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Stagnation pressure

 
Wikipedia: Stagnation pressure

In fluid dynamics, stagnation pressure is the static pressure at a stagnation point in a fluid flow.[1] At a stagnation point the fluid velocity is zero and all kinetic energy has been converted into pressure energy. Stagnation pressure is equal to the sum of the free-stream dynamic pressure and free-stream static pressure.[2] Stagnation pressure is sometimes referred to as pitot pressure because it is measured using a pitot tube.

Contents

Magnitude

The magnitude of stagnation pressure can be derived from the Bernoulli Equation.[3][1] For incompressible flow,


Total Pressure = Dynamic Pressure + Static Pressure

or

P_\text{total}=\tfrac{1}{2} \rho v^2 + P_\text{static}

where: P_\text{total}\; is the total pressure in pascals
\rho\; is the fluid density in kg/m3
v\; is the velocity of fluid in m/s at any point
P_\text{static}\; is the static pressure in pascals at any point.

At a stagnation point, the velocity of the fluid is zero. Therefore the stagnation pressure (which is the static pressure at a stagnation point) is equal to total pressure.[1]
P_\text{total}=0 + P_\text{stagnation}\;

In compressible flow the stagnation pressure is equal to total pressure only if the fluid entering the stagnation point is brought to rest isentropically.[4] For many purposes in compressible flow, the stagnation enthalpy or stagnation temperature plays a role similar to the stagnation pressure in incompressible flow.

Compressible flow

Stagnation pressure is the static pressure a fluid retains when brought to rest isentropically from Mach number M.[5]

\frac{p_t}{p} = \left(1 + \frac{\gamma -1}{2} M^2\right)^{\frac{\gamma}{\gamma-1}}\,

or, assuming an isentropic process, the stagnation pressure can be calculated from the ratio of stagnation temperature to static temperature:

\frac{p_t}{p} = \left(\frac{T_t}{T}\right)^{\frac{\gamma}{\gamma-1}}\,

where:

p_t =\, stagnation (or total) pressure

p =\, static pressure

T_t =\, stagnation (or total) temperature in kelvin

T =\, static temperature in kelvins

\gamma\ =\, ratio of specific heats

The above derivation holds only for the case when the fluid is assumed to be calorically perfect. For such fluids, specific heats and γ are assumed to be constant and invariant with temperature (See also, a thermally perfect fluid).

See also

Notes

  1. ^ a b c Clancy, L.J., Aerodynamics, Section 3.5
  2. ^ Stagnation Pressure at Eric Weisstein's World of Physics (Wolfram Research)
  3. ^ Equation 4, Bernoulli Equation - The Engineering Toolbox
  4. ^ Clancy, L.J. Aerodynamics, Section 3.12
  5. ^ Equations 35,44, Equations, Tables and Charts for Compressible Flow

References

  • Clancy, L.J. (1975), Aerodynamics, Pitman Publishing Limited, London. ISBN 0 273 01120 0

External links


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