Allowance for motion in a steady-state thermal flux pattern

被引:0
作者
Shmeleva, O. P. [1 ]
Krasil'nikova, L. L. [1 ]
Sukhova, N. S. [1 ]
机构
[1] Moscow MV Lomonosov State Univ, Moscow, Russia
关键词
TEMPERATURE;
D O I
10.1134/S0016793210040079
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
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.
引用
收藏
页码:471 / 474
页数:4
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