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 N sub e-N sub mu and N sub e-N sub gamma

Muraki, Y.

English

NASA Technical Reports Server

177' OG 5. i-ii
A New method to determine the Chemical Composition of the
Cosmic Rays beyond 1015eV
Y. Muraki
Inst. for Cosmic Ray Research, Univ. Of Tokyo, Tanashi, Tokyo
abstract
The chemical composition of primary cosmic rays beyond
1015eV could not be measured by the direct method. Here
I would like to propose more sensitive method to determine
the chemical composition. The idea has been checked by the
simulation and compared with the exsisting data concerning on
N -N and N -N
e _ e y.
The simulation will be also cmpared with the experimental
results coming from ANI experiment in a near future.
https://ntrs.nasa.gov/search.jsp?R=19850025739 2020-03-20T18:01:56+00:00Z


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

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