Density Behind Oblique Shock Formula:
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The density behind oblique shock formula calculates the air or fluid density after passing through an oblique shock wave. This is a fundamental equation in compressible flow and aerodynamics that describes how density changes across an oblique shock wave.
The calculator uses the density behind oblique shock formula:
Where:
Explanation: The formula calculates the density ratio across an oblique shock wave based on the normal component of the upstream Mach number and the specific heat ratio of the fluid.
Details: Calculating density behind oblique shocks is crucial for analyzing compressible flows, designing supersonic aircraft components, understanding shock wave behavior, and predicting aerodynamic performance in high-speed applications.
Tips: Enter density ahead of shock in kg/m³, specific heat ratio (typically 1.4 for air), and upstream Mach normal to oblique shock. All values must be positive with specific heat ratio ≥ 1.
Q1: What is an oblique shock wave?
A: An oblique shock wave is a shock wave that forms at an angle to the flow direction, typically occurring when supersonic flow encounters a compression corner or obstacle.
Q2: How does this differ from normal shock density calculation?
A: The formula is similar to normal shock density calculation but uses the normal component of the Mach number relative to the shock wave rather than the full Mach number.
Q3: 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, triatomic gases = 1.33.
Q4: When is this formula applicable?
A: This formula applies to perfect gases experiencing oblique shock waves where the flow is steady, adiabatic, and without external forces.
Q5: What are the limitations of this calculation?
A: The formula assumes ideal gas behavior, constant specific heats, and that the shock wave is thin and straight. It may not be accurate for very strong shocks or non-ideal gases.