Solution
ID: past-exam-of-the-astrophysical-fluid-dynamics-course-of-the-university-of-cambridge/2019/section-b/4/solution
Past exam of the astrophysical fluid dynamics course of the University of Cambridge 2019 Section B 4 Solution by
Codex 0 2026-10-18
Following a fluid element. Let be a pathline, satisfying . The material derivative, also called the Lagrangian time derivative, is the rate observed while following that element. The multivariable chain rule givesThe partial derivative holds position fixed; the advection term accounts for motion through a spatially varying field. For a vector field, the same formula applies component by component in fixed Cartesian axes.
Momentum balance. For an inviscid flow, pressure is the only surface stress. A small material volume has net pressure force , obtained by the divergence theorem. Its mass is and its material acceleration is . Applying Newton's second law gives the Euler equations for an inviscid fluid,This is the local momentum conservation equation when viscosity and physical body forces are absent. A prescribed body force per unit mass would add on the right.
Changing to rotating coordinates. In a rotating frame with constant angular velocity , the lab acceleration is the rotating-frame material acceleration plus . ThereforeFor uniform rotation,With constant , this gives the Euler equation in a uniformly rotating frame,The term subtracted from is the equilibrium centrifugal contribution. Dividing the bracket by defines a reduced pressure , with units . The Coriolis acceleration remains a velocity-dependent term.
Linear disturbances. Linearize about rest in the rotating coordinates, with the equilibrium part of removed. The advective acceleration is quadratic in disturbance amplitude, so the linearized Euler equations and incompressible flow condition areTaking the curl removes the pressure gradient. The identitygives the inertial-wave vorticity equation,
Plane-wave frequencies. Let and use the given plane wave convention. Incompressible flow requires , and the vorticity equation givesFor a nonzero frequency, apply again, using . It follows thatThis is the inertial-wave dispersion relation. If is the angle of the wavevector to the rotation axis, the positive angular frequency is . It is largest, , for a parallel wavevector, decreases to zero for a perpendicular one, and is independent of the magnitude of the wavenumber at fixed direction. The two signs describe the two oscillatory polarization branches. When , the zero-frequency result is obtained directly from the linear equations rather than by dividing by ; it describes the nonoscillating balanced limit.
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