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  2. Incompressible flow - Wikipedia

    en.wikipedia.org/wiki/Incompressible_flow

    In fluid dynamics, a flow is considered incompressible if the divergence of the flow velocity is zero. However, related formulations can sometimes be used, depending on the flow system being modelled. Some versions are described below: Incompressible flow: =. This can assume either constant density (strict incompressible) or varying density flow.

  3. Stagnation temperature - Wikipedia

    en.wikipedia.org/wiki/Stagnation_temperature

    q = Heat per unit mass added into the system. Strictly speaking, enthalpy is a function of both temperature and density. However, invoking the common assumption of a calorically perfect gas, enthalpy can be converted directly into temperature as given above, which enables one to define a stagnation temperature in terms of the more fundamental property, stagnation enthalpy.

  4. Navier–Stokes equations - Wikipedia

    en.wikipedia.org/wiki/Navier–Stokes_equations

    The incompressible flow assumption typically holds well with all fluids at low Mach numbers (say up to about Mach 0.3), such as for modelling air winds at normal temperatures. [16] the incompressible Navier–Stokes equations are best visualized by dividing for the density: [17]

  5. Euler equations (fluid dynamics) - Wikipedia

    en.wikipedia.org/wiki/Euler_equations_(fluid...

    Thus for an incompressible inviscid fluid the specific internal energy is constant along the flow lines, also in a time-dependent flow. The pressure in an incompressible flow acts like a Lagrange multiplier, being the multiplier of the incompressible constraint in the energy equation, and consequently in incompressible flows it has no ...

  6. Derivation of the Navier–Stokes equations - Wikipedia

    en.wikipedia.org/wiki/Derivation_of_the_Navier...

    The flow is incompressible and Newtonian. Coordinates are orthogonal. Flow is 2D: u 3 = ⁠ ∂u 1 / ∂x 3 ⁠ = ⁠ ∂u 2 / ∂x 3 ⁠ = 0; The first two scale factors of the coordinate system are independent of the last coordinate: ⁠ ∂h 1 / ∂x 3 ⁠ = ⁠ ∂h 2 / ∂x 3 ⁠ = 0, otherwise extra terms appear. The stream function has ...

  7. Prandtl condition - Wikipedia

    en.wikipedia.org/wiki/Prandtl_condition

    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.

  8. Hagen–Poiseuille equation - Wikipedia

    en.wikipedia.org/wiki/Hagen–Poiseuille_equation

    For a compressible fluid in a tube the volumetric flow rate Q(x) and the axial velocity are not constant along the tube; but the mass flow rate is constant along the tube length. The volumetric flow rate is usually expressed at the outlet pressure. As fluid is compressed or expanded, work is done and the fluid is heated or cooled.

  9. Fluid parcel - Wikipedia

    en.wikipedia.org/wiki/Fluid_parcel

    In fluid dynamics, a fluid parcel, also known as a fluid element or material element, is an infinitesimal volume of fluid, identifiable throughout its dynamic history while moving with the fluid flow. [1] As it moves, the mass of a fluid parcel remains constant, while—in a compressible flow—its volume may change, [2] [3] and its shape ...