Primary cosmic ray mass composition from simulation of Cerenkov pulse height spectrum.

Details Primary cosmic ray mass composition from simulation of Cerenkov pulse height spectrum. Primary cosmic ray mass composition from simulation of Cerenkov pulse height spectrum.

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ijpap..28..628b&link_type=abstract

Indian J. Pure Appl. Phys., Vol. 28, No. 11, p. 628 - 631

Physics

Cosmic Rays: Cerenkov Radiation

Scientific paper

Pulse height distribution of Cerenkov radiation associated with extensive air showers (EAS) of primary energy Ep ≥ 1016eV, detected at the Gauhati University air shower array, have been simulated for four different primary mass composition models assuming (1) Cerenkov intensity to be proportional to the track-length integral and (2) lateral distribution as an exponential function. The technique of simulation has been given in detail. Comparison of the simulation results with the experimental data favours a composition having predominantly protons above 1016eV.

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