Geodesic
Применение методов Адамса к решению уравнений движения больших планет, Луны и Солнца
Matematicheskoe Modelirovanie i Kraevye Zadachi, Proceedings of the Third All-Russian Scientific Conference (29–31 May 2006). Part 3, Tome 3 (2006), pp. 13-19.

Voir la notice de l'article provenant de la source Math-Net.Ru

@article{MMKZ_2006_3_a1,
     author = {V. V. Abramov},
     title = {{\CYRP}{\cyrr}{\cyri}{\cyrm}{\cyre}{\cyrn}{\cyre}{\cyrn}{\cyri}{\cyre} {\cyrm}{\cyre}{\cyrt}{\cyro}{\cyrd}{\cyro}{\cyrv} {{\CYRA}{\cyrd}{\cyra}{\cyrm}{\cyrs}{\cyra}} {\cyrk} {\cyrr}{\cyre}{\cyrsh}{\cyre}{\cyrn}{\cyri}{\cyryu} {\cyru}{\cyrr}{\cyra}{\cyrv}{\cyrn}{\cyre}{\cyrn}{\cyri}{\cyrishrt} {\cyrd}{\cyrv}{\cyri}{\cyrzh}{\cyre}{\cyrn}{\cyri}{\cyrya} {\cyrb}{\cyro}{\cyrl}{\cyrsftsn}{\cyrsh}{\cyri}{\cyrh} {\cyrp}{\cyrl}{\cyra}{\cyrn}{\cyre}{\cyrt}, {{\CYRL}{\cyru}{\cyrn}{\cyrery}} {\cyri} {{\CYRS}{\cyro}{\cyrl}{\cyrn}{\cyrc}{\cyra}}},
     journal = {Matematicheskoe Modelirovanie i Kraevye Zadachi},
     pages = {13--19},
     publisher = {mathdoc},
     volume = {3},
     year = {2006},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/MMKZ_2006_3_a1/}
}
TY  - JOUR
AU  - V. V. Abramov
TI  - Применение методов Адамса к решению уравнений движения больших планет, Луны и Солнца
JO  - Matematicheskoe Modelirovanie i Kraevye Zadachi
PY  - 2006
SP  - 13
EP  - 19
VL  - 3
PB  - mathdoc
UR  - http://geodesic.mathdoc.fr/item/MMKZ_2006_3_a1/
LA  - ru
ID  - MMKZ_2006_3_a1
ER  - 
%0 Journal Article
%A V. V. Abramov
%T Применение методов Адамса к решению уравнений движения больших планет, Луны и Солнца
%J Matematicheskoe Modelirovanie i Kraevye Zadachi
%D 2006
%P 13-19
%V 3
%I mathdoc
%U http://geodesic.mathdoc.fr/item/MMKZ_2006_3_a1/
%G ru
%F MMKZ_2006_3_a1
V. V. Abramov. Применение методов Адамса к решению уравнений движения больших планет, Луны и Солнца. Matematicheskoe Modelirovanie i Kraevye Zadachi, Proceedings of the Third All-Russian Scientific Conference (29–31 May 2006). Part 3, Tome 3 (2006), pp. 13-19. http://geodesic.mathdoc.fr/item/MMKZ_2006_3_a1/

[1] Kholl Dzh., Uatt Dzh., Sovremennye chislennye metody resheniya obyknovennykh differentsialnykh uravnenii, Mir, M., 1979

[2] Zausaev A. F., Zausaev A. A., Katalog orbitalnoi evolyutsii korotkoperiodicheskikh komet s 1900 po 2100 gg., Mashinostroenie–1, M., 2005

[3] Standish E. M., “JPL Planetary and Lunar Ephemerides, DE 405 / LE 405”, Jet Prop Lab Technical Report. IOM 312. F-048., 1998, 1–7

[4] Newhall X. X., Standish E. M., Williams Jr. and j. g., “DE 102: a numerically integrated ephemeris of the Moon and planets spanning forty-four centuries”, Astron. Astrophys., 1983, no. 125, 150–167 | Zbl

[5] Everhart E., “Implicit single methods for integrating orbits”, Celestial mechanics, 1974, no. 10, 35–55 | DOI | MR | Zbl

[6] Zausaev A. F., Zausaev A. A., Olkhin A. G., “Primenenie metoda Everkharta 31 poryadka dlya resheniya uravnenii dvizheniya bolshikh planet”, VAK-2004. Gorizonty Vselennoi, Tez. dokl. na Vseros. astronom. konf., MGU, GAISh, M., 2004, 209