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Astron. Astrophys. 329, 769-775 (1998)


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The determination of the parameters of fragmenting meteoroids

G.G. Novikov 1, P. Pecina 2 and N.A. Konovalova 3

1 Novgorod State University, 173003 Novgorod, Russian Federation
2 Astronomical Institute of the Academy of Sciences of the Czech Republic, 251 65 Ondejov, Czech Republic
3 Astrophysical Institute, Tadzhik Academy of Sciences, 734670 Dushanbe, Tadzhik Republic

Received 2 April 1996 / Accepted 27 June 1997

Abstract

Taking into account the quasi-continuous fragmentation of meteor particles, the formulae describing the variation of both light and ionization along the atmospheric trajectory of meteoroids, are derived. Two methods of data processing are presented enabling the determination of the parameters of quasi-continuous fragmentation, [FORMULA], and [FORMULA], characterizing the parent body and the fragmentation products, as well as the bulk density of the parent meteoroid from the light and/or ionization curve. The use of these methods is shown by means of two examples of processing of model curves.

Key words: meteors, meteoroids

Send offprint requests to: P. Pecina

© European Southern Observatory (ESO) 1998

Online publication: December 8, 1997
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