Journal of the Society of Motion Picture Engineers (1930-1949)

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1949 SCHLIEREN PHOTOGRAPHY 541 will coincide with the tangential and sagital image of the source. The separation of these two images is given by , sin2 a AS =/ cos a (29) To keep the light source out of the collimated beam, it must be displaced from the optic axis by a distance equal to at least one half the Fig. 15 — Light-intensity distribution in the image of a disturbance of Fig. 5 with a source 1.25 X 10~2-mm width for several knife-edge positions. A = 10, a = 1, <£ = 0.125 X, /= 250 cm. aperture of the system. If a is small, cos a = 1, sin a = a = A/L Equation (29) then becomes A5=/(^). (30) Since for most wind-tunnel systems the aperture A will be fixed by other than optical considerations, the only variable involved in controlling the astigmatic distance S will be focal length /. To keep S as small as possible, the focal length of the mirrors should be large.