Treatment of Viscosity in the Shock Waves Observed After Two Consecutive Coronal Mass Ejection Activities CME08/03/2012 and CME15/03/2012

dc.authoridCavus, Huseyin/0000-0003-4224-7039
dc.contributor.authorCavus, Huseyin
dc.date.accessioned2025-01-27T20:59:39Z
dc.date.available2025-01-27T20:59:39Z
dc.date.issued2016
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractA coronal mass ejection (CME) is one of the most the powerful activities of the Sun. There is a possibility to produce shocks in the interplanetary medium after CMEs. Shock waves can be observed when the solar wind changes its velocity from being supersonic nature to being subsonic nature. The investigations of such activities have a central place in space weather purposes, since; the interaction of shocks with viscosity is one of the most important problems in the supersonic and compressible gas flow regime (Blazek in Computational fluid dynamics: principles and applications. Elsevier, Amsterdam 2001). The main aim of present work is to achieve a search for the viscosity effects in the shocks occurred after two consecutive coronal mass ejection activities in 2012 (i.e. CME08/03/2012 and CME15/03/2012).
dc.identifier.doi10.1007/s11038-016-9492-3
dc.identifier.endpage101
dc.identifier.issn0167-9295
dc.identifier.issn1573-0794
dc.identifier.issue2-3
dc.identifier.scopus2-s2.0-84978630883
dc.identifier.scopusqualityQ3
dc.identifier.startpage91
dc.identifier.urihttps://doi.org/10.1007/s11038-016-9492-3
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26768
dc.identifier.volume118
dc.identifier.wosWOS:000387221700003
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofEarth Moon and Planets
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.titleTreatment of Viscosity in the Shock Waves Observed After Two Consecutive Coronal Mass Ejection Activities CME08/03/2012 and CME15/03/2012
dc.typeArticle

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