This page is the "no case left behind" companion to 3.3.15 Under-expanded nozzle — Prandtl-Meyer expansion, efficiency loss (Hinglish) 's English parent. We march through every kind of situation an under-expanded nozzle problem can hand you — every sign of the pressure gap, the degenerate "just barely" cases, the extreme limits, a real flight problem, and an exam trap — and solve each one fully.
Before line one, one promise: nothing gets used before it is built. Let us build the three tools we lean on.
Definition Pressure ratio
p e / p ∞ — the "who's stronger" number
p e is the exit static pressure : how hard the exhaust pushes sideways on its own gas as it leaves the nozzle mouth. p ∞ is the ambient pressure : how hard the surrounding air pushes back.
Their ratio r = p e / p ∞ is a single number that tells the whole story:
r > 1 → exhaust wins → gas keeps expanding outside → under-expanded (our topic).
r = 1 → tie → perfectly expanded , no waves.
r < 1 → air wins → gas gets squeezed by shocks → over-expanded (see 3.3.14-Over-expanded-nozzle-shock-diamonds ).
M — "how many times the speed of sound"
M = v / a , where v is the gas speed and a is the local speed of sound. M > 1 is supersonic . It matters here because supersonic gas cannot send warnings upstream — that is why the expansion has to happen through a fan of waves and not a smooth uniform swell. This idea comes straight from 3.2.7-Isentropic-flow-area-Mach-relation .
Definition Prandtl-Meyer function
ν ( M ) — the "turning bank account"
Think of ν ( M ) as a running total of how far the flow has already turned to reach speed M , starting the clock at M = 1 where ν = 0 .
ν ( M ) = γ − 1 γ + 1 arctan ( γ + 1 γ − 1 ( M 2 − 1 ) ) − arctan ( M 2 − 1 )
Rule of use: to turn flow from M 1 to M 2 costs a turning angle θ = ν ( M 2 ) − ν ( M 1 ) . That is the ONLY equation we ever apply it with.
γ (gamma) is the heat-capacity ratio of the gas: air ≈ 1.4 , hot rocket exhaust ≈ 1.2 –1.3 . It sets how "springy" the gas is.
Every under-expanded problem is one (or a blend) of these cells. Each example below is tagged with the cell it fills.
Cell
What makes it special
Example
A. Baseline
r > 1 , ordinary supersonic exit
Ex 1
B. Degenerate r = 1
pressure tie — the "zero turn" boundary
Ex 2
C. Wrong-sign trap
student is given r < 1 — must reject the P-M method
Ex 3
D. Small mismatch limit
r → 1 + , tiny angle, thrust loss → 0
Ex 4
E. Large mismatch limit
high altitude, big r , big turn
Ex 5
F. Thrust-force accounting
uses F = m ˙ v e + A e ( p e − p ∞ )
Ex 6
G. Real-world word problem
rocket climbs, p ∞ falls with altitude
Ex 7
H. Exam twist
different γ , asks for the loss factor 1 − cos θ
Ex 8
Worked example Example 1 — Cell A: the baseline under-expanded jet
Given: M e = 3.5 , p e = 1.5 atm, p ∞ = 1.0 atm, γ = 1.3 .
Find: M plume and the turning angle θ turn .
Forecast: Guess — will M plume be bigger or smaller than 3.5 ? Will θ be a few degrees or tens of degrees?
Confirm the regime. r = 1.5/1 = 1.5 > 1 → under-expanded.
Why this step? The whole method only applies when the gas is still over-pressured; check first.
Plume Mach. Exponent γ / ( γ − 1 ) = 1.3/0.3 = 4.333 ; and 2 γ − 1 = 0.15 .
Denominator bracket = 1 + 0.15 ( 3. 5 2 ) = 1 + 0.15 ( 12.25 ) = 2.8375 .
1.5 = ( 2.8375 1 + 0.15 M plume 2 ) 4.333
So 1 + 0.15 M plume 2 = 2.8375 ⋅ 1. 5 1/4.333 = 2.8375 ( 1.0964 ) = 3.111 .
Thus M plume 2 = ( 3.111 − 1 ) /0.15 = 14.07 , giving M plume ≈ 3.75 .
