On the Azimuthal Asymmetry of Cosmic-Ray Intensity above the Atmosphere at the Geomagnetic Equator

Details On the Azimuthal Asymmetry of Cosmic-Ray Intensity above the Atmosphere at the Geomagnetic Equator On the Azimuthal Asymmetry of Cosmic-Ray Intensity above the Atmosphere at the Geomagnetic Equator

Jul 1950

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1950phrv...79...51v&link_type=abstract

Physical Review, vol. 79, Issue 1, pp. 51-53

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By means of Geiger-Mueller tube telescopes in an Aerobee sounding rocket fired to high altitude at the geomagnetic equator, information on the azimuthal asymmetry of the cosmic-ray intensity above the atmosphere has been obtained. These results, in conjunction with previously reported vertical intensities and specific ionizations at λ=0° and λ=41°N, are consistent with the hypothesis that most of the primaries are positively charged protons with differential number spectrum of the form dN=KE-1.9dE in the energy region 5 to 23 Bev.

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