Diabatic ross-isentropic dispersion in the lower stratosphere.


L. C. Sparling, J. A. Kettleborough, P. H. Haynes, and M. E. McIntyre
Centre for Atmospheric Science at the
Department of Applied Mathematics and Theoretical Physics
Cambridge University
J. E. Rosenfield, M. R. Schoeberl, and P. A. Newman
Atmospheric Chemistry and Dynamics Branch,
Code 916, NASA/Goddard Space Flight Center,
Greenbelt, MD 20771
A revised version (NB) has appeared in J. Geophys. Res., 102, 25817-25829 (1997).

Abstract

A significant contribution to vertical dispersion of tracers in the stratosphere arises from the variability in the diabatic heating of air parcels. Air parcels starting on a given isentropic surface experience different time histories of diabatic heating, which causes vertical dispersion across isentropic surfaces. We refer to this process as ``diabatic cross-isentropic dispersion'', or ``diabatic dispersion'' for brevity. The present study investigates diabatic dispersion in the lower stratosphere by computing parcel trajectories initialized uniformly over the 500K surface on 1 Jan 1993. Parcels are followed for two months using analyzed winds and diabatic heating rates computed from analyzed temperatures. Two independent datasets and radiation schemes are used.

Diabatic dispersion depends on the statistics of the large-scale horizontal eddy motion as well as on the spatial structure, be it steady or time varying, of the diabatic heating field. The trajectory statistics suggest that the polar vortex, winter hemisphere surf zone, tropics, and extratropical summer hemisphere are to varying extents isolated from each other by eddy transport barriers. The character and magnitude of the diabatic dispersion for parcels that stay within each of these four regions is distinctly different. The diabatic dispersion in both the surf zone and southern hemisphere extratropics is initially advective, with potential temperature variance (dtheta(t)²) increasing like as time t increases. After about one month, on the 500K isentropic surface, the dispersion becomes diffusive. Strictly this would be better as "quasi-diffusive" in the sense that (dtheta(t)²) ~ 2K_ss t and with a diffusivity K_ss in the range 2-6 K² day^(-1), roughly equivalent to
K_zz ~ 0.1-0.2m² s^(-1) on the 500K isentropic surface. The emergence of a diffusive regime is discussed in terms of loss of memory of diabatic heating along parcel paths, as measured by the decay of the Lagrangian autocorrelation function. Diabatic dispersion within the tropics and polar vortex over the two month period is more than an order of magnitude smaller, and is less clearly diffusive. Some parcels do not remain within any of the four regions defined above, and show entirely different dispersion characteristics. The diabatic dispersion of parcels moving poleward out of the tropics into either hemisphere is faster than either differential advection or diffusion, and is consistent with a transient shear dispersion model in which (dtheta(t)²) increases like . For the total ensemble of all parcels, the potential temperature variance increases like , consistent with global-scale differential advection by the mean diabatic circulation. This is inconsistent, at least on the two-month timescale considered here, with a one-dimensional diffusive model of global-scale vertical diffusive dispersion.


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