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Last modified
7/28/2009 2:40:35 PM
Creation date
4/24/2008 2:52:55 PM
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Weather Modification
Title
The Feasibility of Enhancing Streamflow in the Silver Iodide in the Sevier River Basin of Utah bt Seeding Winter Mountain Clouds
Date
12/1/1991
Weather Modification - Doc Type
Report
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<br />effectiveness CUIVe for the type of AgI used, active modes of nucleation and their rates, dispersion of the <br />seeding agent, etc. However, stonns with higher SL W amounts tend to be wanner which compounds the <br />potential problem of providing insufficient ice nuclei. But these wanner, wetter stonns also tend to have <br />embedded convection present Impressions gained during the 1991 field season strongly suggest that <br />convection can transport AgI from even low-level valley generators to altitudes well above the barrier <br />where temperatures may be cold enough for nucleation. <br /> <br />Larger SL W amounts tend to occur with shallow clouds having wann tops that often are inefficient <br />precipitation producers due to a lack of natural ice crystals. Deep clouds with high, cold tops generally <br />produce high concentrations of ice crystals which can settle through the SL W condensate produced near <br />the mountain slopes and convert much of it to snowflakes or graupel. Huggins et al. (1989) showed <br />evidence for this tendency in that mesoscale bands had 2 to 4 times higher precipitation rates than adjacent <br />periods between bands but the latter had greater SL W amounts. This suggests considerable variability in <br />stonn seedability not only from stonn-to-stonn but throughout a stonn passage. Similar variability was <br />shown by Rauber et al. (1986) and Heggli and Rauber (1988). The bands shown by Huggins (~t al. (1989) <br />were only 5 to 15 kIn wide, Similar structure has been shown for winter stonns over the Cascade Range <br />in Washington, the Sierra Nevada of California, and the Mogollon Rim of northern Arizona.. <br /> <br />As discussed earlier, the flux of SL W over the crest of a barrier represents the absolute maximum amount <br />of liquid that seeding could convert to ice crystals. Only a fraction of the ice crystals might reach the <br />surface as additional snowfall. Thus, seeding-induced precipitation will never exceed the SL W flux over <br />a barrier, but will be some fraction of that flux, The specific fraction that can be converted to <br />precipitation would be expected to vary with stonn conditions and seeding effectiveness and is difficult <br />to quantify with present knowledge. <br /> <br />Estimates of SL W flux were made for several Tushar data sets. Rauber and Grant (1987) estimated the <br />amount of SLW passing the crest for a single stonn in February 1983. This was done with rawinsonde <br />wind data for the elevation of the barrier crest and scanning microwave radiometer measurements collected <br />about 20 kIn west of the crest at a much lower elevation. It was necessary to nonnalize the radiometer <br />data to the zenith so the obselVations may not totally represent conditions over the crestline. However, <br />precipitation was very limited so most of the flux should have passed the downwind crestline as excess <br />SL W. The resulting estimate of total SL W flux for a 13-hour period was equivalent to approximately 13 <br />percent of the mean annual runoff from the Beaver River which drains the west slopes of the Tushars (the <br />east slopes drain into the Sevier River).. This case study appeared to have substantial seeding potential. <br /> <br />Long (1986) reported on early 1985 data from the Tushar Mountains, also based on microwave radiometer <br />and rawinsonde windspeed measurements. During this season, the radiometer was at a significantly higher <br />elevation than during 1983, located only about 5 kIn west of the barrier crest. Similar data were presented <br />by Huggins (1990a) for the 1987 field season when the radiometer was located at the same site as in 1985. <br />Liquid water flux estimates for early 1989, given by Huggins (1990b), were again for the west slope <br />radiometer site used the previous two obselVational seasons. <br /> <br />During the above noted Tushar field programs the tenn "stonn" was used to designate a period with <br />significant cloud cover over the research area perceived to have some probability of producing <br />precipitation. As a minimum that meant a broken to overcast mid-level or lower level cloud deck. <br />Research periods coincided with stonn periods. It is of interest to consider a summary of SL W flux <br />estimates for stonn episodes during the 1985, 1987 and 1989 seasons. This provides the beginnings of <br />a "climatology" of possibly seed able events over the Sevier River Basin. While only three relatively short <br />field seasons are involved, actual SL W obselVations are much more relevant to the question of seeding <br /> <br />11 <br />
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