR"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Emoto, Kazuma"}], "nameIdentifiers": [{"nameIdentifier": "34731", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Takao, Yoshinori"}], "nameIdentifiers": [{"nameIdentifier": "714", "nameIdentifierScheme": "WEKO"}, {"nameIdentifier": "80552661", "nameIdentifierScheme": "e-Rad", "nameIdentifierURI": "https://kaken.nii.ac.jp/ja/search/?qm=80552661"}]}, {"creatorNames": [{"creatorName": "Kuninaka, Hitoshi"}], "nameIdentifiers": [{"nameIdentifier": "34733", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2018-11-06"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "32_1.pdf", "filesize": [{"value": "2.5 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 2500000.0, "url": {"label": "32_1.pdf", "url": "https://ynu.repo.nii.ac.jp/record/9379/files/32_1.pdf"}, "version_id": "968707e6-daf8-430f-a6cf-fa21e2cb933e"}]}, "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": "journal article", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "A Preliminary Study on Radiation Shielding Using Martian Magnetic Anomalies", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "A Preliminary Study on Radiation Shielding Using Martian Magnetic Anomalies"}]}, "item_type_id": "2", "owner": "3", "path": ["496"], "permalink_uri": "http://hdl.handle.net/10131/00012049", "pubdate": {"attribute_name": "公開日", "attribute_value": "2018-11-06"}, "publish_date": "2018-11-06", "publish_status": "0", "recid": "9379", "relation": {}, "relation_version_is_last": true, "title": ["A Preliminary Study on Radiation Shielding Using Martian Magnetic Anomalies"], "weko_shared_id": 3}
A Preliminary Study on Radiation Shielding Using Martian Magnetic Anomalies
http://hdl.handle.net/10131/00012049
http://hdl.handle.net/10131/000120497a770587-6f9b-47cb-b53d-6c8fedd96679
名前 / ファイル | ライセンス | アクション |
---|---|---|
32_1.pdf (2.5 MB)
|
|
Item type | 学術雑誌論文 / Journal Article(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2018-11-06 | |||||
タイトル | ||||||
タイトル | A Preliminary Study on Radiation Shielding Using Martian Magnetic Anomalies | |||||
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_6501 | |||||
資源タイプ | journal article | |||||
著者 |
Emoto, Kazuma
× Emoto, Kazuma× Takao, Yoshinori× Kuninaka, Hitoshi |
|||||
著者所属 | ||||||
Department of Systems Integration, Yokohama National University | ||||||
著者所属 | ||||||
Division of Systems Research, Yokohama National University | ||||||
著者所属 | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency | ||||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | We propose radiation shielding using Martian magnetic anomalies to protect human crews on the Martian surface. We have simulated the trajectories of energetic protons using the Buneman-Boris method to measure how magnetic anomalies affect the impact rate on the Martian surface. Protons from the west can be completely eliminated, while those from the east are concentrated on the area between the magnetic poles. This would mean crews would need to concern themselves about radiation from the vertex and east only. A Martian magnetic anomaly can therefore be used to realize continuous and efficient radiation shielding. | |||||
書誌情報 |
Biological Sciences in Space 巻 32, p. 1-5, 発行日 2018-04 |
|||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 09149201 | |||||
DOI | ||||||
関連タイプ | isIdenticalTo | |||||
識別子タイプ | DOI | |||||
関連識別子 | info:doi/10.2187/bss.32.1 | |||||
権利 | ||||||
権利情報 | © 2018 by Japanese Society for Biological Sciences in Space | |||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
出版者 | ||||||
出版者 | Japanese Society for Biological Sciences in Space |