对火星轨道变化问题的最后解释(第5/16页)
ection 6also discuss the longternbsp;stabilitythe plary tion and its possible cause.
2 descriptionthe nurical integrations
本部分涉及比较复杂的积分计算，作者君就不贴上来了，贴上来了起点也不一定能成功显示。
2.3 nurical thod
we utilizecondorder wisdoholn sylectic pourintegration thod wisdonbsp;& holn 1991; kinoshita， yoshida & nakai 1991 witpecial startup procedurereduce the truncation errorangle variables，warnbsp;startsaha & treine 1992， 1994.
the stepsize for the nurical integrations8 d throughout all integrationsthe nine pls n1，2，3， whichabout 111the orbital periodthe innersor the deternationstepsize，partly follow the previous nurical integrationall nine plssussn & wisdonbsp;1988， 7.2 d and saha & treine 1994， 22532 d.rounded the decil partthe their stepsizes8ke the stepsiztiple2orderreduce the ulationroundoff errorthe&nbspputatio relationthis， wisdonbsp;& holn 1991 perford nurical integrationsthe outer five plary orbits using the sylectiittepsize400 d， 110.83the orbital perioesult seebe urate enough， which partly justifies our thoddeterning th， since the entricityjupiter 0.05ch sller than thatmercury 0.2，needcare when we&nbsppare these integrations silyterstepsizes.
in the integrationthe outer five pls f，fixed the stepsize400 d.
we adopt gauss&039; f anunctionsthe sylectiother with the thirdorder halley thod danby 1992a solver for keple nuerxinbsp;iterationssethalley&039;s thod15， but they never reached the xinbsp;in anr integrations.
the intervalthe data output200 000 d 547for
本章未完，请点击下一页继续阅读 》》
2 descriptionthe nurical integrations
本部分涉及比较复杂的积分计算，作者君就不贴上来了，贴上来了起点也不一定能成功显示。
2.3 nurical thod
we utilizecondorder wisdoholn sylectic pourintegration thod wisdonbsp;& holn 1991; kinoshita， yoshida & nakai 1991 witpecial startup procedurereduce the truncation errorangle variables，warnbsp;startsaha & treine 1992， 1994.
the stepsize for the nurical integrations8 d throughout all integrationsthe nine pls n1，2，3， whichabout 111the orbital periodthe innersor the deternationstepsize，partly follow the previous nurical integrationall nine plssussn & wisdonbsp;1988， 7.2 d and saha & treine 1994， 22532 d.rounded the decil partthe their stepsizes8ke the stepsiztiple2orderreduce the ulationroundoff errorthe&nbspputatio relationthis， wisdonbsp;& holn 1991 perford nurical integrationsthe outer five plary orbits using the sylectiittepsize400 d， 110.83the orbital perioesult seebe urate enough， which partly justifies our thoddeterning th， since the entricityjupiter 0.05ch sller than thatmercury 0.2，needcare when we&nbsppare these integrations silyterstepsizes.
in the integrationthe outer five pls f，fixed the stepsize400 d.
we adopt gauss&039; f anunctionsthe sylectiother with the thirdorder halley thod danby 1992a solver for keple nuerxinbsp;iterationssethalley&039;s thod15， but they never reached the xinbsp;in anr integrations.
the intervalthe data output200 000 d 547for
本章未完，请点击下一页继续阅读 》》