Soft X-Ray Pulsations in Solar Flares

@article{Simes2015SoftXP,
  title={Soft X-Ray Pulsations in Solar Flares},
  author={P J A Sim{\~o}es and Hugh S Hudson and Lyndsay Fletcher},
  journal={Solar Physics},
  year={2015},
  volume={290},
  pages={3625-3639}
}
  • P J A Simões, Hugh S Hudson, Lyndsay Fletcher
  • Published 2015
  • Physics
  • Solar Physics
  • The soft X-ray emissions (hν>1.5 keV) of solar flares mainly come from the bright coronal loops at the highest temperatures normally achieved in the flare process. Their ubiquity has led to their use as a standard measure of flare occurrence and energy, although the overwhelming bulk of the total flare energy goes elsewhere. Recently Dolla et al. (Astrophys. J. Lett.749, L16, 2012) noted quasi-periodic pulsations (QPP) in the soft X-ray signature of the X-class flare SOL2011-02-15, as observed… CONTINUE READING

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