Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...2e..12u&link_type=abstract
On the Present and Future of Pulsar Astronomy, 26th meeting of the IAU, Joint Discussion 2, 16-17 August, 2006, Prague, Czech Re
Astronomy and Astrophysics
Astronomy
Scientific paper
Radio emission of single pulses for five pulsars (PSR 0809+74; 0834+06; 0950+08; 0943+10; 1133+16) was found at frequencies 18-30 MHz. The radio emission is caused by the strong sub-pulses that have peak intensity of more than 20 times larger than peak intensity of average profiles. The intensity of single pulses has a strong variation in frequency and time. The probability of detection of the anomalous intense pulses does not exceed several percents at Decameter wave range. Usually such pulses are detected in short series (not more than 10 pulses). Typical band values of detection for the pulses with anomalous intensities lie in the range from 0.2 to 0.5 octaves.
Konovalenko Aleksander
Lecacheux Alain
Rosolen Carlo
Rucker Helmet O.
Ulyanov Oleg M.
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