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STABILITY OF THE TOROIDAL MAGNETIC FIELD IN STELLAR RADIATION ZONES

机译:星状辐射带中环形磁场的稳定性

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The stability of the magnetic field in radiation zones is of crucial importance for mixing, angular momentum transport, etc. We consider the stability properties of a star containing a predominant toroidal field in spherical geometry by means of a linear stability in the Boussinesq approximation taking into account the effect of thermal conductivity. We calculate the growth rate of instability and analyze in detail the effects of stable stratification and heat transport. We argue that the stabilizing influence of gravity can never entirely suppress the instability caused by electric currents in radiation zones. However, the stable stratification can essentially decrease the growth rate of instability
机译:辐射区中磁场的稳定性对于混合,角动量传输等至关重要。通过考虑Boussinesq近似的线性稳定性,我们考虑了球体几何中包含主要环形场的恒星的稳定性。考虑导热系数的影响。我们计算不稳定的增长率,并详细分析稳定分层和热传递的影响。我们认为,重力的稳定作用永远无法完全抑制辐射区内电流引起的不稳定性。但是,稳定的分层实质上可以降低不稳定的增长率

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