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GMT AO system requirements and error budgets in the preliminary design phase

机译:GMT AO系统要求和错误预算在初步设计阶段

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Error budgets are an indispensable tool for assuring that project requirements can be and are being met. An error budgetwill typically include terms associated with subsystems which are being designed by different teams of engineers, andfabricated by different vendors. It is a useful tool at all levels of design since it provides a means to negotiate designtrades in the broadest possible context. Error budgeting is in many ways fundamental to the mission of systemsengineering and of course to the overall project success.In this paper we will describe the GMT Adaptive Optics System flow down requirements and their integration with theirwavefront error budgets. We will focus on the GMT Adaptive Optics wavefront error budgets for the followingobserving modes: Natural Guide Star Adaptive, Laser Tomography Adaptive Optics and Ground Layer Adaptive Optics.Finally, a description of the error budgets and the close link between the error budgets and other parameter such as skycoverage, zenith angle, etc., will be discussed in this paper.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:错误预算是一个不可或缺的工具,以确保可以和正在满足项目要求。错误预算版本通常包括与子系统相关联的术语,该子系统是由不同的工程团队设计的,由不同的供应商和特征为由。它是所有级别设计中的有用工具,因为它提供了在最广泛的环境中协商设计贸易的手段。错误预算符在Systemengering的使命基础上是在许多方面,当然还要达到整体项目成功。本文将描述GMT自适应光学系统的流量下降要求及其与其Wavefront错误预算的集成。我们将专注于GMT自适应光学波前错误预算为以下服务模式:自然导向星自适应,激光断层扫描自适应光学和地层自适应光学器件。最后,错误预算的描述和错误预算与其他参数之间的关闭链接如Skycoverage,天顶角等,将在本文中讨论。©(2012)光学仪表工程师(SPIE)的版权协会。仅供个人使用的摘要下载。

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