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reducing squared uncertainty e 2 . In large-eddy simulation of atmospheric boundary
layers, for example, we can average the calculated fields over homogeneous hori-
zontal planes. In this way one “snapshot” of a simulated field on a sufficiently large
plane can yield a good estimate of the ensemble average.
2.5 The turbulence spectrum and the eddy velocity scale
In Chapter 1 we introduced the velocity scales u, υ and length scales , η of the
energy-containing and dissipative eddies, respectively, and showed that
R 3 / t , with R t the large-eddy Reynolds number u/ν . R t varies from less than 10 3
in some engineering flows to about 10 8 in the convective atmospheric boundary
layer and perhaps 10 10 in a supercell thunderstorm; over that range varies from
about 10 2 to 10 7 .
The power spectral density of the turbulent velocity field (loosely called “the
turbulence spectrum”) allows the velocity scale u of the energy-containing eddies
to be generalized to u(r) , the velocity scale of an eddy of size r , with
η .We
shall present here an informal derivation of the turbulence spectrum, beginning for
simplicity with a homogeneous scalar function of a single variable. Part III contains
a more formal presentation.
r
2.5.1 The spectrum of a one-dimensional, real, random,
homogeneous scalar function
Let f(x) be a real, homogeneous function, the sumof an ensemble-mean part F and
a fluctuation f(x) , defined over record of length L . It could be a spatial record of
temperature or a velocity component in a turbulent flow, for example. We can
approximate f(x) through a Fourier series, a sum of sines and cosines of
wavelengths L/n, n
=
0 ,...,N :
a n cos 2 πnx
L
b n sin 2 πnx
L
.
N
N
a 0
2 +
f(x)
+
(2.39)
n = 1
n = 1
The coefficients a n and b n are real numbers called Fourier coefficients .
Since each of the sine and cosine terms in Eq. (2.39) integrates to zero over the
record length, it follows that the average of
f(x) over the record length is
L
1
L
a 0
f(x)dx =
2 .
(2.40)
0
f(x) with x .
The other Fourier components together represent the variation of
 
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