On the Modelling of Rotational Effects in the Lower Convective Region of the Sun

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dc.authoridCavus, Huseyin/0000-0003-4224-7039
dc.contributor.authorCavus, H.
dc.contributor.authorKarafistan, A. I.
dc.date.accessioned2025-01-27T20:59:37Z
dc.date.available2025-01-27T20:59:37Z
dc.date.issued2010
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractThe purpose of this work is to study effects of differential rotation in the lower convective region of the Sun. Similar to MHD case; the governing equations are separated in variables, allowing numerical integration in this layer. This algorithm facilitates solutions of more complicated systems, with less computing time. Two different known rotation profiles are used in order to fit the model. The fitting procedure is accomplished by making use of sphericity and density shape parameters related to the rotation profiles. It is also shown that the most important feature of rotation is to break the spherical symmetric distribution of density in this layer. As in the MHD effects found before, differential rotation changes considerably the density of the reference model for both cases.
dc.identifier.doi10.1590/S0103-97332010000200006
dc.identifier.endpage165
dc.identifier.issn0103-9733
dc.identifier.issue2
dc.identifier.scopus2-s2.0-77955519511
dc.identifier.scopusqualityQ3
dc.identifier.startpage160
dc.identifier.urihttps://doi.org/10.1590/S0103-97332010000200006
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26753
dc.identifier.volume40
dc.identifier.wosWOS:000280286400006
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofBrazilian Journal of Physics
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20250125
dc.subjectHydrodynamics-Sun
dc.subjectgeneral-Sun
dc.subjectinterior-Sun
dc.subjectrotation-Sun
dc.subjectfundamental parameters
dc.titleOn the Modelling of Rotational Effects in the Lower Convective Region of the Sun
dc.typeArticle

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