4.6 Article

IBEX RIBBON: WHAT COULD IT TELL ABOUT THE LOCAL INTERSTELLAR MAGNETIC FIELD?

期刊

ASTROPHYSICAL JOURNAL LETTERS
卷 727, 期 2, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/727/2/L48

关键词

ISM: atoms; ISM: magnetic fields; magnetohydrodynamics (MHD); plasmas; solar wind; Sun: heliosphere

资金

  1. Polish Ministry of Science and Higher Education [N N203 4159 33, N NS-1260-11-09]

向作者/读者索取更多资源

We show that the shape of the IBEX Ribbon can be reproduced assuming energetic neutral atoms originate in regions beyond the heliopause where the interstellar magnetic field is the strongest and perpendicular to radial directions from the Sun. The best fit to the observed ribbon was obtained for the local interstellar magnetic field B-infinity = 3.0 +/- 1.0 mu G pointing from ecliptic/galactic coordinates (lambda, beta)/(l, b) = (225 degrees +/- 5 degrees, 35 degrees +/- 5 degrees)/(27 degrees +/- 5 degrees, 51 degrees +/- 5 degrees) close to the apparent ribbon center (lambda, beta)/(l, b) = (221 degrees, 39 degrees)/(33 degrees, 55 degrees). The geometrical considerations presented below should prove useful in identifying the mechanism of ribbon formation.

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。

评论

主要评分

4.6
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据