Nonlinear magneto-hydrodynamical modeling of solar envelope


ÇAVUŞ H. , KARAFISTAN A. I.

7th International Conference of the Hellenic-Astronomical-Society, Lixourion, Greece, 8 - 11 September 2006, vol.848, pp.207-208 identifier identifier

  • Publication Type: Conference Paper / Full Text
  • Volume: 848
  • Doi Number: 10.1063/1.2347979
  • City: Lixourion
  • Country: Greece
  • Page Numbers: pp.207-208

Abstract

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.