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Comparing magnetic field extrapolations with measurements of magnetic loops

  • T. Wiegelmann
  • , A. Lagg
  • , S. K. Solanki
  • , B. Inhester
  • , J. Woch

Research output: Contribution to journalArticlepeer-review

90 Citations (Scopus)

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 languageEnglish
Pages (from-to)701-705
Number of pages5
JournalAstronomy and Astrophysics
Volume433
Issue number2
DOIs
Publication statusPublished - Apr 2005

Keywords

  • Sun: chromosphere
  • Sun: corona
  • Sun: magnetic fields

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