Titlebook: High-Precision Earth Rotation and Earth-Moon Dynamics; Lunar Distance and R O. Calame Conference proceedings 1982 D. Reidel Publishing Comp

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The Pole Position in October 1980 as Determined from Lageos Laser DataOn the basis of 223 passes of Lageos Laser Tracking data taken in October 1980 during the MERIT short arc campaign from 13 tracking sites, the pole position was determined in the orbit correction program MGM along with the initial state vector. This analysis was done for a varying time resolution (5–1 days).

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Dependence of the Lunisolar Perturbations in the Earth Rotation on the Adopted Earth ModelIf no perturbation exists, the motion of the Earth around its center of mass would be a rigid rotation around a fixed axis in space with constant angular velocity.

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für etwas verlangsamte Teilnehmende, als auch für Menschen mit leichten kognitiven Beeintr?chtigungen. Weiterführende übungen erg?nzen das Angebot.. .Die Autorinnen führen seit Jahrzehnten Ged?chtnistrainings durch und kennen die Herausforderungen der Praxis. Das Arbeitsbuch bietet Unterstützung bei

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für etwas verlangsamte Teilnehmende, als auch für Menschen mit leichten kognitiven Beeintr?chtigungen. Weiterführende übungen erg?nzen das Angebot.. .Die Autorinnen führen seit Jahrzehnten Ged?chtnistrainings durch und kennen die Herausforderungen der Praxis. Das Arbeitsbuch bietet Unterstützung bei

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Earth rotation from a simultaneous reduction of LLR and LAGEOS laser ranging dataesent the first stages of an investigation to combine LAGEOS and lunar laser ranging observations. It is hoped that the proper implementation of such a process might eliminate the shortcomings inherent in each technique, while accentuating the advantages of each. This has the potential of producing

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Intercomparison of Lunar Laser and Traditional Determinations of Earth Rotationn of UT1, corresponding to a Gaussian filter of the form exp{?t./2σ.} with σ = 10 or 12 days, will usually be a good representation of Earth rotation. However, there appear to be short episodes of high acceleration revealed by the LLR data, showing that there are intervals during which frequent obse