求多变量函数极值的算法及其在天文光学系统自动设计中的应用

Su Ding-qian, Wang Ya-nan, Zhou Bi-fang, Lu Sheng-dong
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引用次数: 0

摘要

结果表明,当等势为n维椭球时,流线会向代表最小势的椭球中心收敛,并且流线会越来越靠近椭球的最长存在线。基于以上考虑,提出了一种求函数φ = Σfi2的最小值点的算法。在每次迭代中,我们对fi进行线性展开,并沿着与结果近似φ对应的流线进行,其中等势为椭球体。当我们接近椭球体的最长轴时,我们沿着连接当前点到椭球体中心的线进行适当的跳跃,开始下一次迭代。该方法在天文光学系统的自动设计中得到了很好的应用。给出了三个例子。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
An algorithm for finding the extreme values of a function of many variables and its application in the automatic design of astronomical optical systems

It is shown that if the equipotentials are n-dimensional ellipsoids, then the streamlines will converge to the centre of the ellipsoids representing minimum potential, and in doing so, the streamlines will get closer and closer to the longest axist of the ellipsoids.

Based on the above consideration, an algorithm is presented for finding the minimum point of the function φ = Σfi2. At each iteration, we take the linear expansions of fi and proceed along the streamlines corresponding to the resulting, approximate φ, of which the equipotentials are ellipsoids. When we are close to the longest axis of the ellipsoids, we take a suitable leap along the line joining the current point to the centre of the ellipsoid, to begin the next iteration. This method has been found effective in the automatic design of astronomical optical systems. Three examples are given.

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