Isentropic Flow Calculator
Determine the properties of fluid flow during an isentropic process using the Isentropic flow calculator.
The formula
T₀/T = 1 + (γ−1)M²/2; A/A* = (1/M)[2(1+(γ−1)M²/2)/(γ+1)]^((γ+1)/2(γ−1))
Stagnation heating is not friction
Bringing a fast-moving gas to rest converts its kinetic energy into internal energy, raising the temperature by (γ−1)M²/2 times the static value. At Mach 2 that is already 80% hotter; at Mach 6 it is more than sevenfold. This happens in an ideal, frictionless, reversible flow — it is compression, not rubbing, and it is why hypersonic vehicles have a thermal problem no amount of surface smoothness can fix.
Why nozzles have a throat
The area ratio A/A* has a minimum of exactly 1 at Mach 1 and rises on both sides, so every area ratio corresponds to two Mach numbers — one subsonic, one supersonic. A purely converging nozzle can therefore accelerate flow only up to Mach 1 at its exit, no further. Going supersonic requires the passage to converge to a throat and then DIVERGE, which reverses the usual intuition that narrowing speeds a flow up.
Once the pressure ratio falls below about 0.528 for air the throat chokes at Mach 1 and the mass flow stops responding to further reductions downstream. That is why a compressed-air line delivers a fixed flow regardless of what is downstream of the orifice.
Shocks destroy pressure, not energy
Across a normal shock the stagnation temperature is unchanged — no energy leaves the flow. Stagnation pressure, however, always falls, because the shock is irreversible. What is lost is not energy but the ability to do work with it, and recovering pressure efficiently is the entire design problem of a supersonic inlet.
The downstream flow is always subsonic, no matter how fast the upstream flow, and the density ratio saturates at (γ+1)/(γ−1) — six for air — however strong the shock becomes.