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第76章 对火星轨道变化问题的最后解释(6/12)

ionsofallninelas(±1,2,3),andabout8000000d(~21903yr)fortheintegrationoftheouterfivelas(±).

lthoughnooututfilteringasdonehenthenumericalintegrationsereinrocess,ealiedalo-assfiltertotheraorbitaldataafterehadletedallthecalculations.eeection4.1formoredetail.

2.4rrorestimation

2.4.1elativeerrorsintotalenergyandangularmomentum

ordingtooneofthebasicroertiesofsymlecticintegrators,hichconservethehysicallyconservativequantitiesell(totalorbitalenergyandangularmomentum),ourlong-termnumericalintegrationsseemtohavebeenerformedithverysmallerrors.heaveragedrelativeerrorsoftotalenergy(~10?9)andoftotalangularmomentum(~10?11)haveremainednearlyconstantthroughouttheintegrationeriod(ig.1).hesecialstarturocedure,armstart,ouldhavereducedtheaveragedrelativeerrorintotalenergybyaboutoneorderofmagnitudeormore.

elativenumericalerrorofthetotalangularmomentumδ0andthetotalenergyδ0inournumericalintegrations±1,2,3,hereδandδaretheabsolutechangeofthetotalenergyandtotalangularmomentum,resectively,and0and0aretheirinitialvalues.hehorizontalunitisyr.

otethatdifferentoeratingsystems,differentmathematicallibraries,anddifferenthardarearchitecturesresultindifferentnumericalerrors,throughthevariationsinround-offerrorhandlingandnumericalalgorithms.ntheueranelofig.1,ecanrecognizethissituationinthesecularnumericalerrorinthetotalangularmomentum,hichshouldberigorouslyreservedutomachine-recision.

2.4.2rrorinlaarylongitudes

incethesymlecticmasreservetotalenergyandtotalangularmomentumof-bodydynamicalsystemsinherentlyell,thedegreeoftheirreservationm
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