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<br />- <br /> <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 />accumulated precipitation forecasts was generated with both the dump-bucket and <br />microphysics versions of the forecast model. Both sets of output were compared to a set <br />of 167 community-based station reports, and to a set of 32 Snotel stations. Climatological <br />station precipitation forecasts were improved on the average by correcting for the <br />difference between a station's actual elevation and the cell-averaged topography used by <br />the model. The model had more problems with the precise timing and geographical <br />location of the precipitation features, probably due in part to the influence of other model <br />physics, the failure of the model to resolve adequately winter-time convection events, and <br />lack of mesoscale detail in the initializations. Wetzel et al. (2002,2003) further <br />demonstrated RAMS accuracy in predicting snowfall amounts in high-mountain terrain, <br />specifically the Park Range of Colorado. As in the Gaudet and Cotton (1998) study, the <br />best agreement occurred at the higher elevation sites and the worst in the valleys. This <br />could be a related to the inability of the model to represent the valley features correctly <br />since emphasis is placed on getting the mountain high terrain forcing in the model. In <br />addition, RAMS exhibited a warm-temperature bias, which may be a consequence of <br />using ETA model forecast data for initialization and nudging; the ETA model is known to <br />have such a warm temperature bias. <br /> <br />The current prototype real-time forecast version ofRAMS@CSU is based on version 4.3. <br />The model is set up on a cluster ofPCs. The forecast model configuration has three <br />interactive nested grids. Grid #1 has 48 km grid spacing and covers the entire <br />conterminous U.S. Grid #2 has 12 km grid spacing and covers all of Colorado, most of <br />Wyoming, and portions of adjacent states, and Grid #3 has 3 km grid spacing covering a <br />240 km x 240 km area that is relocatable anywhere within Grid #2. Vertical grid spacing <br />on all grids starts with 150-km spacing at the lowest levels and is stretched to 1000m <br />aloft, with a total of 36 vertical levels extending into the stratosphere. The model is <br />initialized with OOUTC ETA model analysis fields and run for a period of 48h, with the <br />lateral boundary region of the coarse grid nudged to the ETA 3-hourly forecast fields. A <br />48-h run typically begins about 03 UTC or 8 P.M. MST (when the 00 UTC ETA forecast <br />data are available), takes 4-5 h of computer time to finish, and is available for real-time <br />operational use by 2 A.M. MST. Because RAMS has been able to reproduce high- <br />elevation snow fall amounts with considerable accuracy (Gaudet and Cotton, 1998; <br />Wetzel et aI., 2002; 2003), we believe that RAMS can be useful in forecasting the effects <br />of cloud seeding on precipitation for an entire winter season. <br /> <br />The microphysics in RAMS is quite sophisticated. Instead of using continuous accretion <br />approximations as had been the norm in cloud parameterizations, RAMS uses solutions <br />to the full stochastic collection equation. Walko et al. (1995) describe the <br />implementation ofthis approach in RAMS for prediction of hydro meteor mixing ratios. <br />An important aspect of the implementation strategy was the use oflook-up tables that <br />enabled fast and accurate solutions to the collection equations. Meyers et al. (1997) then <br />extended this approach to two-moments of the hydrometeor spectra: mixing ratio and <br />number concentration. Also in Verlinde et al. (1990) and subsequent implementations in <br />RAMS, the Kessler-type exponential or Marshall-Palmer basis function for hydrometeor <br />spectra was abandoned in favor of a generalized gamma distribution function, <br /> <br />11-8 <br />