(meteorology) That horizontal wind velocity for which the Coriolis acceleration exactly balances the horizontal pressure force.
| Sci-Tech Dictionary: geostrophic wind |
(meteorology) That horizontal wind velocity for which the Coriolis acceleration exactly balances the horizontal pressure force.
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| Sci-Tech Encyclopedia: Geostrophic wind |
A hypothetical wind based upon the assumption that a perfect balance exists between the horizontal components of the Coriolis force and the horizontal pressure gradient force per unit mass, with the implication that viscous forces and accelerations are negligible. The geostrophic wind blows parallel to the isobars (lines of equal pressure) with lower pressure to the left of the direction of the wind in the Northern Hemisphere and to the right in the Southern Hemisphere. It represents a good approximation to the actual wind at elevations greater than about 3000 ft (900 m), except in instances of strongly curved flow and in the vicinity of the Equator.
The term thermal wind denotes the net change in the geostrophic wind over some specific vertical distance. This change arises because the rate of change of pressure in the vertical is different in two air columns of different air density, so that the horizontal component of the pressure gradient force per unit mass varies in the vertical. The thermal wind is directed approximately parallel to the isotherms of air temperature with cold air to the left and warm air to the right in the Northern Hemisphere, and vice versa in the Southern Hemisphere. Thus, for example, the increasing predominance of westerly winds aloft may be viewed as a consequence of the warmth of tropical latitudes and the coldness of polar regions. See also Coriolis acceleration; Gradient wind; Wind; Wind stress.
| Geography Dictionary: geostrophic wind |
A theoretical wind, occurring when the force exerted on the air by the pressure gradient is equal to the opposing Coriolis force (assuming straight or nearly straight isobars; when the isobars are strongly curved, the effect of centrifugal force should be added in). The net result is a wind blowing parallel to the isobars, with speeds proportional to the pressure gradient. Except in low latitudes, where the Coriolis force is minimal, the actual wind direction is the same as that of the geostrophic wind.
Supergeostrophic flow describes wind speeds greater than the expected geostrophic wind. It occurs at a jet entry, where winds are experiencing linear acceleration. Subgeostrophic flow describes wind speeds less than the expected geostrophic wind.
| Wikipedia: Geostrophic wind |
The geostrophic wind (pronounced /dʒiːɵˈstrɒfɨk/ or /dʒiːɵˈstroʊfɨk/) is the theoretical wind that would result from an exact balance between the Coriolis effect and the pressure gradient force. This condition is called geostrophic balance. The geostrophic wind is directed parallel to isobars (lines of constant pressure at a given height). This balance seldom holds exactly in nature. The true wind almost always differs from the geostrophic wind due to other forces such as friction from the ground or the centrifugal force from curved fluid flow. Thus, the actual wind would equal the geostrophic wind only if there were no friction and the isobars were perfectly straight. Despite this, much of the atmosphere outside the tropics is close to geostrophic flow much of the time and it is a valuable first approximation.
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Air naturally moves from areas of high pressure to areas of low pressure, due to the pressure gradient force. As soon as the air starts to move, however, the Coriolis "force" deflects it. The deflection is to the right in the northern hemisphere, and to the left in the southern hemisphere. As the air moves from the high pressure area, its speed increases, and so does its Coriolis deflection. The deflection increases until the Coriolis and pressure gradient forces are in geostrophic balance: at this point, the air flow is no longer moving from high to low pressure, but instead moves along an isobar. (Note that this explanation assumes that the atmosphere starts in a geostrophically unbalanced state and describes how such a state would evolve into a balanced flow. In practice, the flow is nearly always balanced.) The geostrophic balance helps to explain why, in the northern hemisphere, low pressure systems spin counterclockwise and high pressure systems spin clockwise, and the opposite in the southern hemisphere.
Flow of ocean water is also largely geostrophic. Just as multiple weather balloons that measure pressure as a function of height in the atmosphere are used to map the atmospheric pressure field and infer the geostrophic wind, measurements of density as a function of depth in the ocean are used to infer geostrophic currents. Satellite altimeters are also used to measure sea surface height anomaly, which permits a calculation of the geostrophic current at the surface. Geostrophic flow in air or water is a zero-frequency inertial wave.
The effect of friction, between the air and the land, breaks the geostrophic balance. Friction slows the flow, lessening the effect of the Coriolis force. As a result, the pressure gradient force has a greater effect and the air still moves from high pressure to low pressure, though with great deflection. This explains why high pressure system winds radiate out from the center of the system, while low pressure systems have winds that spiral inwards.
The geostrophic wind neglects frictional effects, which is usually a good approximation[citation needed] for the synoptic scale instantaneous flow in the midlatitude mid-troposphere. Although ageostrophic terms are relatively small, they are essential for the time evolution of the flow and in particular are necessary for the growth and decay of storms. Quasigeostrophic and Semigeostrophic theory are used to model flows in the atmosphere more widely. These theories allow for divergence to take place and for weather systems to then develop.
Assuming geostrophic balance, the geostrophic wind components (ug,vg) on a constant-pressure surface can be derived as:


where g is the acceleration due to gravity (9.81 m.s−2), f is the Coriolis parameter (approximately 10−4 s−1, varying with latitude) and Z is the geopotential height of the constant pressure surface. The validity of this approximation depends on the local Rossby number. It is invalid at the equator, because f is equal to zero there, and therefore generally not used in the tropics.
Other variants of the equation are possible; for example, the geostrophic wind vector can be expressed in terms of the gradient of the geopotential height Φ on a surface of constant pressure:

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