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Pioneer 10 Doppler data analysis: Disentangling periodic and secular anomalies
Authors:A. Levy,B. Christophe,P. Bé  rio,G. Mé  tris,J.-M. Courty,S. Reynaud
Affiliation:1. ONERA/DMPH, 29 av. Division Leclerc, F-92322 Chatillon, France;2. Geoscience Azur, Université Nice Sophia-Antipolis, OCA, Avenue Copernic F-06130 Grasse, France;3. LKB, UPMC, Case 74, CNRS, ENS, F-75252 Paris cedex 05, France
Abstract:
This paper reports the results of an analysis of the Doppler tracking data of Pioneer probes which did show an anomalous behaviour. A software has been developed for the sake of performing a data analysis as independent as possible from that of Anderson et al. [Anderson, J., Laing, P.A., Lau, E.L., Liu, A.S., Nieto, M.M., Turyshev, S.G. Study of the anomalous acceleration of Pioneer 10 and 11. Phys. Rev. D 65, 082004, 2002], using the same data set. A first output of this new analysis is a confirmation of the existence of a secular anomaly with an amplitude about 0.8 nm s−2 compatible with that reported by Anderson et al. A second output is the study of periodic variations of the anomaly, which we characterize as functions of the azimuthal angle φφ defined by the directions Sun–Earth Antenna and Sun-Pioneer. An improved fit is obtained with periodic variations written as the sum of a secular acceleration and two sinusoids of the angles φφ and 2φ2φ. The tests which have been performed for assessing the robustness of these results are presented.
Keywords:Pioneer anomaly   Doppler tracking data   Interplanetary trajectography
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