Observations of low energy interplanetary electrons

Details Observations of low energy interplanetary electrons Observations of low energy interplanetary electrons

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....2..758m&link_type=abstract

In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 2. (A76-26851

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4

Electron Energy, Energy Spectra, Interplanetary Magnetic Fields, Magnetic Effects, Satellite Observation, Imp, Jupiter (Planet), Particle Intensity, Planetary Magnetic Fields, Solar Activity Effects, Time Dependence

Scientific paper

Observations of the temporal behavior of low energy (0.16-6 MeV) at 1 AU are reported. The electron intensity is found to vary by a factor of more than five from one quiet time to another, including short-term enhancements of the type reported at higher electron energies. Over a period of about four months, beginning with the time at which the interplanetary field line first connects earth and Jupiter, the magnitude and frequency of the increases grow abruptly and remain high. The observed longitudinal distribution of Jovian electrons could be the result of the interconnection of the interplanetary field with an extended Jovian magnetotail.

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