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Abstract
Last year the work on the qualitative model of the Geminid meteoroid stream was finished [1, 2]. The mentioned publications summarized the results of 20-years efforts. This model explained most of the Geminid’s structural features, including bimodality, but to find quantitative spatial density distribution of particles we need a more precise model. The first runs of the new numerical model were made, and some preliminary results have been obtained.
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