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Acta Geophysica

, Volume 57, Issue 1, pp 52–63 | Cite as

Flare forecasting based on sunspot-groups characteristics

  • Lidia Contarino
  • Francesca ZuccarelloEmail author
  • Paolo Romano
  • Daniele Spadaro
  • Salvatore L. Guglielmino
  • Viviana Battiato
Article

Abstract

Our comprehension of solar flares is still lacking in many aspects and the possibility of observing active regions during the first phases of flare occurrence is limited by our capability of doing accurate flare forecasting. In order to give a contribution to this aspect, we focused our attention on the characteristics that must be fulfilled by sunspot-groups in order to be flare-productive. We addressed this problem using a statistical approach: first, we analyzed sunspot-groups parameters (i.e., Zürich class, magnetic configuration, area, morphology of the penumbra) and evolution; then, we performed a flare forecasting campaign, based on the results obtained in the first phase and on real-time observations. The results obtained by comparing the flare forecasting probability with the number of flares that have actually occurred are quite encouraging; we plan to improve this procedure by including a bigger statistical sampling.

Key words

solar flares sunspot-groups flare forecasting 

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Copyright information

© © Versita Warsaw and Springer-Verlag Berlin Heidelberg 2009

Authors and Affiliations

  • Lidia Contarino
    • 1
  • Francesca Zuccarello
    • 2
    Email author
  • Paolo Romano
    • 1
  • Daniele Spadaro
    • 1
  • Salvatore L. Guglielmino
    • 2
  • Viviana Battiato
    • 2
  1. 1.INAF Osservatorio Astrofisico di CataniaCataniaItaly
  2. 2.Dipartimento di Fisica e AstronomiaUniversitá di CataniaCataniaItaly

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