The Solar Magnetic Field as a Coronal Hole Extension Forms: Effects of Magnetic Helicity and Boundary Conditions

被引:0
作者
J. R. Clegg
B. J. I. Bromage
P. K. Browning
机构
[1] University of Central Lancashire,Centre for Astrophysics
[2] UMIST,Dept. of Physics
来源
Space Science Reviews | 1999年 / 87卷
关键词
force-free; corona; magnetic fields;
D O I
暂无
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学科分类号
摘要
An analytical solution is presented for linear force fields within a spherical shell, representing the solar corona. Allowing for a global magnetic helicity, we find magnetic fields over the entire corona with realistic inner boundary conditions obtained from transformation and extrapolation of photospheric magnetograms and considering alternative outer boundary conditions. Such fields are found for the well known coronal hole extension event of August 1996.
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页码:145 / 148
页数:3
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[1]  
Wang Y.-M.(1992)On potential field models of the solar corona Ap.J. 392 310-undefined
[2]  
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