Dispersion of Cherenkov radio pulse generated by a cascade shower on the Moon surface

Details Dispersion of Cherenkov radio pulse generated by a cascade shower on the Moon surface Dispersion of Cherenkov radio pulse generated by a cascade shower on the Moon surface

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008tephl..34..139f&link_type=abstract

Technical Physics Letters, Volume 34, Issue 2, pp.139-142

Physics

95.55.Vj

Scientific paper

Phenomena accompanying the propagation of a short bipolar radio pulse with duration of ˜1 ns through the Earth’s ionosphere are considered. Such pulses can be generated by a cascade shower caused by an ultrahigh-speed cosmic particle on the Moon’s surface. It is shown that the width of the radio pulse increases by almost two orders of magnitude as a result of dispersion. A method is proposed for retaining the real sensitivity of a detector. The possibility of using dispersion for separating informative signals from local interferences is considered. The power of a cosmic-particle-induced radio signal is compared to the power of cosmic radio-frequency interferences.

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