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Bringing it all together: a unique approach to requirements for wave-front sensing and control on the James Webb Space Telescope (JWST)

机译:汇集所有内容:一种独特的方法来满足詹姆斯·韦伯太空望远镜(JWST)对波前感测和控制的要求

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The opto-mechanical design of the 6.6 meter James Webb Space Telescope1 (JWST), with its actively-controlled secondary and 18-segment primary mirror, presents unique challenges from a system engineering perspective. To maintain the optical alignment of the telescope on-orbit, a process called wavefront sensing and control (WFS&C) is employed to determine the current state of the mirrors and calculate the optimal mirror move updates. The needed imagery is downloaded to the ground, where the WFS&C algorithms to process the images reside, and the appropriate commands are uploaded to the observatory. Rather than use a dedicated wavefront sensor for the imagery as is done in most other applications, a science camera is used instead. For the success of the mission, WFS&C needs to perform flawlessly using the assets available among the combination of separate elements (ground operations, spacecraft, science instruments, optical telescope, etc.) that cross institutional as well as geographic borders. Rather than be yet another distinct element with its own set of requirements to flow to the other elements as was originally planned, a novel approach was selected. This approach entails reviewing and auditing other documents for the requirements needed to satisfy the needs of WFS&C. Three actions are taken: (1) when appropriate requirements exist, they are tracked by WFS&C; (2) when an existing requirement is insufficient to meet the need, a requirement change is initiated; and finally (3) when a needed requirement is missing, a new requirement is established in the corresponding document. This approach, deemed a "best practice" at the customer's independent audit, allows for program confidence that the necessary requirements are complete, while still maintaining the responsibility for the requirement with the most appropriate entity. This paper describes the details and execution of the approach; the associated WFS&C requirements and verification documentation; and the implementation of the primary database tool for the project, DOORS (Dynamic Object-Oriented Requirements System).
机译:6.6米的詹姆斯·韦伯太空望远镜1(JWST)的光机械设计及其主动控制的辅助和18段主镜,从系统工程的角度提出了独特的挑战。为了维持望远镜在轨的光学对准,采用了称为波前传感和控制(WFS&C)的过程来确定反射镜的当前状态并计算最佳的反射镜移动更新。所需的图像将下载到地面,其中包含用于处理图像的WFS&C算法,并将适当的命令上传到天文台。与其像大多数其他应用一样,不使用专用的波前传感器拍摄图像,而是使用科学相机。为了使任务成功,WFS&C需要使用跨越机构和地理边界的独立要素(地面作战,航天器,科学仪器,光学望远镜等)的组合中的可用资产来完美地执行任务。选择了一种新颖的方法,而不是像原来计划的那样,具有自己的一组要求流向其他元素的另一个独特元素。这种方法需要针对满足WFS&C需求所需的要求,对其他文档进行审核和审核。采取了三项行动:(1)当存在适当的要求时,WFS&C会对其进行跟踪; (2)当现有需求不足以满足需求时,就启动需求变更;最后(3)当缺少所需需求时,在相应文档中建立一个新需求。这种方法在客户的独立审核中被认为是“最佳实践”,它使程序确信必要的要求已经完成,同时仍然由最合适的实体来负责要求的责任。本文描述了该方法的细节和执行;相关的WFS&C要求和验证文档;以及该项目的主要数据库工具DOORS(动态面向对象的需求系统)的实现。

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