Atmospheric tides perturb the temperature, winds, density, and composition
of the mesosphere and lower thermosphere (MLT) and therefore affect daytime
O-2 atmospheric band airglow. O-2 atmospheric band dayglow measurements ma
de by the High Resolution Doppler Imager (HRDI) show clear tidal signatures
in equatorial emission rates during equinox, when diurnal tide amplitudes
are large. During solstice the observed symmetric diurnal variation of dayg
low indicates an emission process controlled by solar absorption. Observati
ons are compared with modeled emissions based on an atmosphere perturbed wi
th diurnal tides predicted by the Tuned Mechanistic Tidal Model (TMTM) for
March 1993. Good data/model agreement indicates enhanced emissions result f
rom tidal advection of atomic oxygen from the lower thermosphere. While tid
es modulate O-2 nightglow by perturbing atomic oxygen recombination rates,
the tidal signatures seen in 02 dayplow are due to increased production of
ozone and O(D-1). These results provide further confirmation of the consist
ency of the HRDI daytime wind, temperature and airglow observations.