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Thirty Meter Telescope (TMT) Narrow Field Infrared Adaptive Optics System (NFIRAOS) real-time controller preliminary architecture

机译:三十米望远镜(TMT)窄场红外自适应光学系统(NFIRAOS)实时控制器初步架构

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摘要

The Narrow Field Infrared Adaptive Optics System (NFIRAOS) is the first light Adaptive Optics (AO) system for the Thirty Meter Telescope (TMT). A critical component of NFIRAOS is the Real-Time Controller (RTC) subsystem which provides real-time wavefront correction by processing wavefront information to compute Deformable Mirror (DM) and Tip/Tilt Stage (TTS) commands. The National Research Council of Canada - Herzberg (NRC-H), in conjunction with TMT, has developed a preliminary design for the NFIRAOS RTC. The preliminary architecture for the RTC is comprised of several Linux-based servers. These servers are assigned various roles including: the High-Order Processing (HOP) servers, the Wavefront Corrector Controller (WCC) server, the Telemetry Engineering Display (TED) server, the Persistent Telemetry Storage (PTS) server, and additional testing and spare servers. There are up to six HOP servers that accept high-order wavefront pixels, and perform parallelized pixel processing and wavefront reconstruction to produce wavefront corrector error vectors. The WCC server performs low-order mode processing, and synchronizes and aggregates the high-order wavefront corrector error vectors from the HOP servers to generate wavefront corrector commands. The Telemetry Engineering Display (TED) server is the RTC interface to TMT and other subsystems. The TED server receives all external commands and dispatches them to the rest of the RTC servers and is responsible for aggregating several offloading and telemetry values that are reported to other subsystems within NFIRAOS and TMT. The TED server also provides the engineering GUIs and real-time displays. The Persistent Telemetry Storage (PTS) server contains fault tolerant data storage that receives and stores telemetry data, including data for Point-Spread Function Reconstruction (PSFR).
机译:窄场红外自适应光学系统(NFIRAOS)是用于30米望远镜(TMT)的第一个光自适应光学(AO)系统。 NFIRAOS的关键组件是实时控制器(RTC)子系统,该子系统通过处理波前信息以计算可变形镜像(DM)和倾斜/倾斜台(TTS)命令来提供实时波前校正。加拿大国家研究委员会-Herzberg(NRC-H)与TMT联合开发了NFIRAOS RTC的初步设计。 RTC的初步体系结构由几个基于Linux的服务器组成。这些服务器被分配了各种角色,包括:高阶处理(HOP)服务器,波前校正控制器(WCC)服务器,遥测工程显示(TED)服务器,持久遥测存储(PTS)服务器以及其他测试和备用角色服务器。最多有六个HOP服务器接受高阶波前像素,并执行并行像素处理和波前重构,以产生波前校正器误差矢量。 WCC服务器执行低阶模式处理,并同步和聚合来自HOP服务器的高阶波阵面校正器误差向量,以生成波阵面校正器命令。遥测工程显示(TED)服务器是TMT和其他子系统的RTC接口。 TED服务器接收所有外部命令,并将它们分配给其余的RTC服务器,并负责汇总报告给NFIRAOS和TMT内其他子系统的多个卸载和遥测值。 TED服务器还提供了工程GUI和实时显示。持久遥测存储(PTS)服务器包含容错数据存储,该数据接收和存储遥测数据,包括用于点扩展功能重构(PSFR)的数据。

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