3.1.7Compressible Flow & Aerodynamics

Isentropic flow tables — P - P₀, T - T₀, ρ - ρ₀ as functions of M

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What is a stagnation state?

WHAT we want: the three ratios TT0, PP0, ρρ0\dfrac{T}{T_0},\ \dfrac{P}{P_0},\ \dfrac{\rho}{\rho_0} purely in terms of MM and γ\gamma.


Derivation from first principles

Step 1 — Energy equation gives T/T0T/T_0

The steady adiabatic energy equation (per unit mass) for a perfect gas:

h+12V2=h0=consth + \tfrac12 V^2 = h_0 = \text{const}

Why this step? No heat, no work ⇒ stagnation enthalpy h0h_0 is conserved. At the stagnation point V=0V=0 so h0h_0 is the enthalpy there.

For a perfect gas h=cpTh=c_p T:

cpT+12V2=cpT0c_p T + \tfrac12 V^2 = c_p T_0

Divide by cpTc_p T:

T0T=1+V22cpT\frac{T_0}{T} = 1 + \frac{V^2}{2 c_p T}

Now we need V2/(cpT)V^2/(c_p T) in terms of MM. Use these two facts:

  • Speed of sound: a2=γRTV2=M2a2=M2γRTa^2=\gamma R T \Rightarrow V^2 = M^2 a^2 = M^2 \gamma R T.
  • cp=γRγ1c_p = \dfrac{\gamma R}{\gamma-1} (from cpcv=Rc_p-c_v=R and γ=cp/cv\gamma=c_p/c_v).

Why this step? These convert velocity into Mach number, the only variable we want.

V22cpT=M2γRT2γRγ1T=γ12M2\frac{V^2}{2c_p T}=\frac{M^2\gamma R T}{2\cdot\frac{\gamma R}{\gamma-1}\,T}=\frac{\gamma-1}{2}M^2

Step 2 — Isentropic relations give P/P0P/P_0 and ρ/ρ0\rho/\rho_0

For an isentropic process of a perfect gas:

P0P=(T0T)γγ1,ρ0ρ=(T0T)1γ1\frac{P_0}{P}=\left(\frac{T_0}{T}\right)^{\frac{\gamma}{\gamma-1}},\qquad \frac{\rho_0}{\rho}=\left(\frac{T_0}{T}\right)^{\frac{1}{\gamma-1}}

Why this step? From Pvγ=Pv^\gamma=const and Pv=RTPv=RT, eliminating vv gives PTγ/(γ1)P\propto T^{\gamma/(\gamma-1)} and ρT1/(γ1)\rho\propto T^{1/(\gamma-1)}. The flow is isentropic, so these link the stagnation and local states.

Substituting the T0/TT_0/T result:

Consistency check (Feynman test): dividing gives P0/Pρ0/ρ=(1+γ12M2)1=T0T\dfrac{P_0/P}{\rho_0/\rho}=\left(1+\frac{\gamma-1}{2}M^2\right)^{1}=\dfrac{T_0}{T}, exactly the ideal-gas law P/ρTP/\rho\propto T. ✓


Figure — Isentropic flow tables — P - P₀, T - T₀, ρ - ρ₀ as functions of M

Reading the "tables"

A table is just these three formulas evaluated for γ=1.4\gamma=1.4 (air) at many MM. Key memory anchors:

MM T/T0T/T_0 P/P0P/P_0 ρ/ρ0\rho/\rho_0
0 1.000 1.000 1.000
0.5 0.9524 0.8430 0.8852
1.0 0.8333 0.5283 0.6339
2.0 0.5556 0.1278 0.2301

Worked examples


Common mistakes


Recall Feynman: explain to a 12-year-old

Imagine running with a balloon. If you suddenly stop the air in front of you, it piles up — gets a little hotter, squishier, and pushes harder. The faster you run (bigger Mach number), the more it piles up when stopped. The "stopped" values are T0,P0,ρ0T_0,P_0,\rho_0. The flowing values are always smaller, and exactly how much smaller depends only on your speed compared to the speed of sound.


