Statistical Study of Short Quiescent Times Between Flares

Details Statistical Study of Short Quiescent Times Between Flares Statistical Study of Short Quiescent Times Between Flares

2000-03-28

arxiv.org/abs/astro-ph/0003420v2

Astronomy and Astrophysics

Astrophysics

4 pages, 1 Postscript figure, submitted to Solar Physics

Scientific paper

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.

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