Su Ding-qian, Wang Ya-nan, Zhou Bi-fang, Lu Sheng-dong
{"title":"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","authors":"Su Ding-qian, Wang Ya-nan, Zhou Bi-fang, Lu Sheng-dong","doi":"10.1016/0146-6364(80)90064-X","DOIUrl":null,"url":null,"abstract":"<div><p>It is shown that if the equipotentials are <em>n</em>-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.</p><p>Based on the above consideration, an algorithm is presented for finding the minimum point of the function <em>φ</em> = <em>Σf</em><sub><em>i</em></sub><sup>2</sup>. At each iteration, we take the linear expansions of <em>f</em><sub><em>i</em></sub> 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.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":"4 1","pages":"Pages 84-89"},"PeriodicalIF":0.0000,"publicationDate":"1980-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0146-6364(80)90064-X","citationCount":"0","resultStr":"{\"title\":\"An algorithm for finding the extreme values of a function of many variables and its application in the automatic design of astronomical optical systems\",\"authors\":\"Su Ding-qian, Wang Ya-nan, Zhou Bi-fang, Lu Sheng-dong\",\"doi\":\"10.1016/0146-6364(80)90064-X\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>It is shown that if the equipotentials are <em>n</em>-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.</p><p>Based on the above consideration, an algorithm is presented for finding the minimum point of the function <em>φ</em> = <em>Σf</em><sub><em>i</em></sub><sup>2</sup>. At each iteration, we take the linear expansions of <em>f</em><sub><em>i</em></sub> 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.</p></div>\",\"PeriodicalId\":100241,\"journal\":{\"name\":\"Chinese Astronomy\",\"volume\":\"4 1\",\"pages\":\"Pages 84-89\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1980-03-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/0146-6364(80)90064-X\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Chinese Astronomy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/014663648090064X\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/014663648090064X","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
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.