STRATOSPHERIC AEROSOL OPTICAL DEPTH OBSERVED BY THE STRATOSPHERIC AEROSOL AND GAS EXPERIMENT .2. DECAY OF THE EL-CHICHON AND RUIZ VOLCANIC PERTURBATIONS

The decay of the El Chichon perturbation to the optical depth of stratospheric aerosols at 1.02-mu-m, 0.525-mu-m, and 0.453-mu-m is calculated from the Stratospheric Aerosol and Gas Experiment II (SAGE II) data set for the period December 1984 to December 1988. It is found that the perturbed optical depths at middle and higher latitudes of both hemispheres exhibited an exponential decay superimposed by a seasonal oscillation with maximum and minimum occurring in local winter and local summer, respectively. Microphysical processes and variation of the tropopause height alone cannot explain this seasonal change of optical depth. The magnitudes of the exponential component at higher latitudes were, in general, larger than those at lower latitudes. For optical depths in tropical regions, the seasonal oscillations were small and were disturbed by the eruption of Nevado del Ruiz on November 13, 1985. The increase in ratio of optical depth at 0.525-mu-m to that at 1.02-mu-m from about 2.0 at the beginning of 1985 to about 3.5 at the end of 1988 indicates the average size of aerosol particles in the stratosphere is diminishing since the eruption of El Chichon. The 1/e folding time for El Chichon decay derived from the SAGE II data set is in reasonably good agreement with those derived by other methods.