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A Markov Chain Monte Carlo–based Hybrid Noise Inference for Continuous Wavelet Power Spectra: With Applications to Solar and Stellar Oscillatory Signals

  • Authors: Song Feng, Lin Li, Ding Yuan

Song Feng et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 5.

GOES 1–8 Å light curve for a quiet-Sun interval. (a) Observed soft X-ray flux. (b) Fourier power spectrum (FFT+MCMC). (c) Wavelet power spectrum from the CWT+AR(1) method. (d) Wavelet power spectrum from the CWT+MCMC method. A localized feature near ∼128 s is present in panel (c) but not in the other representations. Black contours indicate the 95% confidence level.

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