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.
Keep this discovery
Explore connections, maps & timelines
Lee, K., Kennel, C. F., Kindel, J. M.. 1970-08-01. High frequency Hall current instability. https://ntrs.nasa.gov/citations/19730001651
Cite the original work for its findings. Save a collection to share your selection of sources.