Abundances of energy spectra of individual iron-secondary elements

Details Abundances of energy spectra of individual iron-secondary elements Abundances of energy spectra of individual iron-secondary elements

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....1..323i&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 1. (A81-12386 02-93) T

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Abundance, Balloon Sounding, Energy Spectra, Iron, Secondary Cosmic Rays, Atmospheric Attenuation, Cerenkov Counters, Ionization Chambers, Mass Ratios

Scientific paper

Relative abundances of individual Iron-secondary elements have been measured using a balloon-borne 6.6 m ster ionization/Cerenkov detector system. The unusually large geometry factor and single-charge resolution yield empirical atmospheric attenuation curves for individual elements which combine with high statistics at float altitude to yield individual element abundances, extrapolated to the top of the atmosphere, with high precision. Results are presented for top-of-the-atmosphere abundances (relative to iron) of individual elements in the Z range 13-30.

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