A Statistical Study of Distant Consequences of Large Solar Energetic Events
Carolus J. Schrijver, Paul A. Higgins

TL;DR
This study analyzes how large solar flares influence remote solar regions, finding increased activity shortly after such events and a subsequent decrease, suggesting large flares destabilize distant magnetic regions temporarily.
Contribution
It provides a statistical analysis of distant sympathetic solar events associated with large flares, highlighting temporal patterns of increased and decreased activity post-flare.
Findings
Increased distant solar activity within 4 hours of large flares
Decreased activity between 4 and 24 hours after large flares
Large flares influence remote magnetic regions, affecting subsequent solar activity
Abstract
Large solar flares and eruptions may influence remote regions through perturbations in the outer-atmospheric magnetic field, leading to causally related events outside of the primary or triggering eruptions that are referred to as "sympathetic events." We quantify the occurrence of sympathetic events using the full-disk observations by the Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory associated with all flares of GOES class M5 or larger from 01 May 2010 through 31 December 2014. Using a superposed-epoch analysis, we find an increase in the rate of flares, filament eruptions, and substantial sprays and surges more than 20 degrees away from the primary flares within the first four hours at a significance of 1.8 standard deviations. We also find that the rate of distant events drops by two standard deviations, or a factor of 1.2, when comparing intervals between 4…
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