HR: 1340h
AN: U43B-1131 [Abstracts]
TI: Isotropic turbulence, stable layers: atmospheric fictions
AU: Lovejoy, S
EM: lovejoy@physics.mcgill.ca
AF: Physics, McGill University, 3600 University st., Montreal, Qc. H3A 2T8, Canada
AU: Tuck, A
EM: Adrian.F.Tuck@noaa.gov
AF: NOAA, 325 Broadway, Boulder, Co. 80305-3337, United States
AU: Hovde, S
EM: susan.j.hovde@noaa.gov
AF: NOAA, 325 Broadway, Boulder, Co. 80305-3337, United States
AU: * Schertzer, D
EM: Daniel.Schertzer@cereve.enpc.fr
AF: ENPC, 6-8, avenue Blaise Pascal,
Cité Descartes, MARNE-LA-VALLE, 77455, France
AB:
Using state of the art drop sonde data (from 237 sondes over the Pacific) we examine two classical and
fundamental idealizations of atmospheric science showing that they are untenable in the light of the vertical
structure.
The first is the notion of stable atmospheric layers. This is used for understanding atmospheric dynamics and
thermodynamics, including notions such as potential vorticity. Using the drop sonde data, we show that each
apparently stable layer is actually composed of a hierarchy of unstable layers themselves with embedded stable
sublayers, each with unstable sub-sub layers etc. i.e. in a Russian doll-like fractal hierarchy whose dimension we
estimate. We therefore argue that the notion is untenable and must be replaced by modern scaling notions.
Although the same basic conclusion follows for conditional, dynamical and convective stability, we showed that
their correlation exponent (quantifying their sparsenesses) were 0.36±0.056, 0.22±0.037, 0.15±0.016
respectively.
The second idealization we examine is the turbulence assumption of isotropy. If we include intermittency,
Kolmorogov's landmark proposal that fully developed turbulence has an "inertial subrange" with isotropic energy
spectrum E(k) ≈ k**-β with β≈5/3 has apparently been spectacularly confirmed in both
the horizontal direction and in the time domain (k is a wavenumber). For gradients over a horizontal distance
Δx this implies Δv≈Δz**Hh (Hh=1/3 corresponds to β=5/3; "<.>" indicates ensemble
averaging). Remarkably, Hv for gradients over vertical distances Δz (Δv≈Δz**Hv) has not
been seriously investigated. Using drop sonde data of horizontal wind, we find that from scales of 5 m to >10 km
from the surface layer through to the top of the troposphere, Hv is close to (or larger) than the Bolgiano-Obukhov
value 3/5. Hv>Hh implies that a) the atmosphere becomes progressively less stratified at smaller scales
although in a scaling way; b) that at most a single (roughly) isotropic "sphero-scale" exists (often in the range 1-
100 cm).
DE: 0300 ATMOSPHERIC COMPOSITION AND STRUCTURE
DE: 3379 Turbulence (4490)
DE: 4440 Fractals and multifractals
DE: 4475 Scaling: spatial and temporal (1872, 3270, 4277)
SC: Union [U]
MN: 2007 Fall Meeting