Cosmic ray zenith angle distribution at low geomagnetic latitude

Details Cosmic ray zenith angle distribution at low geomagnetic latitude Cosmic ray zenith angle distribution at low geomagnetic latitude

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sbarm...6..243a&link_type=abstract

SBARMO Bulletin, vol. 6, Dec. 1977, p. 243-261.

Physics

2

Balloon-Borne Instruments, Cosmic Rays, Geomagnetic Latitude, Zenith, Geiger Counters, Radiation Distribution

Scientific paper

The intensity of secondary charged cosmic rays at different zenith angles was measured by narrow angle Geiger-Mueller telescopes up to an atmospheric depth of 2 g per sq cm. The angular distribution observed at high altitudes is nearly flat at small angles around the vertical and suggests that the particle intensity peaks at large zenith angles, close to the horizon.

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