The Jovian relativistic electron distribution in interplanetary space from 1 to 11 AU - Evidence for a continuously emitting 'point' source

Details The Jovian relativistic electron distribution in interplanetary space from 1 to 11 AU - Evidence for a continuously emitting 'point' source The Jovian relativistic electron distribution in interplanetary space from 1 to 11 AU - Evidence for a continuously emitting 'point' source

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...215l..89p&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 215, July 15, 1977, p. L89-L93.

Astronomy and Astrophysics

Astrophysics

10

Electron Distribution, High Energy Electrons, Interplanetary Space, Jupiter Atmosphere, Relativistic Particles, Pioneer 10 Space Probe, Planetary Environments, Planetary Magnetospheres, Proton Energy, Spatial Distribution

Scientific paper

From observations of Jovian electrons with instrumentation on the Pioneer 10 spacecraft, it is concluded from both their spatial distribution and their modulation in interplanetary space by solar corotating interaction regions (CIRs) that, whatever the scale size of the Jovian magnetotail, the escape of relativistic electrons occurs within 1 AU of the planet. Thus, on the large scale of the heliosphere, Jupiter appears as a continuously emitting 'point source'. The close approach of the spacecraft at 9.6 AU to a possible extension of a magnetotail early in 1976 is discussed. From recurring intensity increases of approximately 1-MeV protons, it is concluded that CIRs have not dissipated even at about 11 AU.

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