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<br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />About the Cover <br /> <br />I <br /> <br />The cover figure represents the development of numerical models by the numerical <br />modeling group at the Institute of Atmospheric Sciences. The 1960s panel shows a <br />result for the initiation of a cloud over a 3000-foot mountain ridge. The primary <br />airflow is from left to right so that the cloud forms over the right mountain slope. The <br />1970s result is for our simulation of a rain shower in a 10 km by 10 km domain that <br />includes the same size mountain ridge as the previous result. The shaded region <br />depicts the rain field. The 165 number in the upper right comer indicates that the <br />results are for 165 minutes of simulated real time. The next panel shows results for <br />the numerical simulation of a hailstorm, published in 1977. The dashed lines are <br />streamlines and the solid line outlines the storm. The darker symbols, extending from <br />deep in the cloud to near the surface, indicate hail falling out of the cloud with some <br />melting into rain over the mountain ridge. Some rain to the right of the ridge is being <br />recycled back into the cloud. The domain is 20 km by 20 km. The 1986 color panel <br />shows the total condensate in a numerical simulation of a thunderstorm that produced <br />a strong microburst near Huntsville, Alabama. The dark red region indicates copious <br />amounts of precipitation falling out of the storm to create strong outflow at the earth's <br />surface. The last panel (1990s) shows three-dimensional modeling results after two <br />hours of real-time simulation of a North Dakota hailstorm on a grid 60 km on a side <br />and 20 km deep. The dynamics of the model is that of Terry Clark at the National <br />Center for Atmospheric Research and the microphysics is that of the lAS, Richard <br />Farley the principal investigator. <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br /> <br />I <br />