The study of the statistical distribution of short quiescent times (≤ 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.
@article{arxiv.astro-ph/0003420,
title = {Statistical Study of Short Quiescent Times Between Flares},
author = {Sebastien Galtier},
journal= {arXiv preprint arXiv:astro-ph/0003420},
year = {2015}
}
Comments
4 pages, 1 Postscript figure, submitted to Solar Physics