Large-scale structure of the solar corona magnetic field

被引：0
|
作者：
V. L. Merzlyakov
L. I. Starkova
机构：
[1] Russian Academy of Sciences,Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation
来源：
Geomagnetism and Aeronomy | 2012年 / 52卷
关键词：
Solar Corona; Solar Eclipse; Neutral Line; Heliospheric Current Sheet; Total Solar Eclipse;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The configuration of the solar corona magnetic field has been studied. Data on the position of the K-corona emission polarization plane during the solar eclipses of September 21, 1941; February 25, 1952; and August 1, 2008, were used as an indicator of the magnetic field line orientation. Based on an analysis of these data, a conclusion has been made that the studied configuration has a large-scale organization in the form of a cellular structure with an alternating field reversal. The estimated cell size was 61° ± 6° (or 36° ± 2°) in longitude with a latitudinal extension of 40°–50° in the range of visible distances 1.3–2.0 RSun. A comparison of the detected cellular structure of the coronal magnetic field with synoptic {ie908-1} maps indicated that the structure latitudinal boundaries vary insignificantly within 1.1–2.0 RSun.
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收藏
页码：908 / 912
页数：4
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