Prandtl Meyer Expansion Calculator

Calculate supersonic flow properties after expansion waves using Prandtl-Meyer theory

Expansion Wave Calculations

Typical values: Air γ = 1.4, Diatomic gas γ = 1.4

Must be supersonic (M₁ > 1)

Surface turning angle (positive for expansion)

Upstream Flow Properties

Expansion Wave Results

Mach Numbers and Angles

1.0000
M₂ (downstream)
90.00°
μ₁ (upstream)
90.00°
μ₂ (downstream)
0.00°
Flow deflection

Prandtl-Meyer Functions

0.00°
ν₁ (upstream)
0.00°
ν₂ (downstream)

Prandtl-Meyer function: ν(M) = √((γ+1)/(γ-1)) × arctan(√((γ-1)(M²-1)/(γ+1))) - arctan(√(M²-1))

Expansion relation: ν₂ = ν₁ + θ

Flow type: Isentropic expansion through Prandtl-Meyer fan

Validation

⚠️ Upstream Mach number must be supersonic (M₁ > 1) for expansion wave analysis.

Example Calculation

Supersonic Flow Expansion

Initial conditions:

• Upstream Mach number: M₁ = 1.5

• Deflection angle: θ = 15°

• Specific heat ratio: γ = 1.4

• Pressure: P₁ = 1 atm

• Temperature: T₁ = 288 K

Solution Steps

1. Calculate ν₁ = 11.91° (upstream Prandtl-Meyer function)

2. Calculate ν₂ = ν₁ + θ = 11.91° + 15° = 26.91°

3. Solve for M₂ using inverse Prandtl-Meyer function: M₂ = 2.0

4. Calculate flow properties using isentropic relations

Result: M₂ = 2.0, P₂ = 0.469 atm, T₂ = 230 K

Key Concepts

📐

Expansion waves form when supersonic flow turns away from itself

🌊

Prandtl-Meyer fan consists of infinite Mach lines

Flow accelerates and pressure decreases through expansion

🔄

Process is isentropic (entropy constant)

📊

Total temperature and pressure remain constant

Typical Values

Air (γ)1.4
Helium (γ)1.67
Steam (γ)1.3
CO₂ (γ)1.28
Max θ (γ=1.4)130.45°

Understanding Prandtl-Meyer Expansion Theory

What are Expansion Waves?

Expansion waves occur when a supersonic flow encounters a surface that turns away from the flow direction. Unlike shock waves, expansion waves are continuous and isentropic, meaning the entropy remains constant throughout the process.

Key Characteristics

  • Flow accelerates (Mach number increases)
  • Pressure and temperature decrease
  • Density decreases
  • Total properties remain constant

Prandtl-Meyer Function

ν(M) = √((γ+1)/(γ-1)) × arctan(√((γ-1)(M²-1)/(γ+1))) - arctan(√(M²-1))

ν₂ = ν₁ + θ

  • ν(M): Prandtl-Meyer function (radians or degrees)
  • M: Mach number
  • γ: Specific heat ratio
  • θ: Deflection angle

Note: The Prandtl-Meyer function is only valid for supersonic flows (M > 1). The maximum deflection angle depends on the specific heat ratio.