Pressure Ratio Across Expansion Fan Formula:
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The Pressure Ratio Across Expansion Fan is the ratio of downstream and upstream pressure across an expansion fan in supersonic flow. It quantifies the pressure change that occurs when a supersonic flow expands around a corner or through a diverging section.
The calculator uses the expansion fan pressure ratio formula:
Where:
Explanation: The equation relates the pressure change across an expansion fan to the specific heat ratio and Mach numbers before and after the expansion.
Details: Calculating pressure ratio across expansion fans is crucial for analyzing supersonic flow behavior, designing high-speed aerodynamic systems, and understanding shock-expansion theory in compressible flow dynamics.
Tips: Enter specific heat ratio (typically 1.4 for air), Mach number ahead of expansion fan, and Mach number behind expansion fan. All values must be valid (γe > 1, Me1 > 0, Me2 > 0).
Q1: What is an expansion fan in supersonic flow?
A: An expansion fan is a region of continuous expansion that occurs when a supersonic flow turns away from itself, typically around a convex corner.
Q2: What are typical values for specific heat ratio?
A: For air at standard conditions, γ = 1.4. For other gases: monatomic gases ≈ 1.67, diatomic gases ≈ 1.4, polyatomic gases ≈ 1.1-1.3.
Q3: How does Mach number affect pressure ratio?
A: Higher Mach numbers generally result in lower pressure ratios across expansion fans, indicating greater pressure drop during expansion.
Q4: What are the limitations of this formula?
A: This formula assumes isentropic flow, perfect gas behavior, and two-dimensional flow. It may not be accurate for very high Mach numbers or complex flow geometries.
Q5: How is this related to Prandtl-Meyer expansion?
A: This pressure ratio formula is derived from Prandtl-Meyer expansion theory, which describes the turning of supersonic flow through an expansion fan.