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Richardson Number

 

Richardson Number formula

\( f \;=\; \dfrac{ Gr }{ Re^2 }\)     (Richardson Number)

\( Gr \;=\; f \cdot Re^2  \)

\( Re \;=\; \sqrt{ \dfrac{ Gr }{ f } } \) 

Symbol English Metric
\( Ri \) = Richardson Number \(dimensionless\) \(dimensionless\)
\( Gr \) = Grashof Number \(dimensionless\) \(dimensionless\)
\( Re \) = Reynolds Number \(dimensionless\) \(dimensionless\)

Richardson number, abbreviated as \(Ri\), a dimensionless number, in fluid dynamics that quantifies the relative importance of buoyancy forces to inertial (shear) forces in a stratified flow.  It is used primarily in the analysis of atmosphere flows, oceanographic flows, and density-stratified engineering systems where velocity gradients and density gradients coexist.  The parameter provides a stability criterion for shear flows subjected to density stratification.

Richardson Number Interpretation
Low Richardson Number (Ri < 0.25)  -  The flow is dynamically unstable.  Turbulence is likely to develop because the shear (mechanical mixing) dominates over buoyancy forces.  This is often associated with the onset of Kelvin-Helmholtz instability, where waves and mixing occur.
Richardson Number (0.25 < Ri < 1)  -  This is a transitional range.  The flow may still become turbulent under certain conditions, but buoyancy begins to play a more significant role in stabilizing the flow.
High Richardson Number (Ri > 1)  -  The flow is dynamically stable.  Buoyancy forces dominate, suppressing turbulence and maintaining stratification.  Mixing is inhibited, and the fluid tends to remain layered.
low Ri indicates that kinetic energy from velocity shear overcomes the potential energy of stratification, leading to turbulence.
high Ri suggests that the stratification is strong enough to resist mixing, stabilizing the flow.

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