Computer Science
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985p%26ss...33..253l&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 33, March 1985, p. 253-262.
Computer Science
9
Geomagnetic Pulsations, Magnetohydrodynamic Waves, Magnetospheric Electron Density, Magnetospheric Instability, Particle Precipitation, Plasma Resonance, Electron Precipitation, Interplanetary Medium, Linear Polarization, Magnetometers, Modulation, Plasmapause, Riometers
Scientific paper
Hydromagnetic wave and modulated particle precipitation data are reported from conjugate areas near the particle-drift shell L of about 4. A modulation of electrons precipitating from the magnetosphere is observed in the conjugate regions when the accompanying hydromagnetic wave period is about 90 s and the wave polarization is linear. When the wave period changes abruptly to about 30 s and the polarizations at the observing stations are no longer linear, the modulation of the precipitating electrons is no longer observed. The change in hydromagnetic wave characteristics does not appear to be related to interplanetary plasma and magnetic field conditions. Rather, it is proposed to arise from a change in the wave generation mechanism from an internal magnetospheric source near the inner edge of the plasmapause (lower frequency) to an externally driven source outside the magnetosphere (higher frequency). This observation of a change in the wave characteristics (frequency and polarization) associated with modulated electron precipitation appears to be related to two previous examples wherein modulated electron precipitation was reported to be closely associated with the existence of a wave resonance region near the observing site.
Lanzerotti Louis J.
Maclennan Carol G.
Rosenberg T. J.
Wolfe Arthur
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