Automated Classification of Flaring Behavior in Solar Active Regions: Preliminary Results

Details Automated Classification of Flaring Behavior in Solar Active Regions: Preliminary Results Automated Classification of Flaring Behavior in Solar Active Regions: Preliminary Results

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21914516a&link_type=abstract

American Astronomical Society, AAS Meeting #219, #145.16

Physics

Scientific paper

Solar active events are the source of many energetic and geo-effective events such as solar flares and coronal mass ejections (CMEs). Understanding how these complex source regions evolve and produce these events is of fundamental importance, not only to solar physics but also the demands of space weather forecasting. In this poster, we present preliminary results from our analysis of the physical properties of active region magnetic fields using fractal-, gradient-, neutral line-, emerging flux-, and wavelet-based techniques. These analyses look to use the defined physical measures to form a predictive model for flaring behavior in active regions.

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