Comparing magnetic field extrapolations with measurements of magnetic loops

被引:75
作者
Wiegelmann, T [1 ]
Lagg, A [1 ]
Solanki, SK [1 ]
Inhester, B [1 ]
Woch, J [1 ]
机构
[1] Max Planck Inst Sonnensystemforsch, D-37191 Katlenburg Lindau, Germany
关键词
Sun : magnetic fields; Sun : corona; Sun : chromosphere;
D O I
10.1051/0004-6361:20042421
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We compare magnetic field extrapolations from a photospheric magnetogram with the observationally inferred structure of magnetic loops in a newly developed active region. This is the first time that the reconstructed 3D-topology of the magnetic field is available to test the extrapolations. We compare the observations with potential fields, linear force-free fields and non-linear force-free fields. This comparison reveals that a potential field extrapolation is not suitable for a reconstruction of the magnetic field in this young, developing active region. The inclusion of field-line-parallel electric currents, the so called force-free approach, gives much better results. Furthermore, a non-linear force-free computation reproduces the observations better than the linear force-free approximation, although no free parameters are available in the former case.
引用
收藏
页码:701 / 705
页数:5
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