volume 13, issue S337, P376-377 2017
DOI: 10.1017/s1743921317008420
View full text
Samuel J. McSweeney, N. D. Ramesh Bhat, Steven E. Tremblay, Avinash A. Deshpande

Abstract: AbstractWe observed single pulses from PSR J0034-0721 (B0031-07) simultaneously at the MWA (185 MHz) and the GMRT (610 MHz). Correlation analyses reveal that the phase difference of the average profiles at the two frequencies differs from the phase difference observed between individual subpulses, indicating that the individual emission columns above the pulsar’s rotating carousel of sparks do not evolve in frequency in the same way that the global magnetosphere does. This hints at a possible departure from th…

expand abstract