Direct observation of individual cosmic ray showers

Details Direct observation of individual cosmic ray showers Direct observation of individual cosmic ray showers

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976natur.264..727o&link_type=abstract

Nature, vol. 264, Dec. 23-30, 1976, p. 727-729. Research supported by the Science Research Council.

Computer Science

13

Cerenkov Counters, Cosmic Ray Showers, Electron Photon Cascades, Light (Visible Radiation), Computerized Simulation, Electromagnetic Pulses, Imaging Techniques, Incident Radiation, Particle Energy, Protons

Scientific paper

The measurements considered were made during winter 1975-76 with an array of eight Cerenkov light detectors spread over an area of 1 sq km at Haverah Park near Harrogate, U.K. The discussed results are based upon a limited sample of showers in which at least six detectors recorded Cerenkov light pulses at distances in the range from 100 to 600 m from the shower core. It is suggested that the approach used in the studies provides a simple, novel, and economic method for the accurate determination of arrival direction, the estimation of primary energy, and the direct observation of the cascade development in individual showers.

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