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Combined Effect of Magnetic field and Internal Heat Generation on the Onset of Marangoni Convection

机译:磁场和内部热量产生对Marangoni对流爆发的综合影响

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Marangoni convection in a horizontal layer with a uniform internal heat source and vertical magnetic field is analyzed. The boundaries are considered to be rigid, however permeable, and insulated to temperature perturbations. The upper surface of a fluid layer is deformably free. The eigen value equations of the perturbed state obtained from the normal mode analysis are solved by using regular perturbation method with a as wave number. The results show that the critical Marangoni number M_c become larger as the Chandrasekhar number Q increases, internal heat source and the Crispation number Cr decreases.
机译:分析了具有均匀内部热源和垂直磁场的水平层中的Marangoni对流。边界被认为是刚性的,但是是可渗透的,并且不受温度扰动的影响。流体层的上表面没有变形。通过使用以a为波数的常规摄动方法,求解了从正常模式分析获得的摄动状态的特征值方程。结果表明,随着钱德拉塞卡尔数Q的增加,内部热源的临界马兰戈尼数M_c变大,而卷曲数Cr则减小。

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