Analysis of the characteristics of extensive air showers with primary energy less than 2 x 10 to the 14th power eV

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Cosmic Ray Showers, Particle Flux Density, Primary Cosmic Rays, Electron Flux Density, Muons, Photons, Spatial Distribution

Scientific paper

The characteristics of 1354 extensive air showers with a mean particle flux density of 5 to 18 per sq m and 2520 showers with a mean particle flux density greater than 18 per sq m (all of which contained 10,000 to 100,000 electrons) are analyzed. The spatial distribution of electron flux density is examined along with that of the muon component with energy greater than 5 GeV in 'small' showers. The energy flux density of the electron-photon shower component is also investigated. It is found that the energy of the electron-photon component at mountaintop level in a circle 10 m in radius decreases as the number of particles decreases from an initial number of about 30,000 electrons and attains a value of 110 to 140 MeV/electron for showers with approximately 10,000 electrons.

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