Nonlinear magneto-hydrodynamical modeling of solar envelope

dc.authoridCavus, Huseyin/0000-0003-4224-7039
dc.contributor.authorCavus, Huseyin
dc.contributor.authorKarafistan, Aysel I.
dc.date.accessioned2025-01-27T20:31:16Z
dc.date.available2025-01-27T20:31:16Z
dc.date.issued2006
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description7th International Conference of the Hellenic-Astronomical-Society -- SEP 08-11, 2006 -- Lixourion, GREECE
dc.description.abstractIn this study, our objective was to investigate the variation of the physical parameters in the 30 % outermost convective solar layer with the use equations of magneto-hydrodynamics (MHD) for non-linear case. The anelastic approximation was used in our calculations. The variations in physical parameters were performed by Maple. Hydrostatics equilibrium state was taken as a Standard Solar Model (SSM) excluding both rotation and magnetic field.
dc.description.sponsorshipMunicipal Lixourion Pallis,Alexander S Onassis Fdn,Hellen Minist Tourism,Hellen Astron Soc,EUDOXOS Natl Observ Educ,Prefecture Kefallinia & Ithaki,Hellen Natl Comm Astron,Hellen Naval Acad
dc.description.sponsorshipCanakkle Mark University Scientific Research
dc.description.sponsorshipThis work being supported by Canakkle Mark University Scientific Research Project No (2005/113)
dc.identifier.endpage+
dc.identifier.isbn0-7354-0343-0
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-33846528955
dc.identifier.scopusqualityQ4
dc.identifier.startpage207
dc.identifier.urihttps://hdl.handle.net/20.500.12428/23060
dc.identifier.volume848
dc.identifier.wosWOS:000241381900022
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartofRecent Advances in Astronomy and Astrophysics
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectsun : magnetic fields : magneto-hydrodynamics
dc.subjectanelastic approximation
dc.titleNonlinear magneto-hydrodynamical modeling of solar envelope
dc.typeConference Object

Dosyalar