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Aerosol retrievals from METEOSAT-8 - CM SAF

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<strong>SAF</strong> on Climate Monitoring Visiting Scientists Report Doc. No: 1.0<br />

Issue : 1.0<br />

Date : 4 October 2006<br />

Appendix C<br />

Clear sky observations and contribution of the temporal<br />

resolution of MSG/SEVIRI<br />

Dominique Jolivet and Didier Ramon (HYGEOS)<br />

&<br />

Jérôme Riedi and Jean-Marc Nicolas (LOA)<br />

The algorithm to separate cloud free <strong>from</strong> cloud contaminated or cloud filled pixels has been<br />

developed with the intention of being applicable globally without requiring ancillary data such as<br />

surface temperature or atmospheric profiles. Each test implemented within the algorithm has been<br />

designed based on fundamental physical differences (emissivity, spectral behaviour) between<br />

clouds and surface.<br />

Many lessons learned <strong>from</strong> the Moderate Resolution Imaging Spectroradiometer (MODIS),<br />

regarding discrimination between clouds and heavy aerosols events or sunglint for instance (spatial<br />

variability, spectral behaviour), have been taken into account in the design of this cloud detection<br />

scheme. However, the present algorithm shall not be considered as just a simplified MODIS-like<br />

cloud mask because : (i) some tests have been adapted and modified to account for the differences<br />

in spectral channels, calibration and/or spatial resolution and make them applicable to SEVIRI, (ii)<br />

the number of tests used is currently much smaller than the one used in the operational MODIS<br />

algorithm (Ackerman et al. 1998; Platnick et al. 2003) and (iii) the decision logic differs<br />

significantly <strong>from</strong> the one used for MODIS (http://www-loa.univ-lille1.fr/~riedi/).<br />

The input to the SEVIRI cloud detection algorithm consists of normalized reflectances <strong>from</strong> the<br />

visible (0.6 and 0.8 µm) and near-infrared (1.6 µm) channels, whereas brightness temperatures are<br />

used <strong>from</strong> the thermal infrared channels (3.8, 8.7, 10.8 and 12.0 µm). Additionally, the algorithm<br />

uses ancillary data on solar and viewing geometry and a land/sea map but none is required <strong>from</strong><br />

model reanalysis. There are spectral threshold and spatial coherence cloud detection tests that are<br />

different for land and ocean surfaces. The various tests implemented are grouped together in such a<br />

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