On the classic heat conduction in the chromosphere-corona transition region of the solar atmosphere

被引：1
|
作者：
Ptitsyna, O. V. [1 ]
Somov, B. V. [1 ]
机构：
[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia
来源：
MOSCOW UNIVERSITY PHYSICS BULLETIN | 2010年 / 65卷 / 06期
基金：
俄罗斯基础研究基金会;
关键词：
Sun; chromosphere; corona; transition region; thermal conductivity;
D O I：
10.3103/S0027134910060184
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The distribution of the temperature versus the thickness in the chromosphere-corona transition region of the solar atmosphere on the assumption that the plasma heating by classical heat flux is balanced by the energy loss by radiation. It is shown that the transition region between the corona and chromosphere is a thin layer, to which, however, a simple collision approximation may be applied.
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页码：527 / 530
页数：4
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