Peculiarities of Giant Pulses from the Crab Pulsar at Frequencies of 594 and 2228 MHz

Details Peculiarities of Giant Pulses from the Crab Pulsar at Frequencies of 594 and 2228 MHz Peculiarities of Giant Pulses from the Crab Pulsar at Frequencies of 594 and 2228 MHz

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003astl...29..387k&link_type=abstract

Astronomy Letters, vol. 29, p. 387-393 (2003)

Astronomy and Astrophysics

Astronomy

10

Scientific paper

We present the results of our simultaneous observations of giant pulses from the Crab pulsar B0531+21 at frequencies of 594 and 2228 MHz with a high (62.5 ns) time resolution. The pulse broadening by scattering was found to be 25 and 0.4 microsec at 594 and 2228 MHz, respectively. We obtained the original giant-pulse profiles compensated for interstellar scattering. The measured profile widths at the two frequencies are approximately equal, 0.5 microsec; i.e., the giant pulses are narrower than the integrated profile by a factor of about 1000. We detected an extremely high brightness temperature of radio emission, T_b > 1036 K radio emission, which is higher than the previous estimates of this parameter by five orders of magnitude. The decorrelation bandwidth of the radio-spectrum diffraction distortions has been determined for this pulsar for the first time: 10 kHz at 594 MHz and 300 kHz at 2228 MHz.

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