In this paper, we use new viscosity law in which magnetic viscosity is mechanism in stead of that of the standard α-model in order to avoid the thermal instability and viscous instability in the inner region of standard disk.
在轴对称、几何薄、光学厚吸积盘模型的基础上,应用新的粘滞定律(磁粘滞为主)以避免标准吸积盘内区的热不稳定及粘滞不稳定定。