J.
D. Farrara, Y. -J. Kim and C. R. Mechoso, 1997
(Preprints, 7th Conference on Climate Variations, 2-7 February, 1997, Long Beach,
CA, Amer. Meteor. Soc., pp 21-26)
ABSTRACT
This paper discusses aspects of an atmospheric general circulation model (AGCM)
whose improvement can have a significant beneficial impact in the simulation
of the climatology and interannual variability in the stratosphere. The work
is based on the tropospheric-stratospheric version of the UCLA AGCM (top at
1 mb) with both low (5 deg lon. x 4 deg lat.) and high (2.5 deg lon. x 2 deg
lat.) horizontal resolution. The model is the most recent version we use in
climate studies.
We start by contrasting decade-long simulations obtained using distributions
of ozone mixing ratio that are either prescribed (according to an observed climatology)
or predicted (according to a highly simplified photochemistry). Our results
show that errors in predicted ozone in the upper troposphere/lower stratosphere
can result in large cold biases at these levels and unrealistically strong stratospheric
jets. With ozone predicted the simulated zonal mean circulation is much improved.
Next, we focus on updates in the parameterization of shortwave radiative heating.
Specifically, we updated the calculation of the absorption cross-sections for
water vapor and ozone. Again, the results of several simulations for the Northern
Hemisphere winter show significant improvements in the middle and upper stratosphere.
Finally, we consider processes that do not directly affect the stratosphere.
One of these processes concerns the incorporation of vertical mixing of momentum
by dry convective adjustment processes. The other refers to the retention or
elimination of small scales in the depth of the planetary boundary layer predicted
by the AGCM. The results of several simulations for the northern winter show
that these model changes have a relatively minor impact on the troposphere,
but a substantial effect on the stratosphere.
Our results emphasize that the performance of an AGCM in the stratosphere can
depend on several model aspects, and that this dependence can be straightforward
in some cases but subtle in some other cases. We will describe our new results
and the effect that an improved simulation of the seasonal cycle in the stratosphere
can result in improvement of the interannual variability in that region.