On the theory of light curves of video-meteors

Abstract

<i>Aims. <i/>The aim of the article is to show how the light curve of video-meteors can be described theoretically.<i>Methods. <i/>The method of numerical integration of the system of differential equations describing the motion and ablation of a meteoroid during its atmospheric motion is employed.<i>Results. <i/>We have shown that the modification of the ablation equation and the more general assumptions on the meteoroid cross-section behaviour can lead to a better description of light curves of faint video-meteors. The applied method indicates that the traditionally-used statistical parameter F could be replaced by another one, Levin's parameter <i>μ<i/>, which has a physical meaning.