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The Past, Present and Future of Reference Systems for Astronomy and Geodesy

Published online by Cambridge University Press:  19 July 2016

G.A. Wilkins
G.A. Wilkins*
Affiliation:
c/o Royal Greenwich Observatory Madingley Road Cambridge England CB3 OEZ

Abstract

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Standard values of astronomical and geodetic constants were adopted in the late nineteenth century for use in the determination of terrestrial and celestial coordinates, and their values were changed subsequently as better values became known. The great improvements in the precision of observation during the past decade has made it necessary to develop reference systems that also include the models and procedures that are used for the analysis of observations by particular techniques. The accurate detemination of the connections between the corresponding reference frames and the adoption of unified standards are major tasks for the future.

Type
Part 1: The legacy of Pulkovo for inertial systems and reference frames
Information
Symposium - International Astronomical Union , Volume 141: Inertial Coordinate System on the Sky , 1990 , pp. 39 - 46
Copyright
Copyright © Kluwer 1990 

References

Danjon, A., (ed.) 1950. Colloque internationale sur les constantes fondamentales de l'astronomie, Observatoire de Paris, 1950. Bull. Astron. 15, 163–292.Google Scholar
De Sitter, W., 1927. “On the most probable values of some astronomical constants”, Bull. Astron. Inst. Netherlands 4, 57–61.Google Scholar
Duncombe, R.L., Fricke, W., Seidelmann, P.K., and Wilkins, G.A., 1977. “Joint report of the working groups of IAU Commission 4 on precession, planetary ephemerides, units and time-scales”, Trans. IAU 16B, 56–67.Google Scholar
Fricke, W., Brouwer, D., Kovalevsky, J., Mikhailov, A.A., and Wilkins, G.A., 1966. “Report to the [IAU] Executive Committee of the Working Group on the System of Constants”, Trans. IAU 12B, 593–8.Google Scholar
Fricke, W., Schwan, H., and Lederle, T., 1988. Fifth fundamental catalogue (FK5): Part 1 The basic fundamental stars. Veröff. Astron. Rechen-Institut , Heidelberg, No. 32, 1–106. (Distributed 1989.) Google Scholar
Gondhalekar, P.M., (ed.) 1989. Astrometry into the 21st century. Proceedings of workshop held at Abingdon, Oxon, UK, on 1989 May 22-24. Rutherford Appleton Laboratory Report RAL-89-117.Google Scholar
Groten, E. 1989. “Geodesy and astrometry”. In Gondhalekar, 1989, 20–48.Google Scholar
Kovalevsky, J., (ed.) 1965. “XXIe Symposium de l'U.A.I. surle systeme de constantes astronomique”, Bull. Astron. 25, 1–324.Google Scholar
Kovalevsky, J., Mueller, I.I., and Kolaczek, B., (eds) 1989. Reference frames in geodesy and geophysics , Kluwer Academic Publishers, Dordrecht.Google Scholar
McCarthy, D.D., (ed.) 1989. “IERS standards (1989)”, IERS Tech. Note 3.Google Scholar
Melbourne, W., (ed.) 1983. “Project MERIT standards”, US Naval Observatory Circ. No 167.Google Scholar
Mueller, I.I., 1988. “Reference coordinate systems: an update”, Dept. of Geodetic Science and Surveying, Ohio State University , Report No. 394.Google Scholar
IAG 1971. “Geodetic reference system 1967”, Bull. Geodesique Publ. Spec. No. 3.Google Scholar
Moritz, H. 1980. “Geodetic Reference System 1980”, Bull. Geodesique 54, 395–402.Google Scholar
NAO 1961. Explanatory Supplement to the Astronomical Ephemeris , H. M. Stationery Office, London.Google Scholar
NAO 1967. “The introduction of the IAU system of astronomical constants into the Astronomical Ephemeris”, Supplement to the A. E. 1968. Google Scholar
NAO 1983. “The introduction of the improved IAU system of astronomical constants into the Astronomical Almanac”, Supplement to the Astronomical Almanac 1984. Google Scholar
Wilkins, G.A., (ed.) 1980. A review of the techniques to be used during Project merit to monitor the rotation of the Earth. Royal Greenwich Observatory, England, & Institut für Angewandte Geodasie, Germany.Google Scholar
Wilkins, G.A., 1989a. “The connections between terrestrial and celestial reference frames”, In Gondhalekar, 1989, 8–13.Google Scholar
Wilkins, G.A., 1989b. “Standards for terrestrial and celestial reference frames”, In Kovalevsky, et al. 1989, 447–460.Google Scholar
Wilkins, G.A., and Mueller, I.I., 1986. “Joint summary report of the IAU/IUGG working groups on the rotation of the Earth and the terrestrial reference system”, Highlights of Astronomy 7, 771–788.Google Scholar