Active-recall flashcards

What conditions define a stagnation state?
Decelerate the flow to zero velocity isentropically (adiabatic + reversible).
Formula for T0/TT_0/T in terms of MM?
T0/T=1+γ12M2T_0/T = 1+\frac{\gamma-1}{2}M^2.
Formula for P0/PP_0/P?
(1+γ12M2)γ/(γ1)\left(1+\frac{\gamma-1}{2}M^2\right)^{\gamma/(\gamma-1)}.
Formula for ρ0/ρ\rho_0/\rho?
(1+γ12M2)1/(γ1)\left(1+\frac{\gamma-1}{2}M^2\right)^{1/(\gamma-1)}.
Exponents for T, ρ, P (air, γ=1.4)?
1, 2.5, 3.5.
Why is T0T_0 constant along an adiabatic flow even with friction?
Stagnation enthalpy is conserved (energy eq.); but P0P_0 drops if irreversible.
Critical pressure ratio P/P0P^*/P_0 for air?
1.23.50.5281.2^{-3.5}\approx0.528.
Which ratio falls fastest with M and why?
Pressure, because its exponent γ/(γ1)=3.5\gamma/(\gamma-1)=3.5 is largest.
Can you use these tables across a normal shock?
No — entropy rises, P0P_0 is not conserved; treat each side separately.
Given P/P0=0.3P/P_0=0.3, M for air?
Solve (1+0.2M2)3.5=1/0.3M1.42(1+0.2M^2)^{3.5}=1/0.3\Rightarrow M\approx1.42.

Connections

Concept Map

conserves h0

decelerate to rest

for perfect gas

converts V

converts V

substituted into

via isentropic link

gives

gives

divide by

divide by

verifies

Adiabatic energy eq h + half V2 = h0

Stagnation state V=0 isentropic

T0/T = 1 + k-1 /2 M2

a2 = gamma R T

cp = gamma R / gamma-1

Mach number M = V/a

Isentropic relations P v gamma const

P0/P ratio power gamma/ gamma-1

rho0/rho ratio power 1/ gamma-1

Consistency P ratio / rho ratio = T0/T

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, idea simple hai: jab gas smoothly (bina shock, bina friction) flow karti hai, toh uska ek "total energy account" hota hai jise hum stagnation properties T0,P0,ρ0T_0, P_0, \rho_0 kehte hain — yeh wahi values hain jo milengi agar gas ko reversibly rok do (V=0). Jab gas move kar rahi hoti hai, toh thodi energy kinetic form mein chali jaati hai, isliye local T,P,ρT, P, \rho hamesha stagnation se chhote hote hain. Aur kitne chhote? Yeh sirf aur sirf Mach number MM par depend karta hai.

Derivation ka core: energy equation cpT+12V2=cpT0c_pT+\frac12 V^2=c_pT_0 se T0/T=1+γ12M2T_0/T=1+\frac{\gamma-1}{2}M^2 nikalta hai. Phir isentropic relation PTγ/(γ1)P\propto T^{\gamma/(\gamma-1)} aur ρT1/(γ1)\rho\propto T^{1/(\gamma-1)} laga do, bas teeno ratios ready. Yaad rakhne ka shortcut — exponents: T ke liye 1, rho ke liye 2.5, pressure ke liye 3.5 (air, γ=1.4\gamma=1.4). Isliye pressure sabse tezi se girta hai.

Yeh "tables" koi magic nahi — bas γ=1.4\gamma=1.4 daal ke har M par yeh formulas calculate kiye hote hain. Exam mein agar value di ho (jaise P/P0=0.3P/P_0=0.3) toh ulta solve karke M nikal lo. Sabse important real-life use: nozzle choking — jab pressure 0.528P00.528\,P_0 tak gir jaye toh throat par M=1M=1 ho jaata hai.

Ek galti se bachna: yeh formulas sirf isentropic flow ke liye valid hain. Shock ke aar-paar mat lagana, kyunki entropy badhti hai aur P0P_0 gir jaata hai. Aur T/T0T/T_0 ko hamesha reciprocal ke roop mein lo — clean factor T0/TT_0/T hota hai, T/T0T/T_0 nahi.

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Connections