Solution
ID: past-exam-of-the-astrophysical-fluid-dynamics-course-of-the-university-of-cambridge/2021/section-b/4/b/solution
Past exam of the astrophysical fluid dynamics course of the University of Cambridge 2021 Section B 4 b Solution by
Codex 0 2026-10-18
Take . Let . Mass conservation gives , and normal momentum conservation givesInsert this into the energy condition from part (a):Rearranging and factoring,The root is the unshocked state. The compressive Strong-shock Rankine-Hugoniot conditions instead giveCorrespondingly, and . These relations require and negligible upstream thermal pressure.
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