Construction of the New High-Precision Moon Rotation Series at a Long Time Intervals
By: V. Pashkevich and G. Eroshkin
Open Access
|Jan 2012References
- 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.
- 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).
- 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.
- Newhall X X and Williams J.G. (1997): Estimation of the lunar physical librations, Celestial Mechanics and Dynamical Astronomy, 66, pp. 21-30.
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
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© 2012 V. Pashkevich, G. Eroshkin, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons License.