The chemical composition of cosmic ray nuclei above 1.3 GeV n-1 and 23 GeV n-1

Details The chemical composition of cosmic ray nuclei above 1.3 GeV n-1 and 23 GeV n-1 The chemical composition of cosmic ray nuclei above 1.3 GeV n-1 and 23 GeV n-1

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..28..101b&link_type=abstract

Astrophysics and Space Science, Volume 28, Issue 1, pp.101-109

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

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.

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