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Introduction

Date: January 14, 2021
Time: 10:00am – 11:00am PT
Duration: 1 hour


Stencil operations are used widely in HPC applications and pose an optimization challenge on both CPUs and GPUs. On GPUs, fine-tuned optimizations can be formulated using low-level APIs such as CUDA, but many large established codes prefer a portable, higher-level API such as OpenACC. Although OpenACC lacks the fine-tuning of CUDA, it does allow for some tuning through a variety of parallelization constructs and loop directives. Here, we try various OpenACC directive options to optimize the computationally heaviest stencil operation within our production solar physics research code Magnetohydrodynamics Around a Sphere (MAS).

By attending this webinar, you will:
  • Explore numerous OpenACC directive options, including tile, cache, and collapse, and compare their performance over several problem types and sizes;
  • Learn which combination of options yields the overall optimal result and see how it appears in a full-scale simulation analyzed with Nsight Systems and Nsight Compute; and
  • Be aware of cautionary cases where using the "wrong" directives can yield very poor performance.

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DGX Station Datasheet

Get a quick low-down and technical specs for the DGX Station.
DGX Station Whitepaper

Dive deeper into the DGX Station and learn more about the architecture, NVLink, frameworks, tools and more.
DGX Station Whitepaper

Dive deeper into the DGX Station and learn more about the architecture, NVLink, frameworks, tools and more.

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Speaker

Ronald M. Caplan

Computational Scientist, Predictive Science Inc. (PSI)

Dr. Caplan is a computational scientist at Predictive Science Inc. (PSI) with over ten years of experience in applying computational methods in applied mathematics and physics. His main research interests are in developing and optimizing numerical methods for simulating physics-based models and their implementations in parallel high-performance-computing environments including GPU accelerators. His research currently focuses on the continued development and optimization of PSI's thermodynamic magnetohydrodynamic code (MAS) used to study the solar corona and heliosphere, as well as providing computational solutions for additional projects including data analysis of solar images.

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Date & Time: Wednesday, April 22, 2018