Saharan dust in nighttime thermal imagery: Detection and reduction of related biases in retrieved sea surface temperature

被引:95
作者
Merchant, C. J. [1 ]
Embury, O.
Le Borgne, P.
Bellec, B.
机构
[1] Univ Edinburgh, Inst Atmospher & Environm Sci, Edinburgh, Midlothian, Scotland
[2] Ctr Meteorol Spatiale, Meteo, France
基金
英国自然环境研究理事会;
关键词
Saharan dust; tropospheric aerosol; sea surface temperature; Spinning Enhanced Visible and Infrared Radiometer; thermal remote sensing;
D O I
10.1016/j.rse.2006.03.007
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
Guided by radiative transfer modelling of the effects of Saharan dust (aerosol) on brightness temperatures at 3.9, 8.7, 11 and 12 lam measured by the Spinning Enhanced Visible and Infrared Imager (SEVIRI), we propose an indicator of the presence of Saharan dust in nighttime (infrared-only) SEVIRI imagery. Radiative transfer modelling is performed using a fast atmospheric transmittance model and a delta-Eddington approximation for scattering. Using aerosol single scattering properties appropriate to simulation of Saharan dust gives qualitatively good simulations of dust-affected brightness temperatures. From these simulations, we show that aerosol-free brightness temperatures are tightly clustered around the principal axis (explaining 99% of variance) in a 3-dimensional brightness-temperature difference space (the axes being 3.9 mu m minus 8.7 mu m, 3.9 mu m minus 12 mu m, and 11 mu m minus 12 mu m); in contrast, brightness temperatures affected by aerosol are simulated to be significantly off-axis when transformed into this space. Although the detailed effects of aerosol on brightness temperatures are not quantitatively reproduced by our simulations, this off-axis characteristic is empirically found to be also true of Saharan-dust-affected brightness temperatures in observations. The second principal component of the brightness-temperature difference space is identified as a useful index for Saharan dust. Comparisons with independent satellite measurements of aerosol optical depth (AOD, at 0.55 mu m) show that the new Saharan dust index (SDI) is loosely correlated with AOD (r=0.34). The correlation is loose because the SDI is also sensitive to the height distribution of aerosol, which affects the aerosol's thermal emission. The SDI is used to develop an empirical correction scheme for SST retrievals affected by Saharan dust. Application of the SDI correction scheme removes an independent error of 0.2 K from SEVIRI SSTs validated against buoys from all latitudes. (c) 2006 Elsevier Inc. All rights reserved.
引用
收藏
页码:15 / 30
页数:16
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