On the possible radio-frequency emission from the nuclear active particles in EAS

Details On the possible radio-frequency emission from the nuclear active particles in EAS On the possible radio-frequency emission from the nuclear active particles in EAS

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....6..253b&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 6 (A85-2

Physics

Cosmic Ray Showers, Electron Photon Cascades, Nuclear Particles, Radio Emission, Protons, Radiation Distribution, Space Charge

Scientific paper

The possible contribution of the positively charged nuclear active particles near the core of an extensive air shower to the radio emission is theoretically investigated in order to substantiate the noncorrelation between the very high and the very low radio-frequency emission. The radiation field created by the proton disk and by the electron-positron disk are calculated for frequencies from 2 to 220 MHz at distances R = 40 and 200 m from the axis. The proton field intensity is found to be much lower than that of the electron-positron disk, and is a decreasing function of frequency, which conforms to a previous analysis (Allan, J. R., 1982) of the noncorrelation.

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