Extended Data Fig. 3: The pulses of PSR B2111+46 observed by FAST in the session on 2020-09-17. | Nature Astronomy

Extended Data Fig. 3: The pulses of PSR B2111+46 observed by FAST in the session on 2020-09-17.

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

Extended Data Fig. 3

The left-most panel is the train of individual pulses for 885 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 the period No. 136 and partial nulling in the period No. 137. The detailed polarization profiles for 4 pulses are presented in the right 4 panels, each with total intensity I, linear polarization L and circular polarization 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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