Please use this identifier to cite or link to this item: http://openarchive.nure.ua/handle/document/248
Title: К проблеме метеорных орбит с большими значениями эксцентриситетов при радиолокационных наблюдениях
Authors: Коломиец, С. В.
Keywords: Кащеев Б.Л.
гиперболические метеоры
метеорное тело
геоцентрическая скорость
солнечная система
метеорная орбита
Issue Date: 2005
Publisher: ХНУРЭ
Citation: Коломиец, С. В. К проблеме метеорных орбит с большими значениями эксцентриситетов при радиолокационных наблюдениях / С. В. Коломиец // Прикладная радиоэлектроника. Состояние и перспективы развития (МРФ’2005) : сб. науч. тр. 2-го Междунар. радиоэлектронного форума. – Х. : ХНУРЭ, 2005. – Т. 1. – С. 224–227.
Abstract: The most of meteors observed instrumentally belong to the Solar system. Nevertheless, the Solar system is not closed. It is permeable for the particles and even large bodies flying inward and outward. Since a meteoroid with a hyperbolic heliocentric velocity may have an usual geocentric velocity then a possibility to record a hyperbolic meteor is no more connected with a great error of determination of its velocity'. Presence of interstellar particles in the observation data is not proved till now because the accuracy of measurements and calculations is not good enough to check the reliability of these data. "We analyze meteor orbits with high eccentricities that were registered in 1972-1978 in Kharkov (Ukraine). The orbital data of the KHNURE electronic catalogue are received from observations of radiometeors with masses 103-10'6g.
URI: http://openarchive.nure.ua/handle/document/248
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