Multistep Methods for Integrating the Solar System

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/1721.1/6832

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DC Field	Value	Language
dc.creator	Skordos, Panayotis S.	-
dc.date	2004-10-20T20:00:38Z	-
dc.date	2004-10-20T20:00:38Z	-
dc.date	1988-07-01	-
dc.date.accessioned	2013-10-09T02:47:10Z	-
dc.date.available	2013-10-09T02:47:10Z	-
dc.date.issued	2013-10-09	-
dc.identifier	AITR-1055	-
dc.identifier	http://hdl.handle.net/1721.1/6832	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/xmlui/handle/1721	-
dc.description	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.	-
dc.format	101 p.	-
dc.format	10517978 bytes	-
dc.format	3936933 bytes	-
dc.format	application/postscript	-
dc.format	application/pdf	-
dc.language	en_US	-
dc.relation	AITR-1055	-
dc.subject	numerical integration	-
dc.subject	error analysis	-
dc.subject	solar system	-
dc.subject	stwo-body problem	-
dc.subject	multistep integrators	-
dc.subject	roundoff error	-
dc.title	Multistep Methods for Integrating the Solar System	-
Appears in Collections:	MIT Items

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