Currents in the cometary atmosphere

Research output: Contribution to journalArticlepeer-review

12 Scopus citations

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.

Original languageEnglish
Pages (from-to)121-125
Number of pages5
JournalPlanetary and Space Science
Volume27
Issue number2
DOIs
StatePublished - Feb 1979

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