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dc.contributor.authorKieokaew, R
dc.contributor.authorFoullon, C
dc.date.accessioned2019-05-30T13:20:38Z
dc.date.issued2019-05-22
dc.description.abstractMagnetopause Kelvin‐Helmholtz (KH) waves are rich in complex magnetic and flow structures which are key to understand the role of these waves in facilitating the solar wind plasma transport into the Earth's magnetosphere. Four spacecraft in tetrahedral configuration provide the tools necessary for characterizing in situ magnetic geometry and vortical flow. We apply the tools on KH waves observed by Cluster inside an electron boundary layer on the duskside magnetopause. Magnetic curvature and flow vorticity properties of the KH waves are obtained for various solar wind conditions. Smaller curvature radius and higher‐positive vorticity are found for longer wavelength. Changes in KH wavelengths observed with relatively fixed tetrahedron size allow us to resolve magnetic curvature in multiscales. For the first time in a space plasma, we report the dependence of the curvature radius measurement on the ratio of the tetrahedron size to the wavelength, consistent with nonlinear spatial variations of magnetic structures that would be resolved by nested cross‐scale spacecraft tetrahedrons. Negative vorticity is found to develop in the rolled‐up vortex, adjacent to positive vorticity in the vortex core. The strength of negative vorticity is found to increase with the solar wind proton density and proton bulk flow speed. This study provides observational evidence of multiscale magnetic structures and is useful for understanding the development of rolled‐up vortex signatures during various stages of solar wind‐controlled KH wave evolution.en_GB
dc.description.sponsorshipScience and Technology Facilities Councilen_GB
dc.description.sponsorshipUniversity of Exeteren_GB
dc.identifier.citationVol. 124en_GB
dc.identifier.doi10.1029/2019JA026484
dc.identifier.grantnumberST/I003649/1en_GB
dc.identifier.urihttp://hdl.handle.net/10871/37307
dc.language.isoenen_GB
dc.publisherAmerican Geophysical Union (AGU) / Wileyen_GB
dc.rights©2019. The Authors. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.en_GB
dc.titleKelvin-Helmholtz Waves Magnetic Curvature and Vorticity: Four-spacecraft Cluster Observationsen_GB
dc.typeArticleen_GB
dc.date.available2019-05-30T13:20:38Z
dc.identifier.issn2169-9402
dc.descriptionThis is the final version. Available on open access from AGU via the DOI in this recorden_GB
dc.descriptionData used in this study obtained from CLWeb at IRAP (http://clweb.irap.omp.eu/cl/clweb.php)en_GB
dc.identifier.journalJournal of Geophysical Research: Space Physicsen_GB
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2019-04-17
exeter.funder::Science and Technology Facilities Councilen_GB
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2019-04-26
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2019-05-30T09:55:08Z
refterms.versionFCDAM
refterms.dateFOA2019-05-30T13:20:45Z
refterms.panelBen_GB


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©2019. The Authors.

This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
Except where otherwise noted, this item's licence is described as ©2019. The Authors. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.