Generalized models are obtained for barycentric pulsar time intervals in reference systems moving in space. It is shown that the observed intervals are determined by pulsar rotation parameters whose values agree in inertial and moving reference systems with an estimated error. Barycentric and topocentric time intervals are compared for pulsars B1937+21 and B0329+54.
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Translated from Izmeritel’naya Tekhnika, No. 5, pp. 40–45, April, 2009.
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Avramenko, A.E. Form invariance of coordinate pulsar time metrics. Meas Tech 52, 501–508 (2009). https://doi.org/10.1007/s11018-009-9298-z
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DOI: https://doi.org/10.1007/s11018-009-9298-z