A NUMERICAL SIMULATION FOR THE PROPAGATION OF DISTURBANCE IN THE SOLAR CORONA (II) THE EFFECTS OF THERMAL CONDUCTION AND RADIATION

Using the magnetohydrodynamic equations with complete energy equation,the dynamical response under the magnetostatic equilibrium in the solar cornna caused by the radial ejection of cold mass at the solar surface is studied numerically.The results may explain the formation of the solar prominence and the propagation of accompanying coronal disturbance.It is also show that the effects of thermal conduction and radiative loss on the fundamental property of a disturbance propagation is very small,and may be they play a role of no importance in the formation of prominence.