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Sod shock tube : ウィキペディア英語版
Sod shock tube

]
The Sod shock tube problem, named after Gary A. Sod, is a common test for the accuracy of computational fluid codes, like Riemann solvers, and was heavily investigated by Sod in 1978.
The test consists of a one-dimensional Riemann problem with the following parameters, for left and right states of an ideal gas.


\left( \begin\rho_L\\P_L\\v_L\end\right)
=
\left( \begin1.0\\1.0\\0.0\end \right)

,

\left( \begin\rho_R\\P_R\\v_R\end\right)
=
\left( \begin0.125\\0.1\\0.0\end\right)


where
::
*\rho is the density
::
*P is the pressure
::
*v is the velocity
The time evolution of this problem can be described by solving the Euler equations,
which leads to three characteristics, describing the propagation speed of the
various regions of the system. Namely the rarefaction wave, the contact discontinuity and
the shock discontinuity.
If this is solved numerically, one can test against the analytical solution,
and get information how well a code captures and resolves shocks and contact discontinuities
and reproduce the correct density profile of the rarefaction wave.
==Analytic derivation==
The different states of the solution are separated by the time evolution of the
three characteristics of the system, which is due to the finite speed
of information propagation. Two of them are equal to the speed
of sound of the both states
::cs_1 = \sqrt}
::cs_5 = \sqrt}
The first one is the position of the beginning of the rarefaction wave while
the other is the velocity of the propagation of the shock.
Defining:
::\Gamma = \frac, \beta = \frac
The states after the shock are connected by the Rankine Hugoniot
shock jump conditions.
::\rho_4 = \rho_5 \frac
But to calculate the density in Region 4 we need to know the pressure in that region.
This is related by the contact discontinuity with the pressure in region 3 by
::P_4 = P_3
Unfortunately the pressure in region 3 can only be calculated iteratively, the right
solution is found when u_2 equals u_4
::u_4 = \left(P_3' - P_5\right)\sqrt}
::u_2 =\left(P_1^\beta-P_3'^\beta\right) \sqrt}
::u_2 - u_4 = 0
This function can be evaluated to an arbitrary precision thus giving the pressure in the
region 3
::P_3 = \operatorname(P_3,s,s,,)
finally we can calculate
::u_3 = u_5 + \frac((\gamma+1)P_3 +(\gamma-1)P_5)}}
::u_4 = u_3
and \rho_3 follows from the adiabatic gas law
::\rho_3 = \rho_1 \left(\frac\right)^

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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