Modelling of the new formation structures in the near space

Complex numerical model of young meteor stream formation taking into account reactive deceleration of cometary nucleus and its form change in the process of stream formation is discussed. The model made it possible to predict the existence of fine and superfine structures for young meteor streams, t...

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Bibliographic Details
Published inAdvances in space research Vol. 12; no. 4; p. 71
Main Authors Kulikova, N V, Pivnenko, E A
Format Journal Article
LanguageEnglish
Published England 1992
Subjects
Astronomical Phenomena
Astronomy
Extraterrestrial Environment
Ice
Mathematics
Meteoroids
Models, Theoretical
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Summary:Complex numerical model of young meteor stream formation taking into account reactive deceleration of cometary nucleus and its form change in the process of stream formation is discussed. The model made it possible to predict the existence of fine and superfine structures for young meteor streams, the characteristics of which agree with the observational data on the Draconid and Leonid meteor showers.
ISSN:0273-1177
DOI:10.1016/0273-1177(92)90157-S