Structure of the PBL
Structure of the PBL
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DOI:
10.1007/978-1-935704-16-4_2
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发表时间:
1988
期刊:
影响因子:
--
通讯作者:
J. Wyngaard
中科院分区:
文献类型:
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作者:
J. Wyngaard
Even the most casual observer notices the changes in the wind. Though it has a certain persistence in time, the details of its swirls and eddies seem infinitely variable. Its strength changes day to day as weather systems evolve, and day to night as the sun rises and sets. It is modulated strongly by terrain features and by urban architecture. How can we hope to describe such a complicated phenomenon? The answer, of course, is that even though the wind fluctuates randomly, its behavior-even in its minuscule details-is not without order. We believe that it satisfies the Navier-Stokes equation, and for over 100 years we have used that equation, in conjunction with measurements, to study the behavior of the wind in the lower atmosphere. Although its instantaneous, local details are essentially unpredictable, as anyone who watches the continuously changing, meandering plume from a smokestack might conclude, we do understand the behavior of the average wind-its dependence on stability, distance from the surface, mean weather conditions, and the likeat least in uncomplicated terrain. We also understand much about its turbulent fluctuations. Today we can estimate the" most likely" behavior in many important turbulent dispersion problems in the planetary boundary layer (PBL), in spite of the chaos of the actual process.I shall outline some of the knowledge about the PBL and its turbulence that allows us to deal successfully with applications such as dispersion. This knowledge rests principally on observations, but there is room for a good deal of individuality in interpreting these observations and fabricating useful conceptual models from them. Thus, the interpretations and explanations in this chapter reflect to some extent my own way of viewing the PBL. I shall concentrate on