Characterizing the Quiet Sun Scale Magnetic Field

被引：0
|
作者：
Title, Alan [1 ]
机构：
[1] Lockheed Martin Adv Technol Ctr, Palo Alto, CA 94304 USA
来源：
ASTROPHYSICAL DYNAMICS: FROM STARS TO GALAXIES | 2011年 / 271期
关键词：
Sun: magnetic fields;
D O I：
10.1017/S1743921311017480
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Observations with the Solar Optical Telescope on Hinode indicate that the Quiet Sun magnetic field occurs on every scale of convection including granulation. Data reported here show that, regardless of the position on the disk, the polarity in the inner network regions are balanced to 1 part in 72. This is consistent with both local dynamo processes or the creation of surface features by the granulation downflows.
引用
收藏
页码：86 / 93
页数：8
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