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<br />o ('lO2 2!, <br /> <br />4.3 Differences Between Experimental Areas <br /> <br />In most significant respects, the two study areas are similar for purposes of experimentation. <br />Each barrier rises over a kilometer above it.<; upwind valley, is over 20 km wide, and has a <br />maximum elevation of about 3.4 km. Accordingly, the experimental design will be written for a <br />single area, and the discussion in this section and in section 5 will apply to both the Grand <br />Mesa and the Wasatch Plateau. Similar experimental designs will provide replication of results, <br />an approach commonly used to test the plausibility of experimental findings. <br /> <br />The application of the design will differ somewhat between the barriers, because of the <br />operational differences to be noted. Future field operations plans will deal with these <br />dissimilarities_ <br /> <br />The two mountain barriers have a number of differences, the most obvious being their <br />orientation. The Wasatch Plateau is a north-south oriented barrier. The crestline of the Grand <br />Mesa lies approximately east-west. However, on both barriers the terrain influences the <br />low-level flow which tends to turn perpendicular to the barrier crest (upslope). Significant SLW <br />production has been observed over both barriers with large-scale flow between south-southwest <br />and nDrthwest_ The difference in crestline orientation is not expected to significantly affect <br />cloud responses to seeding. <br /> <br />Three other significant differences exist between the experimental areas. First, the Wasatch <br />Plateau has an excellent all-weather highway system, which will permit on-top, cross-plume <br />sampling of AgI, tracer gas, and ice crystals by an instrumented four-wheel drive vehicle. <br />Highways do not cross over the eastern portion of the Grand Mesa but do reach well up it.<; <br />slopes. OversnDw travel is required to reach and traverse the Mesa top, and such travel is " <br />practical as the terrain is not rugged. An instrumented DversnDw vehicle will be used for <br />cross-plume sampling on the Mesa. However, large Dversnow vehicles are slow, and surface <br />vehicle sampling clearly will playa larger role on the Plateau because of it.<; highway system. F <br /> <br />Second, a WSR-88D advanced Doppler weather radar is scheduled to be installed on top the <br />Mesa in September 1995, near it.<; northwest end. This radar will be part of the NEXRAD (Next <br />Generation Weather Radar) network now being established nationwide for the National <br />Weather Service and other agencies. Transmission of WSR-88D measurement.<; by radio for <br />real-time use in the CREST operations center and recording for later analysis should be <br />possible, which would eliminate the need for the program to operate a sophisticated surveillance <br />radar on the Mesa. Some cost.<; would be incurred in obtaining the WSR-88D observations, but a <br />significant net savings would result. This savings would be partially offset, however, by higher <br />travel costs on the Mesa caused by more DversnDw travel. WSR-88D unit.<; scheduled for Utah <br />will be too distant to serve a similar function for the Wasatch Plateau. <br /> <br />The third noteworthy difference is that an upwind barrier, the San Pitch Mountains, lies <br />parallel to the Wasatch Plateau at about 30 km distance (about 1.5 h travel time with typical <br />winds). Seeding the Plateau from near the top of the San Pitch Mountains may be feasible, and <br />that possibility will be tested during the direct detection phase. Seeding from the upwind <br />barrier would provide considerably more time for AgI dispersion, and more time for ice crystal <br />growth and fallout, two significant advantages. <br /> <br />20 <br />