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arXiv · 2407.03639

Quasi-periodic oscillations of flare loops and slipping motion of ribbon substructures during a C-class flare

Yining Zhang·Ting Li·Jing Ye
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Abstract

Quasi-periodic oscillations in solar flaring emission have been observed over the past few decades. To date, the underpinning processes resulting in the quasi-periodic oscillations remain unknown. In this paper, we report a unique event that exhibits both the long-duration quasi-periodic intensity oscillations of flare loops and the quasi-periodic slipping motion of ribbon substructures during a C9.1-class flare (SOL2015-03-15-T01:15), using the observations from Solar Dynamics Observatory and Interface Region Imaging Spectrograph. The high-temperature flare loops rooted in the straight part of ribbons display a "bright-dim" intensity oscillation, with a period of about 4.5 minutes. The oscillation starts just after the flare onset and lasts over 3 hours. Meanwhile, the substructures within the ribbon tip display the quasi-periodic slipping motion along the ribbon at 1400 \AA images which has a similar periodicity to the stationary intensity oscillation of the flare loops in the straight part of the flare ribbons. We suggest that the quasi-periodic pattern is probably related to the loop-top dynamics caused by the reconnection outflow impinging on the flare loops.

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Yining Zhang, Ting Li, Jing Ye. 2024-07-04. Quasi-periodic oscillations of flare loops and slipping motion of ribbon substructures during a C-class flare. https://arxiv.org/abs/2407.03639

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