Solution

ID: past-exam-of-the-astrophysical-fluid-dynamics-course-of-the-university-of-cambridge/2022/section-b/6/c/solution

Use complex amplitudes and take their real parts at the end. Write the radial surface displacement as and the combined potential as
The linear kinematic boundary condition is . Differentiate it once more in time and use the radial momentum equation, , evaluated at the unperturbed radius :
With , the mode amplitudes therefore satisfy
The prime differentiates the Modified Bessel function of the first kind with respect to its dimensionless argument, rather than with respect to . The result has units , as required because is a potential. It applies to ; the uniform limit requires separate treatment.

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