Library of rough hailstone backscattering coefficients at 2.8 GHz

Abstract The rough hailstone scattering library is created to fill the need for results of non-spheroidal hailstone backscattering characteristics. The listed backscattering coefficients at the S-band (2.8 GHZ) are specifically tailored for computing the polarimetric variables. The National Weather...

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Main Authors: Djordje Mirkovic, Dusan S. Zrnic
Format: Article
Language:English
Published: Nature Portfolio 2023-07-01
Series:Scientific Data
Online Access:https://doi.org/10.1038/s41597-023-02352-3
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author Djordje Mirkovic
Dusan S. Zrnic
author_facet Djordje Mirkovic
Dusan S. Zrnic
author_sort Djordje Mirkovic
collection DOAJ
description Abstract The rough hailstone scattering library is created to fill the need for results of non-spheroidal hailstone backscattering characteristics. The listed backscattering coefficients at the S-band (2.8 GHZ) are specifically tailored for computing the polarimetric variables. The National Weather Service’s radar operates in this band; hence the library is pertinent to those studying hail in the USA. The library contains several axis ratios and a range of hail sizes from 5 mm to 100 mm. Moreover, hailstone surface roughness is expressed as a percentage of the equatorial diameter. Our computational electromagnetic approach to modeling hailstones is compared with typically employed simpler methods. The polarimetric variables calculated using our models can be compared to observations. Furthermore, we illustrate the potency of the CEM approach to hydrometeors with extreme axis ratios for which simpler methods (i.e., the T-matrix) fail.
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spelling doaj.art-3775ddf475f94604b4721d38dec21f762023-07-16T11:09:07ZengNature PortfolioScientific Data2052-44632023-07-011011710.1038/s41597-023-02352-3Library of rough hailstone backscattering coefficients at 2.8 GHzDjordje Mirkovic0Dusan S. Zrnic1Cooperative Institute for Severe and High-Impact Weather Research and Operations (CIWRO)National Severe Storms Laboratory/NOAA (OAR)Abstract The rough hailstone scattering library is created to fill the need for results of non-spheroidal hailstone backscattering characteristics. The listed backscattering coefficients at the S-band (2.8 GHZ) are specifically tailored for computing the polarimetric variables. The National Weather Service’s radar operates in this band; hence the library is pertinent to those studying hail in the USA. The library contains several axis ratios and a range of hail sizes from 5 mm to 100 mm. Moreover, hailstone surface roughness is expressed as a percentage of the equatorial diameter. Our computational electromagnetic approach to modeling hailstones is compared with typically employed simpler methods. The polarimetric variables calculated using our models can be compared to observations. Furthermore, we illustrate the potency of the CEM approach to hydrometeors with extreme axis ratios for which simpler methods (i.e., the T-matrix) fail.https://doi.org/10.1038/s41597-023-02352-3
spellingShingle Djordje Mirkovic
Dusan S. Zrnic
Library of rough hailstone backscattering coefficients at 2.8 GHz
Scientific Data
title Library of rough hailstone backscattering coefficients at 2.8 GHz
title_full Library of rough hailstone backscattering coefficients at 2.8 GHz
title_fullStr Library of rough hailstone backscattering coefficients at 2.8 GHz
title_full_unstemmed Library of rough hailstone backscattering coefficients at 2.8 GHz
title_short Library of rough hailstone backscattering coefficients at 2.8 GHz
title_sort library of rough hailstone backscattering coefficients at 2 8 ghz
url https://doi.org/10.1038/s41597-023-02352-3
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