2020
DOI: 10.48550/arxiv.2005.07244
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Low-frequency observations of giant pulses from ordinary pulsars

A. N. Kazantsev,
M. Yu. Basalaeva

Abstract: We present our results of investigation of the rate of emission of the giant radio pulses (GRPs) from several second period pulsars, observed with Large Phased Array radio telescope of Pushchino Radio Astronomy Observatory at 111 MHz. It was found that for all pulsars detected rate was not constant and changed with time significantly. Abrupt jumps in the rate of GRPs generation were detected for PSR B0950+08 and PSR B1112+50. We found that GRPs of all pulsars have demonstrated very different clustering propert… Show more

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“…5). Meanwhile, Kazantsev & Basalaeva (2020) reported on occurrence of strong pulses at frequencies close to 100 MHz, which come predominantly from the leading part of the two-peaked MP component. This is not supported by our observations (Fig.…”
Section: Phase Of Occurrencementioning
confidence: 99%
“…5). Meanwhile, Kazantsev & Basalaeva (2020) reported on occurrence of strong pulses at frequencies close to 100 MHz, which come predominantly from the leading part of the two-peaked MP component. This is not supported by our observations (Fig.…”
Section: Phase Of Occurrencementioning
confidence: 99%