Observations of ultraheavy cosmic ray particles at 10 GV cutoff rigidity

Details Observations of ultraheavy cosmic ray particles at 10 GV cutoff rigidity Observations of ultraheavy cosmic ray particles at 10 GV cutoff rigidity

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..111y&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 111-114 (SEE N85-34006 22-93)

Computer Science

Sound

Balloon Sounding, Energy Spectra, Gamma Ray Absorption, Primary Cosmic Rays, Balloon-Borne Instruments, Iron, Particle Tracks, Plastics, Radiant Flux Density, Ratios

Scientific paper

Ultraheavy cosmic ray particles with Z > 45 and Fe were observed in two balloon flights at a mean geomagnetic cutoff rigidity of 10 GV. Fluxes of these particles at the top of the atmosphere are presented. A ratio of (Z > 45)/(Fe) is compared with other experimental results. The ratio decreases with increasing energy in the energy range from 1 to 10 GeV/amu. A possibility is presented to explain the variation of the ratio with energy.

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