Statistical Study of Short Quiescent Times Between Flares
classification
🌌 astro-ph
keywords
flaresquiescentshortstatisticaltimesbeenbehaviourdistribution
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.