Differential Reflectivity (Zdr) is a residual of two large quantities of limited absolute accuracy. The accuracies of the larger quantitiies (the H and V polarized system-derived reflectivities) is a function of system calibration and signal statistics. If the H and V reflectivity calibrations are stable, there is likely to be a bias in Zdr due to the inaccuracies of those reflectivity calibrations; under such circumstances, it is possible to apply a bias correction to Zdr, even if there is a relatively large uncertainty in the absolute calibration of the H and V subsystems.
Note that high accuracy in Zdr is desired when Zdr is applied to precipitation accumulation estimates. For precipitation estimates, a change of 0.3 dB in Zdr will result in a 17% change in estimated accumulation (as estimated from typical Z/Zdr algorithms).
Since S-Pol is a research radar system, particular attention is given to ensuring the accuracy of all parameters. Every effort is made to minimize the error in Zdr, with the goal of obtaining accuracies of .1 dB, or better.For IHOP_2002, analysis indicates that there was a bias of -.08 dB in Zdr, and that this bias was stable throughout the field experiment. Variations in the bias estimate were small, on the order of .02 dB.
In light of the bias and the stability of that bias, ATD applied a bias correction of +.08 dB to Zdr for the entire period of the IHOP_2002 experiment. Details of the techniques used and individual bias analyses are provided.
To estimate Zdr bias, we require a well-characterized, non-biased, system-independent data set for analysis. Such a data set can be obtained from viewing rainfall at vertical incidence.
For purposes of Zdr bias estimation, there is no consistent axial asymmetry in raindrop shape when viewed from directly below. In the case of a strongly sheared environment, there might arguably be preferential orientation of a collection of hydrometeors. Fortunately, preferential orientation effects can be reliably removed by rotating the vertically pointing antenna in azimuth and averaging results over several rotations. It may also be surmised that ice crystals can serve for bias determination; experience with frozen hydrometeors shows that this is indeed the case, but that there is somewhat greater variablility in results (larger standard deviation in the Zdr spectrum, and somewhat greater variability introduced into the inter-case mean).
Antenna rotation is important for a second reason: neutralization of side-lobe effects. The antenna 90-degree side lobes can show a significant bias in Zdr when the antenna is pointed vertically. This bias is typically evident at a certain azimuth, and typically shows a repetition pattern with a 45 or 90 degree azimuthal periodicity (periodicity is dependent upon feedhorn strut location, as evidenced in the radar's antenna pattern). Under the best circumstances, rotation of the antenna, combined with sufficient averaging time (i.e., number of rotations), cancels out bias due to clutter. (For documentation of S-Pol 90° sidelobes, see S-Pol Sidelobe Artifacts)
Every attempt is made to process appropriate cases in a very consistent way. Vertical-pointing scans are transferred to a data processing system. A script is used to drive the SOLO analysis package, performing parameter thresholding and general data selection, on through production of a histogram of Zdr values for qualifying data. The only operator interaction is in the definition of a broad boundary in order to time-window the data and to eliminate obvious artifacts.
Table 1 summarizes the automatic thresholding criteria applied to vertical pointing data. Note that original criteria used in the field during TRMM-LBA were different from the criteria detailed in the table. These modifications were made to bring procedure into conformance with enhancements introduced during MAP (Sep/Oct 1999). For TRMM-LBA, there is no substantive difference between early Zdr bias estimates and current Zdr bias estimates.
In Table 1, if two conditions are shown for the same threshold parameter, the more restrictive condition is used. In most cases, when two conditions are listed, the second condition indicates criteria that are specific to S-Pol, and may be adjusted for other radars or other S-Pol projects.
Description | Exclusion Condition | Reason |
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eliminate data when received power is too high | DM > -45.0 dBm | avoid regions of non-linear receiver response |
DM > -70.0 dBm | restrict data to a portion of receiver response that is most likely to be used during operational data collection; this limit is dictated in part by S-Pol automatic gain control (AGC) | |
eliminate data in regions of weak signal | DM < -105 dBm (flexible criteria) | limit variablity due to poor signal statistics |
eliminate bright band and regions of wet hydrometeors | LDR > -13.0 dB | Zdr can have a very wide distribution in these regions |
avoid regions close to radar | range < 1.2 km | eliminates regions of TR tube recovery, and selects data in far-field, only |
range < 3.0 km | eliminates regions of differential TR tube recovery, a special issue for the S-Pol receiver configuration | |
remove data above the atmosphere | range > 14.0 km | also eliminates inadvertant inclusion of S-Pol test pulse |
For IHOP_2002, only 5 separate events of vertical pointing were logged. Of these, one was considered to be unsuitable for use. Within the 5 events, subsets were occasionally deliniated and processed separately. These subsets provide an indicator of the short-term consistency of the procedure and results. All events are listed in Table 2. Each independent event is separated by a horizontal line; within each event, any subsets are shown on their own line. For determination of gross conclusions, subsets are first combined to provide a single set of event values. Within the table, links are provided to images of the data (time section of received power, DM, and Zdr, both raw and thresholded: ZDR or TZDR, respectively), or the histogram produced in the analysis.
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020524 | 0122 |
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