Precipitation of Inner-Zone Electrons by Whistler-Mode Waves from the VLF Transmitters UMS and NWC
Abstract
The precipitation of energetic electrons which are commonly observed in the drift loss cone east of 60 deg longitude between L approximates 1.6 and L approximates 1.8 can be accounted for by a doppler-shifted cyclotron resonance between the electrons and nonducted whistler-mode waves from high-power, ground- based VLF transmitters. A ray-tracing analysis using a diffusive-equilibrium model shows that 17.1 kHz waves starting with vertical wave normals between 23 and 31 deg magnetic latitude cross the magnetic equator between L approximates 1.6 and L approximates 1.8 with wave normals of approximately 63 deg. A relativistic cyclotron-resonance analysis for the same model plasmasphere using the ray-tracing results gives an energy vs L-shell dependence for the precipitated electrons which is in excellent agreement with the observed dependence. The VLF transmitter is most likely the UMS transmitter located near Gorki, U.S.S.R. It transmits on 17.1 kHz. VLF records covering this frequency band were available for only three of the time periods when electrons were observed. In two cases UMS was transmitting at the time period required to account for the observations. In the third case a higher frequency is required to fit the data. At the time, the NWC transmitter at North West Cape, Australia was operating at 22.3 kHz. These data are consistent with a model in which weak pitch-angle scattering by whistler-mode waves from NWC does not completely fill the drift loss cone at the longitude of NWC. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Dec 01, 1980
- Accession Number
- ADA092919
Entities
People
- A. L. Vampola
- B. C. Edgar
- Harry C. Koons
Organizations
- The Aerospace Corporation