{"title":"高性能、低成本波前重构系统的性能表征","authors":"S. Rogers, S. McDermott","doi":"10.1364/adop.1996.athc.32","DOIUrl":null,"url":null,"abstract":"Logicon RDA has participated in the Air Force Phillips Laboratory imaging efforts under the direction of Dr. J. Gonglewski during the past years. We just finished supporting an adaptive optics experiment using a 197 actuator deformable mirror that was installed on the 3.5 m telescope located at Starfire Optical Range in Albuquerque NM. The experiment initially called for all centroid and wavefront reconstruction calculations be performed using a CSPI multiple i860 processor board. It was quickly determined that the resulting bandwidth would be insufficient to support the experiment objectives so Logicon RDA was tasked with designing and implementing a hardware based centroid and wavefront reconstructor.\n A deformable mirror with a large number of actuators and a requirement for high speed control leads towards the current trend to dedicate a single processing element per actuator. While this allows flexible control with enhanced diagnostic capabilities, the size and complexity of the system increases as does the number of interfaces. Our approach, to quickly provide the needed bandwidth for this experiment, was to use a small number of inexpensive parallel processing paths that are capable of keeping up with the camera frame rate of 1000 fps. This reduced the size of our system (3, 6U VME boards) and kept the number of interfaces to a manageable number.\n The centroid areas used for each actuator are completely reconfigurable (size and location) via the host processor as is the matrix used to reconstruct the wavefront. The matrix multiply is a brute force approach with no shortcuts implemented allowing the user to tailor the matrix to account for local effects if needed.\n We believe that our approach is an inexpensive method to control a medium sized deformable mirror (up to 500 actuators) running at frame rates of up to 2000 fps.\n We discuss the processing system configuration, the methods used to predict and measure the performance of the Deformable Mirror system, actual system performance results and show a cost breakdown and photographs of the centroid calculator and the wavefront reconstructor.","PeriodicalId":256393,"journal":{"name":"Adaptive Optics","volume":"24 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Performance Characterization of High Performance, Low Cost Wavefront Reconstructor System\",\"authors\":\"S. Rogers, S. McDermott\",\"doi\":\"10.1364/adop.1996.athc.32\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Logicon RDA has participated in the Air Force Phillips Laboratory imaging efforts under the direction of Dr. J. Gonglewski during the past years. We just finished supporting an adaptive optics experiment using a 197 actuator deformable mirror that was installed on the 3.5 m telescope located at Starfire Optical Range in Albuquerque NM. The experiment initially called for all centroid and wavefront reconstruction calculations be performed using a CSPI multiple i860 processor board. It was quickly determined that the resulting bandwidth would be insufficient to support the experiment objectives so Logicon RDA was tasked with designing and implementing a hardware based centroid and wavefront reconstructor.\\n A deformable mirror with a large number of actuators and a requirement for high speed control leads towards the current trend to dedicate a single processing element per actuator. While this allows flexible control with enhanced diagnostic capabilities, the size and complexity of the system increases as does the number of interfaces. Our approach, to quickly provide the needed bandwidth for this experiment, was to use a small number of inexpensive parallel processing paths that are capable of keeping up with the camera frame rate of 1000 fps. This reduced the size of our system (3, 6U VME boards) and kept the number of interfaces to a manageable number.\\n The centroid areas used for each actuator are completely reconfigurable (size and location) via the host processor as is the matrix used to reconstruct the wavefront. 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引用次数: 0
摘要
在过去几年里,Logicon RDA在J. Gonglewski博士的指导下参与了空军菲利普斯实验室的成像工作。我们刚刚完成了一个自适应光学实验,该实验使用了一个197驱动器可变形镜,该镜安装在位于Albuquerque NM的Starfire光学靶场的3.5 m望远镜上。该实验最初要求使用CSPI多个i860处理器板执行所有质心和波前重建计算。很快就确定,由此产生的带宽不足以支持实验目标,因此Logicon RDA的任务是设计和实现基于硬件的质心和波前重构器。具有大量致动器和高速控制要求的可变形镜导致了当前的趋势,即每个致动器专用单个处理元件。虽然这允许灵活的控制和增强的诊断功能,但系统的大小和复杂性随着接口数量的增加而增加。为了快速提供这个实验所需的带宽,我们的方法是使用少量廉价的并行处理路径,这些路径能够跟上1000 fps的相机帧速率。这减少了我们的系统(3,6 u VME板)的大小,并将接口数量保持在可管理的数量。用于每个执行器的质心区域是完全可重构的(大小和位置),通过主机处理器是用于重建波前的矩阵。矩阵乘法是一种蛮力方法,没有实现快捷方式,允许用户根据需要定制矩阵以考虑局部效果。我们相信我们的方法是一种廉价的方法来控制一个中等大小的可变形镜子(多达500个驱动器)以高达2000帧/秒的帧速率运行。我们讨论了处理系统的配置,用于预测和测量变形镜系统性能的方法,实际系统性能结果,并展示了质心计算器和波前重构器的成本分解和照片。
Performance Characterization of High Performance, Low Cost Wavefront Reconstructor System
Logicon RDA has participated in the Air Force Phillips Laboratory imaging efforts under the direction of Dr. J. Gonglewski during the past years. We just finished supporting an adaptive optics experiment using a 197 actuator deformable mirror that was installed on the 3.5 m telescope located at Starfire Optical Range in Albuquerque NM. The experiment initially called for all centroid and wavefront reconstruction calculations be performed using a CSPI multiple i860 processor board. It was quickly determined that the resulting bandwidth would be insufficient to support the experiment objectives so Logicon RDA was tasked with designing and implementing a hardware based centroid and wavefront reconstructor.
A deformable mirror with a large number of actuators and a requirement for high speed control leads towards the current trend to dedicate a single processing element per actuator. While this allows flexible control with enhanced diagnostic capabilities, the size and complexity of the system increases as does the number of interfaces. Our approach, to quickly provide the needed bandwidth for this experiment, was to use a small number of inexpensive parallel processing paths that are capable of keeping up with the camera frame rate of 1000 fps. This reduced the size of our system (3, 6U VME boards) and kept the number of interfaces to a manageable number.
The centroid areas used for each actuator are completely reconfigurable (size and location) via the host processor as is the matrix used to reconstruct the wavefront. The matrix multiply is a brute force approach with no shortcuts implemented allowing the user to tailor the matrix to account for local effects if needed.
We believe that our approach is an inexpensive method to control a medium sized deformable mirror (up to 500 actuators) running at frame rates of up to 2000 fps.
We discuss the processing system configuration, the methods used to predict and measure the performance of the Deformable Mirror system, actual system performance results and show a cost breakdown and photographs of the centroid calculator and the wavefront reconstructor.