Prandtl Condition
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fluid mechanics Fluid mechanics is the branch of physics concerned with the mechanics of fluids (liquids, gases, and plasma (physics), plasmas) and the forces on them. Originally applied to water (hydromechanics), it found applications in a wide range of discipl ...
the Prandtl condition was suggested by the German physicist Ludwig Prandtl to identify possible
boundary layer In physics and fluid mechanics, a boundary layer is the thin layer of fluid in the immediate vicinity of a Boundary (thermodynamic), bounding surface formed by the fluid flowing along the surface. The fluid's interaction with the wall induces ...
separation points of
incompressible fluid In fluid mechanics, or more generally continuum mechanics, incompressible flow is a flow in which the material density does not vary over time. Equivalently, the divergence of an incompressible flow velocity is zero. Under certain conditions, t ...
flows.


Prandtl condition-in normal shock

In the case of normal shock, flow is assumed to be in a steady state and thickness of shock is very small. It is further assumed that there is no friction or heat loss at the shock (because heat transfer is negligible because it occurs on a relatively small surface). It is customary in this field to denote x as the upstream and y as the downstream condition. Since the mass flow rate from the two sides of the shock are constant, the mass balance becomes, \rho_.U_=\rho_.U_ As there is no external force applied, momentum is conserved. Which give rises to the equation P_-P_=\rho_.^2-\rho_.^2 Because heat flow is negligible, the process can be treated as adiabatic. So the energy equation will be C_.T_+\frac=C_.T_+\frac From the equation of state for perfect gas, P=\rho R T As the temperature from both sides of the shock wave is discontinuous, the speed of sound is different in these adjoining medium. So it is convenient to define the star mach number that will be independent of the specific mach number. From star condition, the speed of sound at the critical condition can also be a good reference velocity. Speed of sound at that temperature is, c^* = \sqrt And additional Mach number which is independent of specific mach number is, M^* = \frac =\frac Since energy remains constant across the shock, \frac+\frac = \frac+\frac =\frac dividing mass equation by momentum equation we will get \frac+U_=\frac+U_ From above equations, \frac\left frac-\frac\rightU_ = \frac\left frac-\frac\rightU_ it will give rises to U_.U_ = ^2 ''Which is called the prandtl condition in normal shock''


References

{{Reflist Fluid dynamics