Skip to main content
Log in

Microflares and the Statistics of X-ray Flares

  • Published:
Space Science Reviews Aims and scope Submit manuscript

Abstract

This review surveys the statistics of solar X-ray flares, emphasising the new views that RHESSI has given us of the weaker events (the microflares). The new data reveal that these microflares strongly resemble more energetic events in most respects; they occur solely within active regions and exhibit high-temperature/nonthermal emissions in approximately the same proportion as major events. We discuss the distributions of flare parameters (e.g., peak flux) and how these parameters correlate, for instance via the Neupert effect. We also highlight the systematic biases involved in intercomparing data representing many decades of event magnitude. The intermittency of the flare/microflare occurrence, both in space and in time, argues that these discrete events do not explain general coronal heating, either in active regions or in the quiet Sun.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to I. G. Hannah.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Hannah, I.G., Hudson, H.S., Battaglia, M. et al. Microflares and the Statistics of X-ray Flares. Space Sci Rev 159, 263 (2011). https://doi.org/10.1007/s11214-010-9705-4

Download citation

  • Received:

  • Accepted:

  • Published:

  • DOI: https://doi.org/10.1007/s11214-010-9705-4

Keywords

Navigation