Correlation of the Amplitude of Successive Pulses of CP 0328

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Abstract

AN investigation of the variation in amplitude of individual pulses from pulsars was undertaken on June 29–31 using the 46 m antenna at Algonquin Radio Observatory with the receiver usually used in the long baseline interferometer programme. The system specifications were: right-hand circular polarization, a centre frequency of 408 MHz, r.f. bandwidth of 4 MHz, and a system noise of 300 K. The signals were detected, passed through a low-pass filter of variable bandwidth with the cut-off frequency set to 10 Hz for the observations reported here, and recorded on a high-speed chart recorder. Of the twenty-six pulsars investigated only CP 0328 had sufficiently intense pulses to warrant further analysis. A typical record is shown in Fig. 1.

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References

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    Jones, B., and Wielebinski, R., Astrophys. Lett., 5, 17 (1970).

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SHUTER, W., McCUTCHEON, W. Correlation of the Amplitude of Successive Pulses of CP 0328. Nature 227, 1331–1333 (1970) doi:10.1038/2271331a0

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