D. Osullivan et Tj. Dunkerton, SEASONAL DEVELOPMENT OF THE EXTRATROPICAL QBO IN A NUMERICAL-MODEL OFTHE MIDDLE ATMOSPHERE, Journal of the atmospheric sciences, 51(24), 1994, pp. 3706-3721
The seasonal (wintertime) development of middle atmosphere circulation
in opposite phases of the equatorial quasi-biennial oscillation (QBO)
was simulated with a three-dimensional nonlinear numerical model. In
the stratosphere, the effect of equatorial QBO was generally consisten
t with the extratropical QBO observed by Holton and Tan, namely, a str
onger midwinter polar vortex in the westerly phase, and vice versa. Ho
wever, the extratropical response to the QBO was sensitive to other fa
ctors such as mesospheric gravity wave drag and the amplitude of Rossb
y waves specified at the model's lower boundary. The extratropical QBO
was realistic only when a drag parameterization was included and Ross
by wave amplitudes lay in an intermediate range close to the observed.
At somewhat stronger forcing, the model's response was largest in the
mesosphere where (in this case) westerlies were stronger in the easte
rly phase of equatorial QBO. This was apparently due to a shielding ef
fect. The theory of planetary wave-mean flow interaction suggests that
the sensitivity to equatorial QBO should be greatest for wave forcing
s near a ''bifurcation'' point. Below this threshold the stratosphere
approaches radiative equilibrium, shutting off vertical propagation of
planetary waves. Supercritical forcing leads to a major warming. The
model's sensitivity to forcing, while consistent with this idea, was m
ost apparent in perpetual solstice runs without parameterized wave dra
g. Seasonal integrations with wave drag produced a more realistic extr
atropical QBO, making the bifurcation less conspicuous.