Title of article :
Contribution of laser ranging to Earthʹs sciences
Author/Authors :
Exertier، نويسنده , , Pierre and Bonnefond، نويسنده , , Pascal and Deleflie، نويسنده , , Florent and Barlier، نويسنده , , François and Kasser، نويسنده , , Michel and Biancale، نويسنده , , Richard and Ménard، نويسنده , , Yves، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2006
Abstract :
Satellite and Lunar Laser Ranging (SLR and LLR, respectively) are based on a direct measurement of a distance by exactly measuring the time transit of a laser beam between a station and a space target. These techniques have proven to be very efficient methods for contributing to the tracking of both artificial satellites and the Moon, and for determining accurately their orbit and the associated geodynamical parameters, although hampered by the non-worldwide coverage and the meteorological conditions. Since more than 40 years, the French community (today ‘Observatoire de la Côte dʹAzur’, CNES, ‘Observatoire de Paris’, and IGN) is largely involved in the technological developments as well as in the scientific achievements. The role of the laser technique has greatly evolved thanks to the success of GPS and DORIS; the laser technique teams have learnt to focus their effort in fields where this technique is totally specific and irreplaceable.
le of SLR data in the determination of terrestrial reference systems and in the modelling of the first terms of the gravity field (including the terrestrial constant GM that defines the scale of orbits) has to be emphasized, which is of primary importance in orbitography, whatever the tracking technique used. In addition, the role of LLR data (with two main stations, at Mac Donald (United States) and Grasse (France), since 30 years) has been of particular importance for improving solar system ephemeris and contributing to some features of fundamental physics (equivalence principle). Today, the role of the SLR technique is (i) to determine and to maintain the scale factor of the global terrestrial reference frame, (ii) to strengthen the vertical component (including velocity) of the positioning, which is crucial for altimetry missions and tectonic motions, (iii) to locate the geocenter with respect to the Earthʹs crust, (iv) to avoid any secular and undesirable drift of geodetic systems thanks to a very good accuracy.
he future of this technique is to enlarge the technical capability of laser ranging stations for long distances, that is the tracking of space targets orbiting through the Solar System. In addition, the laser technique should participate into time transfer experiments and improve, with mobile systems like the FTLRS and the new SLR2000 concept, the coverage of the international laser network (ILRS). To cite this article: P. Exertier et al., C. R. Geoscience 338 (2006).
Keywords :
Space geodesy , Terrestrial reference frame , Laser ranging , géodésie spatiale , Système de référence , Télémétrie laser sur satellites et sur la Lune , Métrologie optique
Journal title :
Comptes Rendus Geoscience
Journal title :
Comptes Rendus Geoscience