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268                 17. The Physics of the Atmosphere



























          Fig. 17-23. Aerodynamic flow around a cube: (a) side view, (b) plan view. Source: After
        Halitsky (5).


        with strong turbulence and mixing, a wake extending downwind from
        the cavity a distance equivalent to a number of structure side lengths, a
        displacement zone where flow is initially displaced before entering the
        wake, and a region of flow that is displaced away from the structure but
        does not get caught in the wake. Wind tunnels, water channels, and/or
        towing tanks are extremely useful in studying building wake effects.


                           V. GENERAL CIRCULATION

          Atmospheric motions are driven by the heat from incoming solar radia-
        tion and the redistribution and dissipation of this heat to maintain constant
        temperatures on the average. The atmosphere is inefficient, because only
        about 2% of the received incoming solar radiation is converted to kinetic
        energy, that is, air motion; even this amount of energy is tremendous
        compared to that which humans are able to produce. As was shown in
        Section I, a surplus of radiant energy is received in the equatorial regions
        and a net outflux of energy occurs in the polar regions. Many large-scale
        motions serve to transport heat poleward or cooler air toward the equator.
          If the earth did not rotate or if it rotated much more slowly than it
        does, a meridional (along meridians) circulation would take place in the
        troposphere (Fig. 17-24). Air would rise over the tropics, move poleward,
        sink over the poles forming a subsidence inversion, and then stream equa-
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