User:Milton Beychok/Sandbox

(PD) Drawing: Milton Beychok
Drawing of a classical Venturi tube per ASME Standard MFC-3M-1989.

A Venturi tube (or simply a venturi) is a section of piping consisting of an inlet converging conical section leading to a small diameter cylindrical section called the throat, followed by a diverging conical section leading to a cylindrical exit (see the adjacent drawing).

The volumetric flow rate, Q (e.g., m³/s), of a fluid flowing through the venturi at any given point is the product of the cross-sectional area, A (e.g., m²) at that point multiplied by the fluid's linear velocity, v (e.g., m/s), at that point. Since the volumetric flow rate is the same at any point within the venturi, the linear velocity of the fluid traveling through the smaller diameter throat of the venturi must increase which results in a decrease of pressure due to the conservation of energy, one of the conservation laws.

The gain in kinetic energy resulting from the increased linear velocity in the throat is offset (i.e., balanced) by the decrease of pressure in the throat. The reduction in pressure which occurs when the fluid flows through the throat is called the Venturi effect and is named after the Italian physicist Giovanni Battista Venturi (1746 - 1822) who first observed the effect.

Thus, referring to the adjacent drawing, the pressure p₂ and the cross-sectional area A₂ in the throat are smaller than the pressure p₁ and the cross-sectional area A₁ in the cylindrical inlet section. The linear velocity v₂ in the throat is higher than the linear velocity v₁ in the inlet section.

A venturi tube may also consist of non-cylindrical ducting rather than piping.

Measuring fluid flow rate with a venturi

Incompressible fluid

Venturi tubes are used to accurately measure the volumetric flow of an ideal fluid, meaning that the fluid satisfies these conditions:

• The fluid is nonviscous: There is no internal friction between layers of the fluid.
• The fluid is incompressible: The density of the fluid is constant (as is the case with liquids)
• The fluid flows without any turbulence: No element of the fluid has any angular velocity about its center, so there are no eddy currents present.
• The fluid flow is steady: The velocity, density and pressure at each point in the fluid does not change with time.

Starting with a common form of the Bernoulli equation for fluid flow:

 $p_{1}+{\tfrac {1}{2}}\,\rho _{1}\,v_{1}^{2}+\rho _{1}\,g\,h_{1}=p_{2}+{\tfrac {1}{2}}\,\rho _{2}\,v_{2}^{2}+\rho _{2}\,g\,h_{2}$

where ρv²/2 denotes kinetic energy, ρgh denotes gravitational potential energy and:

$p$	= the fluid's static pressure
$\rho$	= the fluid's density
$v$	= the fluid's linear velocity
$g$	= the gravitational acceleration
$h$	= the height of a given point (in the fluid flow) above any reference plane designated as having zero height

For an incompressible fluid with a constant density and a venturi with a horizontal centerline, the equation simplifies to:

 $p_{1}+{\tfrac {1}{2}}\,\rho \,v_{1}^{2}=p_{2}+{\tfrac {1}{2}}\,\rho \,v_{2}^{2}$

or to:

 $p_{1}-p_{2}={\tfrac {1}{2}}\,\rho \,(v_{2}^{2}-v_{1}^{2})$

Since the volumetric flow rate Q is the same at all points in the venturi by the equation of continuity:

 $Q=A_{1}\,v_{1}=A_{2}\,v_{2}$

then:

 $p_{1}-p_{2}={\tfrac {1}{2}}\,\rho \left({\frac {Q^{2}}{A_{2}^{2}}}-{\frac {Q^{2}}{A_{1}^{2}}}\right)$

which can be re-arranged to:

 $Q=A_{2}{\sqrt {\frac {\rho (p_{1}-p_{2})}{2[1-({\frac {A_{2}}{A_{1}}})^{2}]}}}$