A solar tornado triggered by flares?
N. K. Panesar, D. E. Innes, S. K. Tiwari, and B. C. Low

TL;DR
This study investigates the potential causal link between solar flares and tornado-like prominence activity, proposing that flares may trigger tornado formation through magnetic field interactions and cavity expansion.
Contribution
It introduces a new mechanism suggesting flares can trigger solar tornadoes via magnetic field contraction and cavity expansion, supported by multi-instrument observational analysis.
Findings
Flares and EUV waves occurred within 10 hours of tornado onset.
Tornado rotations started after the second flare.
Cavity expansion and tornado acceleration followed the third flare.
Abstract
Solar tornados are dynamical, conspicuously helical magnetic structures mainly observed as a prominence activity. We investigate and propose a triggering mechanism for the solar tornado observed in a prominence cavity by SDO/AIA on September 25, 2011. High-cadence EUV images from the SDO/AIA and the Ahead spacecraft of STEREO/EUVI are used to correlate three flares in the neighbouring active-region (NOAA 11303), and their EUV waves, with the dynamical developments of the tornado. The timings of the flares and EUV waves observed on-disk in 195\AA\ are analyzed in relation to the tornado activities observed at the limb in 171\AA. Each of the three flares and its related EUV wave occurred within 10 hours of the onset of the tornado. They have an observed causal relationship with the commencement of activity in the prominence where the tornado develops. Tornado-like rotations along the side…
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