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A Universal Scaling between Damping Time and Period of Quasi-periodic Pulsations from Solar Extreme-Ultraviolet Brightenings to X-Ray Stellar Flares

  • Authors: Daye Lim, Tom Van Doorsselaere, Valery M. Nakariakov, S. Krishna Prasad, David Berghmans, Laura A. Hayes, Kyung-Suk Cho, Sujin Kim

Daye Lim et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 2.

Time-series analysis of the events illustrated in Figure 1. Panels (a)–(c) show the EUV brightening, and panels (d)–(f) show the solar flare. (a), (d) Example EUV light curves (black), with background trends derived using EMD (blue solid curves). (b), (e) Detrended signals composed of IMFs, together with the best-fitting damped harmonic oscillation models (blue dashed curves). (c), (f) Power spectra of the detrended signals. The vertical blue line marks the fitted period, while the purple, red, and yellow curves denote the 99%, 95%, and 90% confidence levels, respectively.

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