Dependence of the canopy height of solar magnetic flux tubes on its definition

被引：6

作者：

Zhang, M ^{[1
]}

Zhang, HQ

机构：

[1] Chinese Acad Sci, Beijing Astron Observ, Beijing 100080, Peoples R China

[2] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China

来源：

SOLAR PHYSICS | 2000年 / 194卷 / 01期

基金：

中国国家自然科学基金;

关键词：

D O I：

10.1023/A:1005290924416

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

By analyzing a canopy tube described by Athay, we point out the possibility that the different canopy heights given by different authors are caused by different definitions of canopy heights. For the same canopy tube, those heights where the magnetic field has horizontal components, where neighboring magnetic tubes meet each other and where the magnetic field becomes uniform or vertical range from near the solar photosphere to the solar corona.

引用

页码：29 / 33

页数：5

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