A statistical correlation of sunquakes based on their seismic, white light, and X-ray emission
J.C. Buitrago-Casas, J.C. Martinez Oliveros, C. Lindsey, B., Calvo-Mozo, S. Krucker, L. Glesener, S. Zharkov

TL;DR
This study investigates the correlation between sunquakes, high-energy X-ray emissions, and white-light enhancements during solar flares, revealing a strong link between seismic activity and visible continuum increases.
Contribution
It provides the first comprehensive correlation analysis linking sunquakes with X-ray and white-light emissions, using data from RHESSI and SDO/HMI.
Findings
18 sunquakes identified out of 75 flares
All sunquakes associated with visible continuum enhancement
Strong correlation between seismic detection methods and sunquake occurrence
Abstract
Several mechanisms have been proposed to explain the transient seis- mic emission, i.e., sunquakes, from some solar flares. Some theories associate high-energy electrons and/or white-light emission with sunquakes. High-energy charged particles and their subsequent heating of the photosphere and/or chro- mosphere could induce acoustic waves in the solar interior. We carried out a correlative study of solar flares with emission in hard-X rays (HXRs), enhanced continuum emission at 6173{\AA}, and transient seismic emission. We selected those flares observed by RHESSI (Reuven Ramaty High Energy Solar Spectroscopic Imager) with a considerable flux above 50 keV between January 1, 2010 and June 26, 2014. We then used data from the Helioseismic and Magnetic Imager onboard the Solar Dynamic Observatory (SDO/HMI) to search for excess visible continuum emission and new sunquakes not previously…
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