Dust Tail Modelling for Comet Hale-Bopp

Details Dust Tail Modelling for Comet Hale-Bopp Dust Tail Modelling for Comet Hale-Bopp

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ysc..conf...57k&link_type=abstract

YSC'15 Proceedings of Contributed Papers (eds. Choliy V. Ya., Ivashchenko G.), pp. 57-59

Computer Science

Scientific paper

The results of dynamic modelling of the dust tail formation of comet C/1995 O1 (Hale-Bopp) are presented. To simulate the dust tail the trajectories of 2×10^6 dust particles were traced. Their sizes, ejection moments, outflow directions and velocities were defined by a Monte Carlo algorithm. The obtained three-dimensional modelled tail was projected on the sky plane to compare with the observed images.

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