Recently, additional ozone production mechanisms have been proposed to
resolve the ozone deficit problem, which arises from greater ozone de
struction than production in several photochemical models of the upper
stratosphere and lower mesosphere. A detailed ozone model budget anal
ysis was performed with simultaneous observations of O-3, HCl, H2O, CH
4, NO, and NO2 from the Halogen Occultation Experiment (HALOE) an the
Upper Atmosphere Research Satellite (UARS) under conditions with the s
trongest photochemical control of ozone. The results indicate that an
ozone deficit may not exist. On the contrary, the use of currently rec
ommended photochemical parameters leads to insufficient ozone destruct
ion in the model.