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The three major phenomena of subpulse drifting, nulling and mode changing associated with single pulse variations are prominently seen in these observations. The pulsar has a single component conal profile and the single pulses are primarily in the ``normal'' drift mode with periodicity ($P_3$) 11.1$\\pm$0.5 $P$ for 96\\% of the observing duration, while the shorter duration ``slow-drift'' mode has $P_3$ = 15.7$\\pm$1.2 $P$. 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