Abstract
Since 1953 regular observations have been carried out with the Polar photographic tube at Pulkovo [1, 2, 3]. A detailed description of the observational procedure, the data reduction technique, and error sources were given by Potter [4].
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References
Bakhrakh, N.M. (1971) “Short period nutation from observations with the Pulkovo Polar tube”, Izv. Glav. Astron. Obs. Pulkovo, No. 187, 97–108. In Russian.
Bakhrakh, N.M., Kotreleva, O.V., Naumov, V.A. (1988) “Observation results with the Pulkovo Polar tube in 1953–1974”, in Yatskiv, Ya.S. (ed), The Study of the Earth as a Planet by Methods of Geophysics, Geodesy and Astronomy, Naukova Dumka, Kiev, 13–15. In Russian.
Bakhrakh, N.M., Naumov, V.A. (1988) “The Pulkovo Polar tube”, Izv. Glav. Astron. Obs. Pulkovo, No. 205, 18–19. In Russian.
Potter, H.I. (1956) “A method for reducing photographs obtained with a Polar tube”, Izv. Glav. Astron. Obs. Pulkovo, No. 157, 101–119. In Russian.
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© 1990 IAU
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Kotreleva, O.V. (1990). Determination of Nutation Based on Observations with the Pulkovo Polar Tube. In: Lieske, J.H., Abalakin, V.K. (eds) Inertial Coordinate System on the Sky. International Astronomical Union / Union Astronomique Internationale, vol 141. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0613-6_58
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DOI: https://doi.org/10.1007/978-94-009-0613-6_58
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