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12 - An excursion into spectral turbulence theory

Published online by Cambridge University Press:  05 June 2012

Wilford Zdunkowski
Affiliation:
Johannes Gutenberg Universität Mainz, Germany
Andreas Bott
Affiliation:
Rheinische Friedrich-Wilhelms-Universität Bonn
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Summary

The phenomenological theory discussed in the previous chapter did not permit the parameterization of the energy dissipation. In this chapter spectral turbulence theory will be presented to the extent that we appreciate the connections among the turbulent exchange coefficient, the energy dissipation, and the turbulent kinetic energy. In the spectral representation we think of the longer waves as the averaged quantities and the short waves as the turbulent fluctuations. Since the system of atmospheric prediction equations is very complicated we will be compelled to apply some simplifications.

Fourier representation of the continuity equation and the equation of motion

Before we begin with the actual transformation it may be useful to briefly review some basic concepts. For this reason let us consider the function a(x) which has been defined on the interval L only. In order to represent the function by a Fourier series, we extend it by assuming spatial periodicity. Using Cartesian coordinates we obtain a plot as exemplified in Figure 12.1. The period L is taken to be large enough that averaged quantities within L may vary, i.e. the averaging interval Δx ≪≪ L.

Certain conditions must be imposed on a(x) in order to make the expansion valid. The function a(x) must be a bounded periodic function that in any one period has at most a finite number of local maxima and minima and a finite number of points of discontinuity.

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Dynamics of the Atmosphere
A Course in Theoretical Meteorology
, pp. 326 - 348
Publisher: Cambridge University Press
Print publication year: 2003

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