Solution
ID: past-exam-of-the-astrophysical-fluid-dynamics-course-of-the-university-of-cambridge/2022/section-b/4/d/solution
Past exam of the astrophysical fluid dynamics course of the University of Cambridge 2022 Section B 4 d Solution by
Codex 0 2026-10-18
For , write and choose either signed branch , with . These two branches cover the roots of the squared dispersion relation. The group velocity of an internal gravity wave isIf instead the positive-frequency root is chosen for both signs of , set and multiply the displayed components by , away from the cusp .
Taking the dot product with the wave vector givesThus the group velocity, which describes the travel of a narrow wave packet and its energy, is perpendicular to the wave vector, and hence perpendicular to the phase velocity . This is the internal-wave phase and group velocity geometry. It also follows from phase-group orthogonality for degree-zero dispersion: the frequency depends only on the direction of , not its magnitude. For , the group velocity is zero, consistent with the stationary extremum .
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