Multistep Methods for Integrating the Solar System
| dc.date.accessioned | 2004-10-20T20:00:38Z | |
| dc.date.accessioned | 2018-11-24T10:22:03Z | |
| dc.date.available | 2004-10-20T20:00:38Z | |
| dc.date.available | 2018-11-24T10:22:03Z | |
| dc.date.issued | 1988-07-01 | en_US |
| dc.identifier.uri | http://hdl.handle.net/1721.1/6832 | |
| dc.identifier.uri | http://repository.aust.edu.ng/xmlui/handle/1721.1/6832 | |
| dc.description.abstract | High order multistep methods, run at constant stepsize, are very effective for integrating the Newtonian solar system for extended periods of time. I have studied the stability and error growth of these methods when applied to harmonic oscillators and two-body systems like the Sun-Jupiter pair. I have also tried to design better multistep integrators than the traditional Stormer and Cowell methods, and I have found a few interesting ones. | en_US |
| dc.format.extent | 101 p. | en_US |
| dc.format.extent | 10517978 bytes | |
| dc.format.extent | 3936933 bytes | |
| dc.language.iso | en_US | |
| dc.subject | numerical integration | en_US |
| dc.subject | error analysis | en_US |
| dc.subject | solar system | en_US |
| dc.subject | stwo-body problem | en_US |
| dc.subject | multistep integrators | en_US |
| dc.subject | roundoff error | en_US |
| dc.title | Multistep Methods for Integrating the Solar System | en_US |
Files in this item
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| AITR-1055.pdf | 3.936Mb | application/pdf | View/ |
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