Comparison of Raindrop Size Distribution between NASA’s S-Band Polarimetric Radar and Two-Dimensional Video Disdrometers

The ground-based-radar-derived raindrop size distribution (DSD) parameters—mass-weighted drop diameter D mass and normalized intercept parameter NW —are the sole resource for direct validation of the National Aeronautics and Space Administration (NASA) Global Precipitation Measurement (GPM) mission...

Full description

Saved in:
Bibliographic Details
Published inJournal of applied meteorology and climatology Vol. 59; no. 3; pp. 517 - 533
Main Authors Tokay, Ali, D’Adderio, Leo Pio, Marks, David A., Pippitt, Jason L., Wolff, David B., Petersen, Walter A.
Format Journal Article
LanguageEnglish
Published Goddard Space Flight Center American Meteorological Society 01.03.2020
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary:The ground-based-radar-derived raindrop size distribution (DSD) parameters—mass-weighted drop diameter D mass and normalized intercept parameter NW —are the sole resource for direct validation of the National Aeronautics and Space Administration (NASA) Global Precipitation Measurement (GPM) mission Core Observatory satellite-based retrieved DSD. Both D mass and NW are obtained from radar-measured reflectivity ZH and differential reflectivity Z DR through empirical relationships. This study uses existing relationships that were determined for the GPM ground validation (GV) program and directly compares the NASA S-band polarimetric radar (NPOL) observables of ZH and Z DR and derived D mass and NW with those calculated by two-dimensional video disdrometer (2DVD). The joint NPOL and 2DVD datasets were acquired during three GPM GV field campaigns conducted in eastern Iowa, southern Appalachia, and western Washington State. The comparative study quantifies the level of agreement for ZH , Z DR, D mass, and log(NW ) at an optimum distance (15–40 km) from the radar as well as at distances greater than 60 km from radar and over mountainous terrain. Interestingly, roughly 10%–15% of the NPOL ZH –Z DR pairs were well outside the envelope of 2DVD-estimated ZH –Z DR pairs. The exclusion of these pairs improved the comparisons noticeably.
Bibliography:GSFC
Goddard Space Flight Center
ISSN:1558-8424
1558-8432
1558-8432
1558-8424
DOI:10.1175/JAMC-D-18-0339.1