In the stratosphere the relaxation times for transport and ozone photochemistry in a n oxygen-hydrogen-nitrogen system are approximately comparable. Therefore, realistic models used to calculate ozone variations need to be based on the interaction of t h e photochemistry and dynamics in this region.The model used in the present study is the three-dimensional global circulation model developed at the National Center for Atmospheric Research. The photochemical calculations for ozone are carried out as time dependent in a three-dimensional 0-H-N system.The dynamic model is started from an atmosphere initially at rest and then spun up t o a steady state circulation corresponding to mid-January. An initial observed ozone distribution is added and the model is then run through 30 simulated days. Analysis of t h e time variation of the ozone distribution shows that photochemistry dominates the ozone changes in the sub-solar middle stratosphere, and transport processes redistribute t h e ozone poleward and downward into the troposphere. Although the general pattern of ozone changes seem to be correct, the model produces too much ozone in the Southern hemisphere subtropical stratosphere and transports too much ozone into the Northern subtropical troposphere. The conlputed lower boundary flux of about 5 X 10'' cm-' s-' corresponds quite well to estimates given in the literature.Dans la stratosphtre, les temps de relaxation de transport et la photochimie de l'ozone dans un systkme oxygene-hydrogtne-azote sont approximativement comparables. P a r consequent, des modeles rtalistes utilists pour calculer les variations d e l'ozone se doivent d'Ctre basCs sur I'interaction de 121 photochimie et de la dynamique dans cette rCgion.Le modtle utilist dans 1'Ctude actuelle est le modtle tridimensionnel de circulation globale, dCveloppC au Centre National de Recherches AtmosphCriques. Les calculs photochimiques pour l'ozone sont effectuCs comme dCpendant du temps dans le systkme tri-