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Construction of the Numerical and Semi-Analytical Solutions of the Rigid Earth Rotation at a Long Time Intervals Cover

Construction of the Numerical and Semi-Analytical Solutions of the Rigid Earth Rotation at a Long Time Intervals

By: V.V. Pashkevich  
Open Access
|Feb 2013

References

  1. Eroshkin G.I. (2000): High-Precision method of the Numerical Solution of the Celestial Mechanic problems based on Chebyshev Polynomial Interpolation, In: Book of abstracts, Astrometry, Geodynamics and Celestial Mechanics at the turn of XXIth century, (eds. A.M.Finkelstein et al.) The Conference of the St.Petersburg in the IPA RAS, 19-23 June 2000}, pp. 229-230 (in Russian).
  2. Bretagnon P., Francou G., Rocher P., Simon J.L. (1998) SMART97: a new solution for the rotation of the rigid Earth, Astron. Astrophys., Vol. 329, pp. 329-338.
  3. Eroshkin G.I., Pashkevich V.V. and Brzeziński A. (2002): Extension of the high-precision numerical theory of the rigid Earth rotation to the case of a long time interval, Artificial Satellites, 37, 4, pp. 169-183.
  4. Pashkevich V. V., Eroshkin G. I. (2005) Application of the spectral analysis for the mathematical modelling of the rigid Earth rotation, Artificial Satellites, Vol. 40, No. 4, pp. 251-259.
  5. Standish E. M. (1998) JPL Planetary and Lunar Ephemerides, DE405/LE405, JPL Interoffice Memorandum 312.F-98-048.
DOI: https://doi.org/10.2478/arsa-2013-0003 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859
Language: English
Page range: 25 - 37
Published on: Feb 12, 2013
Published by: Polish Academy of Sciences, Space Research Centre
In partnership with: Paradigm Publishing Services
Publication frequency: 4 issues per year

© 2013 V.V. Pashkevich, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons License.