The Non-Potential Structure of Solar Active Regions

Details The Non-Potential Structure of Solar Active Regions The Non-Potential Structure of Solar Active Regions

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...208.6508d&link_type=abstract

American Astronomical Society Meeting 208, #65.08; Bulletin of the American Astronomical Society, Vol. 38, p.145

Astronomy and Astrophysics

Astronomy

Scientific paper

Various methods for constructing 3D models of the coronal field are discussed. The flux-rope insertion method is found to give a good fit to TRACE observations of coronal loops near an H-alpha filament. Data from the Advanced Stokes Polarimeter is used for extrapolating photospheric vector fields into the corona. Tests indicate that models based on chromospheric vector-field data are more reliable than those based on photospheric data.

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