Non-linear Force-free Modeling: Applications To Solar Data

Details Non-linear Force-free Modeling: Applications To Solar Data Non-linear Force-free Modeling: Applications To Solar Data

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.1805d&link_type=abstract

American Astronomical Society, SPD meeting #37, #18.05; Bulletin of the American Astronomical Society, Vol. 38, p.247

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Scientific paper

Understanding the conditions under which solar magnetic fields can destabilizeto cause flares and other eruptive events requires a quantitativeunderstanding of the coronal magnetic field and of the currents that itcarries. Because no direct measurements of magnetic fields and current withincoronal volumes exist, the coronal field is typically modeled usinginformation contained in photospheric vector magnetograms, to be compared toH-alpha images of the chromosphere and EUV and X-ray imagery of the corona.We report on recent results of a team effort to further understand theintricacies of non-linear force-free extrapolations of the coronal magneticfield, presenting results from several solar and solar-like test cases. Wealso consider the use of such coronal field modeling in the upcoming Solar-Band SDO missions.

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