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- W2025683429 endingPage "1038" @default.
- W2025683429 startingPage "1035" @default.
- W2025683429 abstract "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." @default.
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- W2025683429 date "1972-10-09" @default.
- W2025683429 modified "2023-09-26" @default.
- W2025683429 title "Detection of Interplanetary Electrons from 18 keV to 1.8 MeV during Solar Quiet Times" @default.
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- W2025683429 doi "https://doi.org/10.1103/physrevlett.29.1035" @default.
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