Peculiarities of radio emission from new pulsars at 111 MHz

Peculiarities of radio emission from new pulsars at 111 MHz

Blog Article

The analysis of radio emission of three new pulsars discovered at the Pushchino Radio Astronomy Observatory is presented.The detailed observations were carried out at a frequency of 111 MHz using the large phase array and the standard Cypress digital receiver with a total bandwidth of 2.245 MHz and a time resolution of 2.

46 or 5.12 ms.All pulsars exhibit features of their radiation, the subpulse drift is observed in J0220+3622, the flare activity is exhibited in V Neck Sweaters J0303+2248, and the nulling phenomenon has been detected in J0810+3725.