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Last modified
7/28/2009 2:40:53 PM
Creation date
4/24/2008 2:55:57 PM
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Weather Modification
Title
Snow Accumulation Algorithm for the WSR-80D Radar: Second Annual Report
Date
6/1/1997
Weather Modification - Doc Type
Report
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<br />nly 7 percent of the gage observations of figure 3 were greater than 0.050 inch h-1, and the largest value <br />as 0.150 inch h-1. (Of the 1794 hours with detectable snowfall along the line of all five gages located <br />est-northeast of Cleveland, only 2 hours exceeded 0.150 inch.) So estimates of the Ze-S relation for <br />s owfall accumulations greater than 0.050 inch h-1 are based on limited sample sizes. Consequently, the <br />r commended Ze-S relation should be used with some caution for heavier snowfalls. <br /> <br /> <br />onsiderable overplotting of data pairs at the lighter hourly accumulations exists on figure 3 because of <br />e highly skewed distribution of the hourly snowfall accumulations. Median hourly accumulations are <br />nly about 0.01 inch for both gages 1 and 2. As discussed by Super and Holroyd (1996), similar median <br />alues were found for all Cleveland and Denver gages. <br /> <br />he average gage-observed and radar-estimated hourly accumulations for the data of figure 3 are the <br />s e, 0.019 inch, as required by the optimization technique. But figure 3 shows that the optimized <br />I' lation results in frequent radar overestimation at light hourly accumulations and frequent <br />u derestimation at heavy accumulations. This feature is common in similar plots for Denver gages, and <br />h s been noted with Ze-R relations as well where R is rainfall (see Smith et al., 1984). At least a partial <br />e planation for this "mismatch" is likely related to the several orders of magnitude differences in <br />pling volume between the radar range bins and the gages (or snow board) used in table 5. <br /> <br /> <br />lthough 1 hour temporal averaging has been used in this analysis, significant spatial variations <br />s metimes likely existed over the volume of a range bin. Assume that during a given hour, a gage <br />h ppened to sample near a spatial maximum, as should occasionally occur. That gage point measurement <br />ould then be markedly greater than the radar's spatial average sampled in the overlying range bin. Such <br />a point would appear on figure 3 as a radar underestimation associated with a high gage measurement. <br />a similar manner, assume that the gage happened to sample near a spatial minimum, markedly less than <br />t e radar's overhead spatial average. This point would appear on figure 3 as a radar overestimate <br />sociated with a light gage measurement. Because of the inherently very large differences in sampling <br />v lumes between the two measurement methods, one cannot be certain of the "true" snowfall. A very <br />d nse gage network over an area larger than a range bin would be required to measure "true" snowfall <br />o the same spatial scale as the radar. But it is usually very difficult to find representative gage sites well- <br />p otected from the wind as discussed by Super and Holroyd (1996). So finding many adequate sites near <br />t one another is impractical in almost all situations. In summary, one cannot be certain whether the <br />a parent "mismatches" of figure 3 are simply caused by the differences in sampling volume of gages and <br />I' dar, or by other factors such as an improper choice of CTF or even limitations in equation (1). <br /> <br /> <br />5 2 SAA Development for Albany <br /> <br />large volunteer network of snow "spotters" were organized and maintained by Albany NWS WFO <br />P rsonnel. The spotters made hourly measurements of SWE and SD in the area around Albany, NY, <br />d ring the 1995-96 winter as discussed in section 3.2 of Super and Holroyd (1996). Only that portion <br />o the network expected to receive dry snow (no bright band) was activated for each storm. These data <br />ere carefully reviewed and provided by John Quinlan of the Albany NWS WFO for 12 events with <br />u eful surface data, but one had missing radar data. So useable observations are available from the 11 <br />s ow storms listed in table 6. <br /> <br />16 <br />
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