Abstract

Abstract. It is a challenge to calibrate differential reflectivity ZDR to within 0.1–0.2 dB uncertainty for dual-polarization weather radars that operate 24∕7 throughout the year. During operations, a temperature sensitivity of ZDR larger than 0.2 dB over a temperature range of 10 ∘C has been noted. In order to understand the source of the observed ZDR temperature sensitivity, over 2000 dedicated solar box scans, two-dimensional scans of 5∘ azimuth by 8∘ elevation that encompass the solar disk, were made in 2018 from which horizontal (H) and vertical (V) pseudo antenna patterns are calculated. This assessment is carried out using data from the Hohenpeißenberg research radar which is identical to the 17 operational radar systems of the German Meteorological Service (Deutscher Wetterdienst, DWD). ZDR antenna patterns are calculated from the H and V patterns which reveal that the ZDR bias is temperature dependent, changing about 0.2 dB over a 12 ∘C temperature range. One-point-calibration results, where a test signal is injected into the antenna cross-guide coupler outside the receiver box or into the low-noise amplifiers (LNAs), reveal only a very weak differential temperature sensitivity (<0.02 dB) of the receiver electronics. Thus, the observed temperature sensitivity is attributed to the antenna assembly. This is in agreement with the NCAR (National Center for Atmospheric Research) S-Pol (S-band polarimetric radar) system, where the primary ZDR temperature sensitivity is also related to the antenna assembly (Hubbert, 2017). Solar power measurements from a Canadian calibration observatory are used to compute the antenna gain and to validate the results with the operational DWD monitoring results. The derived gain values agree very well with the gain estimate of the antenna manufacturer. The antenna gain shows a quasi-linear dependence on temperature with different slopes for the H and V channels. There is a 0.6 dB decrease in gain for a 10 ∘C temperature increase, which directly relates to a bias in the radar reflectivity factor Z which has not been not accounted for previously. The operational methods used to monitor and calibrate ZDR for the polarimetric DWD C-band weather radar network are discussed. The prime sources for calibrating and monitoring ZDR are birdbath scans, which are executed every 5 min, and the analysis of solar spikes that occur during operational scanning. Using an automated ZDR calibration procedure on a diurnal timescale, we are able to keep ZDR bias within the target uncertainty of ±0.1 dB. This is demonstrated for data from the DWD radar network comprising over 87 years of cumulative dual-polarization radar operations.

Highlights

  • Dual-polarization weather radars have become the standard in European weather radar networks

  • One-point-calibration results, where a test signal is injected into the antenna crossguide coupler outside the receiver box or into the low-noise amplifiers (LNAs), reveal only a very weak differential temperature sensitivity (< 0.02 dB) of the receiver electronics

  • This is in agreement with the NCAR (National Center for Atmospheric Research) S-Pol (S-band polarimetric radar) system, where the primary ZDR temperature sensitivity is related to the antenna assembly (Hubbert, 2017)

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Summary

Introduction

Dual-polarization (dualpol) weather radars have become the standard in European weather radar networks. In Hubbert (2017) systematic ZDR temperature dependence was found using an analysis of solar scan data, cross-polar measurements and transmit power monitoring. The diurnal variation in solar differential power S is used to assess the operational ZDR monitoring results from birdbath scans and S measurements derived from solar interferences extracted from operational data This analysis is complemented with results from continuous onepoint-calibration data, where a test signal is injected either in the antenna coupler (before the TR limiter) or just before the low-noise amplifier (LNA) by using a built-in test signal generator (TSG). The S temperature dependence is investigated in terms of antenna gain which is determined from solar power measurements at the C-band (Sirmans and Urell, 2001) This provides an insight into how well the two receiver chains are calibrated.

Operational ZDR adjustment
Solar box scans
Analysis of pseudo ZDR antenna patterns
Antenna gain based on solar power measurements
Temperature dependence of differential solar power S and gain g
Long-term ZDR monitoring in the DWD weather radar network
Examples of antenna gain retrievals from the radar network
10 Summary and conclusions
Findings
Jul 2018
Full Text
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