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<br />of Reclamation and the National Science Foundation to better understand <br />the complex dynamics, thermodynamics and microphysical mechanisms of <br />convective precipitation evolution. The purpose of this dissertation <br />is to develop a better understanding of the physical structure of meso- <br />scale convective triggering mechanisms that produce rainfall and to <br />stratify precipitation events into more homogeneous classes. To achieve <br />this, an automated objective analysis technique, graphical display sys- <br />tem and numerical model were used to describe kinematic and thermody- <br />namic properties of precipitation events. The technique will be useful <br />for analysis of the CCOPE data sets to better understand mesoscale <br />characteristics of convective storms. <br /> <br />In order to test the technique, a set of hypotheses of kinematic <br />and thermodynamic characteristics of the four classes of precipitation <br />events was proposed. Then, all 1979 Texas HIPLEX events were stratified <br />using visible and infrared geosynchronous satellite photographs. <br />Thermodynamic and kinematic analyses of rawinsonde data were performed <br />and temporal and spatial characteristics of mesoscale features were <br />described. Rain gage, radar echo, and satellite-observed cloud charac- <br />teristics were also analyzed and combined with the thermodynamic results <br />to provide a comprehensive description of each precipitation class and <br />its natural variability. <br /> <br />1.1 Problem definition <br /> <br />Extremely large natural variations in convective rainfall from <br />mesoscale thunderstorms are observed in apparently heterogeneous samples <br />of mesoscale forcing. Such heterogeneous samples make it difficult to <br />plan, organize, conduct and evaluate weather modification experiments. <br />2 <br />