The interplanetary magnetic field and energetic electrons from Jupiter

Details The interplanetary magnetic field and energetic electrons from Jupiter The interplanetary magnetic field and energetic electrons from Jupiter

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976georl...3..281j&link_type=abstract

Geophysical Research Letters, vol. 3, May 1976, p. 281-283.

Physics

7

High Energy Electrons, Interplanetary Magnetic Fields, Jupiter (Planet), Planetary Radiation, Random Walk, Magnetic Field Configurations, Power Spectra, Relativistic Particles, Solar Wind

Scientific paper

The reported four-month 'season' for observation of Jovian electron events at AU is shown to be a plausible consequence of field-line random walk in the solar wind. Values of the field-line random-walk coefficient deduced earlier in connection with observations of solar protons, photospheric supergranulation, and the interplanetary magnetic-field power spectrum, lead to an approximate value for the spread of Jovian electrons at 1 AU, which corresponds to an approximate four-month duration of events. This model is consistent with a point source at Jupiter.

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