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Journal of Geodesy

, Volume 91, Issue 7, pp 867–880

First Online: 16 January 2017Received: 31 August 2016Accepted: 19 December 2016DOI: 10.1007-s00190-016-0992-8

Cite this article as: Plank, L., Hellerschmied, A., McCallum, J. et al. J Geod 2017 91: 867. doi:10.1007-s00190-016-0992-8


The possibility of observing satellites with the very long baseline interferometry VLBI technique has been discussed for several years in the geodetic community, with observations of either existing satellites of the global navigation satellite systems or of satellites dedicated to realise a space tie. Such observations were carried out using the Australian telescopes in Hobart and Ceduna which, for the first time, integrated all the necessary steps: planning the observations automated scheduling, correlation of the data and the generation of a series of time delay observables suitable for a subsequent geodetic analysis. We report on the development of new and the adaptation of existing routines for observing and data processing, focusing on technology development. The aim was to use methods that are routinely used in geodetic VLBI. A series of test experiments of up to six hours duration was performed, allowing to improve the observations from session to session and revealing new problems still to be solved. The newly developed procedures and programs now enable more observations. Further development assumed, this bears the prospect of being directly applied to the observation of dedicated space-tie satellites.

KeywordsSpace tie Co-location in space Very long baseline interferometry VLBI VLBI satellite tracking Global navigation satellite systems GNSS 

Autor: Lucia Plank - Andreas Hellerschmied - Jamie McCallum - Johannes Böhm - Jim Lovell

Fuente: https://link.springer.com/

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