Observations from three optical ground stations and the wind imaging interf
erometer on the upper atmosphere research satellite have been combined to d
escribe a "springtime transition" in atomic oxygen. At each station the tra
nsition is characterized by a rapid 2-day rise in the night-time oxygen air
glow emission rate by a factor of between 2 and 3, with a subsequent decrea
se by a factor of about 10 in the same period of time. This latter state of
extremely weak oxygen airglow indicates a depletion of atomic oxygen that
persists for many days. The characteristic signature is similar at both mid
-latitude and high-latitude stations and is also observed in the hydroxyl a
i;glow, except that immediately following the enhancement, the hydroxyl emi
ssion rate does not fall below the value it had before the event. Airglow r
otational temperatures behave coherently with the emission rate. WINDII dat
a show that the airglow emission rate perturbation is a planetary scale fea
ture associated with strong vertical motions and that the event may be asso
ciated with the winter-to-summer zonal wind reversal. Data from the norther
n springtimes of 1992 and 1993 are reported upon in detail, with additional
data from 1995 to confirm the persistence: of the phenomenon.