The two-day wave is observed in the Upper Atmosphere Research Satellite Mic
rowave Limb Sounder temperature data around 40-58 km. Between December 1991
and September 1994, the two-day wave temperature signature is most signifi
cant after each solstice when the derived easterly winds near the stratopau
se extend across the equator to at least 20 degrees latitude in the winter
hemisphere, and the zonal mean winds near the equator are inertially unstab
le with observed inertial instability disturbances. The observed two-day wa
ve consists of a 2.0-day period zonal wavenumber-3 and a 1.8-day period zon
al wavenumber-4 component, named (3, 2.0) and (4, 1.8), respectively. The (
3, 2.0) component is dominant during two of the three available austral sum
mers, but its amplitude is much weaker than the (4, 1.8) component during t
he two observed boreal summers.
During the austral summers, correspondence between amplification of the two
-day wave temperature signatures, regions of reversed potential vorticity g
radient due to meridional curvature of the zonal mean flow, and the critica
l lines for the (3, 2.0) and (4, 1.8) modes suggest barotropic instability
as a source of both wave components. Momentum redistribution by observed in
ertial instability appears to barotropically destabilize the equatorward fl
ank of the easterly jet where the wave components subsequently grow. During
the boreal summers, the (4, 1.8) component appears to be excited by instab
ility that is associated with vertical shear and curvature of the flow seat
ed above the observational domain. The boreal (3, 2.0) mode appears unrelat
ed to the zonal flow instability within the observational domain and may re
flect a normal-mode-like response during these periods.