On the viscosity effects in the shock wave observed in the solar wind after the December 13, 2006 coronal mass ejection

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dc.authoridCavus, Huseyin/0000-0003-4224-7039
dc.contributor.authorCavus, H.
dc.date.accessioned2025-01-27T20:54:29Z
dc.date.available2025-01-27T20:54:29Z
dc.date.issued2015
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractCoronal mass ejections (CMEs) and solar wind are the main results of solar activity. These events can drive interplanetary shock waves and produce geomagnetic storms. The study of these events is very important for space weather purposes. The shock waves occur where the solar wind changes its characteristics from being supersonic (with respect to the surrounding interplanetary medium) to being subsonic. In the supersonic regime of compressible gas flow, the interaction of shock waves with viscosity is one of the central problems. The main purpose of this study is to search for the effects of viscosity in the shock wave observed after the December 13, 2006 coronal mass ejection.
dc.description.sponsorshipResearch Foundation of the Canakkale Onsekiz Mart University [2011/012]
dc.description.sponsorshipThe author acknowledges with thanks the technical and computing support from the Research Foundation of the Canakkale Onsekiz Mart University (project No. 2011/012). He also thanks the anonymous referee concerning the improvement of this manuscript.
dc.identifier.doi10.1134/S1990341315010137
dc.identifier.endpage122
dc.identifier.issn1990-3413
dc.identifier.issn1990-3421
dc.identifier.issue1
dc.identifier.scopus2-s2.0-84923838924
dc.identifier.scopusqualityQ3
dc.identifier.startpage117
dc.identifier.urihttps://doi.org/10.1134/S1990341315010137
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26089
dc.identifier.volume70
dc.identifier.wosWOS:000350562200013
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherMaik Nauka/Interperiodica/Springer
dc.relation.ispartofAstrophysical Bulletin
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectsolar wind
dc.subjectSun: coronal mass ejections (CMEs)
dc.subjectSun: activity
dc.titleOn the viscosity effects in the shock wave observed in the solar wind after the December 13, 2006 coronal mass ejection
dc.typeArticle

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