Rossby number

The Rossby number (Ro), named for Carl-Gustav Arvid Rossby, is a dimensionless number used in describing fluid flow. The Rossby number is the ratio of inertial force to Coriolis force, terms $, \mathbf \cdot \nabla \mathbf, \sim U^2 / L$ and $\Omega \times \mathbf \sim U\Omega$ in the Navier–Stokes equations respectively. It is commonly used in geophysical phenomena in the oceans and atmosphere, where it characterizes the importance of Coriolis accelerations arising from planetary rotation. It is also known as the Kibel number.

The Rossby number (Ro, not R_o) is defined as

: $\text = \frac,$

where ''U'' and ''L'' are respectively characteristic velocity and length scales of the phenomenon, and $f = 2\Omega \sin \phi$ is the Coriolis frequency, with $\Omega$ being the angular frequency of planetary rotation, and $\phi$ the latitude.

A small Rossby number signifies a system strongly affected by Coriolis forces, and a large Rossby number signifies a system in which inertial and centrifugal forces dominate. For example, in tornadoes, the Rossby number is large (≈ 10³), in low-pressure systems it is low (≈ 0.1–1), and in oceanic systems it is of the order of unity, but depending on the phenomena can range over several orders of magnitude (≈ 10⁻²–10²). As a result, in tornadoes the Coriolis force is negligible, and balance is between pressure and centrifugal forces (called ''cyclostrophic balance''). Cyclostrophic balance also commonly occurs in the inner core of a tropical cyclone. In low-pressure systems, centrifugal force is negligible, and balance is between Coriolis and pressure forces (called '' geostrophic balance''). In the oceans all three forces are comparable (called '' cyclogeostrophic balance''). For a figure showing spatial and temporal scales of motions in the atmosphere and oceans, see Kantha and Clayson.

When the Rossby number is large (either because ''f'' is small, such as in the tropics and at lower latitudes; or because ''L'' is small, that is, for small-scale motions such as flow in a bathtub; or for large speeds), the effects of planetary rotation are unimportant and can be neglected. When the Rossby number is small, then the effects of planetary rotation are large, and the net acceleration is comparably small, allowing the use of the geostrophic approximation.

See also

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References and notes

Further reading

For more on numerical analysis and the role of the Rossby number, see:
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For an historical account of Rossby's reception in the United States, see
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{{NonDimFluMech
Atmospheric dynamics
Dimensionless numbers of fluid mechanics