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NASA NTRS · 19730001651

High frequency Hall current instability

Abstract

The Hall current electrojet instability was studied to determine if it generates VLF hiss in the auroral zone of magnetic substorms. Using the kinetic equations with particle conserving Krook collision operator for electrons and ions, and Poisson's equation, it is shown that in the low frequency region, the range of frequency of unstable modes increases as the electron density increases, and that the high frequency component must be taken into account in calculations of turbulent saturation of the Hall current instability driven beyond threshold. It is concluded that Hall currents can generate waves in the VLF hiss frequency band which are related to local auroral electrojet activity.

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BibTeXRIS

Lee, K., Kennel, C. F., Kindel, J. M.. 1970-08-01. High frequency Hall current instability. https://ntrs.nasa.gov/citations/19730001651

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