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.
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页码：462 / 465
页数：3
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