Energetic particle events /greater than or equal to 30 keV/ of Jovian origin observed by Voyager 1 and 2 in interplanetary space

Details Energetic particle events /greater than or equal to 30 keV/ of Jovian origin observed by Voyager 1 and 2 in interplanetary space Energetic particle events /greater than or equal to 30 keV/ of Jovian origin observed by Voyager 1 and 2 in interplanetary space

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jgr....86.8125z&link_type=abstract

Journal of Geophysical Research, vol. 86, Sept. 30, 1981, p. 8125-8140. Research sponsored by the U.S. Department of Energy;

Physics

45

Energetic Particles, Ion Motion, Jupiter Atmosphere, Planetary Radiation, Voyager Project, Interplanetary Medium, Planetary Magnetospheres, Radiation Counters, Spacecraft Instruments, Temporal Distribution, Jupiter, Particles, Origin, Voyager 1, Voyager 2, Ions, Flux, Lecp, Low Energy Charged Particle Instrument, Observations, Energy, Protons, Helium, Spectrum, Flow, Alfven Speed, Magnetosheath, Magnetosphere, Interplanetary Magnetic Field, Bow Shock, Waves, Acceleration, Models, Data, Composition, Electron

Scientific paper

Detailed observations of ion events of Jovian origin as observed by the low energy charge particle (LECP) instrumentation on Voyager 1 and 2 during the inbound and outbound pass for both spacecraft are reported. The general characteristics of these events are examined, and a comparison is made with similar observations at earth. Careful attention is given to the compositional signature of the Jovian ion events. Two of the specific events discussed in detail are selected to display the range of variability and complexity of the Jovian-produced interplanetary ion events. The observations are seen as strongly implying that the Jovian magnetosphere is the source of a significant fraction of the particles.

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