A Continuum Description of Rarefied Gas Dynamics (III)--- The Structures of Shock Waves

Details A Continuum Description of Rarefied Gas Dynamics (III)--- The Structures of Shock Waves A Continuum Description of Rarefied Gas Dynamics (III)--- The Structures of Shock Waves

2001-05-20

arxiv.org/abs/astro-ph/0105348v1

Astronomy and Astrophysics

Astrophysics

18 pages, 12 figures

Scientific paper

10.1103/PhysRevE.65.036304

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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