2000
DOI: 10.1029/2000jd900529
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On satellite scatterometer model functions

Abstract: Abstract. Satellite scatterometer model functions are the empirical correlations between observed backscatter and geophysical parameters. One problem is the choice of "surface truth" for the latter. Currently, buoy data and general circulation model surface analyses have been used to establish 10 rn neutrally stratified wind model functions. The correlation between backscatter and surface winds has been the foundation of the scatterometers. The backscatter is anisotropic with respect to wind direction, allowin… Show more

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Cited by 19 publications
(9 citation statements)
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“…The correlation analysis between the coarse grid cells of the scatterometer and, for example, buoy data can suffer from smaller scale gradients within the cells that are averaged out. Furthermore calibration data from buoys and ships may suffer errors due to flow distortion, tilting and displacement (Brown 2000a,b, Atlas et al 2001. Improvements to the current algorithms are ongoing as the global dataset collocated with buoys and model data becomes larger.…”
Section: Satellite Sar and Wind Mapsmentioning
confidence: 99%
“…The correlation analysis between the coarse grid cells of the scatterometer and, for example, buoy data can suffer from smaller scale gradients within the cells that are averaged out. Furthermore calibration data from buoys and ships may suffer errors due to flow distortion, tilting and displacement (Brown 2000a,b, Atlas et al 2001. Improvements to the current algorithms are ongoing as the global dataset collocated with buoys and model data becomes larger.…”
Section: Satellite Sar and Wind Mapsmentioning
confidence: 99%
“…These factors generally cause the selected wind flow to appear ''noisy''. For a discussion on GMF inaccuracies and the limitations of the comparison data, see Brown [2000].…”
Section: Introductionmentioning
confidence: 99%
“…A GMF can been written as: σ0=normalGnormalMnormalF|V10s,ϕ,θ,p,λ,SST, where V10s is the stress‐equivalent wind speed at a height of 10 m [ Edson , ; Liu and Tang , ; De Kloe et al ., ], ϕ is the wind direction with respect to the radar range direction, p is the radar emitted and received polarization, θ is the incidence angle, and λ is the radar wavelength [ Wentz et al ., ; Wentz and Smith , ; Brown , ; Gohil et al ., ; Hersbach et al ., ; Ricciardulli and Wentz , ]. Several studies have shown that it is necessary to take SST into account for a Ku‐band GMF, while for C‐band SST effects are much smaller [ Grodsky et al ., ; Bentamy et al ., ; Bentamy et al ., ; Wang et al ., ].…”
Section: Introductionmentioning
confidence: 99%