Effect of Viscosity on Shock Waves Observed After Two Different Coronal Mass Ejection Activities CME20/11/2003 and CME11/04/2010

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dc.authoridCavus, Huseyin/0000-0003-4224-7039
dc.contributor.authorCavus, H.
dc.contributor.authorZeybek, G.
dc.date.accessioned2025-01-27T20:59:39Z
dc.date.available2025-01-27T20:59:39Z
dc.date.issued2017
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractCoronal mass ejections are the main results of powerful solar activity. These activities are capable of generating shock waves in the interplanetary medium. The shock waves happen when the solar particles change their velocities from supersonic to subsonic. Since the interaction of shock waves with viscosity is one of the central problems in the supersonic regime of compressible gas flow, investigations of these events play a crucial role in space weather research [1]. The main purpose of this study is to study the effects of viscosity on the shock waves observed after the CMEs of 20/11/2003 and CME11/04/2010.
dc.identifier.doi10.1007/s10511-017-9466-9
dc.identifier.endpage110
dc.identifier.issn0571-7256
dc.identifier.issn1573-8191
dc.identifier.issue1
dc.identifier.scopus2-s2.0-85017181624
dc.identifier.scopusqualityQ4
dc.identifier.startpage100
dc.identifier.urihttps://doi.org/10.1007/s10511-017-9466-9
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26767
dc.identifier.volume60
dc.identifier.wosWOS:000399232800009
dc.identifier.wosqualityQ4
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer/Plenum Publishers
dc.relation.ispartofAstrophysics
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectShock waves
dc.subjectViscosity
dc.subjectReynolds number
dc.subjectCoronal mass ejection
dc.titleEffect of Viscosity on Shock Waves Observed After Two Different Coronal Mass Ejection Activities CME20/11/2003 and CME11/04/2010
dc.typeArticle

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