Abstract
A new method of synchronization of atomic timekeepers on the basis of pulsar time that has been synthesized on the basis of observations of the rotation parameters of a pulsar is considered. An analysis of the attainable synchronization precision is presented.
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A. E. Avramenko, Izmer. Tekh., No. 6, 39 (2006); Measurement Techniques, 49, No. 6, 585 (2006).
B. Guinot and G. Petit, Astron. Astrophys., 248, 292 (1991).
GOST 8.567-99, GSI, Measurement of Time and Frequency: Terms and Definitions [in Russian].
Yu. S. Domain, “Fundamental and applied coordinate-time assurance (KVO-2005),” Proc. All-Russia Conf., St. Petersburg, 2005, p. 105.
G. Petit and P. Tavella, Astron. Astrophys., 308, 290 (1996).
S. I. Donchenko and A. N. Kroshkin, Izmer. Tekh., No. 7, 3 (1999); Measurement Techniques, 42, No. 7, 619 (2006).
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Translated from Izmeritel’naya Tekhnika, No. 7, pp. 23–28, July, 2007.
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Avramenko, A.E. Synchronization on the basis of pulsar time. Meas Tech 50, 725–732 (2007). https://doi.org/10.1007/s11018-007-0139-7
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DOI: https://doi.org/10.1007/s11018-007-0139-7