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<br />for precipitation characterization and for comparison with the aspirated <br />2D-C, in a size range where the measurements overlap. <br /> <br />The probe will be operated at KGV during experimental units. The data <br />acquisition system (DAS), formatter, and tape drive will be located in the <br />radiometer along with the DAS for the 2D-C. This is particularly important <br />as the DAS for the grey scale probe requires frequent checking since it <br />occasionally needs to be restarted. <br /> <br />c. Photomicrographs of snow crystals collected in petri dishes will be <br />used to document crystal habit and degree of riming. Four or five photo- <br />micrographs will be taken of snow crystals collected at approximately 5-10 <br />minute intervals during operational periods. The photographs will be taken <br />randomly in an attempt to characterize the snowfall collected. Also a <br />manual record of the crystal habits and degree of riming will be kept as a <br />backup in case of loss of the film log. The equipment consists of a <br />microscope with camera, automatic exposure control unit, and cold stage <br />attachments. Tri-X black and white film is used. Negatives of the photo- <br />mi crographs will be contact pri nted into a time seri es format for 1 ater <br />analysis. <br /> <br />d. Concurrent with the photomicrographs, shadowgraphs will be collected at <br />5-10 minute intervals. These Polaroid pictures provide a ~rue size snap- <br />shot of the characteri stics of the preci pitat ion. Each photograph wi 11 <br />represent a 10 second exposure to the snowfall. These observations are <br />aimed at obtaining a chronology of aggregation, the habit and degree of <br />riming of the crystals forming the aggregates, and the approximate number <br />of crystals per aggregate. Additional observations of habit and rime of <br />unaggregated crystals can be useful as a backup to photomicrograph obser- <br /> <br />III-20 <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 />