New trends in numerical simulation of the motion of small bodies of the solar system

DOI10.1023/A:1012241624469zbMath1002.70010OpenAlexW1614669645MaRDI QIDQ5955268

Alexandr Chernitsov, Tatyana Bordovitsyna, Victor A. Avdyushev

Publication date: 22 April 2002

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1012241624469

zbMATH Keywords

dynamicssolar systemsmall bodiesdomain of motionshigh-accuracy numerical simulation

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Celestial mechanics (70F15) Research exposition (monographs, survey articles) pertaining to mechanics of particles and systems (70-02)

Related Items (4)

Nonlinear methods of statistic simulation of virtual parameter values for investigating uncertainties in orbits determined from observations ⋮ Special perturbation theory methods in celestial mechanics. I: Principles for the construction and substantiation of the application ⋮ Intrinsic nonlinearity and method of disturbed observations in inverse problems of celestial mechanics ⋮ Transition methods for stochastic simulation of parametric uncertainty in inverse problems of orbital dynamics

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