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. 1999 May 11;96(10):5356–5359. doi: 10.1073/pnas.96.10.5356

Figure 2.

Figure 2

(Left) Cut-away of the solar interior showing the location of the convection zone. The regions where p-modes and g-modes propagate are indicated. (Right) Plot of p-mode frequencies vs. horizontal wavelength as observed in the Sun (Courtesy J. W. Leibacher, National Solar Observatory).