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. © ESO 2005.
CITATION STYLE
Wiegelmann, T., Lagg, A., Solanki, S. K., Inhester, B., & Woch, J. (2005). Comparing magnetic field extrapolations with measurements of magnetic loops. Astronomy and Astrophysics, 433(2), 701–705. https://doi.org/10.1051/0004-6361:20042421
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