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Representing the larger scale eddy energy as E
2 ∝ .
WE
2
(1.46)
The length scale ratio R 1 / R 2 therefore represents fractional probability P (Eqs. 1.16
and 1.20) of occurrence of large eddy energy E in the environment of the primary
small-scale eddy energy K B T (Eq. 1.45). The expression for P is obtained from
Eq. (1.44) as follows:
E
K B .
(1.47)
T
Pe
The above is the same as Boltzmann's equation (Eq. 1.40).
The derivation of Boltzmann's equation from general systems theory concepts
visualizes the eddy energy distribution as follows: (1) the primary small-scale eddy
represents the molecules whose eddy kinetic energy is equal to K B T as in classi-
cal physics. (2) The energy pumping from the primary small-scale eddy generates
growth of progressive larger eddies (Selvam 1990 ). The r.m.s circulation speeds W
of larger eddies are smaller than that of the primary small-scale eddy (Eq. 1.1). (3)
The space-time fractal fluctuations of molecules (atoms) in an ideal gas may be
visualized to result from an eddy continuum with the eddy energy E per unit volume
relative to primary molecular kinetic energy (K B T ) decreasing progressively with
increase in eddy size.
The eddy energy probability distribution (  P ) of fractal space-time fluctua-
tions also represents the Boltzmann distribution for each stage of hierarchical eddy
growth and is given by Eqs. (1.16) and (1.20) derived earlier, namely
τ
4
P =
.
The general systems theory concepts are applicable to all space-time scales ranging
from microscopic scale quantum systems to macroscale real-world systems such as
atmospheric flows.
References
Bak PC, Tang C, Wiesenfeld K (1988) Self-organised criticality. Phys Rev A 38:364-374
Beck C (2009) Generalized information and entropy measures in physics. Contemp Phys 50:495-
510 (arXiv:0902.1235v2) [cond-mat.stat-mech]
Boers R (1989) A parametrization of the depth of the entrainment zone. J Atmos Sci 28:107-111
Boltzmann L (1872) Weitere Studien Äuber das WÄarmegleichgewicht unter GasmolekÄulen.
Wien Ber 66:275-370 (WA, B and I, pp 316-402)
Brown RA (1980) Longitudinal instabilities and secondary flows in the planetary boundary layer.
Rev Geophys Space Phys 18:683-697
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