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A Survey of Unsteady Hypersonic Flow Problems

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- 26 -<br />

This simple form <strong>of</strong> the method ignores the<br />

disturbances frcm the body surface at the shock wave<br />

gradient in the flow, and. the picture <strong>of</strong> the flow 33<br />

effect <strong>of</strong> the reflection <strong>of</strong><br />

ana from regions <strong>of</strong> entropy<br />

consisting <strong>of</strong> a straight<br />

shock wave from the nose followed by a simple expansion is not in general<br />

adequate for the whole field. The significance <strong>of</strong> these reflections has been<br />

examined. in Ref. 28 and it is found that, at the body surface, the reflected<br />

disturbances tend to cancel each other for the condition y > l-3. Since this<br />

condition holds for most flows <strong>of</strong> practical interest, the simple theory is<br />

adequate to give surface pressure information.<br />

For thin two-dimensional sections undergoing small-amplitude sinusozdal<br />

distortions about zero mean incidence in flow3 <strong>of</strong> sufficiently high Mach numbers,<br />

the expressions for the nose shock conditions and for the Prandtl-Meyer relation<br />

can be simplified and, as a result, a closed-form expression for the lift<br />

distribution can be developed. For a symmetrical section the expression is 19 :<br />

Pe‘PU = ze ikt<br />

PC0<br />

c &[(8)"-II+1<br />

(y-1 1<br />

1 +- Ei.J 'ii(x)<br />

+ 2 3<br />

- k(O)<br />

X? - + ikg(0) 1 emilm +<br />

CL ax<br />

+ yi& [miq x) -1 J<br />

2y/(v-1)<br />

h(O)<br />

- + ikg(O)] emikx +[z + ikg]] . . . (2.49)<br />

ax<br />

where g(x) is the complex amplitude <strong>of</strong> the time-dependent motion; n and m<br />

are the rates-<strong>of</strong> change <strong>of</strong> pressure and Mach number at the nose with change <strong>of</strong><br />

nose angle; "N is the value <strong>of</strong> the Mach number at the nose for sero distortion;<br />

@ is the value <strong>of</strong> the shock inclination angle for zero distortion; and z(x)<br />

is the turning angle <strong>of</strong> the flow from the nose due to thichess alone.<br />

For conditions where the simplified expressions for the nose conditions<br />

and the expansion could not be applied, where the amplitude was not small, or<br />

when real gas effect3 became important, numerical methods would have tL be<br />

employed.<br />

The shock-expansion method can be applied to slender three-dimensional<br />

bodies for which MS is greater than a limit around unity (the limit is not<br />

rigid; errors become greater as unity is approached) because it can be shown<br />

for such bodies that the flow on the body surface is locally two-d' TJym; :",<br />

planes normal to the body surface and tangential to the streamlines<br />

as a consequence <strong>of</strong> this, the Prandtl-Meyer relation can be applied along the<br />

surface streamlines. The surface streamlines can be shown to follow closely the<br />

surface geodesics through the nose. A geodesic is a line on a surface such that<br />

at any point its projection on the tangent plane at that point has zero curvature;<br />

it is determined by the geometry <strong>of</strong> the surface so that once the initial direction<br />

<strong>of</strong> the surface streamlines is known the expansion conbtiona can, in principle,<br />

be determined from the geometry <strong>of</strong> the surface. The condition3 at the nose <strong>of</strong><br />

the body must, <strong>of</strong> course, be found from the flow over a cone hating the 3ame<br />

cross-section as the body at the nose. This presents a limitation for the<br />

application <strong>of</strong> the method since the flow is known only for cones with certain<br />

simple cross-sections at small angles <strong>of</strong> yaw.<br />

x

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