Detection of Interplanetary Electrons from 18 keV to 1.8 MeV during Solar Quiet Times

Details Detection of Interplanetary Electrons from 18 keV to 1.8 MeV during Solar Quiet Times Detection of Interplanetary Electrons from 18 keV to 1.8 MeV during Solar Quiet Times

Oct 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972phrvl..29.1035l&link_type=abstract

Physical Review Letters, vol. 29, Issue 15, pp. 1035-1038

Physics

12

Scientific paper

We have observed a quiet-time component of interplanetary electrons having energies above solar-wind energies and below those characterized as cosmic radiation. Its energy spectrum generally falls with energy from 18 keV to 1.8 MeV, but shows a feature in the 100-300-keV range. The observed temporal variations of the intensity suggest that the 18-100-keV portion is solar and the 0.3-1.8-MeV portion is galactic in origin. Solar and terrestrial neutron-decay electrons appear inadequate to explain the 100-300-keV feature.

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