First detection of transverse vertical oscillation during the expansion of coronal loops
Qingmin Zhang, Chuan Li, Dong Li, Ye Qiu, Yanjie Zhang, and Yiwei Ni

TL;DR
This study reports the first observation of transverse vertical oscillation of coronal loops during the expansion phase of a solar flare, revealing new insights into flare-loop interactions and coronal dynamics.
Contribution
It introduces a novel observation of transverse vertical oscillation during coronal loop expansion and proposes a unified scenario explaining both contraction and expansion phenomena.
Findings
EUV wave propagates at 740-860 km/s, indicating a fast-mode shock.
Oscillation periods of 253 s and 275 s observed in different wavelengths.
Interaction between EUV wave and coronal loops causes contraction, expansion, and oscillation.
Abstract
In this Letter, we perform a detailed analysis of the M5.5-class eruptive flare occurring in active region 12929 on 2022 January 20. The eruption of a hot channel generates a fast coronal mass ejection (CME) and a dome-shaped extreme-ultraviolet (EUV) wave at speeds of 740860 km s. The CME is associated with a type II radio burst, implying that the EUV wave is a fast-mode shock wave. During the impulsive phase, the flare shows quasi-periodic pulsations (QPPs) in EUV, hard X-ray, and radio wavelengths. The periods of QPPs range from 18 s to 113 s, indicating that flare energy is released and nonthermal electrons are accelerated intermittently with multiple time scales. The interaction between the EUV wave and low-lying adjacent coronal loops (ACLs) results in contraction, expansion, and transverse vertical oscillation of ACLs. The speed of contraction in 171, 193, and 211 {\AA}…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Gamma-ray bursts and supernovae
