Abstract

The Global Precipitation Measurement mission is a major U.S.–Japan joint mission to understand the physics of the Earth’s global precipitation as a key component of its weather, climate, and hydrological systems. The core satellite carries a dual-precipitation radar and an advanced microwave imager which provide measurements to retrieve the drop size distribution (DSD) and rain rates using a Combined Radar-Radiometer Algorithm (CORRA). Our objective is to validate key assumptions and parameterizations in CORRA and enable improved estimation of precipitation products, especially in the middle-to-higher latitudes in both hemispheres. The DSD parameters and statistical relationships between DSD parameters and radar measurements are a central part of the rainfall retrieval algorithm, which is complicated by regimes where DSD measurements are abysmally sparse (over the open ocean). In view of this, we have assembled optical disdrometer datasets gathered by research vessels, ground stations, and aircrafts to simulate radar observables and validate the scattering lookup tables used in CORRA. The joint use of all DSD datasets spans a large range of drop concentrations and characteristic drop diameters. The scaling normalization of DSDs defines an intercept parameter NW, which normalizes the concentrations, and a scaling diameter Dm, which compresses or stretches the diameter coordinate axis. A major finding of this study is that a single relationship between NW and Dm, on average, unifies all datasets included, from stratocumulus to heavier rainfall regimes. A comparison with the NW–Dm relation used as a constraint in versions 6 and 7 of CORRA highlights the scope for improvement of rainfall retrievals for small drops (Dm < 1 mm) and large drops (Dm > 2 mm). The normalized specific attenuation–reflectivity relationships used in the combined algorithm are also found to match well the equivalent relationships derived using DSDs from the three datasets, suggesting that the currently assumed lookup tables are not a major source of uncertainty in the combined algorithm rainfall estimates.

Highlights

  • This suggests that the OceanRain NW –Dm relationship would be an appropriate constraint for global space-borne radar-based precipitation algorithms, such as the Global Precipitation Measurement (GPM) combined algorithm

  • A comparison between the operational NW –Dm relation used as a constraint in versions 6 and 7 of the combined algorithm and the OceanRain relation shows deficiencies in the combined relation for small drops (Dm < 1 mm) and large drops (Dm > 2 mm)

  • The implementation of the OceanRain relation in the combined algorithm is likely to result in more accurate precipitation estimates and a better agreement between the NW –Dm distributions estimated by the combined algorithm and the NW –Dm distributions from the three datasets investigated in this study

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Summary

Introduction

The GPM-dual-precipitation radar (or DPR) and CMB algorithms currently use the legacy standard gamma model for h(x) with one shape parameter, μ, fixed at 2 or 3, which gives a convex down shape for a small x (

Instrumentation and Data Collection
The ‘Intrinsic’ DSD Shape
Figures and
Application to the CMB Algorithm
Findings
Discussion and Summary
Full Text
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