Abstract
ON time-scales of 0.1 to 10 ms radio signals from pulsars exhibit irregularities which include sub-millisecond bursts1,2, marching subpulses3, and variations of polarization4,5. We now describe a search for such irregularities in signals from the pulsar NP 0532 in the Crab Nebula.
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References
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STAELIN, D., SUTTON, J. Observed Shapes of Crab Nebula Radio Pulses. Nature 226, 69–70 (1970). https://doi.org/10.1038/226069a0
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DOI: https://doi.org/10.1038/226069a0
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