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  2. ΔP - Wikipedia

    en.wikipedia.org/wiki/ΔP

    Given that the head loss h f expresses the pressure loss Δp as the height of a column of fluid, Δ p = ρ ⋅ g ⋅ h f {\displaystyle \Delta p=\rho \cdot g\cdot h_{f}} where ρ is the density of the fluid.

  3. Bernoulli's principle - Wikipedia

    en.wikipedia.org/wiki/Bernoulli's_principle

    Bernoulli's principle is a key concept in fluid dynamics that relates pressure, density, speed and height. Bernoulli's principle states that an increase in the speed of a parcel of fluid occurs simultaneously with a decrease in either the pressure or the height above a datum. [1]:

  4. Maxwell relations - Wikipedia

    en.wikipedia.org/wiki/Maxwell_relations

    is pressure, temperature, volume, entropy, coefficient of thermal expansion, compressibility, heat capacity at constant volume, heat capacity at constant pressure. Maxwell's relations are a set of equations in thermodynamics which are derivable from the symmetry of second derivatives and from the definitions of the thermodynamic potentials .

  5. Shallow water equations - Wikipedia

    en.wikipedia.org/wiki/Shallow_water_equations

    The pressure gradient term (c) describes how pressure changes with position, and since the pressure is assumed hydrostatic, this is the change in head over position. The friction term (d) accounts for losses in energy due to friction, while the gravity term (e) is the acceleration due to bed slope.

  6. Coandă effect - Wikipedia

    en.wikipedia.org/wiki/Coandă_effect

    If the ⁠ h / r ⁠ ratio (ratio of the width of the jet to the radius of curvature of the wall) is less than 0.5, a true Coandă effect is observed, with the wall pressures along the curved wall remaining at this low (sub-ambient pressure) level until the jet reaches the end of the wall (when the pressure rapidly returns to ambient pressure).

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  8. Navier–Stokes equations - Wikipedia

    en.wikipedia.org/wiki/Navier–Stokes_equations

    The pressure field is obtained from the velocity field as = ‖ ‖ / (where and are reference values for the pressure and density fields respectively). Since both the solutions belong to the class of Beltrami flow , the vorticity field is parallel to the velocity and, for the case with positive helicity, is given by ω = 3 k u {\displaystyle ...

  9. Vertical pressure variation - Wikipedia

    en.wikipedia.org/wiki/Vertical_pressure_variation

    Vertical pressure variation is the variation in pressure as a function of elevation. Depending on the fluid in question and the context being referred to, it may also vary significantly in dimensions perpendicular to elevation as well, and these variations have relevance in the context of pressure gradient force and its effects.