A new analysis of GOES soft X-ray data finds that larger flares in isolated active regions tend to be followed by longer waiting times until the next flare, a 'saturation' pattern that supports the build-up/release model of solar flares.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2019 1verdicts
REJECT 1representative citing papers
citing papers explorer
-
A Correlation in the Waiting-time Distributions of Solar Flares
A new analysis of GOES soft X-ray data finds that larger flares in isolated active regions tend to be followed by longer waiting times until the next flare, a 'saturation' pattern that supports the build-up/release model of solar flares.