Abstract
This paper presents the results of a recent flight campaign conducted over the Great Lakes region and reports the first observations of the W-band normalized backscattered cross section ( $\sigma _{0}$ ) for V and H polarization and the linear depolarization ratios (LDRs) from different types of surfaces at moderate incidence angles ( $\sigma _{0}$ behaves as previously reported at small incidence angles, it features a marked decrease with increasing incidence angles between 20° and 50°. There is a strong dependence of normalized backscattered cross sections both on the wind speed and on the wind direction, with larger values found in the presence of higher wind speeds and when the radar antenna is looking upwind. This is in line with theoretical models (though models tend to overpredict the range of variability at a given incidence angle) and with observations at lower frequencies. The LDRs are steadily increasing from values certainly lower than −30 dB, at vertical incidence, to the values of about −10 dB, at the incidence angles of about 60°–70°, with a good matching between observations and theoretical predictions. On the other hand, land surface backscattering properties are not characterized by a strong angular dependence: $\sigma _{0}$ and LDR values typically range between −20 and 0 dB and between −15 and −5 dB, respectively. This paper is relevant for spaceborne concepts of W-band radars, which envisage moderate incidence angles to achieve a broad swath needed for global coverage.
Highlights
Direct observations of the vertical structure of winds are the fundamental observables needed for further advancing numerical weather prediction, [1]
This paper presents the results of a recent flight campaign conducted over the Great Lakes Region and reports the first observations of the W-band normalized backscattered cross section (σ0) for V and H polarization and the Linear Depolarization Ratios (LDR) from different types of surfaces at moderate incidence angles (
There is a strong dependence of normalized backscattered cross sections both on the wind speed and on the wind direction, with larger values found in the presence of higher wind speeds and when the radar antenna is looking up-wind
Summary
Direct observations of the vertical structure of winds are the fundamental observables needed for further advancing numerical weather prediction, [1]. Whilst Doppler-lidar technology is mature, the radar scientific community has been active in the last 5 years in proposing different space-borne Doppler radar system concepts focused at capturing the structure of winds within clouds and precipitating systems. Following previous work based on groundbased observations [3] and space-borne notional studies [4] recent ESA-funded studies have recommended the use of polarization diversity to overcome the range-Doppler dilemma and the short decorrelation times associated with the Doppler fading inherent to millimeter radar systems mounted on fast moving LEO platforms [5]. 1) A conically scanning Dopplerised 94 GHz radar is key to the WIVERN project [6] that aims to provide global in-cloud winds and improve forecasts of hazardous weather. To achieve global coverage an 800 or 1700 km swath is envisaged, so it is important to know the vertical extent of surface returns at 40 to 60◦ incidence angle and how these returns will restrict the minimum height above the surface where winds can be derived. 2) A stereoradar configuration for observing the microphysical and dynamical structures of cloud systems, including disturbed mesoscale convective systems, [7]
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More From: IEEE Transactions on Geoscience and Remote Sensing
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