Two parallel 5-year climate simulations have been carried out to asses
s the effect of changing from an Eulerian to a semi-Langrangian formul
ation of a general circulation model's dynamical core with the physica
l parameterizations unchanged. It has been found that the change in fo
rmulation leads to significant differences in the simulated climates,
both for fields determined mainly by the dynamics, such as sea level p
ressure, and for those determined mainly by the physics, such as preci
pitation. The differences result both directly from the changes in the
dynamics and indirectly from the interactions of the dynamics with th
e physics. Compared to the simulation with the Eulerian model, the pri
ncipal improvement with the semi-Lagrangian model is a significant red
uction in, or even elimination of, the cold bias in the polar upper tr
oposphere and lower stratosphere in both hemispheres. This improvement
is evident in both the winter and summer seasons. It results from the
more efficient poleward heat transport in the semi-Lagrangian model.
The effect on other simulated fields can give results either closer to
or farther from the corresponding analyses and observations. The phys
ical parameterizations used in the semi-Lagrangian model have been dev
eloped and tuned for the Eulerian model. To optimize the performance o
f the semi-Lagrangian model, it will be necessary to tune the physical
parameterizations explicitly for this mode.