Source variations of interplanetary Jovian electrons - Voyagers 1 and 2 results

Details Source variations of interplanetary Jovian electrons - Voyagers 1 and 2 results Source variations of interplanetary Jovian electrons - Voyagers 1 and 2 results

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....5..374c&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 5. (A81-12386 02-93) T

Astronomy and Astrophysics

Astronomy

Electron Flux Density, High Energy Electrons, Interplanetary Space, Jupiter Atmosphere, Plasma-Particle Interactions, Spaceborne Astronomy, Cosmic Rays, High Energy Interactions, Planetary Magnetospheres, Solar Wind, Voyager 1 Spacecraft, Voyager 2 Spacecraft

Scientific paper

The large intensity of interplanetary Jovian electrons at 1 AU and near the Jovian magnetosphere have been attributed to the large scale solar wind structure. The only variations that can be definitely attributed to the source (i.e. the magnetosphere) are the 10 hour variations observed within about 1 AU of Jupiter. During the pre-Jupiter-encounter period, the Voyagers 1 and 2 spacecraft are separated by about 1 corotation day, facilitating the separation of variations due to corotating streams, which occur 1 day apart on the two spacecraft

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