Polar coronal holes in the solar activity cycle

被引：2

作者：

Stepanian, N. N. ^{[1
]}

Shtertser, N. I. ^{[1
]}

机构：

[1] Taras Shevchenko Natl Univ Kyiv, Crimean Astrophys Observ, Nauchnyi, Crimea, Ukraine

来源：

ADVANCES IN SPACE RESEARCH | 2015年 / 55卷 / 03期

关键词：

Coronal holes; Polar magnetic field;

D O I：

10.1016/j.asr.2014.05.018

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The area of coronal holes, located at solar latitudes of more than 60, is compared with the evolution of the large-scale magnetic fields on the Sun's surface. We found a decrease in the area of the coronal holes as well as growth of their low-latitude boundaries in connection with a reversal of the polar magnetic field. (C) 2014 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：795 / 797

页数：3