用于高速4位天体物理数据处理的GPU内核

P. Klages, K. Bandura, N. Denman, A. Recnik, J. Sievers, K. Vanderlinde
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引用次数: 12

摘要

干涉射电望远镜通常依赖于计算昂贵的O(N2)相关计算;幸运的是,这些计算很好地映射到大规模并行加速器,如低成本gpu。本文介绍了一种新型混合FX相关器的基于GPU的x引擎开发的OpenCL内核。来自f引擎的信道化数据以4位、偏移编码的实整数和虚整数的形式提供给gpu。由于数据的位深较低,两个值可以打包到一个32位寄存器中,允许使用单个融合的乘加指令对多个值进行乘法和加法运算。使用这些内核,在4.3 TOPS的GPU上可以执行多达5.6有效的每秒万亿次操作(TOPS)。通过设计,这些内核允许关联扩展到大量输入元素,并且仅受GPU上最大缓冲区大小的限制。这个代码目前正在与加拿大BC省的CHIME探路者相关器一起工作。
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GPU kernels for high-speed 4-bit astrophysical data processing
Interferometric radio telescopes often rely on computationally expensive O(N2) correlation calculations; fortunately these computations map well to massively parallel accelerators such as low-cost GPUs. This paper describes the OpenCL kernels developed for the GPU based X-engine of a new hybrid FX correlator. Channelized data from the F-engine is supplied to the GPUs as 4-bit, offset-encoded real and imaginary integers. Because of the low bit-depth of the data, two values may be packed into a 32-bit register, allowing multiplication and addition of more than one value with a single fused multiply-add instruction. With these kernels, as many as 5.6 effective tera-operations per second (TOPS) can be executed on a 4.3 TOPS GPU. By design, these kernels allow correlations to scale to large numbers of input elements, and are limited only by maximum buffer sizes on the GPU. This code is currently working on-sky with the CHIME Pathfinder Correlator in BC, Canada.
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