It is shown that there is a parametric connection between the dispersion measure and the observed pulsar rotation period. The conditions for them to agree are determined, and theoretical relations and numerical estimates are obtained.
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Translated from Izmeritel’naya Tekhnika, No. 5, pp. 43–48, May, 2010.
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Avramenko, A.E. Parametric matching of the dispersion measure in observed pulsar time intervals. Meas Tech 53, 525–532 (2010). https://doi.org/10.1007/s11018-010-9537-3
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DOI: https://doi.org/10.1007/s11018-010-9537-3