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Construction of the New High-Precision Moon Rotation Series at a Long Time Intervals Cover

Construction of the New High-Precision Moon Rotation Series at a Long Time Intervals

By: V. Pashkevich and  G. Eroshkin  
Open Access
|Jan 2012

References

  1. Belikov M.V. (1990): Methods of numerical integration with uniform and mean square approximation for solving problems of ephemeris astronomy and satellite geodesy, Manus. Geod., 15, No4, pp.182-200.
  2. Eroshkin G.I., Taibatorov K.A., Trubitsina A.A. (1993): Constructing the specialized numerical ephemerides of the Moon and the Sun for solving the problems of the Earth's artificial satellite dynamics, ITA RAS, Preprint No 31, (in Russian).
  3. Pashkevich V.V., Eroshkin G.I. (2010): Application of the spectral analysis for modeling the rotations of the Moon, Artificial Satellites, 45, 4, pp. 153-162.
  4. Newhall X X and Williams J.G. (1997): Estimation of the lunar physical librations, Celestial Mechanics and Dynamical Astronomy, 66, pp. 21-30.
DOI: https://doi.org/10.2478/v10018-011-0013-3 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859
Language: English
Page range: 63 - 73
Published on: Jan 3, 2012
Published by: Polish Academy of Sciences, Space Research Centre
In partnership with: Paradigm Publishing Services
Publication frequency: 4 issues per year

© 2012 V. Pashkevich, G. Eroshkin, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons License.

Volume 46 (2011): Issue 2 (June 2011)