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Last modified
7/28/2009 2:40:19 PM
Creation date
4/24/2008 2:48:25 PM
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Weather Modification
Title
Observations of Silver Iodide Plumes over the Grand Mesa of Colorado
Date
10/10/1988
State
CO
Weather Modification - Doc Type
Report
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<br />1136 <br /> <br />4.5 <br /> <br />JOURNAL OF APPLIED METEOROLOGY <br /> <br />VOLUME 27 <br /> <br /> <br />860214 <br /> <br /> 4.0 <br />;;; <br />E <br />E <br />'" <br /> 3.5 <br />w <br />0 I <br />::::l <br />>- <br />5 <br /><J: <br /> 3,0 e ee <br /> <br /> <br />2.5 <br />290 <br /> <br /> <br />FIG. 3, An example of the variability of vertical profiles of potential <br />and equivalent potential temperature during a mission, <br /> <br />below appears to have been mixing with 60 warmer <br />air from above as a result of strong speed shear and <br />flow perturbations caused by the mountain. The <br />acoustic sounder recorded winds of about 4 m s - I at <br />3.4 km, increasing linearly to about 15 m S-I at 3.8 <br />km with about 400 of angular shear. <br />The situation presented in Fig. 3 was selected because <br />it illustrates the process well. In the less extreme ex- <br />amples, the AgI was still detectable to near the altitudes <br />where the warmest potential temperature of the seeding <br />site equaled the coldest potential temperature at flight <br />level. Beyond that level only trace amounts were found. <br />The normal temperature profile of an upwind sounding <br />never shows variations like those illustrated in Fig. 3 <br />and is therefore not a reliable indicator of the highest <br />level of plume rise, because the mountain barrier can <br />sometimes lift stable air if the wind momentum is suf- <br />ficiently great. <br />Figure 4 presents vertical cross sections of the plumes <br />in the plane near their middle positions, as shown in <br />Fig. 2. The approximate terrain within 1.5 km of that <br />plume center line is given for reference. The left side <br />of each cross section in Fig. 4 is shaded (with a dot <br />pattern) to show the approximate altitudes of stable <br />layers as indicated by profiles like that in Fig. 3. The <br />individual dots near the plumes indicate the locations <br />where a pass initially detected (or failed to detect) an <br /> <br />320 <br /> <br />AgI or ice particle plume. The horizontal lines indicate <br />the positions through which an ice particle plume was <br />detected on passes along the wind. The vertical extents <br />of the seeding plumes were determined when the air- <br />craft passes failed to detect the AgI or ice signatures, <br />or found only weak ones. When such null data were <br />available, the boundary line in Fig. 4 is solid. When <br />the boundary can only be approximated, it is dotted. <br />The approximate vertical thicknesses of the plumes as <br />they crossed the crests are listed in Table 1. If the top <br />was not determined, the highest measured position is <br />given with a plus sign. In one case, the plume continued <br />to rise and was at a higher position over the southwest <br />arm than over the northwest arm of the mesa. The <br />median plume thickness over the crest exceeded 500 <br />m. The range of thicknesses was about a factor of two <br />from the median. <br />The twelve experiments illustrated in Fig. 4 are <br />identified by the letters a-I. In Fig. 4a, an inversion <br />limited vertical development. An opposing air flow at <br />the crest prevented the plume from continuing over <br />the crest in its original flow direction. The downwind <br />extent in Fig. 4b was not well determined and the <br />plume may have been transported downhill by subsi- <br />dence. The plume rose rapidly to the stable layer in <br />Fig. 4c, but the vertical extent far downwind was not <br />determined. The same is true for Fig. 4d, where the <br />plume position over the southwest arm of the mesa <br />was only measured near the surface. The plume top in <br />Fig. 4e was near a weak stable layer over the northwest <br />arm and continued to rise to a second stable layer near <br />the tip of the southwest arm. In the experiment shown <br />in Fig. 4f there were no barriers until 4.4 km, and no <br />pass was made that was above the plume. The strong <br />flow that created a lenticular cloud in the plume po- <br />sition in Fig. 4g was probably responsible for the very <br />rapid rise of the plume to near cloud base. The plume <br />was below the aircraft on a few passes near the down- <br />wind escarpment, being transported down by subsiding <br />air. Another rapid rise is shown in Fig. 4h, where the <br />plume rose in cloudy conditions, creating ice particles <br />in air that had no stable layers. The upwind edge of <br />the plume was well-determined but not its vertical or <br />downwind extent. In Fig. 4i the stable layer began at <br />4.6 km, and the plume actually rose to that altitude. <br />The plume in Fig. 4j was repeatedly detected but only <br />at one position and altitude; it was not detected for <br />passes at 4.5 km, but that did not provide much res- <br />olution for determining the vertical extent in an at- <br />mosphere that had a stable layer at about 4.4 km. The <br />plumes in Figs. 4k and 41 rose to the tops of the stra- <br />tocumulus clouds and were detected by ice particles as <br />well as by AgI. <br />In an extreme example not illustrated here, AgI <br />smoke was released in an open meadow on top of the <br />mesa at about sunset on 5 February 1986 and was <br />trapped in a drainage flow. Sensors at a nearby PROBE <br />station showed rapid radiational cooling at the surface <br /> <br />\, <br /> <br />
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