ИСТИНА

For various plasma flux velocities specified on the lower boundary of the chromosphere-corona transition region, we find temperature dependencies of plasma concentration, velocity and pressure along magnetic tube with one end immersed in the chromosphere and the other end located in the corona. We also obtain stationary temperature distributions along magnetic tube. At each point of the distribution, there is a balance between the heating by the classical heat flux, the energy losses through the radiation of optically thin plasma and the energy transport associated with plasma flow.