Lesson 5 of 11

Combustion Performance

When does a combustor stop working? Deriving the stability loop from the Damköhler number, why altitude relight is a race against heat loss, and the loading parameter θ that sizes every combustor.

7 min3 live simulations
you are here
The question

Every combustor has a hidden map of where it lives and where it dies. Can we draw that map from first principles, using only the ideas we already have?

We can, and it takes exactly one ratio.

Lefebvre frames performance as three questions a designer must answer at every point in the flight envelope:

  1. Is the fuel's energy actually released? (efficiency)
  2. Will the flame stay lit? (stability)
  3. If it goes out, can we light it again? (ignition and relight)

All three turn out to be the same contest, between how long the gas stays and how long the chemistry takes.

One ratio to rule them: the Damköhler number

Gas spends a finite time in the primary zone, the residence time τflow∼L/U\cair{\tau_\text{flow}} \sim L/\cair{U}. The chemistry needs its own time to complete, τchem\cflame{\tau_\text{chem}}, and from Lesson 2 we know that time depends exponentially on temperature. Their ratio is the Damköhler numberDa = τ_flow / τ_chem, residence time over chemical time. Above 1 the flame survives; below 1 it blows out.:

Da=τflowτchem\text{Da} = \frac{\cair{\tau_\text{flow}}}{\cflame{\tau_\text{chem}}}

If Da>1\text{Da} > 1, the chemistry finishes before the gas leaves: the flame lives. If Da<1\text{Da} < 1, reacting gas is swept out before it can sustain the reactions behind it: the flame dies.

Now watch what happens when we combine this with the two ingredients from Lesson 2. The chemical time scales like e+Ea/RTad(ϕ)e^{+E_a/RT_{ad}(\phi)}, and Tad(ϕ)T_{ad}(\phi) is our bell curve. So the velocity at which the flame blows out is

Ublow-off(ϕ)  ∝  L P n exp⁡ ⁣(−EaR Tad(ϕ))U_\text{blow-off}(\phi) \;\propto\; L\, P^{\,n}\, \exp\!\left(-\frac{E_a}{R\,T_{ad}(\phi)}\right)

A bell-shaped temperature, pushed through an exponential, gives a sharply peaked curve. Plot the boundary Da=1\text{Da} = 1 in the plane of velocity and mixture and you get this:

DeriveThe stability loop is just Damköhler = 1
0204060800.511.522.53air velocity through the primary zone (m/s)equivalence ratio φSTABLEblow-off velocity 35 m/slean blowout ↑rich blowout ↓Da = 2.78
1.00 atm
Low pressure = high altitude
300 K
1.00×
Bigger volume → longer residence time
Damköhler number2.78τ_flow / τ_chem
Lean-blowout mixture0.77at 12 m/s
Margin23%fuel you can remove before blowout
Comfortably inside the loop: chemistry finishes with time to spare.
Challenges0/3
  • Blow the flame out with a throttle chop.
  • Find the fastest flow that can still burn at 1 atm and 300 K (the tip of the loop).
  • Keep a flame alive at 0.3 atm with the flow at 10 m/s or faster. What must you change?
For every mixture φ, the flame survives while the gas stays long enough for chemistry to finish: τ_flow > τ_chem. Because chemistry speed follows the bell-shaped flame temperature through Arrhenius, the Da = 1 boundary traces Lefebvre's famous 'peaked hat'. Drag the operating point.

This is Lefebvre's stability loop, the "peaked hat", and you just derived it. Everything inside is stable. The lower edge is Lean blowoutFlame-out caused by too little fuel: the chemistry slows until it can no longer keep up with the flow., the upper edge rich blowout, and the tip is the maximum velocity at which the combustor can burn at all, found slightly rich of stoichiometric where the flame is hottest.

Now use the sliders to see why designers care about each variable:

  • Pressure enlarges the loop (faster chemistry). That makes high altitude, where pressure is low, the dangerous corner of the envelope.
  • Inlet temperature lifts TadT_{ad} and enlarges the loop, so a cold ground start is harder than a hot one.
  • Combustor volume raises the residence time and the whole boundary moves out. Stability is bought with size and weight.

Modern lean-burn combustors deliberately live with smaller lean-blowout margins than older designs, and manage the risk with pilot flames (a small, richer, very stable zone that keeps the main zone lit), fuel staging schedules, and fast control logic.

Combustion efficiency

Combustion efficiency is the fraction of the fuel's chemical energy actually released:

ηc=ΔTactualΔTideal≈1−m˙CO HCO+m˙UHC HUHCm˙f Hf\eta_c = \frac{\Delta T_\text{actual}}{\Delta T_\text{ideal}} \approx 1 - \frac{\dot m_\text{CO}\, H_\text{CO} + \dot m_\text{UHC}\, H_\text{UHC}}{\dot m_f\, H_f}

At take-off, ηc>99.9%\eta_c > 99.9\%. At idle it can fall to 97–99%. That sounds small, but it is almost entirely CO and unburned hydrocarbons, precisely the pollutants regulated around airports.

