期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 278, 期 1-2, 页码 181-184出版社
KLUWER ACADEMIC PUBL
DOI: 10.1023/A:1013102711400
关键词
-
The large scale magnetic fields of our Galaxy have been mostly revealed by rotation measures (RMs) of pulsars and extragalactic radio sources. In the disk of our Galaxy, the average field strength over a few kpc scale is about 1.8 muG, while the total field, including the random fields on smaller scales, has a strength of about 5 muG. The local regular field, if it is part of the large scale field of a bisymmetric form, has a pitch angle of about -8 degrees. There are at least three, and perhaps five, field reversals from the Norma arm to the outer skirt of our Galaxy.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据