Study on the structure functions of electrons and the energy flow in the soft component of cosmic-ray extensive air showers

Details Study on the structure functions of electrons and the energy flow in the soft component of cosmic-ray extensive air showers Study on the structure functions of electrons and the energy flow in the soft component of cosmic-ray extensive air showers

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ncimc..13..677b&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 13 C, July-Aug. 1990, p. 677-689.

Computer Science

1

Cosmic Ray Showers, Electron Density (Concentration), Electron Distribution, Iterative Solution, Monte Carlo Method

Scientific paper

Cosmic-ray air shower structure functions for the distance dependence of electron density in cosmic-ray air showers in the size range 10 to the 4th - 10 to the 8th have been computed for their intercomparison and comparison with Monte Carlo simulation results and measurements from recent experiments. The analysis has yielded the present status of theoretical structure functions vis a vis experimental results and Monte Carlo simulation distributions. The effect of core location error on the lateral distribution of electrons is also discussed from the point of view of different theoretical and experimental results. The energy flow in the soft component of air showers of size 4 x 10 to the 5th has been evaluated within a ring of radius 10 m about the axis of the showers.

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