Why does efficiency fall at low power? Pressure and inlet temperature drop (chemistry slows), the fuel spray coarsens (Lesson 6) and the combustor is suddenly too small for the job. Lefebvre condensed all of that into one Loading parameter θLefebvre’s P^1.75·A·D^0.75·e^(T₃/300)/ṁ: bundles pressure, temperature, size and airflow into one predictor of efficiency.:

θ=P31.75 Aref Dref0.75 exp⁡(T3/300)m˙A\theta = \frac{P_3^{1.75}\, A_\text{ref}\, D_\text{ref}^{0.75}\, \exp(T_3/300)}{\dot m_A}

Pressure (to a high power), temperature (exponentially) and size in the numerator; air flow in the denominator. Large θ\theta is a lightly loaded, efficient combustor. Remarkably, data from very different combustors collapse onto one S-shaped curve of efficiency against θ\theta:

ExploreIs the combustor big enough? The θ parameter
10⁻⁴10⁻³10⁻²10⁻¹10⁰10¹0%25%50%75%100%θ relative to the take-off design point (log)combustion efficiencyTake-offCruiseGround idleWindmill relight
20.0 bar
800 K
100% of take-off
1.00×
Relative loading1.00θ / θ at take-off
Combustion efficiency99.97%
Challenges0/2
  • Get ground idle (4 bar, 460 K, 25% air) above 99% efficiency. What had to grow?
  • Find a combination that drops efficiency below 50%.
Lefebvre's loading parameter θ = P¹·⁷⁵ A D⁰·⁷⁵ e^(T₃/300) / ṁ bundles pressure, temperature, size and airflow into one number. Every combustor falls on roughly one S-shaped efficiency curve against it.

Try the presets. Take-off sits comfortably on the plateau. Cruise does too. Idle begins to slip down the shoulder, and a windmilling relight at altitude is far down the slope. This is the sizing equation: if the engine's air flow doubles and the combustor doesn't grow, θ\theta halves.

Check your intuition
An engine derivative pushes 15% more air through an unchanged combustor at the same pressure and temperature. What happens to θ and to low-power efficiency?

Ignition: a race against heat loss

Starting a combustor happens in three acts:

  1. Kernel formation: a spark creates a small ball of very hot gas in a combustible pocket of mixture.
  2. Kernel growth: the ball must grow. It releases heat in proportion to its volume and loses heat to the cold surroundings through its surface. Small kernels lose; big kernels win. So there is a critical size, roughly the quenching distance, below which the kernel dies.
  3. Propagation: the flame spreads through the primary zone and around the annulus (remember the light-around in Lesson 1).

Now go to altitude. The air is thinner and colder, the fuel is colder and more viscous, and the spray is coarser. Every one of these effects works against you twice: the spark's energy makes a smaller kernel, and the critical size gets bigger. The minimum ignition energy climbs roughly as P−2P^{-2}.

Estimate first
At 11 km the air pressure is about 22% of sea level. If minimum ignition energy scales as P⁻², how many times more spark energy does relight need up there?
1101001,000
Drag along the line to place your guess — each tick is ten times the last.
SimulateRelight at 35,000 feet
0.0 km · 0 ft
288 K · 1.00 atm
2.0 J
Typical high-energy igniters: 2–20 J
Kernel ÷ critical size3.43
Energy needed here0.05 Jminimum ignition energy ∝ roughly P⁻²
Predict first: will a 2.0 J spark light the combustor at 0.0 km? Then fire.
Challenges0/2
  • Relight the engine at 10 km (33,000 ft) or higher.
  • Find an altitude where even a 19 J spark fizzles.
A spark makes a small ball of hot gas. It survives only if it is bigger than a critical size — below it, heat leaks out faster than chemistry makes it. Thin, cold air shrinks the kernel and enlarges the critical size at the same time.

The result is a finite relight envelope: a region of altitude and flight speed inside which the engine must demonstrate reliable relight for certification. It is one of the most demanding requirements a combustor faces, and it often fights with emissions. A primary zone tuned lean for low NOₓ at cruise is exactly the wrong primary zone for lighting at 30,000 ft.

Check your intuition
An engine struggles to relight at altitude. Which change would help the most, based on this lesson?
Recap
What to carry forward
  • The Damköhler number Da=τflow/τchem\text{Da} = \tau_\text{flow}/\tau_\text{chem} decides survival: > 1 lit, < 1 blown out.
  • Combine Da with the bell-shaped Tad(ϕ)T_{ad}(\phi) and Arrhenius and you get the stability loop, with lean blowout as its operationally critical edge.
  • Pressure, inlet temperature and volume enlarge the loop; throttle chops and lean low-NOₓ operation push toward its edge.
  • Efficiency collapses onto one curve of the loading parameter θ, which is also the combustor's sizing rule.
  • Ignition is a race between kernel growth and heat loss; altitude attacks both, bounding the relight envelope.

All of this assumed the fuel was already vapour, mixed with air. In reality it arrives as a liquid, and turning it into a fine mist is the next problem.

Finished this lesson?Mark it complete to track your progress through the course (saved in this browser).
Up next · Lesson 6Fuel InjectionHow do you turn a liquid into vapour in a millisecond?Keep going →