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On the Determination of UT1 by the BIH and the U.S.S.R. Time Service

Published online by Cambridge University Press:  14 August 2015

Ya. S. Yatskiv ,
A. A. Korsun'  and
N. T. Mironov
Ya. S. Yatskiv
Affiliation:
Main Astronomical Observatory Ukrainian Academy of Sciences Kiev, U.S.S.R.
A. A. Korsun'
Affiliation:
Main Astronomical Observatory Ukrainian Academy of Sciences Kiev, U.S.S.R.
N. T. Mironov
Affiliation:
Main Astronomical Observatory Ukrainian Academy of Sciences Kiev, U.S.S.R.

Abstract

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The reference systems for the determination of UT1 and polar coordinates are discussed. Some arguments are given in support of the adoption of the mean pole origin (MPO) defined by the mean latitudes of the observatories. Taking into account the frequency response of the filters used by the BIH and the U.S.S.R. Time Service, the effects of the errors of the adopted nutational coefficients and tidal variations of the vertical are estimated.

Type
Part I: Time
Information
Symposium - International Astronomical Union , Volume 82: Time and the Earth's Rotation , 1979 , pp. 29 - 39
Copyright
Copyright © Reidel 1979 

References

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