Why this step? Pressure falling to p ∞ forces the flow faster — the isentropic relation is the only bridge from a pressure ratio to a Mach number.
Turning angle with ( γ + 1 ) / ( γ − 1 ) = 2.3/0.3 = 2.769 :
ν ( 3.5 ) = 2.769 arctan ( 2.769 1 11.25 ) − arctan 11.25 = 66.3°
ν ( 3.75 ) = 2.769 arctan ( 2.769 1 13.06 ) − arctan 13.06 = 71.0°
θ turn = ν ( 3.75 ) − ν ( 3.5 ) = 71.0° − 66.3° = 4.7°
Why this step? The turning bank account: cost of going from M e to M plume is the difference of the two totals.
Verify: M plume > M e ✓ (faster, as pressure dropped). θ ≈ 4.7° is a "few degrees" — matches the parent's 3 –5° estimate for r = 1.5 . Look at the fan geometry below.
The red waves are the centered expansion fan; the violet arrow is the exit flow, the orange arrow the deflected plume — the small angle between them is your θ turn .
Worked example Example 2 — Cell B: the degenerate tie
p e = p ∞
Given: M e = 3.5 , p e = 1.0 atm, p ∞ = 1.0 atm, γ = 1.3 .
Find: M plume and θ turn .
Forecast: With no pressure gap, does the gas turn at all?
Regime. r = 1.0 exactly → perfectly expanded, the boundary of our topic.
Plume Mach. The right side must equal 1 , so numerator bracket = denominator bracket, i.e. M plume = M e = 3.5 .
Why this step? No pressure to shed means no further expansion.
Turn. θ turn = ν ( 3.5 ) − ν ( 3.5 ) = 0° .
Why this step? Same Mach in the bank account both sides → zero withdrawal.
Verify: θ = 0 and M plume = M e — the flow leaves perfectly straight, maximum axial thrust, zero loss. This is the limit every real design chases (3.3.13-Optimal-expansion-ratio ).
Worked example Example 3 — Cell C: the wrong-sign trap
Given: M e = 3.5 , p e = 0.7 atm, p ∞ = 1.0 atm, γ = 1.3 . A student blindly applies Prandtl-Meyer.
Find: What is actually happening, and why the P-M method is illegal here.
Forecast: Is this even an under-expanded nozzle?
Regime. r = 0.7 < 1 → p e < p ∞ → over-expanded , not under-expanded.
Why this step? The sign of r − 1 decides which physics runs. Here ambient wins.
Why P-M fails. Expansion fans drop pressure. Here the gas must raise its pressure to reach p ∞ . Pressure-raising in supersonic flow happens through oblique shocks , not expansion fans — see 4.1.3-Oblique-shock-theory and 3.3.14-Over-expanded-nozzle-shock-diamonds .
The plume Mach direction. If you did force the isentropic formula: 1 + 0.15 M plume 2 = 2.8375 ⋅ 0. 7 1/4.333 = 2.8375 ( 0.9192 ) = 2.608 , giving M plume 2 = ( 2.608 − 1 ) /0.15 = 10.72 , M plume ≈ 3.27 < M e .
Why this step? A Mach that dropped is the mathematical fingerprint of compression — the formula is quietly telling you a shock, not a fan, is needed.
Verify: M plume = 3.27 < 3.5 ✓ — deceleration = compression = shock regime. Do not use ν ( M ) for turning angle here. Correct tool: oblique shock relations.
Common mistake The classic sign slip
Seeing a pressure mismatch and reaching for Prandtl-Meyer regardless of direction . Always compute r = p e / p ∞ first: r > 1 → fan (this page); r < 1 → shock (the over-expanded page).
Worked example Example 4 — Cell D: the vanishing-mismatch limit
Given: M e = 3.5 , p e = 1.02 atm, p ∞ = 1.0 atm, γ = 1.3 .
Find: θ turn and confirm the thrust loss → 0 .
Forecast: As r → 1 + , does θ shrink smoothly to zero?
Plume Mach. 1 + 0.15 M plume 2 = 2.8375 ⋅ 1.0 2 1/4.333 = 2.8375 ( 1.00458 ) = 2.8505 .
