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Identification of radiants of low-light-level meteors from double station TV observations during autumnal equinox of 2001 and 2003

Published online by Cambridge University Press:  05 March 2015

Pavlo M. Kozak ,
Olexander O. Rozhilo  and
Yuriy G. Taranukha
Pavlo M. Kozak
Affiliation:
Astronomical Observatory, Kyiv National Taras Shevchenko University, 3, Observatorna Str., Kyiv, 04053, Ukraine email: kozak@observ.univ.kiev.ua
Olexander O. Rozhilo
Affiliation:
Astronomical Observatory, Kyiv National Taras Shevchenko University, 3, Observatorna Str., Kyiv, 04053, Ukraine email: kozak@observ.univ.kiev.ua
Yuriy G. Taranukha
Affiliation:
Astronomical Observatory, Kyiv National Taras Shevchenko University, 3, Observatorna Str., Kyiv, 04053, Ukraine email: kozak@observ.univ.kiev.ua
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Abstract

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Results of double-station TV meteor observations which were carried out during autumnal equinox in 2001 and 2003 are used for the confirmation of existing meteor showers and for a search for probable new micro-showers. Seven existing September showers were confirmed, two of them by meteors from both years. Fourteen new groups were proposed to be considered as new meteor micro-showers. Taking into account similar kinematical parameters two of them can be supposed to be a part of already existing showers.

Keywords

TV observations of meteorsmeteor radiantnew meteor stream
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 178
Copyright
Copyright © International Astronomical Union 2015 

References

Jopek, T. J. & Jenniskens, P. M. 2011, in Cooke, W. J., Moser, D. E., Hardin, B. F., and Janches, D. (eds.), Proc. Meteoroids Conf. Breckenridge, Colorado, USA, NASA/CP-2011-216469. p. 7Google Scholar
Kozak, P. 2008, EM&P 102, 1–4, 277Google Scholar