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Observed Frequency Variations of Solar p‐Mode Travel Times as Evidence for Surface Effects in Sunspot Seismology

  • Authors: D. C. Braun and A. C. Birch

Braun & Birch 2006 The Astrophysical Journal Letters 647 L187.

  • Provider: AAS Journals

Caption: Fig. 3.

(a) Mean travel‐time perturbations, averaged over all sunspot umbrae in the four spot groups observed, divided by the group travel times as functions of the phase speed w, where the orange, red, green, and blue symbols indicate results for ﹩\nu _{0}=2﹩, 3, 4, and 5 mHz, respectively. The open circles indicate the filter and frequency combinations which are dominated by the ﹩p_{1}﹩‐mode. Horizontal bars indicate the range of ﹩w﹩ present within the filter and frequency bandpass, and the vertical bars indicate the standard deviation of the mean. The colored lines indicate the predicted values computed from a sound‐speed proxy (see text), where the colors indicate the same ﹩\nu _{0}﹩ as the observations. (b) Fractional travel‐time perturbations as a function of the inverse of the mean mode mass.

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