A Possible Selection Rule for Flares Causing Sunquakes
Ruizhu Chen, Junwei Zhao

TL;DR
This study proposes a hypothesis that sunquakes are more likely to occur when solar flares impact areas with downward oscillations, supported by analysis of 60 strong flares and helioseismic data from Solar Cycle 24.
Contribution
The paper introduces a new hypothesis linking background oscillations to sunquake occurrence and verifies it through helioseismic analysis of multiple solar flares.
Findings
Majority of sunquakes occur during downward oscillations in the 3-5 mHz and 5-7 mHz bands.
Helioseismic holography effectively reconstructs oscillatory velocities during flares.
Results support the hypothesis that downward background oscillations influence sunquake generation.
Abstract
Sunquakes are helioseismic power enhancements initiated by solar flares, but not all flares generate sunquakes. It is curious why some flares cause sunquakes while others do not. Here we propose a hypothesis to explain the disproportionate occurrence of sunquakes: during a flare's impulsive phase when the flare's impulse acts upon the photosphere, delivered by shock waves, energetic particles from higher atmosphere, or by downward Lorentz Force, a sunquake tends to occur if the background oscillation at the flare footpoint happens to oscillate downward in the same direction with the impulse from above. To verify this hypothesis, we select 60 strong flares in Solar Cycle 24, and examine the background oscillatory velocity at the sunquake sources during the flares' impulsive phases. Since the Doppler velocity observations at sunquake sources are usually corrupted during the flares, we…
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