Fig. 4.
Contribution to the frequency shift of p modes by changes to solar structure variables ρ, p, c2, g, and the flow field u caused by a g mode in absolute values. The total frequency shift |δνp| and the contribution from an example term (δℒ3−2, see Eq. (D.21)) are also given for comparison. The azimuthal order of the modes is mp = mg = 0.
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