On the variations of some physical quantities above the sunspot bands near the equatorial plane

dc.authoridCavus, Huseyin/0000-0003-4224-7039
dc.contributor.authorCavus, H.
dc.contributor.authorIlbikci, N.
dc.date.accessioned2025-01-27T20:43:42Z
dc.date.available2025-01-27T20:43:42Z
dc.date.issued2016
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this work, some solutions of magnetohydrodynamic (MHD) equations are searched in order to investigate some large scale physical quantities in the sunspot dominated latitudinal regions near the equatorial plane. Special separation of variables is used to obtain the radial and latitudinal changes in spherical coordinates. Present parametric analysis yields three important parameters which are the sphericity, density and radial components shape parameters in the latitudinal distributions of physical variables. In the region of interest there is a considerable change in physical quantities with respect to regions where sunspots do not appear.
dc.identifier.doi10.1134/S1990341316020115
dc.identifier.endpage248
dc.identifier.issn1990-3413
dc.identifier.issn1990-3421
dc.identifier.issue2
dc.identifier.scopus2-s2.0-84971647421
dc.identifier.scopusqualityQ3
dc.identifier.startpage241
dc.identifier.urihttps://doi.org/10.1134/S1990341316020115
dc.identifier.urihttps://hdl.handle.net/20.500.12428/24338
dc.identifier.volume71
dc.identifier.wosWOS:000376579200011
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherMaik Nauka/Interperiodica/Springer
dc.relation.ispartofAstrophysical Bulletin
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectSun: atmosphere
dc.subjectsunspots
dc.subjectMHD
dc.titleOn the variations of some physical quantities above the sunspot bands near the equatorial plane
dc.typeArticle

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