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Solar Physics

, Volume 153, Issue 1–2, pp 245–254 | Cite as

Searching for nanoflares

  • Jack B. Zirker
  • F. M. Cleveland
Article

Abstract

The evolution of hydrodynamic shocks generated by nanoflares in coronal loops is investigated in order to suggest requirements for future observations. The shocks produced by nanoflares of 1024 ergs decay within a few seconds, which sets stringent requirements for Doppler or transverse velocity measurements. With feasible improvements, the Normal Incidence X-ray Telescope could observe the time-averaged emission from a nanoflare, however. We also consider collisions between shocks and show that these could also be observed.

Keywords

Flare Solar Phys Emission Measure Coronal Loop Flare Energy 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 1994

Authors and Affiliations

  • Jack B. Zirker
    • 1
  • F. M. Cleveland
    • 2
  1. 1.National Solar Observatory/Sacramento PeakNational Optical Astronomy ObservatoriesSunspotUSA
  2. 2.Utility Consultants InternationalCupertinoUSA

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