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258                  17. The Physics of the Atmosphere

       A. Pressure Gradient Force
         Three forces of importance to horizontal motion are the pressure gradient
       force, gravity, and friction. Atmospheric pressure equals mass times the
       acceleration of gravity. Considering a unit volume, p = pg; the gravitational
       force on the unit volume is directed downward. Primarily because of hori-
       zontal temperature gradients, there are horizontal density gradients and
       consequently horizontal pressure gradients. The horizontal pressure gradi-
       ent force p h = Ap/p Ax where Ap is the horizontal pressure difference over
       the distance AJ. The direction of this force and of the pressure difference
       measurement is locally perpendicular to the lines of equal pressure (isobars)
       and is directed from high to low pressure.

       B. Coriolis Force

         If the earth were not rotating, the wind would blow from high to low
       pressure. Close to the earth, it would be slowed by friction between the
       atmosphere and the earth's surface but would maintain the same direction
       with height. However, since the earth undergoes rotation, there is an
       apparent force acting on horizontal atmospheric motions when examined
       from a point of reference on the earth's surface. For example, consider a
                               1
       wind of velocity 10 m s"  blowing at time 1 in the direction of the 0°
       longitude meridian across the north pole (Fig. 17-10). The wind in an
       absolute sense continues to blow in this direction for 1 hr, and a parcel of
       air starting at the pole at time 1 travels 36 km in this period. However,
       since the earth turns 360° every 24 hr, or 15° per hr, it has rotated 15° in
       the hour and we find that at time 2 (60 min after time 1) the 15° meridian
       is now beneath the wind vector. As viewed from space (the absolute frame
       of reference), the flow has continued in a straight line. However, as viewed
       from the earth, the flow has undergone an apparent deflection to the right.
       The force required to produce this apparent deflection is the coriolis force
       and is equal to D = vf where /, the coriolis parameter, equals 2ft sin <£.















         Fig. 17-10. Effect of the coriolis force. The path of air moving from the north pole to the
       south as viewed from space is straight; as viewed from the earth's surface it is curved.
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