Individual accuracy checks for massive bodies and particles in symplectic integration

被引：7

作者：

Mikkola, S ^{[1
]}

Innanen, K

机构：

[1] Univ Turku, Tuorla Observ, Piikkio 21500, Finland

[2] York Univ, Dept Phys & Astron, N York, ON M3J 1P3, Canada

来源：

ASTRONOMICAL JOURNAL | 2002年 / 124卷 / 06期

基金：

英国惠康基金; 英国医学研究理事会; 美国国家卫生研究院;

关键词：

celestial mechanics; methods : n-body simulations; methods : numerical; minor planets; asteroids;

D O I：

10.1086/344485

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A simple device to check the individual accuracies of planet and particle trajectories in symplectic integration is proposed, and some tests are presented. Although the significant new feature of the method is that it provides information about the accuracies of massless particle orbits, it can also be usefully applied to objects with finite mass.

引用

收藏

页码：3445 / 3448

页数：4

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