2006
DOI: 10.1029/2006gl027088
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Cloud fraction errors for trade wind cumuli from EOS‐Terra instruments

Abstract: [1] Errors in the standard cloud fraction products produced by the Moderate Resolution Imaging Spectroradiometer (MODIS) and the Multi-angle Imaging SpectroRadiometer (MISR) on EOS-Terra were examined using 15 m resolution data from the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER). Relative to 124 ASTER scenes containing only trade wind cumuli and having an average cloud fraction of 0.08, MODIS and MISR overestimated cloud fraction by 0.18 and 0.36, respectively. For non-sunglint scen… Show more

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Cited by 94 publications
(117 citation statements)
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“…But in some number of cases it is not possible to identify a combination of phase, particle size, and optical thickness consistent with the observed reflectances at multiple wavelengths. This may occur because the pixel has been mis-classified as cloudy, as is common in regions of sun-glint (Zhao and Girolamo, 2006). In the Collection 5 retrievals used here, pixels adjacent to clear sky are also rejected, as these are subject to retrieval biases.…”
Section: Appendix a Measuring Cloud Fractionmentioning
confidence: 99%
“…But in some number of cases it is not possible to identify a combination of phase, particle size, and optical thickness consistent with the observed reflectances at multiple wavelengths. This may occur because the pixel has been mis-classified as cloudy, as is common in regions of sun-glint (Zhao and Girolamo, 2006). In the Collection 5 retrievals used here, pixels adjacent to clear sky are also rejected, as these are subject to retrieval biases.…”
Section: Appendix a Measuring Cloud Fractionmentioning
confidence: 99%
“…As above, large-scale conditions from ERA-40 determine the ISCCP sample of RICO-like conditions during the period of overlap between the data sets (1984)(1985)(1986)(1987)(1988)(1989)(1990)(1991)(1992)(1993)(1994)(1995)(1996)(1997)(1998)(1999)(2000)(2001). Because of the method used to define cloud fraction, it is likely the ISCCP data set overestimates cloud fraction in this regime (Wielicki and Parker 1992;Di Girolamo and Davies 1997;Zhao and Di Girolamo 2006). As discussed above, the diagnosed cloud amounts in GCMs can differ from results using an ISCCP simulator, which was not available for this analysis for three of the GCMs, but this regime is not expected to contain much obscuring high-level cloud, so differences should be minimal.…”
Section: Zoom In On Rico Conditionsmentioning
confidence: 99%
“…For this reason, the highest resolution available from ASTER (15 m) is targeted, while the need for an operationally complete and globally validated cloud detection algorithm is not required at this time. Still, the manually tedious effort to produce scene-by-scene cloud masks for a multitude of different resolutions based on a single (or more) threshold approach (e.g., Welch, 1986, Zhao andDi Girolamo, 2006) is replaced in favor of a hybrid approach. Here, individual cases are selected based on the presence of low-level water clouds over the ocean and the absence of high-level cirrus that impacts the cloud F. Werner et al: ASTER cloud property retrievals 5873 property retrieval (Wind et al, 2010).…”
Section: Cloud Detection For Astermentioning
confidence: 99%
“…All other pixels are identified as clear (cloudiness flag "3"). These thresholds, which comprise the first step in the new cloud masking scheme, were set through inspection of 210 ASTER MBL scenes sampled off the coast of California and the tropical western Atlantic (Zhao and Di Girolamo, 2006) between April 2003 and July 2007. These observations have been performed at full ASTER resolution, keeping in mind that we are siding on a cloud-conservative cloud mask.…”
Section: Cloud Detection For Astermentioning
confidence: 99%
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