MODELING THE SUN'S OPEN MAGNETIC FLUX AND THE HELIOSPHERIC CURRENT SHEET

被引：44
|
作者：
Jiang, J. [1 ]
Cameron, R. [1 ]
Schmitt, D. [1 ]
Schuessler, M. [1 ]
机构：
[1] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany
来源：
ASTROPHYSICAL JOURNAL | 2010年 / 709卷 / 01期
关键词：
solar-terrestrial relations; Sun: activity; Sun: magnetic fields; COSMIC-RAY MODULATION; AXIAL TILT ANGLES; SOLAR PHOTOSPHERE; MERIDIONAL FLOW; FIELD; CYCLE; EVOLUTION; TRANSPORT; INTERPLANETARY; CORONA;
D O I：
10.1088/0004-637X/709/1/301
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
By coupling a solar surface flux transport model with an extrapolation of the heliospheric field, we simulate the evolution of the Sun's open magnetic flux and the heliospheric current sheet (HCS) based on observational data of sunspot groups since 1976. The results are consistent with measurements of the interplanetary magnetic field near Earth and with the tilt angle of the HCS as derived from extrapolation of the observed solar surface field. This opens the possibility for an improved reconstruction of the Sun's open flux and the HCS into the past on the basis of empirical sunspot data.
引用
收藏
页码：301 / 307
页数：7
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