THE MIDDLE ATMOSPHERIC RESPONSE TO SHORT AND LONG-TERM SOLAR UV VARIATIONS - ANALYSIS OF OBSERVATIONS AND 2D MODEL RESULTS

We have investigated the middle atmospheric response to the 27-day and 11-yr solar UV flux variations at low to middle latitudes using a two -dimensional photochemical model, The model reproduced most features o f the observed 27-day sensitivity and phase lag of the profile ozone r esponse in the upper stratosphere and lower mesosphere, with a maximum sensitivity of +0.51% per 1% change in 205 nm flux. The model also re produced the observed transition to a negative phase lag above 2 mb, r eflecting the increasing importance with height of the solar modulated HOx, chemistry on the ozone response above 45 km. The model revealed the general anti-correlation of ozone and solar UV at 65-75 km, and si mulated strong UV responses of water vapor and HO, species in the meso sphere. Consistent with previous 1D model studies, the observed upper mesospheric positive ozone response averaged over +/-40 degrees was si mulated only when the model water vapor concentrations above 75 km wer e significantly reduced relative to current observations. Including th e observed temperature-UV response in the model to account for tempera ture-chemistry feedback improved the model agreement with observations in the middle mesosphere, but did not improve the overall agreement a bove 75 km or in the stratosphere for all time periods considered. Con sistent with the short photochemical time scales in the upper stratosp here, the model computed ozone-UV sensitivity was similar for the 27-d ay and 11-yr variations in this region. However, unlike the 27-day var iation, the model simulation of the 11-yr solar cycle revealed a posit ive ozone-UV response throughout the mesosphere due to the large deple tion of water vapor and reduced HOx-UV sensitivity. A small negative o zone response at 65-75 km was obtained in the 11-yr simulation when te mperature-chemistry feedback was included. In agreement with observati ons, the model computed a low to middle latitude total ozone phase lag of +3 days and a sensitivity of +0.077% per 1% change in 205 nm flux for the 27-day solar variation, and a total ozone sensitivity of +0.27 % for the 11-yr solar cycle. This factor of 3 sensitivity difference i s indicative of the photochemical time constant for ozone in the lower stratosphere which is comparable to the 27-day solar rotation period but is much shorter than the 11-yr solar cycle.