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Currents in the cometary atmosphere
Authors:W.-H. Ip
Affiliation:Dept. of Applied Physics and Information Science, University of California, San Diego, La Jolla, California 92093 U.S.A.
Abstract:If the structure of the magnetic field and electric current in the cometary type I tail can be represented by an electric current circuit, disruption of the cross-tail current system may lead to a current discharging through the cometary ionosphere, and the dissipation of the magnetic energy stored in the tail. From the point of view of energy budget, a tail-aligned magnetic field on the order of 10γ will be sufficient to produce a strong ionization effect of the cometary atmosphere.
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