Plasma mass density in the plasmatrough: Comparison using ULF waves and CRRES

Physics

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Magnetospheric Physics: Magnetospheric Configuration And Dynamics, Magnetospheric Physics: Mhd Waves And Instabilities, Magnetospheric Physics: Plasma Waves And Instabilities, Magnetospheric Physics: Instruments And Techniques

Scientific paper

Observations of ULF field line resonances detected by seven magnetometers in the Canadian Auroral Network for the OPEN Program Unified Study (CANOPUS) array were used to estimate equatorial cold plasma mass densities in and around the plasmatrough region as a function of both radial distance and time of day. The magnetometers ranged in latitude from Pinawa (L=4.3) to Rankin Inlet (L=12.4). The equatorial cold plasma mass densities were estimated using the T89 magnetic field model, an R-4 plasma density distribution function and the wave equation from cold plasma MHD theory. These ground based plasma mass density estimates were compared to those obtained from the CRRES spacecraft. Typical values obtained from the ground based measurements were ~2H+cm-3 at L~10 to ~10H+cm-3 at L~7. The data recorded on 3 October, 1990 showed excellent agreement with the spacecraft observations for 8.5

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