Nonlinear magneto-hydrodynamical modeling of solar envelope
7th International Conference of the Hellenic-Astronomical-Society, Lixourion, Yunanistan, 8 - 11 Eylül 2006, cilt.848, ss.207-208, (Tam Metin Bildiri)
- Yayın Türü: Bildiri / Tam Metin Bildiri
- Cilt numarası: 848
- Doi Numarası: 10.1063/1.2347979
- Basıldığı Şehir: Lixourion
- Basıldığı Ülke: Yunanistan
- Sayfa Sayıları: ss.207-208
- Çanakkale Onsekiz Mart Üniversitesi Adresli: Evet
Özet
In 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.