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Multitaper Spectral Analysis and Wavelet Denoising Applied to Helioseismic Data

  • Authors: R. W. Komm, Y. Gu, F. Hill, P. B. Stark, and I. K. Fodor

Komm et al. 1999 The Astrophysical Journal 519 407.

  • Provider: AAS Journals

Caption: Fig. 6.

Histograms of the number of good fits (solid line) as a function of frequency for the periodogram, the sine multitaper spectrum, and the corresponding denoised multitaper spectrum of ﹩\ell =30﹩. Each bin contains the modes of a single n‐value summed over all m. The dotted line represents the total number of fits including the bad ones, and the dashed line represents the good fits from the panel above.

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