Abundance enhancements of silicon to iron in solar energetic particles and their implications

Details Abundance enhancements of silicon to iron in solar energetic particles and their implications Abundance enhancements of silicon to iron in solar energetic particles and their implications

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.149..241v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 149, no. 2, Nov. 1988, p. 241-254.

Astronomy and Astrophysics

Astrophysics

2

Energetic Particles, Iron, Silicon, Solar Cosmic Rays, Abundance, Photosphere, Polycarbonates

Scientific paper

Differential energy spectra of low abundant elements between silicon and iron of energetic solar particles (SEP) in the August 4, 1972 event were measured in the energy region of 10 to 40 MeV amu-1 using rocket-borne Lexan detectors. The relative abundances of elements were determined and abundance enhancements, i.e., SEP/photospheric ratios, and their energy dependence were derived in 10 - 40 MeV amu-1 interval. It is found that there are four types of abundance enhancements as a function of energy.

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