Geostrophic Wind

The geostrophic wind is defined as the wind resulting from the balance between the Coriolis force and the pressure gradient force. Frictional effects are neglected, which is usually a very good approximation for the synoptic scale instantaneous flow in the midlatitude mid-troposphere. However, although ageostrophic terms are relatively small, they are important for the time evolution of the flow. The geostrophic wind (u_g,v_g) can be derived from the primitive equations, using the geostrophic approximation:
u_g = - {g \over f} {\partial Z \over \partial y}, v_g = {g \over f} {\partial Z \over \partial x}
where g is the force of gravity (9.81 m/s^2), f is the Coriolis parameter (approximately 1e-4; varies with latitude) and Z is the geopotential height field. The validity of this approximation is dependent on the local Rossby number: It is invalid at the equator because f is zero there, and therefore generally not used in the tropics. Other variants of the equation are possible, e.g. using the pressure field instead of Z, but are slightly more complex.

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