CSSI Elements: EWMS - Event Workflow Management Service

CSSI 元素：EWMS - 事件工作流管理服务

• 批准号: 2103963
• 负责人: Benedikt Riedel
• 金额: $ 59.61万
• 依托单位: University of Wisconsin-Madison
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2021
• 资助国家: 美国
• 起止时间: 2021-07-01 至 2024-09-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2103963&HistoricalAwards=false
• 关键词: CSSI; Elements; EWMS; Event; Workflow

This award will begin developing an Observation Management System Framework which will help alleviating multiple types of astrophysical data and respective workflow management - a burden shouldered now by human researchers who process large numbers of independent pieces of data (“events”). The core element of this framework - Event Workflow Management System (EWMS) - is a workload manager designed for processing events (simulated readouts from a particle physics detector, recorded data points, images, etc.) with complex workflows. EWMS could become a central core for applying novel computer science methods to improve scientific data processing with an initial focus on Multi-Messenger Astrophysics (MMA) - it will transform how ”event”-based computational problems are tackled on the national CI ecosystem through a set of reusable services. This paradigm is applicable across a wide range of science domains, including astrophysics, astronomy, physics, biology, and other disciplines that deal with Big Data flows. The EWMS will benefit three of NSF’s 10 big ideas – “Growing Convergence Research,” “Harnessing the Data Revolution,” and “Windows on the Universe", bringing together data from the particle physics-based detectors (IceCube Neutrino Observatory, High Altitude Water Cherenkov Observatory, Cherenkov Telescope Array), traditional astronomical observatories (large telescopes), and gravitational wave observatories (LIGO, VIRGO, KAGRA). While the data types of each of these experiments or observatories are dramatically different, they all record data in the independent spatio-temporal increments, observations, triggers, events, etc. that are processed and stored separately. The EWMS is applicable to nearly all current workflows in MMA experiments, and by combining these most precise observations via EWMS, scientists will be able to observe the Universe in fundamentally new ways and learn more about its history than any one of these messengers can provide in isolation. Thus, this award addresses and advances the science objectives and goals of the NSF's "Windows on the Universe: The Era of Multi-Messenger Astrophysics" program.This award by the Office of Advanced Cyberinfrastructure is jointly supported by the Windows on the Universe Program, the Physics at the Information Frontier Program, the IceCube Science Program, the Antarctic Astrophysics and Geospace Sciences Program, and the Office of Polar Programs CyberInfrastructure Program.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

该奖项将开始开发一个观测管理系统框架，该框架将有助于减轻多种类型的天体物理数据和各自的工作流程管理——这是处理大量独立数据（“事件”）的人类研究人员现在肩负的负担。该框架 - 事件工作流管理系统 (EWMS) - 是一个工作负载管理器，设计用于处理具有复杂工作流的事件（粒子物理探测器的模拟读数、记录的数据点、图像等），EWMS 可以成为应用新颖的核心。电脑改进科学数据处理的科学方法，最初重点关注多信使天体物理学（MMA）——它将改变通过一组可重用服务在国家 CI 生态系统上解决基于“事件”的计算问题的方式。广泛的科学领域，包括天体物理学、天文学、物理学、生物学和其他处理大数据流的学科，EWMS 将使 NSF 的 10 个重大想法中的三个受益 - “成长”。融合研究”、“利用数据革命”和“宇宙之窗”，汇集了来自粒子物理探测器（冰立方中微子天文台、高空水切伦科夫天文台、切伦科夫望远镜阵列）、传统天文观测站（大型天文台）的数据。望远镜）和引力波天文台（LIGO、VIRGO、KAGRA），而这些实验的数据类型或。观测站的情况截然不同，它们都以独立的时空增量、观测、触发、事件等记录数据，并单独处理和存储。通过 EWMS 的精确观测，科学家将能够以全新的方式观察宇宙，并比任何一位使者单独提供的更多地了解宇宙的历史。因此，该奖项解决并推进了科学目的和目标。 NSF 的“宇宙之窗：多信使天体物理学时代”计划。该奖项由先进网络基础设施办公室颁发，由宇宙之窗计划、信息前沿物理学计划、IceCube 科学计划、南极天体物理和地球空间科学计划以及极地计划办公室网络基础设施计划。该奖项反映了 NSF 的法定使命，并通过使用基金会的智力评估进行评估，认为值得支持优点和更广泛的影响审查标准。