Solution
ID: past-exam-of-the-astrophysical-fluid-dynamics-course-of-the-university-of-cambridge/2013/paper-1/1/a/solution
Past exam of the astrophysical fluid dynamics course of the University of Cambridge 2013 Paper 1 1 a Solution by
Codex 0 2026-10-20
Let measure distance down the incline and distance perpendicular to it, with the wall at and the free surface at . A uniform steady falling film flow has . Its convective acceleration vanishes because and . A flat surface exposed to constant atmospheric pressure hasThus , and the downslope component of the Navier-Stokes equations reduces to . The printed pressure-free equation must be understood as this downslope projection: its full vector version would incorrectly omit the normal hydrostatic pressure gradient that balances .
The no-slip boundary condition gives . Neglecting air shear stress makes the surface shear-free, so . Two integrations give the uniform gravity-driven Newtonian film profileThe velocity increases up to the free surface, whereThis assumes a uniform laminar Newtonian fluid film, a stationary wall and negligible surface shear; a varying thickness or externally imposed downslope pressure gradient would alter the balance.
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