Recent satellite and radar observations suggest that the semiannual oscilla
tion (SAO) in the mesosphere is modulated by the stratospheric quasibiennia
l oscillation (QBO). The modulation is only apparent during the SAO easterl
y phase, which is considerably stronger when QBO winds are westerly than wh
en they are easterly. We use an equatorial beta-plane model to demonstrate
how such a modulation could come about through selective damping of the equ
atorial wave spectrum excited by deep convection. The waves affected most s
trongly are easterly inertia-gravity waves of phase speeds slower than simi
lar to -40 m s(-1). This is close to the zonal wind speed during the easter
ly phase of the QBO (-30 to -35 m s(-1)), so the waves suffer strong therma
l damping or even absorption as they propagate through the stratosphere. Be
cause these waves are important for driving the easterly phase of the mesop
ause SAO in the model, that phase is weaker when the stratospheric QBO wind
s are easterly. A similar modulation of the westerly phase of the SAO does
not occur for two reasons: (I) QBO westerlies are only half as strong as QB
O easterlies, and (2) much of the driving of the westerly phase of the SAO
is accomplished by Kelvin waves of phase speed similar to 40-60 m s(-1). As
a consequence, the QBO winds have negligible influence on the vertical pro
pagation of waves with westerly phase velocity and hence on the westerly ph
ase of the modeled SAG.