Temporal Evolution of Magnetic Properties of Super Active Regions

Details Temporal Evolution of Magnetic Properties of Super Active Regions Temporal Evolution of Magnetic Properties of Super Active Regions

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.57c&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

It is widely accepted that solar flares are manifestations of magnetic reconnection events taking place in the solar atmosphere. Several aspects of these events remain unclear, although many efforts have been devoted to the investigation of magnetic field configurations at flares occurrence.
In this work we investigate some properties of 26 super active regions, observed between Jan 1 2000 and Dec 31 2006 with MDI/SOHO instrument and characterized by a particularly intense flare activity during their passage on the solar disc. We analyzed the temporal evolution of some fractal and multifractal estimators, as well as other parameters like the distorsion of the magnetic inversion line and the number of the singular points in potential fields with the aim to single out the most significant for flare forecasting.

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