Stability of Pulsar Time Scale.

Details Stability of Pulsar Time Scale. Stability of Pulsar Time Scale.

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..16e..62s&link_type=abstract

Nomenclature, Precession and New Models in Fundamental Astronomy, 26th meeting of the IAU, Joint Discussion 16, 22-23 August 200

Astronomy and Astrophysics

Astronomy

Scientific paper

It is well known, that stability of pulsar period in the barycenter of Solar system depends on different effects. The stability is determined by both physical conditions in pulsar and processes along the way of signal propagation which affect the pulse time of arrival (TOA). In the presentation it will be discussed stability of pulsar time scale based on the long term millisecond pulsar timing. It will be considered an influence of the propagation conditions along the pulsar signal way. In this presentation it will be considered an influence of microlensing to TOA, as well. This effect can put a natural limit for pulsar time scale stability.

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