NASA NTRS · 19720039356
Low-energy solar positrons.
Abstract
Fluxes of solar particles, consistent with Kinsey's (1970) measurements and demodulated in a manner consistent with the cosmic-ray transport equations discussed by Gleeson and Axford (1967), are shown to be able to produce low-energy positrons in the solar atmosphere via unstable CNO beta-particle emitters. Computed positron fluxes are presented for various diffusion coefficient values and compared with measurements of Cline and Hones (1970).
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Gregory, C. T.. 1972-03-01. Low-energy solar positrons.. https://ntrs.nasa.gov/citations/19720039356
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