Modelling the magnetic field and differential rotation effects for the vicinity of the base of convective zone in the Sun

作者: Huseyin Cavus

DOI: 10.1016/J.NEWAST.2008.10.008

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摘要: Abstract In this work, some numerical solutions of magnetohydrodynamics equations are investigated in the presence differential rotation with use previously developed algorithm. This algorithm includes thin shell approximation and a special separation variables which were used to obtain radial latitudinal variations physical parameters spherical coordinates. The magnetic field profile is chosen produce comparable fluxes found previous works. sphericity density shape relevant model determined by using two different known profiles. It that strongly dependent there considerable change respect reference model. as well shown symmetric distributions broken for region study.

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