Nonlinear Magneto-Hydrodynamical Modeling Of Solar Envelope

Details Nonlinear Magneto-Hydrodynamical Modeling Of Solar Envelope Nonlinear Magneto-Hydrodynamical Modeling Of Solar Envelope

Publishing date

Aug 2006

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..848..207c&link_type=abstract

Journals

RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP Conferenc

Science

Physics

Additional info 3

Solar Physics, Magnetohydrodynamics And Plasmas

Type

Scientific paper

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.

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