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出 处:《天文学报》1996年第4期368-376,共9页Acta Astronomica Sinica
摘 要:本文根据Markov随机过程理论,给出了周年极移振幅ra序列的一阶Markov链概型,并建立了ra序列增加年R与减小年D游程以及(R十D)游程循环(周年极移循环)的概率分布模式,经统计假设检验,一阶Markov链可以很好拟合。序列的变化过程.得到了ra不同状态的平均首次到达时间矩阵,其值大多与实测符合.ra的基本周期为2年、6.07年、6.54年、7.08-8.50年、21.25-28.33年和85年,而6.07年是它的一个主要周期.由Markov链的遍历性定理得到,预报ra时取用在此之前的第6—13个以内的样本为宜.Based upon Markov's random process theory, a Markov chain probablity model of one order corresponding to the series of amplitute (ra) of annual polar motion is given. The probablity models of runs of R (increasing year) and D (decreasing year),and of their run cycle of (R+D), are also established. By means of the statistical hypothesis test, it seems that the Markov chain of one order fits to the change process of ra series. The obtained matrices of average arrival times of different r'a s show that its basic peroids are 2, 6.07, 6.54, 7.08-8.50, 21.25-28.33 and 85 years,and among them 6.07 years is the main one. From the ergodic theorem of Markov chain, the suitable samples are taken from the 6th to 13th points before the predicted point.
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