http://arxiv.org/abs/2005.07244
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 properties. Finally, we have carried out the phase analysis of the time of arrival for GRPs and detected their phase with reference to the averaged pulse time of arrival.
A. Kazantsev and M. Basalaeva
Mon, 18 May 20
28/43
Comments: 20 pages, 18 figures
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