The floor in the solar wind: status report

被引:6
|
作者
Cliver, E. W.
机构
来源
COMPARATIVE MAGNETIC MINIMA: CHARACTERIZING QUIET TIMES IN THE SUN AND STARS | 2012年 / 286期
关键词
Sun; magnetic fields; solar wind; GEOMAGNETIC-ACTIVITY;
D O I
10.1017/S1743921312004814
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Cliver & Ling (2010) recently suggested that the solar wind had a floor or ground-state magnetic field strength at Earth of similar to 2.8 nT and that the source of the field was the slow solar wind. This picture has recently been given impetus by the evidence presented by Schrijver et al. (2011) that the Sun has a minimal magnetic state that was approached globally in 2009, a year in which Earth was imbedded in slow solar wind similar to 70% of the time. A precursor relation between the solar dipole field strength at solar minimum and the peak sunspot number (SSNMAX) of the subsequent 11-yr cycle suggests that during Maunder-type minima (when SSNMAX was similar to 0), the solar polar field strength approaches zero - indicating weak or absent polar coronal holes and an increase to nearly similar to 100% in the time that Earth spends in slow solar wind.
引用
收藏
页码:179 / 184
页数:6
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