Hydrometeor Identification Using GMI Passive Microwave Brightness Temperatures

Author:

Cecil Daniel J.1,Solomon Michael B.2,Mecikalski Retha2,Leppert Kenneth D.3

Affiliation:

1. a NASA Marshall Space Flight Center, Huntsville, Alabama

2. b University of Alabama in Huntsville, Huntsville, Alabama

3. c University of Louisiana Monroe, Monroe, Louisiana

Abstract

Abstract Using passive microwave brightness temperatures Tb from the Global Precipitation Measurement (GPM) Microwave Imager (GMI) and hydrometeor identification (HID) data from dual-polarization ground radars, empirical lookup tables are developed for a multifrequency estimation of the likelihood a precipitation column includes certain hydrometeor types, as a function of Tb. Eight years of collocated Tb and HID data from the GPM Validation Network are used for development and testing of the GMI-based HID retrieval, with 2015–20 used for training and 2021–22 used for testing the GMI-based HID retrieval. The occurrence of profiles with hail and graupel are both slightly underpredicted by the lookup tables, but the percentage of profiles predicted is highly correlated with the percentage observed (0.98 correlation coefficient for hail and 0.99 for graupel). By having snow appear before rain in the hierarchy, the sample size for rain, without ice aloft, is fairly small, and the percentage of rain profiles is less than snow for all Tb.

Funder

Earth Sciences Division

Publisher

American Meteorological Society

Reference25 articles.

1. Constructing a multifrequency passive microwave hail retrieval and climatology in the GPM domain;Bang, S. D.,2019

2. Berg, W., 2022: GPM GMI common calibrated brightness temperatures collocated L1C 1.5 hours 13 km, v07. Goddard Earth Sciences Data and Information Services Center (GES DISC), accessed 10 September 2023, https://doi.org/10.5067/GPM/GMI/GPM/1C/07.

3. Passive microwave brightness temperatures as proxies for hailstorms;Cecil, D. J.,2009

4. Toward a global climatology of severe hailstorms as estimated by satellite passive microwave imagers;Cecil, D. J.,2012

5. Polarization-corrected temperatures for 10-, 19-, 37-, and 89-GHz passive microwave frequencies;Cecil, D. J.,2018

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