Latitudinally and Seasonally Dependent Zenith-Angle Corrections for Geostationary Satellite IR Brightness Temperatures

Abstract

The equivalent brightness temperature Tb recorded by geosynchronous infrared (geo-IR) ?window? channel (10.7?11.5 ?m) satellite sensors is shown to depend on the zenith angle (local angle from the zenith to the satellite for a pixel?s ground location) in addition to the mix of clouds and surface that would be observed from a direct overhead viewpoint (nadir view). This zenith-angle dependence is characterized, and two corrections are developed from a collection of half-hourly geo-IR pixel data that have been parallax corrected and averaged to a 0.5° ? 0.5° latitude/longitude grid for each geosynchronous satellite separately. First, composites of collocated Tb over tropical regions from the Geostationary Operational Environmental Satellite (GOES)-8/GOES-10 and the Meteosat-5/Meteosat-7 satellite pairs are used to produce robust estimates of isotropic zenith-angle corrections as a function of zenith angle and grid-box-averaged Tb. The corrections range from zero for a zenith angle of ?26.5° to increases of more than 20 K at Tb = 230 K near the limb. Near-limb corrections in clear and very cold thick overcast conditions are smaller but are still positive. This empirical result depends on the surface?tropopause temperature differences, so a second correction was developed. Using collocations from the same two satellite pairs from 60°N to 60°S, differences in uncorrected Tb divided by differences in the corresponding corrected values were accumulated as a function of latitude and season. The resultant ratios smoothly vary from ?1 in the Tropics to ?0.5 at 60°N and 60°S, with a quicker decrease in the winter hemisphere. In comparison with the uncorrected geo-IR data, there is a 50% reduction in the root-mean-square differences between collocated values from adjacent satellites by applying the latitude/season-adjusted zenith-angle corrections. Histograms of corrected geo-IR Tb at large zenith angles closely match histograms from collocated near-nadir-view values. Residual difference maps are smooth and indicate intersatellite differences.