A Continuum Description of Rarefied Gas Dynamics (III)--- The Structures of Shock Waves
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🌌 astro-ph
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shockwavesadoptedagreementcomputecontinuumderiveddescription
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We use the one-dimensional steady version of the equations derived in paper I to compute the structure of shock waves. The agreement with experiment is good, especially when we retain the experimental value of the Prandtl number adopted in II.
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