The chemical composition of cosmic ray nuclei above 1.3 GeV n?1 and 23 GeV n?1 |
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| Authors: | G D Badhwar R W Osborn |
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| Institution: | (1) Cosmic Ray Group, Johnson Space Center, Houston, Tex., U.S.A.;(2) Dept. of Physics Astronomy, University of Rochester, Rochester, N.Y., U.S.A. |
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| Abstract: | Measurements made with a balloon-borne counter telescope having an exposure factor of 774 m2 sr s are reported. The telescope was flown from Palestine, Tex., during the fall of 1971 for a total of 10 h under an average residual atmospheric depth of 4.4 g cm–2. The data analysis indicates that the integral flux ratios above 1.3 Gev n–1 and 23 GeV n–1 are consistent with energy independence.National Academy of Science-Senior Resident Research Associate |
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