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Last modified
7/28/2009 2:41:49 PM
Creation date
4/30/2008 2:42:19 PM
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Weather Modification
Title
Investigations of Winter Storms over the Wasatch Plateau during the 1994 NOAA-Utah Field Research Program - Final Report
Date
7/1/1996
State
UT
Weather Modification - Doc Type
Report
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<br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br />I <br /> <br />depth difference becomes a filLX difference of 3630.4 g m-I S-I. This SLW flux was converted to a <br />precipitation flux over the 9.925 km distance between RRS and TAR, giving the approximate <br />precipitation rate required to completely account for the flux difference. The precipitation flux was <br />computed to be 0.3658 g m-2 s-:. Converting to a conventional precipitation rate. this becomes 1.32 <br />mm h':, the rate necessary to account for the difference in SL W depth between RRS and TAR. <br />The a\'erage precipitation rate at TAR from 0900 to 1100 was 0.875 mm h -'. onlv about 66% <br />of the rate required to remove the excess SL \V. Studies of precipitation over the plateau during a <br />1991 :'\OA<\-Ctah field program by Huggins et al. (1992) showed that the precipitation maximum <br />was generally up\\ind of TAR. For the 1991 season the maximum was between the upwind edge of <br />the plateau and the middle, "\lth TAR precipitation being about 75% of the maximum. This suggests <br />that the average rate between RRS and Tl\R, on 7 February, was likely greater than the average <br />observed at TAR alone. Applying the 1991 percentage to the 7 February case suggests that the <br />precipitation observed could have accounted for about 90% of the SL W difference noted in the <br />radiometer comparison. Given the assumptions used in the simple calculation (such as the <br />representati\'eness of the SLW measurements), and reasonable errors in each parameter, this <br />comparison indicates that the up\vind-dmvnwind difference in SL W can be mostly be accounted for <br />by precipitation removal. To verify this further, a more detailed condensed phase water budget <br />across the plateau would be needed. <br />The tlnal period in Fig. 52b (1100-1200) shows the mobile transect from TAR back to RRS, <br />\\ith depth values again becoming nearly equivalent as the mobile reached RRS at about 1140. The <br />final period of comparison in Fig. 52c shows data from the mobile radiometer when it was near the <br />base of the plateau at HQ. The differences were similar to those noted in Fig. 52a, and reflect the <br />additional condensate that is produced when moist air is lifted over the \"indward slopes of the <br />plateau. It is interesting to note in all panels of Fig. 52 that the temporal trends in SLW were seen <br />in the data from both radiometers, regardless of position, indicating that, although orographic <br />influences were observed, the mesoscale influences were also detectable and in most cases were of <br />equal or greater magnitude. <br /> <br />71 <br />
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