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A Survey of Unsteady Hypersonic Flow Problems

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- 20 -<br />

<strong>of</strong> a disturbance is <strong>of</strong> order sd(= a@). Consequently, the second limitation<br />

can be expressed by<br />

03..<br />

x >> 66<br />

where- X is the wavelength <strong>of</strong> the disturbance.<br />

h/d >> 6 . . . (2.22)<br />

Sychev has shown, in Ref. 25, that a fdrm <strong>of</strong> small disturbance theory<br />

can be developed for bodies at large incidence in hypersonic flow, provided that<br />

the flow on the leeward side <strong>of</strong> the bcdy can be neglected. From this development<br />

<strong>of</strong> the theory it can be shown that on the windward side <strong>of</strong> the body the flow in<br />

a lamina <strong>of</strong> fluid normal to the axis <strong>of</strong> the body can be considered as independent<br />

<strong>of</strong> the flow in adJacent laminae. The form that the equations take will be<br />

illustrated, as before, by considering the general equations <strong>of</strong> motion <strong>of</strong> the<br />

fluid. The equations are presented this time in non-dimensional form as, far<br />

this case, the development can be seen more clearly.<br />

The axes &, '1, C., are taken with origin at the nose <strong>of</strong> the body and<br />

the &-axis in the mean direction <strong>of</strong> the principal body axis and the z-axis in<br />

the plane <strong>of</strong> the &-axis and the flow direction (Fig. 6). The independent<br />

variables are made non-dimensIona by the transformations:<br />

g = -, & 11 T = tu co9 a<br />

;i = --&,<br />

. . . (2.23)<br />

b<br />

where b is the body length, 6 is a ratio representing the maximum surface<br />

slope, a is the angle <strong>of</strong> incidence <strong>of</strong> the body and U is the flow velocity<br />

<strong>of</strong> the free stream.<br />

The dependent variables are made non-dimensional by the transformations:<br />

u cos 01 + u v W<br />

= l+ii, 7 = f w =<br />

u 00s a U sin a U sin a<br />

P P<br />

P = , and p = - . . .<br />

pm ua sFna a<br />

PC0<br />

where u, v, w are the velocity perturbations in the &, i, G directions.<br />

Then the general equations <strong>of</strong> fluid motion become<br />

pm u cos a a;; pm u cos OL as; poou sina a(3 pmU sina a(3<br />

-+ -+ -+<br />

b ax b E b6 a? b& a4<br />

b<br />

(2.24)<br />

poou co.9 a a(3<br />

= - -, . . . (2.25)<br />

b E<br />

u2cos2a<br />

b<br />

I

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