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Gritsevich, M. I.; Guslov, T. S.; Kozhemyakina, D. M.; Novikov, A. D.
Solar system research, 08/2011, Letnik: 45, Številka: 4Journal Article
We explored how justifiable the use of a model with a constant mass loss parameter as applied is to real meteor events. The model with variable mass loss parameter used in this work is based on the calculation of the luminosity parameter and of the radiative heat exchange coefficient at separate points of trajectory. Agreement between models with constant and variable mass loss parameters is demonstrated by the example of observations of two big meteor bodies (MORP 219 and MORP 872).
