3.1.7 · Physics › Compressible Flow & Aerodynamics
Intuition Badi picture (YE ratios exist KYU?)
Jab gas smoothly flow karti hai (koi shock nahi, friction nahi, heat add nahi) aur tum imagine karo ki use reversibly rest pe lao , to tumhe uski stagnation (total) properties P 0 , T 0 , ρ 0 milti hain. Ye aise hain jaise flow ka "total energy bank account". Actual local properties P , T , ρ chhoti hoti hain kyunki us bank account ka kuch hissa motion ki kinetic energy ke roop mein "kharch" ho jaata hai. Jo cheez decide karti hai ki kitna kharch hua, woh sirf Mach number M = V / a hai. Isliye har property ratio ek single clean function of M ban jaata hai — yehi wajah hai ki hum unhe ek baar tabulate karte hain aur hamesha reuse karte hain.
Definition Stagnation (total) properties
Stagnation state woh state hai jo fluid tab reach karta agar use adiabatically aur reversibly (isentropically) zero velocity tak decelerate kiya jaata. T 0 = stagnation temperature, P 0 = stagnation pressure, ρ 0 = stagnation density. Ye ek isentropic flow mein constant rehte hain .
KYA chahiye: teen ratios T 0 T , P 0 P , ρ 0 ρ purely M aur γ ke terms mein.
Steady adiabatic energy equation (per unit mass) ek perfect gas ke liye:
h + 2 1 V 2 = h 0 = const
Ye step kyu? Koi heat nahi, koi work nahi ⇒ stagnation enthalpy h 0 conserved hai. Stagnation point par V = 0 isliye h 0 wahan ki enthalpy hai.
Ek perfect gas ke liye h = c p T :
c p T + 2 1 V 2 = c p T 0
c p T se divide karo:
T T 0 = 1 + 2 c p T V 2
Ab V 2 / ( c p T ) ko M ke terms mein express karna hai. In do facts ka use karo:
Speed of sound: a 2 = γ R T ⇒ V 2 = M 2 a 2 = M 2 γ R T .
c p = γ − 1 γ R (c p − c v = R aur γ = c p / c v se).
Ye step kyu? Ye velocity ko Mach number mein convert karta hai, jo ki humara ek maatra variable hai.
2 c p T V 2 = 2 ⋅ γ − 1 γ R T M 2 γ R T = 2 γ − 1 M 2
Ek perfect gas ke isentropic process ke liye:
P P 0 = ( T T 0 ) γ − 1 γ , ρ ρ 0 = ( T T 0 ) γ − 1 1
Ye step kyu? P v γ = const aur P v = R T se, v eliminate karne par P ∝ T γ / ( γ − 1 ) aur ρ ∝ T 1/ ( γ − 1 ) milta hai. Flow isentropic hai, isliye ye stagnation aur local states ko link karte hain.
T 0 / T result substitute karne par:
Consistency check (Feynman test): divide karne par ρ 0 / ρ P 0 / P = ( 1 + 2 γ − 1 M 2 ) 1 = T T 0 milta hai, jo exact ideal-gas law P / ρ ∝ T hai. ✓
Table bas in teen formulas ko γ = 1.4 (air) ke liye bahut saare M values par evaluate karna hai. Key memory anchors:
M
T / T 0
P / P 0
ρ / ρ 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
P 0 P < ρ 0 ρ < T 0 T hamesha (jab M > 0 ). KYU? Pressure ka exponent sabse bada hai γ − 1 γ = 3.5 , isliye woh sabse tezi se girta hai; temperature ka exponent 1 hai, sabse dheere girta hai.
Worked example Example 1 — Air at
M = 2 , T 0 = 300 K, P 0 = 500 kPa (γ = 1.4 )
2 γ − 1 M 2 = 0.2 × 4 = 0.8 , to base factor = 1.8 .
T = 300/1.8 = 166.7 K. Kyu? T 0 / T = 1.8 .
P = 500/1. 8 3.5 = 500/7.824 = 63.9 kPa. Kyu? exponent γ / ( γ − 1 ) = 3.5 .
