A ground-based and rocket investigation of the response of the neutral
atmosphere to E region auroral heating has been carried out at Poker
Flat, Alaska. The temporal evolution of the atomic oxygen to molecular
nitrogen ratio (O/N-2) in the lower thermosphere has been monitored u
sing the optical emissions from the aurora as a diagnostic. Comparison
s between the changes in the O/N-2 ratio and the auroral Joule and par
ticle heating have shown several examples of close similarity between
the durations of the heating events and the depletions. Using the ther
mospheric winds measured during the rocket flights and the temporal st
ructure of the depletions, the upper limit on the horizontal scale siz
e of the depletions has been estimated at 200-400 km. Moreover, in sit
u rocket measurements of atomic oxygen showed significant differences
at points separated horizontally by approximately 220 km. It is also c
oncluded from the near coincidence between the depletion events and th
e Joule heating events that the dynamical mechanism(s) that drive the
depletions were not far distant from the observing site, that is, loca
l processes are sometimes dominant during periods of moderate auroral
activity. We suggest that the observation of a strong wind shear in th
e 100- to 120-km altitude region [Larsen et al., 1997] could be respon
sible for turbulence that contributes to the changes in minor constitu
ent composition.