Research of stability of solution of motion equations for small bodies of Solar system when using Adams-Moulton method
V. V. Abramov
Vestnik Samarskogo Gosudarstvennogo Tehničeskogo Universiteta. Seriâ: Fiziko-Matematičeskie Nauki · 2007
doi:10.14498/vsgtu510 (opens in a new tab)
We email you when a new notice or a question about this paper appears.
Abstract
Using the Adams-Moulton method we research evolution of orbits of small bodies of Solar system, having few close encounters on chosen time interval. The analysis of stability of numerical integration of motion differential equations is made. The obtained results show the convergence of solution.
Abstract licence: CC BY
References2
2 more references, whose wording the paper’s licence keeps private.
Reads
Read by people on this page
None yet.
Checked or read by AI through naulon
None yet.
A person counts once a day per paper. We keep no cookie and no address: a reader is a hash that changes every day. Any month under five reads shows no number.
Are you an author?
Is this your paper?
Claim it to add your note and be paid when agents cite it. Free.