{"created":"2023-06-20T15:17:43.296971+00:00","id":11655,"links":{},"metadata":{"_buckets":{"deposit":"57804752-0831-4627-bd06-19285cdb6c7b"},"_deposit":{"created_by":20,"id":"11655","owners":[20],"pid":{"revision_id":0,"type":"depid","value":"11655"},"status":"published"},"_oai":{"id":"oai:nifs-repository.repo.nii.ac.jp:00011655","sets":["6:7"]},"author_link":["128102","128101","127837","127835","128103","127198"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2012-03-23","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"3","bibliographicPageStart":"032111","bibliographicVolumeNumber":"19","bibliographic_titles":[{"bibliographic_title":"Physics of Plasmas "}]}]},"item_10001_description_4":{"attribute_name":"著者ID","attribute_value_mlt":[{"subitem_description":"0000-0003-2513-0453","subitem_description_type":"Other"}]},"item_10001_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"Solar wind interaction with a kinetic scale magnetosphere and the resulting momentum transfer process are investigated by 2.5-dimensional full kinetic particle-in-cell simulations. The spatial scale of the considered magnetosphere is less than or comparable to the ion inertial length and is relevant for magnetized asteroids or spacecraft with mini-magnetosphere plasma propulsion. Momentum transfer is evaluated by studying the Lorentz force between solar wind plasma and a hypothetical coil current density that creates the magnetosphere. In the zero interplanetary magnetic field (IMF) limit, solar wind interaction goes into a steady state with constant Lorentz force. The dominant Lorentz force acting on the coil current density is applied by the thin electron current layer at the wind-filled front of the magnetosphere. Dynamic pressure of the solar wind balances the magnetic pressure in this region via electrostatic deceleration of ions. The resulting Lorentz force is characterized as a function of the scale of magnetosphere normalized by the electron gyration radius, which determines the local structure of the current layer. For the finite northward IMF case, solar wind electrons flow into the magnetosphere through the reconnecting region. The inner electrons enhance the ion deceleration, and this results in temporal increment of the Lorentz force. It is concluded that the momentum transfer of solar wind plasma could take place actively with variety of kinetic plasma phenomena, even in a magnetosphere with a small scale of less than the ion inertial length.","subitem_description_type":"Abstract"}]},"item_10001_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"American Institute of Physics "}]},"item_10001_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":" 10.1063/1.3683560 ","subitem_relation_type_select":"DOI"}}]},"item_10001_relation_16":{"attribute_name":"情報源","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"Physics of Plasmas 19, 032111 (2012); https://doi.org/10.1063/1.3683560"}]}]},"item_10001_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"Publisher version   "}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1063/1.3683560","subitem_relation_type_select":"DOI"}}]},"item_10001_rights_15":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"This content may be downloaded for personal use only."},{"subitem_rights":" Any other use requires prior permission of the author and the publisher. "},{"subitem_rights":"This material originally appeared in Physics of Plasmas 19, 032111 (2012) and may be found at https://doi.org/10.1063/1.3683560."},{"subitem_rights":"Copyright 2012 Author(s). "},{"subitem_rights":"This article is distributed under a Creative Commons Attribution (CC BY) License."}]},"item_10001_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA10987555 ","subitem_source_identifier_type":"NCID"}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1070-664X ","subitem_source_identifier_type":"ISSN"}]},"item_10001_text_23":{"attribute_name":"NAIS","attribute_value_mlt":[{"subitem_text_value":"13770"}]},"item_10001_version_type_20":{"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":[{"creatorAffiliations":[{"affiliationNameIdentifiers":[{"affiliationNameIdentifier":""}],"affiliationNames":[{"affiliationName":""}]}],"creatorNames":[{"creatorName":"MORITAKA, Toseo"}],"familyNames":[{}],"givenNames":[{}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"KAJIMURA, Yoshihiro"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"USUI, Hideyuki"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"MATSUMOTO, Masaharu"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"MATSUI, Tatsuki"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"SHINOHARA, Iku"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2023-03-14"}],"displaytype":"detail","filename":"13770_Phys.Plasmas.pdf","filesize":[{"value":"4.2 MB"}],"format":"application/pdf","licensetype":"license_6","mimetype":"application/pdf","url":{"label":"13770_Phys.Plasmas","url":"https://nifs-repository.repo.nii.ac.jp/record/11655/files/13770_Phys.Plasmas.pdf"},"version_id":"56641231-a110-40fe-855a-8c983ca15fcb"}]},"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":"Momentum transfer of solar wind plasma in a kinetic scale magnetosphere","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Momentum transfer of solar wind plasma in a kinetic scale magnetosphere"}]},"item_type_id":"10001","owner":"20","path":["7"],"pubdate":{"attribute_name":"公開日","attribute_value":"2023-03-14"},"publish_date":"2023-03-14","publish_status":"0","recid":"11655","relation_version_is_last":true,"title":["Momentum transfer of solar wind plasma in a kinetic scale magnetosphere"],"weko_creator_id":"20","weko_shared_id":-1},"updated":"2023-09-21T06:35:23.414535+00:00"}