K CORONA AND MAGNETIC SECTOR BOUNDARIES

被引：34

作者：

Hansen, Shirley F. ^{[1
]}

Sawyer, C. ^{[2
]}

Hansen, Richard T. ^{[3
]}

机构：

[1] Natl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80303 USA

[2] Natl Ocean & Atmospher Adm, Sunspot, NM 88349 USA

[3] High Altitude Observ, Kamuela, HI 96743 USA

来源：

GEOPHYSICAL RESEARCH LETTERS | 1974年 / 1卷 / 01期

关键词：

D O I：

10.1029/GL001i001p00013

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

Solar white-light intensity maxima form a characteristic spatial pattern at the solar root of an interplanetary sector boundary, different for +/- and for -/+ boundaries. At a sector boundary, interplanetary magnetic polarities correspond to solar follower fields in the ascending part of the solar activity cycle and to leader fields in the decline.

引用

页数：3

共 12 条

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