Statistical Study of Short Quiescent Times Between Flares

Abstract

The study of the statistical distribution of short quiescent times ($\le$ 30 minutes) between solar flares has been investigated on a 1D MHD model. A power law behaviour is found which indicates the existence of sympathetic flaring. This prediction is supported by recent observations.

4 pages, 1 Postscript figure, submitted to Solar Physics

References in corpus (1)

• The Origin of the Solar Flare Waiting-Time Distribution

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