The pulsating magnetosphere and flux transfer events

Details The pulsating magnetosphere and flux transfer events The pulsating magnetosphere and flux transfer events

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19.1615p&link_type=abstract

Geophysical Research Letters (ISSN 0094-8534), vol. 19, no. 15, Aug. 3, 1992, p. 1615-1618. Research supported by NASA, U.S. Nav

Physics

11

Energetic Particles, Flux Transfer Events, Magnetospheric Instability, Particle Precipitation, Solar Terrestrial Interactions, Ampte (Satellites), Goes Satellites, Solar Wind, Viking Spacecraft

Scientific paper

The possible sources of magnetic field variations in the magnetosphere, the precipitation of energetic particles, and auroral emissions are investigated using magnetic field observations from the GOES 5, GOES 6, AMPTE/CCE, and Viking satellites and a ground station. An analysis of the observations supports the view that the magnetosphere often varies in a periodic way because of its own resonant processes and processes driven by the solar wind. UV images from Viking are used to examine the patterns of precipitating particles in the lower ionosphere.

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