The Rankine body of revolution of Fig. 8.26 could simulate the shape of a pitotstatic tube (Fig.
Question:
The Rankine body of revolution of Fig. 8.26 could simulate the shape of a pitotstatic tube (Fig. 6.30). According to in viscid theory, how far downstream from the nose should the static-pressure holes be placed so that the local surface velocity is within 0.5% of U? Compare your answer with the recommendation x ≈8D in Fig. 6.30.
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