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Zienkiewicz O.C., Taylor R.L. Vol. 3. The finite - tiera.ru

Zienkiewicz O.C., Taylor R.L. Vol. 3. The finite - tiera.ru

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172 Compressible high-speed gas ¯ow<br />

6.<strong>3.</strong>1 Euler equation<br />

Here only ®rst-order derivatives occur and the number of boundary conditions is less<br />

than that for the full Navier±Stokes problem.<br />

For a solid wall boundary, ÿ u, only the normal component of velocity u n needs to be<br />

speci®ed (zero if the wall is stationary). Further, with lack of conductivity the energy<br />

¯ux across the boundary is zero and hence E (and ) remain unspeci®ed.<br />

In general the analysis domain will be limited by some arbitrarily chosen external<br />

boundaries, ÿ s, for exterior or internal ¯ows, as shown in Fig. 6.1 (see also Sec. <strong>3.</strong>6,<br />

Chapter 3).<br />

Here, as discussed in Sec. 2.10.3, it will in general be necessary to perform a<br />

linearized Riemann analysis in the direction of the outward normal to the boundary<br />

n to determine the speeds of wave propagation of the equations. For this linearization<br />

of the Euler equations three values of propagation speeds will be found<br />

1 ˆ u n<br />

2 ˆ un ‡ c<br />

3 ˆ un ÿ c<br />

…6:8†<br />

where un is the normal velocity component and c is the compressible wave celerity<br />

(speed of sound) given by<br />

r<br />

c ˆ<br />

p<br />

…6:9†<br />

As of course no disturbances can propagate at velocities greater than those of Eqs<br />

(6.8) and in the case of supersonic ¯ow, i.e. when the local Mach number is<br />

M ˆ junj 5 1 …6:10†<br />

c<br />

we shall have to distinguish two possibilities:<br />

(a) supersonic in¯ow boundary where<br />

un < ÿc<br />

and the analysis domain cannot in¯uence the exterior, for such boundaries all<br />

components of the vector must be speci®ed; and<br />

Γ u<br />

Γ s<br />

External flow Internal flow<br />

Fig. 6.1 Boundaries of a computation domain. ÿ u, wall boundary; ÿ s, ®ctitious boundary.<br />

Γ s<br />

Γ u<br />

Γ s

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