Cloud and Aerosol Distributions From SAGE III/ISS Observations
M. R. Schoeberl, E. J. Jensen, Tao Wang, Ghassan Taha, Rei Ueyama, Yi Wang, M. T. DeLand, A. E. Dessler
Abstract
Abstract We describe our Solar Aerosol and Gas Experiment (SAGE) III/ISS cloud detection algorithm and observations. We identify three types of clouds: visible cirrus (extinction coefficient > 3 x 10 −2 km −1 ), subvisible cirrus (extinction coefficient between 3 x 10 −2 km −1 and 10 −3 km −1 ), and very low extinction cloud‐aerosol mixtures (extinction coefficient between 10 −3 km −1 and 10 −4 km −1 ). Visible cirrus cannot be quantitatively measured by SAGE because of its high extinction, but we infer the presence of cirrus through the termination of the SAGE vertical scan. We then assume that cirrus layers extend 0.5 km below the scan termination height. SAGE cirrus cloud fraction estimated in this way is in qualitative agreement with Cloud‐Aerosol Lidar with Orthogonal Polarization (CALIOP) measurements. Analyzing 2018–2020 SAGE III/ISS data, we find that visible cirrus and subvisible cirrus have nearly equal abundance in the tropical upper troposphere and the average cloud fraction is about 25%. At 16 km, the highest concentration of visible cirrus and subvisible cirrus is over the Tropical West Pacific, central Africa, and central South America during boreal winter. Latitudinal gaps in zonal mean cloud fraction are aligned with descending branch of the residual mean circulation. Using tropopause relative coordinates, we show that maximum cloud‐top heights are consistently restricted to a narrow region near the tropopause. The aerosol extinction fields also show the latitudinal gaps coincident with the descending residual circulation. We identify four anomalous aerosol extinction periods that can be tentatively assigned to significant volcanic or fire events.