Solution

ID: past-exam-of-the-astrophysical-fluid-dynamics-course-of-the-university-of-cambridge/2021/section-b/4/b/solution

Take . Let . Mass conservation gives , and normal momentum conservation gives
Insert 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 give
Correspondingly, and . These relations require and negligible upstream thermal pressure.

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