Mathematical modelling of the Geminid meteoroid stream

Details Mathematical modelling of the Geminid meteoroid stream Mathematical modelling of the Geminid meteoroid stream

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007mnras.375.1371r&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 375, Issue 4, pp. 1371-1380.

Astronomy and Astrophysics

Astronomy

16

Meteors, Meteoroids

Scientific paper

The Geminid meteoroid stream formation and evolution were studied by the method of nested polynomials. The stream has two layers formed due to differences in orbital parameters of particles ejected from the cometary nucleus before and after perihelion. The shape of the model activity profiles depends on the place where the Earth passes the stream. The importance of observations for calibration of the model is discussed.

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