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Submillisecond Radio Intensity Variations in Pulsars

Nature volume 218, pages 1122–1124 (1968)Cite this article

An Erratum to this article was published on 01 July 1968

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Abstract

Two pulsars have been observed with a time resolution of 0.1 ms using the 1,000 ft radio telescope at Arecibo, revealing structure showing circular polarization within the pulses.

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  • 01 July 1968

    In the article "Submillisecond Radio Intensity Variations in Pulsars" by H. D. Craft, jun., J. M. Cornelia and F. D. Drake (Nature, 218, 1122; 1968) the last sentence of the first paragraph should read "Similar short time structure for CP 0950 at a frequency of 2,295 MHz was also reported at the conference by R.

References

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Authors and Affiliations

  1. Cornell-Sydney University Astronomy Center, Arecibo Ionospheric Observatory, Arecibo, Puerto Rico

    H. D. CRAFT jun., J. M. COMELLA & F. D. DRAKE

Authors
  1. H. D. CRAFT jun.
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  2. J. M. COMELLA
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  3. F. D. DRAKE
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CRAFT, H., COMELLA, J. & DRAKE, F. Submillisecond Radio Intensity Variations in Pulsars. Nature 218, 1122–1124 (1968). https://doi.org/10.1038/2181122a0

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