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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