Unusual emission of iron nuclei from the sun

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Abundance, Heavy Nuclei, Iron, Solar Cosmic Rays, Emission Spectra, Oxygen Spectra, Solar Corona, Solar Corpuscular Radiation, Solar Protons, Solar Spectra

Scientific paper

Sustained emission of low-energy solar particles with a composition richer in iron than oxygen has been observed during the time period May 7-17, 1974. Between 0.7 and 4 MeV per nucleon the relative abundances of C:O:Fe are 0.65:1:1.35. We suggest that these observations provide an indication of the effects of heavy-ion enrichment in the lower corona of the sun.

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