{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360004229805747328.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2016gl068926"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2016GL068926"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL068926"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2016GL068926"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL068926"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"MAVEN observations of partially developed Kelvin‐Helmholtz vortices at Mars"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>We present preliminary results and interpretations for Mars Atmospheric and Volatile EvolutioN (MAVEN) observations of magnetosheath‐ionospheric boundary oscillations at Mars. Using centrifugal force arguments, we first predict that a signature of fully rolled up Kelvin‐Helmholtz vortices at Mars is sheath ions that have a bulk motion toward the Sun. The sheath ions adjacent to a vortex should also accelerate to speeds higher than the mean sheath velocity. We also predict that while the ionospheric ions that are in the vortex accelerate antisunward, they never attain speeds exceeding that of the sheath ions, in stark contrast to KH vortices that arise at the Earth's magnetopause. We observe accelerated sheath and ionospheric ions, but we do not observe sheath ions that have a bulk motion toward the Sun. Thus, we interpret these observations as KH vortices that have not fully rolled up.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004229805747330","@type":"Researcher","foaf:name":[{"@value":"Suranga Ruhunusiri"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy University of Iowa  Iowa City Iowa USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747201","@type":"Researcher","foaf:name":[{"@value":"J. S. Halekas"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy University of Iowa  Iowa City Iowa USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747205","@type":"Researcher","foaf:name":[{"@value":"J. P. McFadden"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747209","@type":"Researcher","foaf:name":[{"@value":"J. E. P. Connerney"}],"jpcoar:affiliationName":[{"@value":"NASA Goddard Space Flight Center  Greenbelt Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747210","@type":"Researcher","foaf:name":[{"@value":"J. R. Espley"}],"jpcoar:affiliationName":[{"@value":"NASA Goddard Space Flight Center  Greenbelt Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747200","@type":"Researcher","foaf:name":[{"@value":"Y. Harada"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747329","@type":"Researcher","foaf:name":[{"@value":"R. Livi"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747331","@type":"Researcher","foaf:name":[{"@value":"K. Seki"}],"jpcoar:affiliationName":[{"@value":"Solar‐Terrestrial Environment Laboratory Nagoya University  Nagoya Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747202","@type":"Researcher","foaf:name":[{"@value":"C. Mazelle"}],"jpcoar:affiliationName":[{"@value":"CNRS IRAP  Toulouse France"},{"@value":"University Paul Sabatier  Toulouse France"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747328","@type":"Researcher","foaf:name":[{"@value":"D. Brain"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747206","@type":"Researcher","foaf:name":[{"@value":"T. Hara"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747207","@type":"Researcher","foaf:name":[{"@value":"G. A. DiBraccio"}],"jpcoar:affiliationName":[{"@value":"NASA Goddard Space Flight Center  Greenbelt Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747204","@type":"Researcher","foaf:name":[{"@value":"D. E. Larson"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747203","@type":"Researcher","foaf:name":[{"@value":"D. L. Mitchell"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747072","@type":"Researcher","foaf:name":[{"@value":"B. M. Jakosky"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004229805747208","@type":"Researcher","foaf:name":[{"@value":"H. Hasegawa"}],"jpcoar:affiliationName":[{"@value":"Institute of Space and Astronautical Science JAXA  Sagamihara Japan"}]}],"contributor":[{"@id":"https://cir.nii.ac.jp/crid/1892272492731716621","@type":"Researcher","foaf:name":[{"@value":"Institut de recherche en astrophysique et planétologie (IRAP) ; Université Toulouse III - Paul Sabatier (UT3) ; Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) ; Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) ; Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)"}]},{"@id":"https://cir.nii.ac.jp/crid/1892272492731716614","@type":"Researcher","foaf:name":[{"@value":"Université de Toulouse (UT)"}]},{"@id":"https://cir.nii.ac.jp/crid/1893118015814864134","@type":"Researcher","foaf:name":[{"@value":"POTHIER, Nathalie"}]},{"@id":"https://cir.nii.ac.jp/crid/1893118015814864002","@type":"Researcher","foaf:name":[{"@value":"Institut de recherche en astrophysique et planétologie (IRAP)"}]},{"@id":"https://cir.nii.ac.jp/crid/1893118015814864128","@type":"Researcher","foaf:name":[{"@value":"Université Toulouse III - Paul Sabatier (UT3)"}]},{"@id":"https://cir.nii.ac.jp/crid/1893118015814864129","@type":"Researcher","foaf:name":[{"@value":"Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)"}]},{"@id":"https://cir.nii.ac.jp/crid/1893118015814864008","@type":"Researcher","foaf:name":[{"@value":"Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)"}]},{"@id":"https://cir.nii.ac.jp/crid/1893118015814864136","@type":"Researcher","foaf:name":[{"@value":"Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00948276"},{"@type":"EISSN","@value":"19448007"}],"prism:publicationName":[{"@value":"Geophysical Research 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