Compressible flow is a branch of fluid mechanics that deals with flows where significant changes in fluid density occur. Unlike incompressible flows, where density is assumed constant (typically valid for liquids and low-speed gases), compressible flow analysis must account for the coupling between density, pressure, and temperature. This behavior is most commonly observed in gases moving at high velocities, but it can also occur under significant pressure or temperature variations even at lower speeds.
The primary parameter used to characterize compressible flow is the Mach number ($M$), defined as the ratio of the flow velocity ($v$) to the speed of sound in the fluid ($a$):
The speed of sound itself is a function of the fluid's properties, specifically the ratio of specific heats ($\gamma$), the gas constant ($R$), and the absolute temperature ($T$):
Based on the Mach number, compressible flows are categorized into distinct regimes, each with unique physical behaviors:
A fundamental concept in analyzing compressible flow is isentropic flowflow that is both adiabatic (no heat transfer) and reversible (no friction). While real flows rarely meet these strict criteria, isentropic relations provide an ideal baseline for designing nozzles, diffusers, and jet engines.
In isentropic flow, the relationship between the static properties (pressure, density, temperature) and the stagnation properties (total properties) are governed by the Mach number. The stagnation temperature ($T_0$) remains constant in adiabatic flow:
Similarly, the ratios for pressure and density are:
One of the most distinct phenomena in compressible flow is the shock wave. A shock wave is an extremely thin region (often only a few mean free paths thick) across which flow properties change almost discontinuously. Shock waves occur when a supersonic flow is decelerated or forced to turn.
A normal shock wave is perpendicular to the flow direction. It is a non-isentropic process, meaning entropy increases across the shock. As flow passes through a normal shock:
When a supersonic flow encounters a corner or a wedge that turns the flow into itself, an oblique shock wave is generated. This shock wave is inclined at an angle ($\beta$) to the upstream flow direction. The flow deflection angle ($\theta$) is related to the shock angle and the upstream Mach number. Unlike normal shocks, the flow downstream of an oblique shock can remain supersonic if the turning angle is small enough.
The counterpart to the oblique shock is the expansion wave (or Prandtl-Meyer expansion). When a supersonic flow turns away from itself, such as flowing over a convex corner, an expansion fan is generated. This process is isentropic. Across an expansion fan:
The behavior of gases in nozzles is a classic application of compressible flow theory. The area-velocity relationship for compressible flow differs fundamentally from incompressible flow:
This equation implies that:
To accelerate a gas from rest to supersonic speeds, a converging-diverging (de Laval) nozzle is required. The flow accelerates in the converging section until it reaches Mach 1 at the throat (the narrowest point). This condition is known as choking. Once choked, the mass flow rate reaches its maximum and cannot be increased by lowering the back pressure further. If the back pressure is low enough, the flow continues to accelerate in the diverging section, becoming supersonic.
Understanding compressible flow is vital in numerous engineering fields:
Compressible flow introduces complex phenomena such as shock waves, choking, and density variations that are absent in incompressible flow analysis. By leveraging the Mach number and isentropic relations, engineers can predict and control these behaviors to design efficient high-speed systems. From breath-taking fighter jets to humble gas pipelines, the principles of compressible flow govern the movement of gases that power modern technology.
