Application of Millisecond Pulsar Timing to the Long-Term Stability of Clock Ensembles

dc.creatorMatsakis, Demetrios N.
dc.creatorFoster, Roger S.
dc.date1995-09-27
dc.date.accessioned2026-07-07T02:20:13Z
dc.date.available2026-07-07T02:20:13Z
dc.descriptionTerrestrial timescales show instabilities due to the physical limitations of the atomic clocks. Stricter environmental isolation and increased numbers of improved cesium clocks and cavity-tuned hydrogen masers have resulted in time scales more accurate by a factor of about five. The use of different clock ensembles results in measurable changes in some millisecond pulsar timing data. We investigate the possible application of millisecond pulsars to define a precise long-term time standard and positional reference system in a nearly inertial reference frame. Although possible quantitative contribution of the two longest studied millisecond pulsars to terrestrial timescales appears minimal, they may prove useful as independent standards in identifying error sources that are difficult to detect due to the finite lifetime and common reference frame of terrestrial clocks. New millisecond pulsars, perhaps some with even better timing properties, may be discovered as a result of the current global pulsar search efforts.
dc.description16 pages, latex, 9 figures, to be published in Amazing Light, Springer-Verlag Press, 1995
dc.identifierhttps://arxiv.org/abs/astro-ph/9509133
dc.identifierhttp://arxiv.org/abs/astro-ph/9509133
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10142
dc.subjectAstrophysics
dc.titleApplication of Millisecond Pulsar Timing to the Long-Term Stability of Clock Ensembles
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