Coronal Heating by Nanoflares and the Variability of the Occurrence Frequency in Solar Flares
- 1 October 1996
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 469 (2) , L135-L138
- https://doi.org/10.1086/310283
Abstract
No abstract availableThis publication has 16 references indexed in Scilit:
- Extended instability criteria in isotropic and anisotropic energy avalanchesPhysica A: Statistical Mechanics and its Applications, 1995
- An explanation for the flare frequency - energy dependenceSolar Physics, 1994
- Energy-crossing number relations for braided magnetic fieldsPhysical Review Letters, 1993
- Variability of the occurrence frequency of solar flares as a function of peak hard X-ray rateThe Astrophysical Journal, 1993
- Avalanches and the distribution of solar flaresThe Astrophysical Journal, 1991
- Solar flares, microflares, nanoflares, and coronal heatingSolar Physics, 1991
- Solar hard X-ray burstsSolar Physics, 1985
- Solar hard X-ray microflaresThe Astrophysical Journal, 1984
- Magnetic Neutral Sheets in Evolving Fields - Part Two - Formation of the Solar CoronaThe Astrophysical Journal, 1983
- ORIGIN OF COSMIC RAYSSoviet Physics Uspekhi, 1966