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  • Article
  • Open Access

Hard X-rays from Slow Flares

Earth, Planets and Space201453:BF03353274

https://doi.org/10.1186/BF03353274

  • Received: 14 June 2000
  • Accepted: 11 January 2001
  • Published:

Abstract

“Slow LDEs” are those for which the rise phase is slow, as well as the decay phase. Such flares follow the Neupert effect, which implies that the non-thermal energy release has a similar relationship to heating as in a normal impulsive flare. Based on a sample of 53 slow LDEs during the first nine years of Yohkoh observations, we find 19 for which substantial overlap occurs with BATSE hard X-ray observations. These events tend strongly to have extended hard X-ray emission even though their hard X-ray emission does not tend to be “impulsive” in the sense of rapid variation. The hard X-ray fluences for these 19 events correlate with the soft X-ray peak fluxes, implying strong non-thermal particle acceleration even for these relatively slow energy-release rates. These events often correspond to the occurrence of “supra-arcade downflows,” a phenomenon consistent with the classical reconnection model for gradual-phase flare energy release. This correspondence suggests a close relationship, not depending strongly upon time scale, between large-scale reconnection and the acceleration of non-thermal electrons.

Keywords

  • Coronal Mass Ejection
  • Magnetic Reconnection
  • Rise Phase
  • Neupert Effect
  • Coronal Reconnection

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