A new method to determine the chemical composition of the cosmic rays beyond 10 to the 15th power eV

Details A new method to determine the chemical composition of the cosmic rays beyond 10 to the 15th power eV A new method to determine the chemical composition of the cosmic rays beyond 10 to the 15th power eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..177m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 177 (SEE N85-34006 22-93)

Computer Science

Chemical Composition, Energy Spectra, Primary Cosmic Rays, Comparison, Simulation, Solar Cosmic Rays, Spectral Signatures

Scientific paper

The chemical composition of primary cosmic rays beyond 10 to the 15th
power eV could not be measured by the direct method. A more sensitive
method to determine the chemical composition is proposed. The method was
checked by simulation and compared with existing data on Ne-N
sub mu and Ne-N sub gamma.

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