Features of the process of comparing atomic scales on the basis of pulsar time intervals are considered. Parametric and numerical dependences of the deviations of the intervals, the observed rotation period of a pulsar, and corrections with respect to an independent time standard are determined. Experimental confirmations of the computed characteristics of comparisons of the quantum cesium standard from timekeeping data of the pulsar J1640 + 22 are obtained.
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I. Yu. Blinov and I. A. Driga, “A study of methods of measuring the spectral density of the power of the phase noise of precision quantum frequency and time standards,” Izmer. Tekhn., No. 10, 12–15 (2009); Measur. Techn., 52, No. 10, 1041–1046 (2009).
A. E. Avramenko, “The parametric stability of pulsar time,” Izmer. Tekhn., No. 7, 32–37 (2008); Measur. Techn., 51, No. 7, 747–754 (2008).
A. E. Avramenko, “Synchronization on the basis of pulsar time,” Izmer. Tekhn., No. 7, 23–28 (2007); Measur. Techn., 50, No. 7, 725–732 (2007).
V. A. Potapov et al., “Results of chronometry of the double millisecond pulsar J1640 + 22 using the RT-64 radio telescope in Kalyazin,” Pisma Astron. Zh., 29, No. 4, 282–287 (2003).
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Translated from Izmeritel’naya Tekhnika, No. 3, pp. 43–47, March, 2011.
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Avramenko, A.E., Blinov, I.Y., Goncharov, A.S. et al. Comparison of atomic scales on the basis of pulsar time. Meas Tech 54, 310–317 (2011). https://doi.org/10.1007/s11018-011-9725-9
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DOI: https://doi.org/10.1007/s11018-011-9725-9