Results of three-frequency monitoring of giant pulses from the crab pulsar

• Published in: Astronomy reports 2008-11, Vol.52 (11), p.900-909
• Main Authors: Popov, M. V., Soglasnov, V. A., Kondrat’ev, V. I., Bilous, A. V., Sazankov, S. V., Smirnov, A. I., Kanevskiĭ, B. Z., Oreshko, V. V., Ilyasov, Yu. P.
• Format: Article
• Language: English
• Subjects: Astronomy; Astrophysics; Observations and Techniques; Physics; Physics and Astronomy; Pulsars; Radio astronomy; Radio telescopes
• ISSN: 1063-7729; 1562-6881
• DOI: 10.1134/S1063772908110048

We present the results of long-term, three-frequency monitoring of giant pulses from the Crab pulsar on the 64-m radio telescope in Kalyazin. The total monitoring time was 160 hours. The signal power was recorded simultaneously at 600, 1650, and 4850 MHz via direct sampling of the received signals in the total receiver bandwidth without any compensation for interstellar dispersion. In total, 1117 and 352 giant pulses were detected at 600 and 4850 MHz, respectively. The frequency band centered at 1650 MHz was contaminated by interference, and was used only to identify events found in other frequency bands. The cumulative energy distribution of the giant pulses follows a power law at 600 and 4850 MHz up to the highest energies. A deep modulation in the radio spectra of individual giant pulses was observed on both large (Δ v/v ≈ 0.5) and small (Δ v/v ≈ (2−4) × 10 −3 ) frequency scales. The simultaneous appearance of giant pulses at the interpulse longitudes at high (4850 MHz) and low (1650 and/or 600 MHz) frequencies testifies to their common origin, in spite of the observed differences in other parameters.