Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-18T11:19:32.806Z Has data issue: false hasContentIssue false

Apport des Observations d’Occultations Stellaires en vue du Rattachement du Systeme Dynamique au Systeme Geometrique

Published online by Cambridge University Press:  12 April 2016

M. Froeschlé
Affiliation:
C.E.R.G.A., Grasse(France)
C. Meyer
Affiliation:
C.E.R.G.A., Grasse(France)

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.

The possibilities of tying the geometrical and dynamical reference frames by use of lunar occultations are reviewed. Actually, the best accuracy available is about 0”.4, essentially limited by stellar positions and limb corrections. One can expect an improvement of one order of magnitude with the accomplishment of POLO and HIPPARCOS Projects.

Type
Research Article
Copyright
Copyright © Reidel 1981

References

Baudry, A.: 1979, Radio astrométrie; principe; précision actuelle et future des mesures de positions, Coll. GS V, Bordeaux.Google Scholar
Calarne, O.: 1975, Etude des mouvements li oratoires lunaires et localisation des stations terrestres à partir de mesures laser de distances, Thèses, Paris.Google Scholar
de Vegt, C., Gehlich, U. K.: 1976, Astron. Astroph., 48, p. 245.Google Scholar
ESA: 1979, HIPPARCOS space astrometry, report on phase A study, SCI (79) 10.Google Scholar
ESA: 1979, Polar orbiting lunar observatory, assessment study, SCI (79) 7.Google Scholar
Evans, D. S.: 1971, in proceedings of the IAU General Assembly, Highlights of Astronomy, de Jager, C. ed., p. 601.Google Scholar
Gaignebet, J.: 1980, Communication personnelle.Google Scholar
Kaula, W. M., Schubert, G., Lingenfelder, R. E., Sjogren, W. L., Wollenhaupt, W. R.: 1974, Proc. Fifth Lunar Conf., 3, p. 3049.Google Scholar
Klock, B. L., Scott, D. K.: 1970, Astr. J., 75, p. 851.Google Scholar
Kovalevsky, J.: 1975, in Space Astrometry, ESRO, SP 108, p. 67.Google Scholar
Kovalevsky, J.: 1979, IAU Symposium No. 82, p. 151.Google Scholar
Meyer, C: 1974, Contribution à la détermination des positions lunaires par l’observation d’occultations au moyen d’un micromètre à double image, Thèses, Paris.Google Scholar
Meyer, C: 1976, The Moon, 16, p. 27.Google Scholar
Meyer, F.: 1978, Méthode pour l’amélioration et l’extension d’un catalogue de profils lunaires, Thèses, Nice.Google Scholar
Migus, A.: 1976, The Moon, 15, p. 165.Google Scholar
Morrison, L. V.: 1971, Proc. IAU Symposium No. 47, p. 395.Google Scholar
Morrison, L. V.: 1979, Mon. Not. R. Astr. Soc., 187, p. 41.Google Scholar
Nather, R. E., Evans, D. S.: 1970, Astr. J., 75, p. 575 and p. 953.Google Scholar
Slade, M. A., Preston, R. A., Harris, A. W., Skjerve, L. J., and Spitzmesser, D. J.: 1977, The Moon, 17, p. 133.CrossRefGoogle Scholar
Valein, J. L.: 1979, Etude de la rotation de la Terre à partir des mesures laser-Lune, Thèses, Paris.Google Scholar
Watts, C. B.: 1963, Astr. Pap. Washington, 17.Google Scholar
Weimer, T.: 1952, Atlas de profils lunaires, Observatoire de Paris.Google Scholar
Weimer, T.: 1954, Recherches sélénographiques: allongement du sélénoide, libration physique, profils lunaires, Thèses, Paris.Google Scholar
Yasuda, H., Miyauchi, N.: 1971, Ann. Tokyo Astr. Obs., 12, p. 188.Google Scholar