WEKO3
アイテム
{"_buckets": {"deposit": "98b7a2b4-1d07-4ae4-a388-a40c1ba5ad26"}, "_deposit": {"created_by": 1, "id": "5018", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "5018"}, "status": "published"}, "_oai": {"id": "oai:jaxa.repo.nii.ac.jp:00005018", "sets": ["948", "1891"]}, "author_link": ["23422", "23417", "23420", "23424", "23418", "23423", "23419", "23421"], "item_5_biblio_info_10": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2010-02-26", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "229", "bibliographicPageStart": "228", "bibliographicVolumeNumber": "JAXA-SP-09-008E", "bibliographic_titles": [{"bibliographic_title": "宇宙航空研究開発機構特別資料:"}, {"bibliographic_title": "JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H", "bibliographic_titleLang": "en"}]}]}, "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": "The 3rd Suzaku international Conference \"Energetic Cosmos : from Suzaku to ASTRO-H\" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan", "subitem_description_type": "Other"}]}, "item_5_description_17": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "The particle acceleration mechanism of pulsars has been an outstanding problem for more than forty years. A breakthrough can be provided by a large particle-simulation for the global magnetosphere showing the formation of the field-aligned electric field. However, this demands heavy calculation of Coulomb interaction. We have resolved this difficulty by use of GRAPE, which is a massively parallel special purpose computer for astronomical N-body problem at National Astronomical Observatory of Japan. Note that GRAPE can calculate Coulomb force as well as gravitational force because of the same inverse-square law and of sign-bit available with GRAPE. In this paper, we present a method of particle simulation for the global magnetosphere including electron-positron pair creation. We show some initial results of the simulation.", "subitem_description_type": "Other"}]}, "item_5_description_19": {"attribute_name": "内容記述(英)", "attribute_value_mlt": [{"subitem_description": "Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science", "subitem_description_type": "Other"}]}, "item_5_description_32": {"attribute_name": "資料番号", "attribute_value_mlt": [{"subitem_description": "資料番号: AA0064574086", "subitem_description_type": "Other"}]}, "item_5_description_33": {"attribute_name": "レポート番号", "attribute_value_mlt": [{"subitem_description": "レポート番号: JAXA-SP-09-008E", "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"}]}, "item_5_publisher_9": {"attribute_name": "出版者(英)", "attribute_value_mlt": [{"subitem_publisher": "Japan Aerospace Exploration Agency (JAXA)"}]}, "item_5_source_id_21": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "1349-113X", "subitem_source_identifier_type": "ISSN"}]}, "item_5_source_id_24": {"attribute_name": "書誌レコードID", "attribute_value_mlt": [{"subitem_source_identifier": "AA11984031", "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: 特別資料"}]}, "item_5_text_40": {"attribute_name": "jaxa出版物種類", "attribute_value_mlt": [{"subitem_text_value": "jaxa出版物種類: SP"}]}, "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": "山形大学大学院理工学研究科"}, {"subitem_text_value": "山形大学理学部"}, {"subitem_text_value": "国立天文台天文学データ解析計算センター"}, {"subitem_text_value": "山形大学大学院理工学研究科"}]}, "item_5_text_7": {"attribute_name": "著者所属(英)", "attribute_value_mlt": [{"subitem_text_language": "en", "subitem_text_value": "Graduate School of Science and Engineering, Yamagata University"}, {"subitem_text_language": "en", "subitem_text_value": "Department of Physics, Yamagata University"}, {"subitem_text_language": "en", "subitem_text_value": "Center for Computational Astrophysics, National Astronomical Observatory of Japan"}, {"subitem_text_language": "en", "subitem_text_value": "Graduate School of Science and Engineering, Yamagata University"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "結城, 伸哉"}], "nameIdentifiers": [{"nameIdentifier": "23417", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "柴田, 晋平"}], "nameIdentifiers": [{"nameIdentifier": "23418", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "和田, 智秀"}], "nameIdentifiers": [{"nameIdentifier": "23419", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "海崎, 