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WFIRST Coronagraph Technology Requirements: Status Update and Systems Engineering Approach

机译:WFIRST日冕仪技术要求:状态更新和系统工程方法

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The Coronagraph Instrument (CGI) on the Wide-Field Infrared Survey Teleseope (WFIRST) will demonstrate technologies and methods for high-contrast direct imaging and spectroscopy of exoplanet systems in reflected light, including polarimetry of circumstellar disks. The WFIRST management and CGI engineering and science investigation teams have developed requirements for the instrument, motivated by the objectives and technology development needs of potential future flagship exoplanet characterization missions such as the NASA Habitable Exoplanet Imaging Mission (HabEx) and the Large UV/Optical/IR Surveyor (LUVOIR). The requirements have been refined to support recommendations from the WFIRST Independent External Technical/Management/Cost Review (WIETR.) that the WFIRST CGI be classified as a technology demonstration instrument instead of a science instrument. This paper provides a description of how the CGI requirements flow from the top of the overall WFIRST mission structure through the Level 2 requirements, where the focus here is on capturing the detailed context and rationales for the CGI Level 2 requirements. The WFIRST requirements flow starts with the top Program Level Requirements Appendix (PLRA), which contains both high-level mission objectives as well as the CGI-specific baseline technical and data requirements (BTR and BDR, respectively). Captured in the WFIRST Mission Requirements Document (MRD), the Level 2 CGI requirements flow from the PLRA objectives, BTRs, and BDRs. There are five CGI objectives in the WFIRST PLRA, which motivate the four baseline technical/data requirements. There are nine CGI level 2 (L2) requirements presented in this work, which have been developed and validated using predictions from increasingly refined observatory and instrument performance models. We also present the process and collaborative tools used in the L2 requirements development and management, including the collection and organization of science inputs, an open-source approach to managing the requirements database, and automating documentation. The tools created for the CGI L2 requirements have the potential to improve the design and planning of other projects, streamlining requirement management and maintenance. The WFIRST CGI passed its System Requirements Review (SRR) and System Design Review (SDR) in May 2018. The SRR examines the functional requirements and performance requirements defined for the system and the preliminary program or project plan and ensures that the requirements and the selected concept will satisfy the mission, and the SDR examines the proposed system architecture and design and the flow down to all functional elements of the system.
机译:广域红外勘测望远镜(WFIRST)上的日冕仪(CGI)将展示反射系外行星系统在反射光下的高对比度直接成像和光谱学的技术和方法,包括圆盘的极化。 WFIRST管理层以及CGI工程和科学调查团队针对潜在的未来旗舰系外行星表征任务(例如NASA宜居系外行星成像任务(HabEx)和大型UV /光学/红外线测量员(LUVOIR)。对要求进行了完善,以支持WFIRST独立外部技术/管理/成本审核(WIETR。)的建议,即WFIRST CGI被归类为技术演示工具而非科学工具。本文描述了CGI需求如何从整个WFIRST任务结构的顶部流向2级需求,这里的重点是捕获CGI 2级需求的详细背景和基本原理。 WFIRST需求流程始于最高计划级别需求附录(PLRA),其中包含高层任务目标以及CGI特定的基准技术和数据需求(分别为BTR和BDR)。在WFIRST任务需求文档(MRD)中捕获的2级CGI需求来自PLRA目标,BTR和BDR。 WFIRST PLRA中有五个CGI目标,这些目标激发了四个基线技术/数据要求。在这项工作中提出了九项CGI 2级(L2)要求,这些要求已使用越来越完善的天文台和仪器性能模型的预测进行了开发和验证。我们还将介绍在L2需求开发和管理中使用的过程和协作工具,包括科学输入的收集和组织,用于管理需求数据库的开源方法以及自动化文档。为CGI L2需求而创建的工具具有改进其他项目的设计和规划,简化需求管理和维护的潜力。 WFIRST CGI于2018年5月通过了系统要求审查(SRR)和系统设计审查(SDR)。SRR检查为系统和初步计划或项目计划定义的功能要求和性能要求,并确保要求和选定的概念将满足任务,SDR会检查建议的系统体系结构和设计以及流程直至系统的所有功能元素。

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