The possibility of searching of cosmic rays in the energy range above 10 to the 20th eV

Details The possibility of searching of cosmic rays in the energy range above 10 to the 20th eV The possibility of searching of cosmic rays in the energy range above 10 to the 20th eV

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...11..420d&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 11 (A85-22801

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Cosmic Ray Showers, Energetic Particles, Particle Energy, Radio Echoes, Radio Emission, E Region, Earth Surface, F Region, Particle Mass, Radio Antennas, Radio Scattering

Scientific paper

The use of radio emission reflected and scattered by the earth surface and then by the ionosphere to detect EAS in the energy range above 20 EeV is proposed. Assuming that the scattering angle is 10 deg (a possible value for the scattering angle of the radio emission of the F or E layer of the ionosphere) and directing the antenna at the angle of 30 deg to the horizon, it is possible to scan an effective area 300 x 600 km. Estimates show that the signal would be about 40 microV/m for primary particles with energy 1000 EeV if they exist, and statistics would be about 10 events/yr, disregarding the relic cutoff.

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