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Primary cosmic ray spectra in the range 20-60 GeV/nEnergy spectra for primary cosmic rays C-Fe above 20 GeV/n were measured on a balloon flight from Greenville S.C. in June 1982 with a hybrid electronic counter-emulsion chamber experiment. Fluxes above the atmosphere appear in general agreement with previously published values. The heavy events included in this data will be used along with the JACEE passive chamber data to provide a heavy composition direct measurement from 10 to the 12th power to approximately 10 to the 15th power eV total energy.
Document ID
19850025702
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Burnett, T. H. (Washington Univ. Huntsville, AL, United States)
Dake, S. (Kobe Univ. Huntsville, AL, United States)
Derrickson, J. H. (NASA Marshall Space Flight Center Huntsville, United States)
Fuki, M. (Okayama Univ. of Science Huntsville, United States)
Fountain, W. F. (NASA Marshall Space Flight Center Krakow, United States)
Gregory, J. C. (Alabama Univ. Huntsville, AL, United States)
Hayashi, T. (Kobe Univ.)
Hayashi, T. (Alabama Univ.)
Holynski, R. (Inst. for Nuclear Physics)
Iwai, J. (Washington Univ.)
Jones, W. V. (NASA Marshall Space Flight Center)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 2
Subject Category
Space Radiation
Report/Patent Number
OG-4.1-9
Accession Number
85N34015
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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