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<br />made above the plateau (Doppler acoustic sounder or profiler), but some estimation errors will still exist. <br />Silver-in-snow concentrations sometimes will be measured at each gauge site to test the estimation method <br />for deciding whether particular gauges were seeded or not. <br /> <br />Relatively high relationships can be expected during nonseeded periods between target gauges along the <br />center (target) portion of each line, and control gauges near the north and south ends of each line. The <br />terrain is reasonably unifonn and the distance along each gauge line will be limited (about 6 miles along <br />the windward edge and about 15 miles along the lee edge line). Relationships established during <br />nonseeded periods with similar meteorological conditions will be used to estimate precipitation at target <br />gauges during physical seeding experiments. Any significant differences from that predicted will be <br />considered due to the seeding. <br /> <br />Many nonseeded periods used to establish target-control gauge relationships will be from nighttime when <br />safely considerations preclude low-level aircraft flight. While daytime in-cloud flight also relies on aircraft <br />instruments, emergency landing is much safer during daylight <br /> <br />Conventional weighing precipitation gauges, modified with orifices providing 5 times the area of 8-in <br />diameter gauges, have been successfully used on the Grand Mesa of Colorado and the Mogollon Rim of <br />Arizona. They provided a resolution of about 0.002 in (0.05 mm), and, with daily rotation gears, a time <br />resolution of about 5 min. Both should be adequate when seeding produces significant snowfall so similar <br />gauges will be used on the Wasatch Plateau to monitor physical seeding experiments. <br /> <br />The duration of a physical seeding experiment is partially detennined by the temporal stability of the <br />atmosphere and partially by the practical flight duration of an instrumented aircraft. The latter is about <br />3 hours on-station time. Thus, a typical seeding experiment will release AgI for about 2 hours, <br />commencing shortly before arrival of the sampling aircraft. The aircraft will continue to sample after <br />generator turnoff to document changes in cloud microphysics as the concentration of seeding material <br />decreases with time.. This approach, used by Super and Heimbach (1988), can provide convincing <br />evidence of changes due to seeding in both space and time. <br /> <br />It is important that measurements be made to monitor natural temporal changes in cloud conditions that <br />are unaffected by seeding. These observations help correctly identify both natural and seeding-caused <br />changes in IPC, precipitation rate, etc. Of course, the purpose of the control gauges is to monitor natural <br />changes in snowfall with time. However, radar coverage of the experimental area also can be helpful by <br />documenting the passage of any mesoscale features (e.g., "precipitation bands") during the course of an <br />experiment <br /> <br />Monitoring available SL W is very important because its presence is necessary for cloud seeding to be <br />effective. A physical seeding experiment would not commence unless SL W were present. Moreover, any <br />natural changes in SL W during the course of an experiment should be known for proper interpretation of <br />results. A zenith-pointing microwave radiometer should be operated on top the plateau, crosswind of the <br />seeded zone, to provide a time history of SL W amount throughout each experiment If a second <br />radiometer were available, it should be located in the seeded zone as often as practical to search for <br />reductions in SL W caused by seeding. A truck-mounted radiometer, such as used in the 1991 field effort, <br />could be driven back and forth along the upwind highway to sample both natural and seeded cloud. <br />Effective seeding should reduce the SL W in the seeded zone. <br /> <br />It is estimated that about three winter field programs, each 4 to 5 months long, would be required for the <br />physical experiment phase. Analyses of the many experiments conducted during that time should provide <br /> <br />51 <br />