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Clear‐sky closure studies of lower tropospheric aerosol and water vapor during ACE‐2 using airborne sunphotometer, airborne in‐situ, space‐borne, and ground‐based measurements
Authors:Beat Schmid  John M Livingston  Philip B Russell  Philip A Durkee  Haflidi H Jonsson  Donald R Collins  Richard C Flagan  John H Seinfeld  Santiago Gassó  Dean A Hegg  Elisabeth Öström  Kevin J Noone  Ellsworth J Welton  Kenneth J Voss  Howard R Gordon  Paola Formenti  Meinrat O Andreae
Institution:Bay Area Environmental Research Institute, San Francisco, CA, USA;;SRI International, Menlo Park, CA, USA;;NASA Ames Research Center, Moffett Field, CA, USA;;Naval Postgraduate School, Monterey, CA, USA;;California Institute of Technology, Pasadena, CA, USA;;University of Washington, Seattle, WA, USA;;Meteorological Institute, Stockholm University, Stockholm, Sweden;;University of Miami, Miami, FL, USA;;Max Planck Institute for Chemistry, Mainz, Germany
Abstract:We report on clear‐sky column closure experiments (CLEARCOLUMN) performed in the Canary Islands during the second Aerosol Characterization Experiment (ACE‐2) in June/July 1997. We present CLEARCOLUMN results obtained by combining airborne sunphotometer and in‐situ (optical particle counter, nephelometer, and absorption photometer) measurements taken aboard the Pelican aircraft, space‐borne NOAA/AVHRR data and ground‐based lidar and sunphotometer measurements. During both days discussed here, vertical profiles flown in cloud‐free air masses revealed 3 distinctly different layers: a marine boundary layer (MBL) with varying pollution levels, an elevated dust layer, and a very clean layer between the MBL and the dust layer. A key result of this study is the achievement of closure between extinction or layer aerosol optical depth (AOD) computed from continuous in‐situ aerosol size‐distributions and composition and those measured with the airborne sunphotometer. In the dust, the agreement in layer AOD (λ=380–1060 nm) is 3–8%. In the MBL there is a tendency for the in‐situ results to be slightly lower than the sunphotometer measurements (10–17% at λ=525 nm), but these differences are within the combined error bars of the measurements and computations.
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