On the distribution and efficiency of sporadic meteor radiants

Physics

Scientific paper

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Scientific paper

A method of determining the efficiency of sporadic meteor radiants for a given distribution model of sources from results of measurements on a forward-scatter path is proposed. From three models under investigation, the most satisfactory is that one with three point-sources in the ecliptical plane situated in the apex and in two points shifted by ±70° ecliptical longitude from it. For this model, the annual efficiency variation of individual sources is shown.

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