{"created":"2021-03-01T06:32:51.090999+00:00","id":24863,"links":{},"metadata":{"_buckets":{"deposit":"90c52311-2f75-419b-9d4b-217f52ab8b62"},"_deposit":{"id":"24863","owners":[],"pid":{"revision_id":0,"type":"depid","value":"24863"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00024863"},"item_10_biblio_info_6":{"attribute_name":"\u66f8\u8a8c\u60c5\u5831","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2017-07-07","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"072307","bibliographicPageStart":"072307","bibliographicVolumeNumber":"24","bibliographic_titles":[{"bibliographic_title":"Physics of Plasmas"}]}]},"item_10_description_4":{"attribute_name":"\u6284\u9332","attribute_value_mlt":[{"subitem_description":"The nonlinear evolution of the Rayleigh-Taylor instability (RTI) at a density shear layer transverse\nto magnetic field in a collisionless plasma is investigated by means of a fully kinetic\nVlasov simulation with two spatial and two velocity dimensions. The primary RTI in the MHD\nregime develops symmetrically in a coordinate axis parallel to gravity as seen in the previous\nMHD simulations. The primary RTI in the Hall-MHD regime develops asymmetrically in a\ncoordinate axis parallel to gravity. A compressible flow is formed at the secondary density shear\nlayer by the Hall effect, which generates a strong scalar pressure gradient of ions. A Hall electric\nfield due to the diamagnetic current results in the asymmetric flow at the tip of the finger structure.\nIn the primary RTI with the ion gyro kinetic effect, secondary RTI with a wavelength\nshorter than the wavelength of the primary RTI is generated at the saturation stage of the primary\nRTI. A seed perturbation for the secondary RTI is excited by another secondary instability\ndue to the coupling between the electron stress tensor and the Hall electric field. The heat\nflux term plays an important role in the time development of the total pressure. On the other\nhand, the contribution of the ion stress tensor is small in both the electric current and the total\npressure.","subitem_description_type":"Abstract"}]},"item_10_identifier_60":{"attribute_name":"URI","attribute_value_mlt":[{"subitem_identifier_type":"DOI","subitem_identifier_uri":"http://doi.org/10.1063/1.4991409"},{"subitem_identifier_type":"HDL","subitem_identifier_uri":"http://hdl.handle.net/2237/27083"}]},"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 2017 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.24, 2017, p.072307) and may be found at (http://dx.doi.org/10.1063/1.4991409)."}]},"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":"Takayuki, Umeda"}],"nameIdentifiers":[{"nameIdentifier":"73964","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Yasutaka, Wada"}],"nameIdentifiers":[{"nameIdentifier":"73965","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":"2018-07-07"}],"displaytype":"detail","filename":"1_4991409.pdf","filesize":[{"value":"4.8 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"1_4991409.pdf \u30d5\u30a1\u30a4\u30eb\u516c\u958b\u65e5:2018/07/07","url":"https://nagoya.repo.nii.ac.jp/record/24863/files/1_4991409.pdf"},"version_id":"2ee61d48-534d-468c-93ff-af0b875b3cdd"}]},"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":"Non-MHD effects in the nonlinear development of the MHD-scale Rayleigh-Taylor instability","item_titles":{"attribute_name":"\u30bf\u30a4\u30c8\u30eb","attribute_value_mlt":[{"subitem_title":"Non-MHD effects in the nonlinear development of the MHD-scale Rayleigh-Taylor instability"}]},"item_type_id":"10","owner":"1","path":["879/880/881"],"pubdate":{"attribute_name":"\u516c\u958b\u65e5","attribute_value":"2017-11-08"},"publish_date":"2017-11-08","publish_status":"0","recid":"24863","relation_version_is_last":true,"title":["Non-MHD effects in the nonlinear development of the MHD-scale Rayleigh-Taylor instability"],"weko_creator_id":"1","weko_shared_id":null},"updated":"2021-03-01T13:51:34.879281+00:00"}