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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. 2.

Scatter plots of ﹩\delta \tau ﹩ against the total magnetic flux density ﹩B_{\mathrm{tot}\,}﹩ (estimated from the MDI line‐of‐sight magnetogram assuming the magnetic field is the gradient of a potential). For clarity, only 1 out of 15 points is plotted. The vertical bars indicate the range of ±1 standard deviation about the mean over bins equally spaced over the logarithm of the flux density. The three cases shown are representative samples of the types of variations observed: (a) shows the results for filter A at ﹩\nu _{0}=5﹩ mHz, (b) shows filter C at 3 mHz, and (c) shows filter E at 4 mHz.

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