Solar cycle evolution of the heliospheric magnetic field: The Ulysses legacy

被引：30

作者：

Smith, E. J. ^{[1
]}

机构：

[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

来源：

JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS | 2011年 / 73卷 / 2-3期

基金：

美国国家航空航天局;

关键词：

Heliosphere; Magnetic field; Solar wind; Solar cycle; NORTH-SOUTH ASYMMETRY; RAPID LATITUDE SCAN; CURRENT SHEET; HELIOGRAPHIC LATITUDES; WIND SPEED; GEOMAGNETIC-ACTIVITY; SECTOR STRUCTURE; INTERPLANETARY; FLUX; SUN;

D O I：

10.1016/j.jastp.2010.03.019

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

Important contributions of Ulysses to understanding the solar cycle evolution of the heliospheric magnetic field (HMF) and solar wind are reviewed: a dramatic reorientation of the HMF as the solar dipole rotates between axial and equatorial orientations; solar cycle variation of the total heliospheric magnetic flux and its response to changes in solar magnetic fields; the unusual on-going solar minimum and its effects; a connection between magnetic flux and solar wind mass flux in the heliosphere and at the source; a recurrent north-south heliospheric asymmetry at solar minimum and the equatorial offset of the solar magnetic dipole. (C) 2010 Published by Elsevier Ltd.

引用

页码：277 / 289

页数：13

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