Supersonic Flow: Shock Waves and the Sound Barrier

simulator intermediate ~10 min
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β = 45.3° shock angle — pressure ratio 2.46 across shock

At Mach 2.0 with a 15° half-wedge angle, an oblique shock forms at 45.3° to the freestream. The pressure jumps by a factor of 2.46 and the downstream Mach number drops to about 1.45.

Formula

θ-β-M relation: tan θ = 2 cot β × (M²sin²β − 1) / (M²(γ + cos 2β) + 2)
Normal shock pressure ratio: P2/P1 = 1 + 2γ/(γ+1) × (Mn² − 1)
Speed of sound: a = √(γ × R × T)

Breaking the Sound Barrier

Below the speed of sound, pressure disturbances propagate ahead of an aircraft, allowing air to 'prepare' for its arrival. Above Mach 1, the aircraft outruns these signals — air encounters the vehicle with no warning and must adjust through shock waves, sudden discontinuities where pressure, temperature, and density spike. Chuck Yeager first exceeded Mach 1 in the Bell X-1 in 1947, proving that controlled flight beyond the sound barrier was possible despite violent buffeting in the transonic regime.

Oblique Shock Geometry

When supersonic flow encounters a wedge or cone, an oblique shock wave forms at a specific angle that depends on the Mach number and deflection angle. The θ-β-M relation — one of the most important equations in compressible flow — connects these three quantities. For a given Mach number, there is a maximum deflection angle beyond which an attached oblique shock cannot exist, and a curved detached bow shock forms instead. This simulation solves the θ-β-M relation numerically to find the shock geometry.

Across the Shock

Crossing an oblique shock, the flow changes abruptly. Pressure and temperature increase while velocity decreases. The normal component of Mach number drops below 1, but the tangential component is preserved — so the total downstream Mach number can remain supersonic. Engineers exploit this by using multiple weak oblique shocks (in supersonic inlets) rather than a single strong normal shock, dramatically reducing total pressure losses.

Expansion and Compression

Supersonic flow turning away from itself (around a convex corner) accelerates through a Prandtl-Meyer expansion fan — a continuous, isentropic process that is the opposite of a shock. By combining oblique shocks (compression) and expansion fans (acceleration), supersonic aerodynamicists can design efficient engine inlets, nozzles, and waverider vehicles that surf their own shock waves for maximum lift-to-drag ratio at hypersonic speeds.

FAQ

What is a shock wave?

A shock wave is an extremely thin region (a few mean free paths thick) where flow properties change discontinuously. When supersonic flow encounters an obstacle, information cannot propagate upstream (since disturbances travel at the speed of sound), so the flow adjusts through a sudden compression — a shock wave. Across a shock, pressure, temperature, and density all increase abruptly while velocity drops.

What is the difference between oblique and normal shocks?

A normal shock is perpendicular to the flow direction and always decelerates supersonic flow to subsonic. An oblique shock is angled to the flow, produced by a wedge or cone, and can leave the downstream flow still supersonic (weak shock solution). Oblique shocks are less dissipative, which is why supersonic inlets use them to decelerate air efficiently.

What causes a sonic boom?

A sonic boom is the ground-level manifestation of shock waves attached to a supersonic aircraft. The conical shock surfaces propagate to the ground as a sudden pressure rise followed by a pressure drop. The boom strength depends on the aircraft's size, altitude, and Mach number. NASA's X-59 is designed to create a quiet 'sonic thump' by carefully shaping the aircraft to prevent shock coalescence.

What is Mach number?

Mach number is the ratio of the object's speed to the local speed of sound. At sea level (15°C), the speed of sound is about 340 m/s. Mach 1 is the speed of sound; below Mach 1 is subsonic, above is supersonic. Above Mach 5 is hypersonic, where molecular dissociation and real-gas effects become important.

Sources

Embed

<iframe src="https://homo-deus.com/lab/aerospace/supersonic-flow/embed" width="100%" height="400" frameborder="0"></iframe>
View source on GitHub