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Determination of Nutation Based on Observations With the Pulkovo Polar Tube

Published online by Cambridge University Press:  19 July 2016

O.V. Kotreleva
O.V. Kotreleva*
Affiliation:
Central Astronomical Observatory, USSR Academy of Sciences Pulkovo 196140 Leningrad USSR

Extract

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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].

Type
Part 3: Concepts, Definitions, Models
Information
Symposium - International Astronomical Union , Volume 141: Inertial Coordinate System on the Sky , 1990 , pp. 160
Copyright
Copyright © Kluwer 1990 

References

1. 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.Google Scholar
2. 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.Google Scholar
3. Bakhrakh, N.M., Naumov, V.A. (1988) “The Pulkovo Polar tube”, Izv. Glav. Astron. Obs. Pulkovo, No. 205, 18–19. In Russian.Google Scholar
4. 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.Google Scholar