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Toward Reliable Benchmarking of Solar Flare Forecasting Methods View all abstracts by submitter

D. Shaun Bloomfield   Submitted: 2012-02-27 09:04

Solar flares occur in complex sunspot groups, but it remains unclearhow the probability of producing a flare of a given magnitude relatesto the characteristics of the sunspot group. Here, we useGeostationary Operational Environmental Satellite X-ray flares andMcIntosh group classifications from solar cycles 21 and 22 tocalculate average flare rates for each McIntosh class and use these todetermine Poisson probabilities for different flare magnitudes.Forecast verification measures are studied to find optimum thresholdsto convert Poisson flare probabilities into yes/no predictions ofcycle 23 flares. A case is presented to adopt the true skill statistic(TSS) as a standard for forecast comparison over the commonly usedHeidke skill score (HSS). In predicting flares over 24 hr, the maximumvalues of TSS achieved are 0.44 (C-class), 0.53 (M-class), 0.74(X-class), 0.54 (>=M1.0), and 0.46 (>=C1.0). The maximum values of HSSare 0.38 (C-class), 0.27 (M-class), 0.14 (X-class), 0.28 (>=M1.0), and0.41 (>=C1.0). These show that Poisson probabilities performcomparably to some more complex prediction systems, but the overallinaccuracy highlights the problem with using average values torepresent flaring rate distributions.

Authors: D. Shaun Bloomfield, Paul A. Higgins, R. T. James McAteer, and Peter T. Gallagher
Projects: None

Publication Status: Published in ApJL
Last Modified: 2012-02-29 08:25
Go to main E-Print page  On the physical meaning of n-distributions in solar flares  Break up of returning plasma after the 7 June 2011 filament eruption by Rayleigh-Taylor instabilities  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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