M plume 2 = ( 2.8505 − 1 ) /0.15 = 12.337 , M plume ≈ 3.513 .
Why this step? Tiny pressure drop → tiny Mach rise.
Turn. ν ( 3.513 ) − ν ( 3.5 ) . Since the change is small, θ ≈ 0.24° .
Why this step? Nearly-equal bank balances → nearly-zero withdrawal.
Loss factor. 1 − cos ( 0.24° ) = 1 − 0.9999912 ≈ 8.8 × 1 0 − 6 → about 0.0009% .
Why this step? Thrust loss scales with ( 1 − cos θ ) , which is ∼ θ 2 /2 for small θ — it dies quadratically .
Verify: θ → 0 and loss → 0 as r → 1 ✓ — continuously matching Example 2's exact zero. The physics has no jump at the boundary.
Worked example Example 5 — Cell E: the big-mismatch (high-altitude) limit
Given: M e = 3.5 , p e = 1.0 atm, p ∞ = 0.1 atm (high up), γ = 1.3 . So r = 10 .
Find: M plume and θ turn .
Forecast: Big pressure ratio — will the turn be large (tens of degrees)?
Plume Mach. 1 + 0.15 M plume 2 = 2.8375 ⋅ 1 0 1/4.333 = 2.8375 ( 1.6885 ) = 4.7912 .
M plume 2 = ( 4.7912 − 1 ) /0.15 = 25.27 , M plume ≈ 5.03 .
Why this step? A tenfold pressure drop demands a much faster plume.
Turn. ν ( 5.03 ) ≈ 88.9° , ν ( 3.5 ) = 66.3° , so θ = 88.9 − 66.3 ≈ 22.6° .
Why this step? Larger M plume → far bigger withdrawal from the bank account.
Loss factor. 1 − cos ( 22.6° ) = 1 − 0.9232 = 0.0768 → up to ∼ 7.7% of the extra expansion momentum thrown sideways.
Why this step? Now θ is large; the small-angle shortcut is invalid, so use full cosine.
Verify: θ jumped from 4.7° (Ex 1) to 22.6° as r went 1.5 → 10 ✓ — bigger mismatch, bigger loss, exactly the trend the parent warns of. This is why altitude-compensation nozzles exist (3.3.16-Altitude-compensation-nozzles ).
Worked example Example 6 — Cell F: full thrust-force accounting
Given: m ˙ = 200 kg/s, v e = 2800 m/s, A e = 0.5 m 2 , p e = 1.5 × 1 0 5 Pa, p ∞ = 1.0 × 1 0 5 Pa.
Find: Thrust F , and the split between momentum and pressure terms.
Forecast: Does the over-pressure add to or subtract from thrust here?
Momentum term. m ˙ v e = 200 × 2800 = 560 , 000 N.
Why this step? Bulk of thrust is momentum flux leaving the nozzle.
Pressure term. A e ( p e − p ∞ ) = 0.5 × ( 1.5 × 1 0 5 − 1.0 × 1 0 5 ) = 0.5 × 5 × 1 0 4 = 25 , 000 N.
Why this step? Under-expanded means p e > p ∞ , so this term is positive — the over-pressure pushes forward on the exit plane.
Total. F = 560 , 000 + 25 , 000 = 585 , 000 N = 585 kN.
Why this step? Momentum theorem: sum the two contributions.
Verify: Units: [ m ˙ v e ] = s kg ⋅ s m = s 2 kg⋅m = N ✓; [ A e p ] = m 2 ⋅ Pa = m 2 ⋅ m 2 N = N ✓. Pressure term is positive ✓ (correct sign for under-expansion). Note: the gain 25 kN is real but is not free lunch — v e here is smaller than a perfectly-expanded nozzle would deliver. See 2.5.12-Thrust-coefficient-definition .
Worked example Example 7 — Cell G: a climbing rocket (word problem)
Given: A rocket keeps p e = 0.8 atm fixed (fixed nozzle, fixed chamber). At launch p ∞ = 1.0 atm; at 11 km altitude p ∞ = 0.22 atm. Exit M e = 4 , γ = 1.2 .
