Fig. 13.
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Relationship between QPP period (P) and lifetime (τ) across different flare scales. Blue, orange, and green dots represent QPPs detected in EUV brightenings (this study), GOES X-ray solar flares (Hayes et al. 2020), and TESS stellar flares (Joshi et al. 2025), respectively. The dashed black line shows a power-law fit to the combined dataset.
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