Abstract
Inference about the origin of the variations can be drawn from measurements of intensity distributions, power spectra and cross correlations between several frequencies.
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References
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LOVELACE, R., CRAFT, H. Intensity Variations of the Pulsar CP 1919. Nature 220, 875–879 (1968). https://doi.org/10.1038/220875a0
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DOI: https://doi.org/10.1038/220875a0
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