ρ / ρ 0 = 1. 8 − 2.5 = 0.2301 . Kyu? exponent 1/ ( γ − 1 ) = 2.5 .
Worked example Example 3 — Inverse problem: given
P / P 0 = 0.3 , M find karo.
( 1 + 0.2 M 2 ) 3.5 = 1/0.3 = 3.333
1 + 0.2 M 2 = 3.33 3 1/3.5 = 1.4036
M 2 = 0.4036/0.2 = 2.018 ⇒ M = 1.42 . Kyu? Hum wahi formula invert karte hain — tables bas is lookup ko precomputed rakhti hain.
T / T 0 = ( 1 + 2 γ − 1 M 2 ) " (bhool gaye ki ye reciprocal hai)
Kyu sahi lagta hai: formula 1 + 2 γ − 1 M 2 itna memorable hai ki tum ise directly T / T 0 par laga dete ho. Fix: clean factor T 0 / T ke barabar hai (≥1). Local T stagnation T se chhoti hoti hai, isliye T / T 0 ≤ 1 — reciprocal lo.
P , ρ , T ke liye same exponent use karna.
Kyu sahi lagta hai: ye sab same base factor se aate hain. Fix: exponents alag hain — T :1, ρ :γ − 1 1 = 2.5 , P :γ − 1 γ = 3.5 (air ke liye). Inhe mix karna #1 numerical error hai.
shock ke across apply karna.
Kyu sahi lagta hai: ye "gas tables" hain. Fix: inhe isentropic flow chahiye. Shock ke across entropy jump karti hai, isliye P 0 girta hai; inhe sirf shock-free points ke beech use karo (ya dono sides par alag P 0 ke saath).
Recall Feynman: ek 12-saal ke bache ko samjhao
Socho tum balloon lekar daud rahe ho. Agar tum apne aage ki hawa ko achanak rokdo, woh pile up hoti hai — thodi si geeli, thodi si squishier, aur zyada push karti hai. Jitna tezi daudoge (bada Mach number), utna zyada pile up hoga jab ruka jaye. "Ruke hue" values T 0 , P 0 , ρ 0 hain. Flowing values hamesha chhoti hoti hain, aur kitni chhoti hain ye sirf tumhari speed aur speed of sound ke comparison par depend karta hai.
T-R-P = 1, 2.5, 3.5 "
Base factor ( 1 + 2 γ − 1 M 2 ) par T emperature, R ho (density), P ressure ke exponents air ke liye 1, 2.5, 3.5 hain. Alphabetical-ish T<R<P ke saath badhta exponent ⇒ pressure sabse tezi se girta hai.
Stagnation state define karne wali conditions kya hain? Flow ko zero velocity tak isentropically decelerate karo (adiabatic + reversible).
T 0 / T ka formula M ke terms mein?T 0 / T = 1 + 2 γ − 1 M 2 .
P 0 / P ka formula?( 1 + 2 γ − 1 M 2 ) γ / ( γ − 1 ) .
ρ 0 / ρ ka formula?( 1 + 2 γ − 1 M 2 ) 1/ ( γ − 1 ) .
T, ρ, P ke exponents (air, γ=1.4)? 1, 2.5, 3.5.
T 0 ek adiabatic flow mein friction ke saath bhi constant kyu rehta hai?Stagnation enthalpy conserved hoti hai (energy eq.); lekin agar irreversible hai to P 0 girta hai.
Air ke liye critical pressure ratio P ∗ / P 0 ? 1. 2 − 3.5 ≈ 0.528 .
Kaun sa ratio M ke saath sabse tezi se girta hai aur kyu? Pressure, kyunki iska exponent γ / ( γ − 1 ) = 3.5 sabse bada hai.
Kya tum ye tables ek normal shock ke across use kar sakte ho? Nahi — entropy badhti hai, P 0 conserved nahi hota; dono sides ko alag treat karo.
Diya hai P / P 0 = 0.3 , air ke liye M? Solve karo ( 1 + 0.2 M 2 ) 3.5 = 1/0.3 ⇒ M ≈ 1.42 .
Adiabatic energy eq h + half V2 = h0
Stagnation state V=0 isentropic
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