KIS 科学数据中心

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Solar Physics Pub Date : 2024-10-15 DOI:10.1007/s11207-024-02388-7
Peter Caligari, Faezeh Aghaei, Janek Beck, Nazaret Bello González, Svetlana Berdyugina, Andreas Bührer, Andrea Diercke, Iaroslav Gorbachev, Andrei Y. Gorobets, Marco Günter, Kamal Hamdan, Alexander Hochmuth, Lea Hohl, Petri Kehusmaa, Markus Knobloch, Sani Patel, Markus Schmassmann, Gangadharan Vigeesh, Taras Yakobchuk, Morten Franz, Thomas Hederer, Carl Schaffer, Manuel Collados
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引用次数: 0

摘要

随着观测能力和数值模拟的不断提高,必须对大量数据进行有效的数据管理。太阳物理研究所(KIS)开发了科学数据中心(SDC),这是一个数据基础设施,用于存储、整理和传播来自德国太阳观测设施和其他合作机构的科学数据。科学数据中心的另一个构想是创建和传播具有附加值的更高级别的数据产品,如光谱测量数据的反演。SDC 档案基础设施包括一个基于 Rucio 科学数据管理和 MongoDB 系统的后端和一个前端网络界面,用户可以根据仪器、日期、波长范围和目标等搜索参数搜索和发现数据。SDC 档案库还通过 API 和 TAP 服务提供数据访问。SDC 目前可访问自 2014 年以来来自 GREGOR 望远镜(特内里费)GRIS 仪器的 1299 个科学就绪数据集、来自真空太阳望远镜(VTT,特内里费)LARS 的一组 610 个光谱以及来自色球层望远镜(ChroTel)的 202 404 个全圆盘太阳图像。空间数据中心还向社区提供可下载的全球资源信息系 统光谱极坐标存档数据的米尔恩-爱丁顿反演以及数据可视化和高级分析工具(如全球资源信息系 统视图工具)。在大型国际数据项目(如地平线 2020 ASTERICS 和 ESCAPE 欧盟资助项目)框架内,根据 FAIR(可查找、可访问、可互操作、可重用)原则开展了许多 SDC 活动。新的和计划中的 SDC 活动包括从 GREGOR 上下文成像仪器获取太阳数据、从 Ondřejov 天文台(捷克共和国)获取耀斑观测数据、内部磁流体动力学模拟的存档和传播,以及利用机器学习创建高级数据产品。韩国天文台科学数据中心是一个先进的数据管理基础设施,负责对可用于科学研究的地基太阳光谱和成像数据进行整理、归档和访问。科学数据中心还提供先进的数据可视化和分析工具,并邀请数据提供者通过科学数据中心的数据档案向太阳物理学界和更广泛的(天体)物理学界发布其数据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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The KIS Science Data Centre

With the steady improvement of the observing capabilities and numerical simulations, an efficient data management of large data volumes has become mandatory. The Institute for Solar Physics (KIS) has developed the Science Data Centre (SDC), a data infrastructure to store, curate, and disseminate science-ready data from the German solar-observing facilities and other partner institutions. The SDC was also conceived to create and disseminate higher-level data products of added value like inversions from spectropolarimetric data. The SDC archive infrastructure consists of a back-end based on the Rucio science data-management and MongoDB systems and a front-end web interface that allows the user to search and discover data based on search parameters like instrument, date, wavelength range, and target. The SDC archive also provides data access via API and TAP services. The SDC currently offers access to 1299 science-ready datasets from the GRIS instrument at the GREGOR telescope (Tenerife) since 2014, a set of 610 spectra from the LARS at the Vacuum Solar Telescope (VTT, Tenerife) and 202 404 full-disc solar images from the Chromospheric Telescope (ChroTel). The SDC also offers to the community Milne–Eddington inversions of the GRIS spectropolarimetric archived data that can be downloaded as well as tools for data visualization and advanced analysis (e.g., GRISView tool). Many SDC activities have been carried out within the framework of large international data projects like the Horizon 2020 ASTERICS and ESCAPE EU-funded projects under the FAIR (Findable, Accessible, Interoperable, Reusable) principles. New and planned SDC activities include the ingestion of solar data from GREGOR context imaging instruments, flare observations from Ondřejov Observatory (Czech Republic), archiving and dissemination of in-house magnetohydrodynamic simulations, and creation of high-level data products using machine learning. The KIS Science Data Centre is a state-of-the-art data-management infrastructure that curates, archives, and provides access to ground-based science-ready spectropolarimetric and imaging solar data. SDC also provides advanced data visualization and analysis tools and invites data providers to publish their data to the solar and broader (astro)physics community via the SDC data archive.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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