Geoscience Reference
In-Depth Information
Table 1.1
Primary eddy growth
Growth step number
±σ
k
Probability (%)
Model predicted
Statistical normal
2
0.9000
0.8864
18.1555
18.4060
3
0.8000
0.7237
24.8304
21.1855
4
0.7000
0.6268
29.9254
24.1964
5
0.6000
0.5606
33.9904
27.4253
6
0.5000
0.5118
37.3412
30.8538
7
0.4000
0.4738
40.1720
34.4578
8
0.3000
0.4432
42.6093
38.2089
9
0.2000
0.4179
44.7397
42.0740
10
0.1000
0.3964
46.6250
46.0172
11
0
0.3780
48.3104
50.0000
tical normal probability density distribution corresponding to the normalized devia-
tion σ values are also given in Table
1.1
.
The model predicted probability density distribution
P
along with the corre-
sponding statistical normal distribution with probability values plotted on linear
and logarithmic scales, respectively, on the left- and right-hand sides are shown in
Fig.
1.8
. The model predicted probability distribution
P
for fractal space-time fluc-
tuations is very close to the statistical normal distribution for normalized deviation
σ values less than 2 as seen on the left-hand side of Fig.
1.8
. The model predicts
progressively higher values of probability
P
for values of σ greater than 2 as seen
on a logarithmic plot on the right-hand side of Fig.
1.8
.
1.6.4
Atmospheric Wind Spectrum and Suspended Particulate
Size Spectrum
The steady-state flux d
N
of CCN at level
z
in the normalized vertical velocity per-
turbation (d
W
)
z
is given as follows:
(1.21)
d
NNWz
= (
d
) .
The logarithmic wind profile relationship for
W
at Eq. (1.4) gives
NNz
w
k
(1.22)
*
d
=
d
(ln .
z
Substituting for
k
from Eq. (1.2)
NNz
w
(1.23)
*
2
d
=
w
Wz z Wz
d
(ln)
=
d
(ln .
z
*
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