{"_buckets": {"deposit": "6e991732-c2fc-4e1b-95d3-590670428022"}, "_deposit": {"id": "22993", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "22993"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00022993"}, "item_10_biblio_info_6": {"attribute_name": "\u66f8\u8a8c\u60c5\u5831", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2016-05-27", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "054506", "bibliographicPageStart": "054506", "bibliographicVolumeNumber": "23", "bibliographic_titles": [{"bibliographic_title": "Physics of Plasmas"}]}]}, "item_10_description_4": {"attribute_name": "\u6284\u9332", "attribute_value_mlt": [{"subitem_description": "In the present paper, the finite-Larmor-radius (gyro-viscous) term [K. V. Roberts and J. B. Taylor, Phys. Rev. Lett. 8, 197\u2013198 (1962)] is evaluated by using a full kinetic Vlasov simulation result of the Kelvin-Helmholtz instability (KHI). The velocity field and the pressure tensor are calculated from the high-resolution data of the velocity distribution functions obtained by the Vlasov simulation, which are used to approximate the Finite-Larmor-Radius (FLR) term according to Roberts and Taylor [Phys. Rev. Lett. 8, 197\u2013198 (1962)]. The direct comparison between the pressure tensor and the FLR term shows an agreement. It is also shown that the anisotropic pressure gradient enhanced the linear growth of the KHI when the inner product between the vorticity of the primary velocity shear layer and the magnetic field is negative, which is consistent with the previous FLR-magnetohydrodynamic simulation result. This result suggests that it is not sufficient for reproducing the kinetic simulation result by fluid simulations to include the FLR term (or the pressure tensor) only in the equation of motion for fluid.", "subitem_description_type": "Abstract"}]}, "item_10_identifier_60": {"attribute_name": "URI", "attribute_value_mlt": [{"subitem_identifier_type": "DOI", "subitem_identifier_uri": "http://dx.doi.org/10.1063/1.4952632"}, {"subitem_identifier_type": "HDL", "subitem_identifier_uri": "http://hdl.handle.net/2237/25177"}]}, "item_10_publisher_32": {"attribute_name": "\u51fa\u7248\u8005", "attribute_value_mlt": [{"subitem_publisher": "AIP Publishing"}]}, "item_10_rights_12": {"attribute_name": "\u6a29\u5229", "attribute_value_mlt": [{"subitem_rights": "Copyright 2016 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing.The following article appeared in (Physics of Plasmas. v.23, 2016, p.054506) and may be found at (http://dx.doi.org/10.1063/1.4952632)."}]}, "item_10_select_15": {"attribute_name": "\u8457\u8005\u7248\u30d5\u30e9\u30b0", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_10_source_id_7": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "1070-664X", "subitem_source_identifier_type": "ISSN"}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Umeda, Takayuki"}], "nameIdentifiers": [{"nameIdentifier": "67926", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Yamauchi, Natsuki"}], "nameIdentifiers": [{"nameIdentifier": "67927", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Wada, Yasutaka"}], "nameIdentifiers": [{"nameIdentifier": "67928", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Ueno, Satoshi"}], "nameIdentifiers": [{"nameIdentifier": "67929", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "\u30d5\u30a1\u30a4\u30eb\u60c5\u5831", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2017-05-27"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "1_4952632.pdf", "filesize": [{"value": "1.6 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 1600000.0, "url": {"label": "1_4952632.pdf \u30d5\u30a1\u30a4\u30eb\u516c\u958b\uff1a2017/05/27", "url": "https://nagoya.repo.nii.ac.jp/record/22993/files/1_4952632.pdf"}, "version_id": "7e31391d-4fc3-4a4d-bb6b-89424a094ed9"}]}, "item_language": {"attribute_name": "\u8a00\u8a9e", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "\u8cc7\u6e90\u30bf\u30a4\u30d7", "attribute_value_mlt": [{"resourcetype": "journal article", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "Evaluating gyro-viscosity in the Kelvin-Helmholtz instability by kinetic simulations", "item_titles": {"attribute_name": "\u30bf\u30a4\u30c8\u30eb", "attribute_value_mlt": [{"subitem_title": "Evaluating gyro-viscosity in the Kelvin-Helmholtz instability by kinetic simulations"}]}, "item_type_id": "10", "owner": "1", "path": ["879/880/881"], "permalink_uri": "http://hdl.handle.net/2237/25177", "pubdate": {"attribute_name": "\u516c\u958b\u65e5", "attribute_value": "2016-12-09"}, "publish_date": "2016-12-09", "publish_status": "0", "recid": "22993", "relation": {}, "relation_version_is_last": true, "title": ["Evaluating gyro-viscosity in the Kelvin-Helmholtz instability by kinetic simulations"], "weko_shared_id": null}