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The chemical composition of cosmic ray nuclei above 1.3 GeV per nucleus and 23 GeV per nucleusMeasurements made with a balloon-borne counter telescope are reported. The telescope was flown from Palestine, Tex., during the fall of 1971 for a total of 10 hours under an average residual atmospheric depth of 4.4 g per sq cm. The data analysis indicates that the integral flux ratios above 1.3 GeV per nucleus and 23 GeV per nucleus are consistent with energy independence.
Document ID
19740048307
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Badhwar, G. D. (NASA Johnson Space Center Cosmic Ray Group, Houston, Tex., United States)
Osborn, R. W. (Rochester, University Rochester, N.Y., United States)
Date Acquired
August 7, 2013
Publication Date
May 1, 1974
Publication Information
Publication: Astrophysics and Space Science
Volume: 28
Subject Category
Chemistry
Accession Number
74A31057
Distribution Limits
Public
Copyright
Other

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