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Normal and Oblique Shock Waves Questions and Answers

Answer: A

No heat crosses the shock, so it is adiabatic, but the steep gradients inside it dissipate energy and raise entropy, so it is irreversible. That combination is why stagnation temperature survives a shock while stagnation pressure does not, a distinction worth keeping firmly in mind.

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Answer: B

The three conservation laws applied across the discontinuity, together with the equation of state, give the complete jump conditions. They are not isentropic relations and must not be confused with them: entropy is an output of the Rankine-Hugoniot analysis, not an assumed constant.

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Answer: C

Immediately behind the nearly normal portion of the bow shock the flow is subsonic. As it expands round the shoulder of the body it accelerates again, and the locus where it passes back through Mach one is the sonic line. Downstream of it the flow is supersonic once more.

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Answer: D

A larger deflection needs a stronger shock, and on the weak branch that means a larger shock angle. The angle grows until the maximum deflection for that Mach number is reached, and any further increase in wedge angle detaches the shock, which then stands off ahead of the leading edge.

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25.

For a fixed wedge angle, raising the upstream Mach number causes the attached oblique shock to

Answer: A

Higher Mach number means a smaller Mach angle and, on the weak branch, a smaller shock angle for the same deflection, so the shock wraps in closer to the surface. At hypersonic speeds the shock lies very close indeed, producing the thin shock layer characteristic of that regime.

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26.

A normal shock stands in a stream at \( M_1 = 2 \). The downstream Mach number is nearest to

Answer: B

The relation is \( M_2^2 = (1 + 0.2 M_1^2)/(1.4 M_1^2 - 0.2) \). Substituting, the numerator is \( 1 + 0.8 = 1.8 \) and the denominator \( 5.6 - 0.2 = 5.4 \), so \( M_2^2 = 0.3333 \) and \( M_2 = 0.577 \). Every normal shock leaves the flow subsonic, so any answer above one would be wrong on principle.

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27.

For a normal shock at \( M_1 = 2 \), the static pressure ratio \( p_2/p_1 \) is

Answer: C

The relation is \( p_2/p_1 = 1 + \frac{2\gamma}{\gamma+1}(M_1^2 - 1) \). With \( \gamma = 1.4 \) the coefficient is \( 2.8/2.4 = 1.1667 \), and \( M_1^2 - 1 = 3 \), so the ratio is \( 1 + 3.5 = 4.5 \). The pressure has more than quadrupled across a discontinuity a fraction of a micron thick.

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28.

For a normal shock at \( M_1 = 2 \), the density ratio \( \rho_2/\rho_1 \) is nearest to

Answer: D

The relation is \( \rho_2/\rho_1 = (\gamma+1)M_1^2 / ((\gamma-1)M_1^2 + 2) \), which gives \( 9.6 / 3.6 = 2.667 \). Compare this with the limiting value of six as the Mach number grows without bound: even at Mach 2 the shock has already achieved nearly half the compression that is available at any speed.

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29.

For a normal shock at \( M_1 = 2 \), the static temperature ratio \( T_2/T_1 \) is nearest to

Answer: A

The equation of state gives the temperature ratio as the pressure ratio divided by the density ratio, so \( 4.5 / 2.667 = 1.688 \). A stream at 250 K would emerge at about 422 K, which is why shock heating matters structurally even at modest supersonic speeds.

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30.

Air approaching an obstacle at \( M = 1.5 \) crosses a normal shock. The Mach number with which it emerges is nearest to

Answer: B

Substituting into \( M_2^2 = (1 + 0.2 M_1^2)/(1.4 M_1^2 - 0.2) \), the numerator is \( 1 + 0.45 = 1.45 \) and the denominator \( 3.15 - 0.2 = 2.95 \), giving \( M_2^2 = 0.4915 \) and \( M_2 = 0.701 \). The weaker shock leaves the flow closer to sonic than the Mach 2 case did.

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