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Elemental abundances of cosmic rays with Z33 as measured on HEAO-3The Heavy Nuclei Experiment on HEAO-3 uses a combination of ion chambers and a Cerenkov counter. During analysis, each particle is assigned two parameters Z sub c and Z sub l proportion signal is double valued, a unique assignment of particle charge, Z, is not possible in general. Previous work was limited to particles of either high rigidity or low energy, for which a unique charge assignment was possible, although those subsets contain less than 50% of the total number of particles observed. The use of the maximum likelihood technique to determine abundances for the complete data set from approximately 1.5 to approximately 80 GeV/amu is studied.
Document ID
19850023733
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Newport, B. J.
(California Inst. of Tech. Pasadena, CA, United States)
Stone, E. C.
(California Inst. of Tech. Pasadena, CA, United States)
Waddington, C. J.
(California Inst. of Tech. Pasadena, CA, United States)
Binns, W. R.
(California Inst. of Tech. Pasadena, CA, United States)
Garrard, T. L.
(California Inst. of Tech. Pasadena, CA, United States)
Israel, M. H.
(California Inst. of Tech. Pasadena, CA, United States)
Klarmann, J.
(California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: Washington Univ. Contrib. to the 19th Intern. Cosmic Ray Conf.
Subject Category
Space Radiation
Accession Number
85N32046
Funding Number(s)
CONTRACT_GRANT: NGR-05-002-160
CONTRACT_GRANT: NAG8-500
CONTRACT_GRANT: NGR-26-008-001
CONTRACT_GRANT: NAG8-498
CONTRACT_GRANT: NAG8-502
CONTRACT_GRANT: NGR-24-005-050
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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