Extended Data Fig. 4: The pulses of PSR B2111+46 observed by FAST in the session on on 2022-03-08. | Nature Astronomy

Extended Data Fig. 4: The pulses of PSR B2111+46 observed by FAST in the session on on 2022-03-08.

From: Strong and weak pulsar radio emission due to thunderstorms and raindrops of particles in the magnetosphere

Extended Data Fig. 4

The left-most panel is the train of individual pulses for 7098 periods, with the mean profile shown in the bottom and the intensity of which is normalized using the peak value. The total energy of every individual pulse is plotted in the immediately right. A segment of the pulse stack is shown in grey for high quality individual pulses, with a dwarf pulse in period of No.5895 and two partial nullings in the period No. 5891 and 5897. The detailed polarization profiles for 4 pulses are presented in the right 4 panels, each with total intensity I, linear polarization L and circularpolarization V in the bottom subpanel and P A in the upper subpanel. The polarization profiles of the mean pulse are shown in dashed line in these subpanels for comparison. The error bar for PA is ± 1σ.

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