Observations of the diurnal propagating solar tide in the mesosphere and lo
wer thermosphere (similar to 50-150 km) indicate substantial annual variati
ons in tidal amplitudes. Observations and modeling efforts suggest that int
eractions with internal gravity waves can result in significant modificatio
ns of the diurnal tide. Herein a two-dimensional (2-D) linear steady-state
tidal model is used in conjunction with hybrid Lindzen/Matsuno gravity wave
parameterization to examine the role of gravity wave interactions in the s
easonal variability of the diurnal tide in the MLT. The analysis indicates
that annual variations of the background atmosphere result in significant a
nnual variations in the eddy diffusion and the diurnal harmonic of the mome
ntum flux divergence (wave stress) produced by breaking gravity waves. The
seasonal variability in these two mechanisms can explain the observed semi-
annual variability in the diurnal tide: amplitude minima at solstice and ma
xima at equinox. The relative roles of wave stress and diffusion are examin
ed and it is shown that both play important roles in tidal modification by
damping its amplitude. The effects of varying inputs to the gravity wave pa
rameterization are explored.