Shear velocity

Shear velocity, also called friction velocity, is a form by which a shear stress may be re-written in units of velocity. It is useful as a method in fluid mechanics to compare true velocities, such as the velocity of a flow in a stream, to a velocity that relates shear between layers of flow.

Shear velocity is used to describe shear-related motion in moving fluids. It is used to describe:

• Diffusion and dispersion of particles, tracers, and contaminants in fluid flows
• The velocity profile near the boundary of a flow (see Law of the wall)
• Transport of sediment in a channel

Shear velocity also helps in thinking about the rate of shear and dispersion in a flow. Shear velocity scales well to rates of dispersion and bedload sediment transport. A general rule is that the shear velocity is between 5% and 10% of the mean flow velocity.

For river base case, the shear velocity can be calculated by Manning's equation.

${\displaystyle u^{*}=\langle u\rangle {\frac {n}{a}}(gR_{h}^{-1/3})^{0.5}}$

• n is the Gauckler–Manning coefficient. Units for values of n are often left off, however it is not dimensionless, having units of: (T/[L^1/3]; s/[ft^1/3]; s/[m^1/3]).
• R_h is the hydraulic radius (L; ft, m);
• the role of a is a dimension correction factor. Thus a= 1 m^1/3/s = 1.49 ft^1/3/s.

Instead of finding ${\displaystyle n}$ and ${\displaystyle R_{h}}$ for the specific river of interest, the range of possible values can be examined; for most rivers, ${\displaystyle u^{*}}$ is between 5% and 10% of ${\displaystyle \langle u\rangle }$:

For general case

${\displaystyle u_{\star }={\sqrt {\frac {\tau }{\rho }}}}$

where τ is the shear stress in an arbitrary layer of fluid and ρ is the density of the fluid.

Typically, for sediment transport applications, the shear velocity is evaluated at the lower boundary of an open channel:

${\displaystyle u_{\star }={\sqrt {\frac {\tau _{b}}{\rho }}}}$

where τ_b is the shear stress given at the boundary.

Shear velocity is linked to the Darcy friction factor by equating wall shear stress, giving:

${\displaystyle u_{\star }={\langle u\rangle }{\sqrt {\frac {f_{\mathrm {D} }}{8}}}}$

where f_D is the friction factor. ^[1]

Shear velocity can also be defined in terms of the local velocity and shear stress fields (as opposed to whole-channel values, as given above).

Friction velocity in turbulence

The friction velocity is often used as a scaling parameter for the fluctuating component of velocity in turbulent flows. ^[2] One method of obtaining the shear velocity is through non-dimensionalization of the turbulent equations of motion. For example, in a fully developed turbulent channel flow or turbulent boundary layer, the streamwise momentum equation in the very near wall region reduces to:

${\displaystyle 0={\nu }{\partial ^{2}{\overline {u}} \over \partial y^{2}}-{\frac {\partial }{\partial y}}({\overline {u'v'}})}$.

By integrating in the y-direction once, then non-dimensionalizing with an unknown velocity scale u_∗ and viscous length scale ⁠ν/u_∗⁠, the equation reduces down to:

${\displaystyle {\frac {\tau _{w}}{\rho }}=\nu {\frac {\partial u}{\partial y}}-{\overline {u'v'}}}$

or

${\displaystyle {\frac {\tau _{w}}{\rho u_{\star }^{2}}}={\frac {\partial u^{+}}{\partial y^{+}}}+{\overline {\tau _{T}^{+}}}}$.

Since the right hand side is in non-dimensional variables, they must be of order 1. This results in the left hand side also being of order one, which in turn give us a velocity scale for the turbulent fluctuations (as seen above):

${\displaystyle u_{\star }={\sqrt {\frac {\tau _{w}}{\rho }}}}$.

Here, τ_w refers to the local shear stress at the wall.

Planetary boundary layer

Within the lowest portion of the planetary boundary layer a semi-empirical log wind profile is commonly used to describe the vertical distribution of horizontal mean wind speeds. The simplified equation that describe it is

${\displaystyle u(z)={\frac {u_{*}}{\kappa }}\left[\ln \left({\frac {z-d}{z_{0}}}\right)\right]}$

where ${\displaystyle \kappa }$ is the Von Kármán constant (~0.41), ${\displaystyle d}$ is the zero plane displacement (in metres).

The zero-plane displacement (${\displaystyle d}$) is the height in meters above the ground at which zero wind speed is achieved as a result of flow obstacles such as trees or buildings. It^{[ clarification needed ]} can be approximated as ²/₃ to ³/₄ of the average height of the obstacles. ^[3] For example, if estimating winds over a forest canopy of height 30 m, the zero-plane displacement could be estimated as d = 20 m.

Thus, you can extract the friction velocity by knowing the wind velocity at two levels (z).

${\displaystyle u_{*}={\frac {\kappa (u(z2)-u(z1))}{\ln \left({\frac {z2-d}{z1-d}}\right)}}}$

Due to the limitation of observation instruments and the theory of mean values, the levels (z) should be chosen where there is enough difference between the measurement readings. If one has more than two readings, the measurements can be fit to the above equation to determine the shear velocity.

References

1. Chanson, Hubert (2004). Environmental Hydraulics for Open Channel Flows. Elsevier Science. p. 83. ISBN   9780080472690.
2. Schlichting, H.; Gersten, K. (2004). Boundary-Layer Theory (8th ed.). Springer 1999. ISBN   978-81-8128-121-0.
3. Holmes JD. Wind Loading of Structures. 3rd ed. Boca Raton, Florida: CRC Press; 2015.

• Whipple, K. X. (2004). "III: Flow Around Bends: Meander Evolution" (PDF). MIT. 12.163 Course Notes.