Allowance for motion in a steady-state thermal flux pattern

We estimated solar plasma streams in the structure and energy balance of the transition layer between the corona and the chromosphere within the framework of the steady-state thermal flux pattern. As well we give the dependence on thermal flux temperature with allowance for convective descending and ascending plasma streams and in the absence of plasma motion. Calculation results show that the contribution of plasma streams to the energy balance of the transition layer is of considerable importance.