Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...200l..45g&link_type=abstract
Astrophysical Journal, vol. 200, Aug. 15, 1975, pt. 2, p. L45-L48.
Astronomy and Astrophysics
Astrophysics
14
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.
Fan Chang-Yun
Gloeckler George
Hovestadt Dieter
Vollmer O.
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