光宏"}], "nameIdentifiers": [{"nameIdentifier": "23420", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Yuki, Shinya", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "23421", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Shibata, Shinpei", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "23422", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Wada, Tomohide", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "23423", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Umizaki, Mitsuhiro", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "23424", "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": "2020-01-16"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "64574086.pdf", "filesize": [{"value": "191.2 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 191200.0, "url": {"label": "64574086.pdf", "url": "https://jaxa.repo.nii.ac.jp/record/5018/files/64574086.pdf"}, "version_id": "672ecc75-d5a6-49e2-8cf1-ccb5c06bf2ae"}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "pulsars: general - magnetic field - plasmas", "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": "Method of Particle Simulation for the Pulsar Magnetosphere by Use of Special Purpose Computer, GRAPE-6", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Method of Particle Simulation for the Pulsar Magnetosphere by Use of Special Purpose Computer, GRAPE-6", "subitem_title_language": "en"}]}, "item_type_id": "5", "owner": "1", "path": ["948", "1891"], "permalink_uri": "https://jaxa.repo.nii.ac.jp/records/5018", "pubdate": {"attribute_name": "公開日", "attribute_value": "2015-03-26"}, "publish_date": "2015-03-26", "publish_status": "0", "recid": "5018", "relation": {}, "relation_version_is_last": true, "title": ["Method of Particle Simulation for the Pulsar Magnetosphere by Use of Special Purpose Computer, GRAPE-6"], "weko_shared_id": -1}
Method of Particle Simulation for the Pulsar Magnetosphere by Use of Special Purpose Computer, GRAPE-6
https://jaxa.repo.nii.ac.jp/records/5018
https://jaxa.repo.nii.ac.jp/records/501850e7ef57-8a21-4e91-832f-0c2462d8fefb
名前 / ファイル | ライセンス | アクション |
---|---|---|
64574086.pdf (191.2 kB)
|
|
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 | Method of Particle Simulation for the Pulsar Magnetosphere by Use of Special Purpose Computer, GRAPE-6 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | pulsars: general - magnetic field - plasmas | |||||
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 | |||||
著者 |
結城, 伸哉
× 結城, 伸哉× 柴田, 晋平× 和田, 智秀× 海崎, 光宏× Yuki, Shinya× Shibata, Shinpei× Wada, Tomohide× Umizaki, Mitsuhiro |
|||||
著者所属 | ||||||
山形大学大学院理工学研究科 | ||||||
著者所属 | ||||||
山形大学理学部 | ||||||
著者所属 | ||||||
国立天文台天文学データ解析計算センター | ||||||
著者所属 | ||||||
山形大学大学院理工学研究科 | ||||||
著者所属(英) | ||||||
en | ||||||
Graduate School of Science and Engineering, Yamagata University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Yamagata University | ||||||
著者所属(英) | ||||||
en | ||||||
Center for Computational Astrophysics, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
Graduate School of Science and Engineering, Yamagata University | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構 | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料: en : JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H 巻 JAXA-SP-09-008E, p. 228-229, 発行日 2010-02-26 |
|||||
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 | The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The particle acceleration mechanism of pulsars has been an outstanding problem for more than forty years. A breakthrough can be provided by a large particle-simulation for the global magnetosphere showing the formation of the field-aligned electric field. However, this demands heavy calculation of Coulomb interaction. We have resolved this difficulty by use of GRAPE, which is a massively parallel special purpose computer for astronomical N-body problem at National Astronomical Observatory of Japan. Note that GRAPE can calculate Coulomb force as well as gravitational force because of the same inverse-square law and of sign-bit available with GRAPE. In this paper, we present a method of particle simulation for the global magnetosphere including electron-positron pair creation. We show some initial results of the simulation. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064574086 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-09-008E |