Search for the Giant Pulses Search for the Giant Pulses - an extreme phenomenon in radio pulsar emission

TL;DR

This study reports a survey at 111 MHz using the LPA telescope that detected regular giant pulses from two northern hemisphere pulsars, expanding understanding of extreme pulsar emission phenomena.

Contribution

It presents the first detection of giant pulses from pulsars B1133+16 and B1237+25 at 111 MHz, demonstrating the occurrence of GPs in these sources.

Findings

Detected GPs from pulsars B1133+16 and B1237+25

Survey conducted at 111 MHz with LPA telescope

Confirmed regular generation of strong pulses as GPs

Abstract

Here we present results of our search for Giant Pulses(GPs) from pulsars of Northern Hemisphere. Our survey was carried out at a frequency of 111 MHz using the Large Phased Array (LPA) radio telescope. Up to now we have detected regular generation of strong pulses satisfying the criteria of GPs from 2 pulsars: B1133+16, B1237+25.