Cavus, HuseyinKarafistan, Aysel I.2025-01-272025-01-2720060-7354-0343-00094-243Xhttps://hdl.handle.net/20.500.12428/230607th International Conference of the Hellenic-Astronomical-Society -- SEP 08-11, 2006 -- Lixourion, GREECEIn 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.eninfo:eu-repo/semantics/closedAccesssun : magnetic fields : magneto-hydrodynamicsanelastic approximationConference Object848207+N/AWOS:0002413819000222-s2.0-33846528955Q4