Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-20T12:36:19.235Z Has data issue: false hasContentIssue false
  • English
  • Français

Comparison of the Coordinates of the Pole as Obtained by Classical Astrometry (IPMS, BIH) and as Obtained by Doppler Measurements on Artificial Satellites (Dahlgren Polar Monitoring Service)

Published online by Cambridge University Press:  27 June 2016

M. Feissel ,
B. Guinot  and
N. Taton
M. Feissel
Affiliation:
Observatoire de Paris and Bureau International de l'Heure
B. Guinot
Affiliation:
Observatoire de Paris and Bureau International de l'Heure
N. Taton
Affiliation:
Observatoire de Paris and Bureau International de l'Heure

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Before combining the coordinates of the pole obtained by the Dahlgren Polar Monitoring Service (DPMS) with those of the Bureau International de l'Heure (BIH) we investigated the systematic differences between the two series and their relative weights.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 48: Rotation of the Earth , 1972 , pp. 104 - 111
Copyright
Copyright © Reidel 1972 

References

Anderle, R. J.: 1970, NWL Technical Report TR 2432 (subsequent data were also used before the introduction of the NWL 9 system).Google Scholar
Guinot, B., Feissel, M., and Granveaud, M.: 1971, BIH Annual Report for 1970.Google Scholar