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III. Laws of Motion                    259

        Here O is the angular speed of the earth's rotation,            2rr/
                                       1
                                    5
        (24 x 60 x 60) = 7.27 x 10~  s" , and 0 is the latitude. It is seen that/
        is maximal at the poles and zero at the equator. The deflecting force is to
        the right of the wind vector in the Northern Hemisphere and to the left in
        the Southern Hemisphere. For the present example/ the deflecting force is
                  3     2
        1,45 x 10~  m s~ , and the amount of deflection after the 36-km movement
        in 1 hr is 9.43 km.

        C. Geostrophk Wind
          Friction between the atmosphere and the earth's surface may generally
        be neglected at altitudes of about 700 m and higher. Therefore, large-scale
        air currents closely represent a balance between the pressure gradient force
        and the coriolis force. Since the coriolis force is at a right angle to the
        wind vector, when the coriolis force is equal in magnitude and opposite
        in direction to the pressure gradient force, a wind vector perpendicular to
        both of these forces occurs, with its direction along the lines of constant
        pressure (Fig. 17-11). In the Northern Hemisphere, the low pressure is to
        the left of the wind vector (Buys Ballot's law); in the Southern Hemisphere,
        low pressure is to the right. The geostrophic velocity is


        When the isobars are essentially straight, the balance between the pressure
        gradient force and the coriolis force results in a geostrophic wind parallel
        to the isobars.

        D. Gradient Wind

          When the isobars are curved, an additional force, a centrifugal force
        outward from the center of curvature, enters into the balance of forces. In
        the case of curvature around low pressure, a balance of forces occurs when
        the pressure gradient force equals the sum of the coriolis and centrifugal
        forces (Fig. 17-12) and the wind continues parallel to the isobars. In the














                    Fig. 17-11. Balance of forces resulting in geostrophic wind.
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