Mathematics
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984stin...8426546f&link_type=abstract
Unknown
Mathematics
Comet Tails, Cometary Magnetospheres, Comets, Magnetic Fields, Magnetohydrodynamics, Magnetospheres, Simulation, Solar Wind, Discontinuity, Interplanetary Magnetic Fields, Mathematical Models, Plasma Interactions, Rotation
Scientific paper
This paper presents results of a numerical magnetohydrodynamic simulation of the interaction of the solar wind with a comet. It states that for a steady solar wind and interplanetary magnetic field (IMF) the cometary plasma has a distinctive structure; a spheroidal head and a long ribbon-like tail. Rotational discontinuities in the IMF lead to changes in the tail structure. It is shown how these effects occur and describe ray-like structures as well as a tail disconnection event. The simulation results provide a simple explanation for a number of observable features in cometary plasma tails.
Brecht Stephen H.
Fedder Joel A.
Lyon John G.
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