Rossby Number
The
Rossby number
, named for
Carl-Gustav Arvid Rossby
, is a
dimensionless number
used in describing
geophysical
phenomena in the
oceans
and
atmosphere
. It characterises the ratio of
inertial
forces in a
fluid
to the
fictitious forces
arising from
planetary
rotation
. It is also known as the
Kibel number
. It is defined as:
R_o=\frac{U}{Lf}
where
U
and
L
are, respectively, characteristic velocity and length scales of the phenomenon and
f
= 2 Ω sin φ is the
Coriolis frequency
, where Ω is the
angular velocity
of
planetary
rotation
and φ the
latitude
. When the Rossby number is large (such as in the tropics and at lower latitudes), 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
geostrophic approximation
is valid.
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