Persistent Quasi-Periodic Pulsations During a Large X-Class Solar Flare
Laura A. Hayes, Peter T. Gallagher, Brian R. Dennis, Jack Ireland,, Andrew Inglis, and Diana E. Morosan

TL;DR
This study documents persistent quasi-periodic pulsations (QPP) throughout a large X8.2 solar flare, revealing different periods during impulsive and decay phases, linked to reconnection dynamics and MHD wave modes in post-flare loops.
Contribution
It provides detailed observations of QPP during both impulsive and decay phases of a major solar flare, highlighting their potential physical origins and evolution.
Findings
QPP with ~65 s period during impulsive phase
QPP with ~150 s period during decay phase
Persistent QPP linked to reconnection and MHD waves
Abstract
Solar flares often display pulsating and oscillatory signatures in the emission, known as quasi-periodic pulsations (QPP). QPP are typically identified during the impulsive phase of flares, yet in some cases, their presence is detected late into the decay phase. Here, we report extensive fine structure QPP that are detected throughout the large X8.2 flare from 2017 September 10. Following the analysis of the thermal pulsations observed in the GOES/XRS and the 131 A channel of SDO/AIA, we find a pulsation period of ~65 s during the impulsive phase followed by lower amplitude QPP with a period of ~150 s in the decay phase, up to three hours after the peak of the flare. We find that during the time of the impulsive QPP, the soft X-ray source observed with RHESSI rapidly rises at a velocity of approximately 17 km/s following the plasmoid/coronal mass ejection (CME) eruption. We interpret…
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The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1Kennicutt et al. (2006) Kennicutt, R. C., Jr., Vishniac, E., & Sneden, C. 2006, Ap J, 652, 847
- 2Kurtz et al. (2000) Kurtz, M. J., Eichhorn, G., Accomazzi, A., et al. 2000, A&AS, 143, 41
- 3Vishniac (2012) Vishniac, E. T. 2012, American Astronomical Society Meeting Abstracts #219, 219, 204.04
