Column-Oriented Data Store for Astrophysical Data

J. Yaghob, D. Bednárek, Martin Kruliš, F. Zavoral
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引用次数: 1

Abstract

Astrophysical databases have used proprietary formats (especially the FITS format) to represent measured data and related metadata. The design of the FITS format was influenced by punch cards, thus it is extremely inappropriate for modern hardware. Even though this format is well established in the domain of astrophysics and will be definitely used as a common ground for data exchange, a new representation is required if the data are to be processed efficiently in a high performance manner. In this paper, we propose a specialized column-oriented format for the measured data, which allows much faster loading from the persistent data storage and direct application of the data in computational operations. Furthermore, we have tested various I/O methods implemented in modern operating systems to accommodate different access patterns that were observed in various use cases. We have created a prototype implementation of the proposed methods and experimentally evaluated their benefits.
面向列的天体物理数据存储
天体物理数据库使用专有格式(特别是FITS格式)来表示测量数据和相关元数据。FITS格式的设计受到打孔卡的影响,因此它非常不适合现代硬件。尽管这种格式在天体物理学领域已经很好地建立起来,并且肯定会用作数据交换的通用基础,但如果要以高性能的方式有效地处理数据,则需要一种新的表示。在本文中,我们提出了一种专门的面向列的测量数据格式,它可以更快地从持久数据存储加载数据,并在计算操作中直接应用数据。此外,我们还测试了在现代操作系统中实现的各种I/O方法,以适应在各种用例中观察到的不同访问模式。我们已经创建了所提出方法的原型实现,并通过实验评估了它们的效益。
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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