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The Cherenkov Telescope Array Observatory Top Level Use Cases

机译:切伦科夫望远镜阵列天文台顶层用例

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Today the scientific community is facing an increasing complexity of the scientific projects, from both a technological and a management point of view. The reason for this is in the advance of science itself, where new experiments with unprecedented levels of accuracy, precision and coverage (time and spatial) are realised. Astronomy is one of the fields of the physical sciences where a strong interaction between the scientists, the instrument and software developers is necessary to achieve the goals of any Big Science Project. The Cherenkov Telescope Array (CTA) will be the largest ground-based very high-energy gamma-ray observatory of the next decades. To achieve the full potential of the CTA Observatory, the system must be put into place to enable users to operate the telescopes productively. The software will cover all stages of the CTA system, from the preparation of the observing proposals to the final data reduction, and must also fit into the overall system. Scientists, engineers, operators and others will use the system to operate the Observatory, hence they should be involved in the design process from the beginning. We have organised a workgroup and a workflow for the definition of the CTA Top Level Use Cases in the context of the Requirement Management activities of the CTA Observatory. Scientists, instrument and software developers are collaborating and sharing information to provide a common and general understanding of the Observatory from a functional point of view. Scientists that will use the CTA Observatory will provide mainly Science Driven Use Cases, whereas software engineers will subsequently provide more detailed Use Cases, comments and feedbacks. The main purposes are to define observing modes and strategies, and to provide a framework for the flow down of the Use Cases and requirements to check missing requirements and the already developed Use-Case models at CTA sub-system level. Use Cases will also provide the basis for the definition of the Acceptance Test Plan for the validation of the overall CTA system. In this contribution we present the organisation and the workflow of the Top Level Use Cases workgroup.
机译:如今,从技术和管理的角度来看,科学界都面临着越来越多的科学项目的复杂性。其原因在于科学本身的进步,在那里实现了具有前所未有的准确性,精确度和覆盖率(时间和空间)水平的新实验。天文学是物理科学的领域之一,科学家,仪器和软件开发人员之间的强大互动对于实现任何大型科学项目的目标都是必不可少的。切伦科夫望远镜阵列(CTA)将是未来几十年最大的地面超高能伽马射线天文台。为了充分发挥CTA天文台的潜力,必须安装该系统以使用户能够高效地操作望远镜。该软件将涵盖CTA系统的所有阶段,从准备观察方案到最终减少数据,还必须适合整个系统。科学家,工程师,操作人员和其他人员将使用该系统来操作天文台,因此他们应该从一开始就参与设计过程。我们已经在CTA天文台的需求管理活动的背景下组织了一个工作组和一个工作流,用于定义CTA顶级用例。科学家,仪器和软件开发人员正在协作和共享信息,以从功能的角度提供对天文台的共识。将使用CTA天文台的科学家将主要提供“科学驱动的用例”,而软件工程师随后将提供更详细的用例,评论和反馈。主要目的是定义观察模式和策略,并为用例和需求的下流提供框架,以在CTA子系统级别检查缺失的需求和已开发的用例模型。用例还将为定义验收测试计划提供基础,以验证整个CTA系统。在此贡献中,我们介绍了顶级用例工作组的组织和工作流程。

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