Abstract
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.
| Original language | English |
|---|---|
| Pages (from-to) | 701-705 |
| Number of pages | 5 |
| Journal | Astronomy and Astrophysics |
| Volume | 433 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - Apr 2005 |
Keywords
- Sun: chromosphere
- Sun: corona
- Sun: magnetic fields
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