On the stability of the solar chromosphere-corona transition region

被引：0
|
作者：
O. V. Ptitsyna
B. V. Somov
机构：
[1] Moscow State University,Sternberg State Institute of Astronomy
来源：
Moscow University Physics Bulletin | 2011年 / 66卷
关键词：
sun; chromosphere; corona; transition region; thermal conductivity;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We prove the stability of a previously obtained temperature-versus-thickness distribution in the solar chromosphere-corona transition region. The temperature distribution has been obtained on the assumption that the plasma heating by classical heat flux is balanced by the energy loss due to radiation.
引用
收藏
页码：462 / 465
页数：3
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