NASA NTRS · 19830068511
Interpretation of satellite-observed thunderstorm anvil structure
Abstract
The radiative characteristics of an anvil plume sensed by satellite radiometers are studied to discern the reason for an observed 'V' pattern of colder temperatures and a corresponding internal warm region. The measured black body temperature is affected by the ice water content and particle distributions in the cloud layer. Attention is given to 'V' anvil structure examined by Haynesfield et al. (1979). The GOES satellite IR data are treated with a plane parallel geometric radiative transfer model and a particle trajectory model is used to simulate ice particle concentrations downwind from a strongly divergent cloud top. Output from the two models indicate the 'V' pattern arises from divergence in the storm anvil. The particle concentration was elevated within the V-shaped region, causing lower temperatures in the V arms. The V is produced by strong upper level flow as well as strong mass and moisture divergence in the storm outflow.
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Heymsfield, G. M., Schotz, S., Blackmer, R. H., Szejwach, G.. 1982-01-01. Interpretation of satellite-observed thunderstorm anvil structure. https://ntrs.nasa.gov/citations/19830068511
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