A magnetohydrodynamic model applied to the lower convective region in the Sun

We have investigated the effects of a toroidal-type magnetic field of 10 T (105 G), in the lower convective region of a standard solar model. From the numerical solution of the magnetohydrodynamic (MHD) equations, distributions of some physical variables are obtained in spherical coordinates for thi...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2007-09, Vol.380 (1), p.142-148
Hauptverfasser:	Cavus, H., Karafistan, A. I.
Format:	Artikel
Sprache:	eng
Schlagworte:	Approximation Astronomy Astrophysics Earth, ocean, space Estimating techniques Exact sciences and technology Magnetic fields MHD Sun Sun: fundamental parameters Sun: general Sun: interior Sun: magnetic fields
Online-Zugang:	Volltext
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