Magnetic Kelvin-Helmholtz instability in the solar atmosphere

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dc.authoridCavus, Huseyin/0000-0003-4224-7039
dc.contributor.authorCavus, Huseyin
dc.contributor.authorKazkapan, Derya
dc.date.accessioned2025-01-27T20:22:53Z
dc.date.available2025-01-27T20:22:53Z
dc.date.issued2013
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractMain aim of this paper is to twofold: firstly, to investigate the formation mechanism and secondly to search the effects of fundamental parameters like magnetic field, shear velocity and wave number on the growth rate of the magnetic Kelvin-Helmholtz instability occured in the solar atmosphere. In this investigation, occurrence and unoccurrence of instability are determined for the different values of magnetic field, shear velocity and wave number in the solar atmosphere. We have obtained the critical values of shear velocity and magnetic field. (C) 2013 Elsevier B.V. All rights reserved.
dc.identifier.doi10.1016/j.newast.2013.04.001
dc.identifier.endpage94
dc.identifier.issn1384-1076
dc.identifier.scopus2-s2.0-84878325863
dc.identifier.scopusqualityQ2
dc.identifier.startpage89
dc.identifier.urihttps://doi.org/10.1016/j.newast.2013.04.001
dc.identifier.urihttps://hdl.handle.net/20.500.12428/22059
dc.identifier.volume25
dc.identifier.wosWOS:000322805300012
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherElsevier Science Bv
dc.relation.ispartofNew Astronomy
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectKelvin Helmholtz instability
dc.subjectSun
dc.subjectSun: atmosphere
dc.subjectSun: magnetic fields
dc.titleMagnetic Kelvin-Helmholtz instability in the solar atmosphere
dc.typeArticle

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