Fast numerics for the spin orbit equation with realistic tidal dissipation and constant eccentricity
Author:
Funder
University of Surrey
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics,Applied Mathematics,Computational Mathematics,Mathematical Physics,Modeling and Simulation
Link
http://link.springer.com/article/10.1007/s10569-017-9760-1/fulltext.html
Reference16 articles.
1. Bartuccelli, M.V., Deane, J.H.B., Gentile, G.: The high-order Euler method and the spin-orbit model: a fast algorithm for solving differential equations with small, smooth nonlinearity. Celest. Mech. Dyn. Astron. 121(3), 233–260 (2015). doi: 10.1007/s10569-014-9599-7
2. Bartuccelli, M.V., Deane, J.H.B., Gentile, G.: Periodic and quasi-periodic attractors for the spin-orbit model with a realistic tidal torque. (2017) (in preparation)
3. Celletti, A., Chierchia, L.: Measures of basins of attraction in spin-orbit dynamics. Celest. Mech. Dyn. Astron. 101(1–2), 159–170 (2008)
4. Celletti, A., Chierchia, L.: Quasi-periodic attractors in celestial mechanics. Arch. Ration. Mech. Anal. 191(2), 311–345 (2009)
5. Correia, A.C.M., Laskar, J.: Mercury’s capture into the 3/2 spin-orbit resonance as a result of its chaotic dynamics. Nature 429, 848–850 (2004)
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