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A new method to determine the chemical composition of the cosmic rays beyond 10 to the 15th power eVThe 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.
Document ID
19850025739
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Muraki, Y. (Tokyo Univ. Tanashi, Japan)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2
Subject Category
Space Radiation
Report/Patent Number
OG-5.1-11
Accession Number
85N34052
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850025693Collected WorksNinteenth International Cosmic Ray Conference. OG Sessions, Volume 2
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