Modeling Non-Potential Fields in Solar Active Regions

Details Modeling Non-Potential Fields in Solar Active Regions Modeling Non-Potential Fields in Solar Active Regions

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.0112b&link_type=abstract

American Astronomical Society, SPD meeting #37, #1.12; Bulletin of the American Astronomical Society, Vol. 38, p.217

Astronomy and Astrophysics

Astronomy

Scientific paper

Many models aim to reproduce the non-linear force-free fields in the solar corona; in this particular study, the magnetofrictional relaxation method is tested. This method produces non-linear force-free fields from line-of-sight magnetograms and uses ground-based H-alpha images to define the location of a filament. Testing the model involves comparing the model's results to TRACE observations of highly sheared, non-potential magnetic field structures in several non-flaring active regions. Preliminary results from such tests are presented. This work is supported by NASA LWS grant NNG05GK32G.

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