The radial HMF in fast and slow solar wind
作者:
X. P. Zhao,
J. T. Hoeksema,
期刊:
AIP Conference Proceedings
(AIP Available online 1999)
卷期:
Volume 471,
issue 1
页码: 103-106
ISSN:0094-243X
年代: 1999
DOI:10.1063/1.58739
出版商: AIP
数据来源: AIP
摘要:
From Ulysses observations of magnetic field and plasma properties during its rapid pole-to-pole scan, we determine the causes of variations in the magnitude of the radial component of the heliospheric magnetic field (HMF). We find that the ambient radial HMF in the slow solar wind is a combination of the ambient radial HMF components of the two hemispheres with opposite polarities. It suggests that the source region of the slow solar wind has the same magnetic topology as the source region of the fast solar wind, i.e., both are open field regions. ©1999 American Institute of Physics.
点击下载:
PDF
(784KB)
返 回