Currents in the cometary atmosphere

研究成果: 雜誌貢獻期刊論文同行評審

12 引文 斯高帕斯(Scopus)

摘要

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.

原文???core.languages.en_GB???
頁(從 - 到)121-125
頁數5
期刊Planetary and Space Science
27
發行號2
DOIs
出版狀態已出版 - 2月 1979

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