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- W3100799333 abstract "Our high-time-resolution observations reveal that individual main pulses from the Crab pulsar contain one or more short-lived microbursts. Both the energy and duration of bursts measured above 1 GHz can vary dramatically in less than a millisecond. These fluctuations are too rapid to be caused by propagation through turbulence in the Crab Nebula or in the interstellar medium; they must be intrinsic to the radio emission process in the pulsar. The mean duration of a burst varies with frequency as ν−2, significantly different from the broadening caused by interstellar scattering. We compare the properties of the bursts to some simple models of microstructure in the radio emission region." @default.
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- W3100799333 date "2010-10-05" @default.
- W3100799333 modified "2023-09-26" @default.
- W3100799333 title "SHORT-LIVED RADIO BURSTS FROM THE CRAB PULSAR" @default.
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