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This article is the second in the series that analyze about 1.87 million
periods of Crab pulsar, observed by the PCA detector aboard the RXTE x-ray
observatory. At these energies the pulsar displays none of the three phenomena
that are often seen in normal radio pulsars – pulse nulling'', systematic
sub pulse drifting’’ and ``mode changing’'. Presence or absence of these three
behavior in the Crab pulsar, at radio wavelengths, something that has not been
rigorously established yet, might be important for a satisfactory understanding
of the above three phenomena.

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