Find: At which altitude is the nozzle under-expanded, and roughly how the turn changes.
Forecast: A fixed nozzle can't be perfect everywhere — where does it flip from over- to under-expanded?
Launch. r = 0.8/1.0 = 0.8 < 1 → over-expanded (shocks, Ex 3 regime). Not our page's job here.
Why this step? At sea level ambient is strong; classify by r .
Altitude. r = 0.8/0.22 = 3.64 > 1 → under-expanded (fan forms).
Why this step? As the rocket climbs, p ∞ collapses; eventually the exhaust over-powers it.
Crossover. Perfect expansion happens when p ∞ = p e = 0.8 atm. Using the barometric-style drop, that is somewhere below 11 km. Above it, plume opens up: with γ = 1.2 , 2 γ − 1 = 0.1 , exponent = 6 , ( γ + 1 ) / ( γ − 1 ) = 11 = 3.317 .
Denominator bracket = 1 + 0.1 ( 16 ) = 2.6 . 1 + 0.1 M plume 2 = 2.6 ⋅ 3.6 4 1/6 = 2.6 ( 1.2405 ) = 3.225 , M plume 2 = 22.25 , M plume ≈ 4.72 .
Why this step? Track the same isentropic bridge with the new γ and r .
Verify: Regime flips from over- (r < 1 ) to under-expanded (r > 1 ) as it climbs ✓ — exactly why altitude-compensating designs are pursued (3.3.16-Altitude-compensation-nozzles ). M plume = 4.72 > 4 ✓ (faster aloft).
Worked example Example 8 — Cell H: exam twist, the loss factor with air-like
γ
Given: M e = 2.5 , p e / p ∞ = 2.0 , γ = 1.4 . Find θ turn and the loss factor 1 − cos θ turn .
Forecast: With springier gas (γ = 1.4 ) does the same r give a bigger or smaller turn than the γ = 1.3 cases?
Constants. 2 γ − 1 = 0.2 , exponent = 1.4/0.4 = 3.5 , ( γ + 1 ) / ( γ − 1 ) = 2.4/0.4 = 6 = 2.449 .
Plume Mach. Denominator bracket = 1 + 0.2 ( 6.25 ) = 2.25 . 1 + 0.2 M plume 2 = 2.25 ⋅ 2 1/3.5 = 2.25 ( 1.2190 ) = 2.7428 , M plume 2 = 8.714 , M plume ≈ 2.952 .
Why this step? Same isentropic bridge, air's γ .
Turn. ν ( 2.5 ) = 2.449 arctan ( 2.449 1 5.25 ) − arctan 5.25 = 39.12° .
ν ( 2.952 ) = 2.449 arctan ( 2.449 1 7.714 ) − arctan 7.714 = 48.78° .
θ turn = 48.78 − 39.12 = 9.66° .
Loss factor. 1 − cos ( 9.66° ) = 1 − 0.98583 = 0.01417 → about 1.4% .
Why this step? The exam wants the fraction of extra momentum lost sideways , not just the angle.
Verify: M plume = 2.95 > 2.5 ✓; loss ≈ 1.4% is modest for r = 2 ✓, consistent with "few-percent" losses at moderate mismatch. Springier air turns a bit more per unit pressure drop than the γ = 1.3 exhaust — a subtle but examinable point.
Recall Quick self-test
Which regime is p e / p ∞ = 1.0 ? ::: Perfectly expanded — zero turn, zero loss (boundary case).
Which tool for p e < p ∞ ? ::: Oblique shocks, NOT Prandtl-Meyer.
Turning angle formula in one line? ::: θ turn = ν ( M plume ) − ν ( M e ) .
Thrust loss scales like? ::: ( 1 − cos θ turn ) ≈ θ 2 /2 for small θ .
Sign of the pressure thrust term when under-expanded? ::: Positive, A e ( p e − p ∞ ) > 0 .
Mnemonic "UP-FAN, DOWN-SHOCK"
Exit pressure UP vs ambient → expansion FAN (under-expanded). Exit pressure DOWN → SHOCK (over-expanded).