Evolution strategies optimization of the multiple Fabry-Perot imaging interferometer for the advanced technology solar telescope

被引:2
作者
Robinson, Brian [1 ,2 ]
Gary, G. Allen [3 ]
Balasubramaniam, K. S. [4 ]
机构
[1] Univ Alabama, Ctr Appl Opt, Huntsville, AL 35899 USA
[2] Univ Alabama, ATST Project Natl Solar Observ, Huntsville, AL 35899 USA
[3] Univ Alabama, Ctr Space Plasma & Aeron Res, Natl Space Sci & Technol Ctr, Huntsville, AL 35899 USA
[4] USAF, Air Force Res Lab, Sunspot, NM 88349 USA
关键词
optical design; evolutionary computation; Fabry-Perot etalons; solar astronomy instrumentation;
D O I
10.1117/1.3002337
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We describe an evolutionary algorithm for the design of an imaging triple-etalon Fabry-Perot interferometer (MFPI), which gives a solution to the multidimensional minimization process through a stochastic search method. The interactions between design variables (the etalon reflectances, interetalon ghost attenuator transmittances, and spacing ratios) are complex, resulting in a fitness landscape that is pitted with local optima. Traditional least-squares and gradient descent algorithms are not useful in such a situation. Instead, we employ a method called evolution strategies in which several preliminary designs are randomly generated subject to constraints. These designs are combined in pairs to produce offspring designs. The offspring population is mutated randomly, and only the fittest designs of the combined population are passed to the next iteration of the evolutionary process. We discuss the evolution strategies method itself, as well as its application to the specific problem of the design of an incoherently coupled triple-etalon interferometer intended for use as a focal plane instrument in the planned National Solar Observatory's Advanced Technology Solar Telescope (NSO's ATST). The algorithm converges quickly to a reasonable design that is well within the constraints imposed on the design variables, and which fulfills all resolution, signal-to-noise, throughput, and parasitic band suppression requirements. (C) 2008 Society of Photo-Optical Instrumentation Engineers. [DOI: 10.1117/1.3002337]
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页数:9
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