Formula Used:
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The continuity equation for shock waves describes the conservation of mass across a normal shock wave. It states that the mass flow rate remains constant, leading to the relationship between densities and velocities upstream and downstream of the shock.
The calculator uses the continuity equation:
Where:
Explanation: This equation is derived from the principle of mass conservation, where the product of density and velocity remains constant across the shock wave.
Details: Calculating density changes across shock waves is crucial for understanding compressible flow behavior, designing supersonic aircraft, analyzing rocket propulsion systems, and studying high-speed aerodynamic phenomena.
Tips: Enter density behind shock in kg/m³, velocity downstream in m/s, and velocity upstream in m/s. All values must be positive and non-zero for accurate calculation.
Q1: What is a normal shock wave?
A: A normal shock wave is a discontinuity in a supersonic flow where the flow becomes subsonic, characterized by sudden changes in pressure, temperature, density, and velocity perpendicular to the wave front.
Q2: Why does density change across a shock wave?
A: Density increases across a normal shock wave due to the compression effect as the flow decelerates from supersonic to subsonic velocities.
Q3: What are typical applications of this calculation?
A: This calculation is used in aerospace engineering for designing supersonic inlets, analyzing shock-boundary layer interactions, and studying high-speed flow phenomena in nozzles and diffusers.
Q4: Are there limitations to this equation?
A: This equation assumes ideal gas behavior, steady flow, and a normal shock (perpendicular to flow direction). It may not accurately represent oblique shocks or real gas effects at extreme conditions.
Q5: How does this relate to other shock wave equations?
A: The continuity equation is one of the three fundamental equations (with momentum and energy) used to completely describe normal shock wave behavior through the Rankine-Hugoniot relations.