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<br />Therefore, the goal of this researcn 1S to understand the factors that <br /> <br />contribute to natural T,esoscale heterogeneities which produce large <br /> <br /> <br />variations in rainfall and, thus, enable us to select more homogeneous <br /> <br />samples within which seeding effects may be detected and measured. <br /> <br />Orlanski (1975) has designated the a, ;S,vscales as those required <br /> <br />to define phenomena having subsynoptic size. These scales are defined <br /> <br />in terms of the system wavelength ~ and time scales as: <br /> <br />Me so a <br />Meso ;3 <br />t'~eso y <br /> <br />250 < L < 2500 km <br />25 < L < 250 km <br />2.5 < L < 25 km <br /> <br />6 < t < 36 h <br />l<t<6h <br />o.T < t < 1 h <br /> <br />These definitions are used throughout this report. <br /> <br />Previous weather modification field experiments ~ave failed to <br /> <br />recognize the need for mesoscale rawinsonde observations and the physi- <br /> <br />cal understanding of mesoscale triggering effects on convective precipi- <br /> <br />tation. Therefore, the Texas HIPLEX data set represents a unique source <br /> <br />of information that provides digital radar, rain gage, rawinsonde and <br /> <br />satellite observations (e.g., Riggio et al., 1982). Fig. 1.1 shows the <br /> <br />location and scale of observations in this experi~ent. Sy~optic and <br /> <br />meso-p scale rawinsonde n~tworks and radar site are shown on the two- <br /> <br />degree grid of the objective analyses. A critical problem in mesoscale <br /> <br />analysis is the automated analysis of mesoscale features and quantita- <br /> <br />tive prediction of the mesoscale triggering effects on cloud development <br /> <br />and precipitation. Anthes et al. (1982) have shown the value of meso- <br /> <br />scale analyses in fine-mesh models to predict mesoscale regions of <br /> <br />severe storm development. This study provides a unique analysis tech- <br /> <br />nique that uses mesoscale objective analyses of vertical motion fields <br /> <br />3 <br />