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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. 1.

(a) MDI intensity, (b) line‐of‐sight magnetogram, and (ch) sample maps of the mean travel‐time perturbation covering a portion of the region studied and showing sunspot group AR 9885. Panels c and d show travel‐time maps for filter C at 3 and 4 mHz, respectively (see Table 1). Panels eh show the travel‐time maps for filter E at 2, 3, 4, and 5 mHz, respectively.

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