Nonlinear magneto-hydrodynamical modeling of solar envelope


ÇAVUŞ H. , KARAFISTAN A. I.

7th International Conference of the Hellenic-Astronomical-Society, Lixourion, Yunanistan, 8 - 11 Eylül 2006, cilt.848, ss.207-208 identifier identifier

  • Cilt numarası: 848
  • Doi Numarası: 10.1063/1.2347979
  • Basıldığı Şehir: Lixourion
  • Basıldığı Ülke: Yunanistan
  • Sayfa Sayıları: ss.207-208

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.