Physics
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jteph..53.1222f&link_type=abstract
Technical Physics, Volume 53, Issue 9, pp.1222-1228
Physics
95.55.Vj
Scientific paper
Possible reasons for the absence of direct observations of individual events in measuring the super-high-energy particle flux by the radio astronomy technique are considered. One of these reasons is probably associated with the choice of extremely high frequencies (˜1.5 GHz) for detecting radio pulses. Calculations show that the radiation intensity attains its peak value at frequencies ˜500 600 MHz and then sharply decreases so that it becomes three orders of magnitude lower even at a frequency of ˜1.5 GHz. The effectiveness of particle detection in the range of high (˜600 MHz) and low (˜60 MHz) frequencies is analyzed.
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