脉冲星搜索加速使用fpga和OpenCL模板

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Julian Oppermann, Mitchell B. Mickaliger, Oliver Sinnen
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引用次数: 1

摘要

平方公里阵列(SKA)是目前正在建设的世界上最大的射电望远镜,它将采用复杂的信号处理来探测新的脉冲星,即高磁化旋转的中子星。本文利用基于OpenCL模板的新的高级设计过程,解决了在现场可编程门阵列(fpga)上对脉冲星搜索的苛刻计算的加速问题,该过程可转移到其他科学问题。成功的FPGA加速大规模科学工作负载需要定制架构,充分利用现代可重构硬件的并行计算能力,并适应大量的设计空间探索。基于opencl的高级合成工具链具有用单一源语言表达相互连接的多内核管道的能力,在这一领域表现出色。然而,可实现的性能很大程度上取决于编译器从代码中推断出所需硬件结构的能力。卓越性能的一个关键方面通常是不间断的、高带宽的数据流进入和通过设计。这在复杂的设计中很难实现,因为数据顺序需要重新排列,例如转置。当读取以非平凡模式发生时,从DDR内存中预取和突发加载同样困难。在本文中,我们提出了使用基于opencl的代码模板来解决这两个问题的新方法。我们通过加速SKA脉冲星搜索管道中的一个关键组件:傅里叶域加速搜索(FDAS)模块,展示了这些方法的实际好处。使用我们提出的方法,我们能够开发出比以前更可扩展的FDAS加速器架构。我们探索了它的设计空间,最终实现了10倍的吞吐量提高,比之前完全优化的纯OpenCL实现。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Pulsar search acceleration using FPGAs and OpenCL templates

Pulsar search acceleration using FPGAs and OpenCL templates

The Square Kilometre Array (SKA) is the world’s largest radio telescope currently under construction, and will employ elaborate signal processing to detect new pulsars, i.e. highly magnetised rotating neutron stars. This paper addresses the acceleration of demanding computations for this pulsar search on Field-Programmable Gate Arrays (FPGAs) using a new high-level design process based on OpenCL templates that is transferable to other scientific problems. The successful FPGA acceleration of large-scale scientific workloads requires custom architectures that fully exploit the parallel computing capabilities of modern reconfigurable hardware and are amenable to substantial design space exploration. OpenCL-based high-level synthesis toolchains, with their ability to express interconnected multi-kernel pipelines in a single source language, excel in this domain. However, the achievable performance strongly depends on how well the compiler can infer desirable hardware structures from the code. One key aspect to excellent performance is commonly the uninterrupted, high-bandwidth streaming of data into and through the design. This is difficult to achieve in complex designs when data order needs to be re-arranged, e.g. transposed. It is equally hard to pre-fetch and burst-load from DDR memory when reading occurs in non-trivial patterns. In this paper, we propose new approaches to these two problems that use OpenCL-based code templates.

We demonstrate the practical benefits of these approaches with the acceleration of a key component in the SKA’s pulsar search pipeline: the Fourier Domain Acceleration Search (FDAS) module. Using our proposed methodology, we are able to develop a more scalable FDAS accelerator architecture than previously possible. We explore its design space to eventually achieve a 10x throughput improvement over a prior, thoroughly optimised implementation in plain OpenCL.

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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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