Silicon to iron abundances in solar cosmic rays and in the sun

Details Silicon to iron abundances in solar cosmic rays and in the sun Silicon to iron abundances in solar cosmic rays and in the sun

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..221v&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 221-224 (SEE N85-34729 23-92)

Computer Science

Charged Particles, Energy Spectra, Iron, Silicon, Solar Cosmic Rays, Comparison, Electron Distribution, Particle Density (Concentration), Solar Atmosphere

Scientific paper

Differential spectra of even charged nuclei between Si and Fe in the August 4, 1972 event are made in the energy region of 10 to 40 MeV/n using rocket borne plastic detectors. The resultant relative abundances of elements and low energy (E < 25 MeV/n) enhancements are obtained. Comparison with spectroscopically determined photospheric abundances is also made. The implications of these relative abundances on the acceleration mechanisms is discussed.

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