Mixed-mode coupling in the red clump - I. Standard single star models

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Fig. A.2.

P, Q, and $\sqrt{PQ}$ $\sqrt{PQ}$ are shown as blue, orange, and black lines respectively. Solid lines show values calculated using the quadratic fit, and dotted lines show values using linear interpolation. The coloured circles show values at mesh points, with small circles being outside the evanescent zone and large circles inside. The vertical grey dashed lines show ±s₀.

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