UDC: 
1 Tolchelnikova S.A.
Year: 
№: 
848
Pages: 
3-11

Central Astronomical Observatory at Pulkovo of RAS

1, 
Abstract:
Astronomers have been using the coordinates of stars (or quasars) in studies of motions of the Earth‘s pole and terrestrial points although the terrestrial coordinate system – λ, Φ – was already established. The method is explained of global solution of the equations of observations from different places on the Earth in order to obtain the mean coordinates λ, Φ and those of stars a, b, – linked to the direction of the plumb line of equatorial observatory А with zero stars – longitude. The relation is shown between motions of the Earth’s pole and observations from point А, and possibility of using it as an initial point of International astronomical-geodetic net.
Citation:
Tolchelnikova S.A., 
(2011) Substantiation of a new method for determination the average motion of the pole and observation stations. Geodesy and cartography = Geodezia i Kartografia, 72(3), pp. 3-11. (In Russian).
Publication History
Published: 20.04.2011

Content

2011 March DOI:
10.22389/0016-7126

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