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<br />OCTOBER 1988 <br /> <br />HOLROYD, McPARTLAND AND SUPER <br /> <br />1127 <br /> <br /> <br />~- <br /> <br />G;, <br />........ <br />'0 <br />~ <br />'9'10: <br />~'S'! <br />~ <br />~ <br />'9'..... <br />~ <br />'''9. <br />Go- <br /> <br /> <br />o <br />. I <br /> <br />2.0 <br /> <br />:::. <br /> <br /> <br />.0 <br /> <br />2~i 3R~~J ~~S~ <br /> <br />5" <br />E"' <br />3-': <br /> <br />... ~ <br />"0 <br /> <br />6- <br /> <br />39CN- <br /> <br />4" <br /> <br />FIG, I. A map of the terrain near the Grand Mesa, Colorado, showing the locations of ground release sites for AgI and weather stations, <br />The seeding sites are identified by numbers here and in Table 1. The weather stations are indicated by letters here and in the text, The <br />contour interval is 500 m, with the terrain below 3000 m shaded as shown in the key in the upper left, <br /> <br />reliably transported up and over the barrier to sufficient <br />height and in sufficient concentrations to produce <br />measurable cloud microphysical effects during typical <br />storms. <br />2. The appropriate spacing between ground gener- <br />ators, based on the lateral spread of ground-released <br />plumes as they cross the target area. <br />3. The lateral diffusion rates of airborne-released <br />lines of AgI and the resulting seeding repetition rate <br />that would be required for plume mergers to occur <br />prior to target cloud entry. <br /> <br />The Grand Mesa is a large, relatively flat-topped <br />mountain that rises steeply about 1500 m from the <br />surrounding valley floors. The maximum mesa ele- <br />vation in the region of the experiments is about 3200 <br />m msl. The orientation of the barrier provides oro- <br />graphic lift for storms from all principal directions <br />(clockwise from South to North). Because of the lack <br />of pronounced vertical relief on the Mesa top, Federal <br />Aviation Administration (FAA) permitted aircraft op- <br /> <br />1- <br /> <br />erations to within about 300 m above the highest point <br />in the research area during IFR conditions. This is 300 <br />m closer to the surface than is usually allowed in <br />mountainous terrain. Figure 1 shows the area and il- <br />lustrates the locations of ground sensors (indicated by <br />letters) and seeding sites (indicated by numbers) in the <br />Grand Mesa area. Table 1 further identifies the seeding <br />sites. <br /> <br />3. Equipment <br /> <br />a, Silver iodide generators <br /> <br />The ground seeding unit was a modified Skyfire-type <br />solution burner developed at Montana State Univer- <br />sity. It utilizes a propane flame into which is injected <br />an acetone solution containing dissolved AgI. A 3% by <br />weight AgI solution complexed with ammonium iodide <br />(NH4I) was used at a consumption rate of about 30 g <br />AgI h -1 . Calibration tests conducted in the isothermal <br />cloud chamber at Colorado State University (CSU) <br />