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, the characteristics of which agree with the observational data on the Draconid and Leonid meteor showers.
Kulikova
N V
NV
Institute of Nuclear Power Engineering, Obninsk, USSR.
Pivnenko
E A
EA
D055580:Astronomical Phenomena; D001256:Astronomy; D005118:Extraterrestrial Environment; D007053:Ice; D008433:Mathematics; D019110:Meteoroids; D008962:Models, Theoretical
D007053:Ice