Numerical examinations of the structures in the dust tail of a comet

Statistics – Computation

Scientific paper

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Comet Nuclei, Comet Tails, Computational Astrophysics, Cosmic Dust, Particle Motion, Astronomical Models, Particle Emission, Particle Trajectories, Rotation

Scientific paper

The consequences of the variation of comet nucleus emission characteristics on the shape of the dust tail are examined. Additionally, the emitted dust quantity is deduced from the dust tail image. The concept behind the process and the resulting algorithm are represented and discussed in detail. Other methods are also examined. The effects that the rotation of the comet nucleus have on the dust tail are examined. Test examinations using the method, which allow the possibilities of back circuits on the behavior of a comet dust emission, are presented.

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