The authors develop a model to compute energy efficiency for GPU-based data processing in LHCb's HLT1 by linking throughput to GPU core count, clock frequency, memory bandwidth, and thermal design power.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Review of helioseismic inversions shows the solar modelling problem remains unsolved with broad implications for stellar seismology and fields relying on precise stellar parameters.
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Energy efficiency of a GPU-based computing system for High Energy Physics experiments
The authors develop a model to compute energy efficiency for GPU-based data processing in LHCb's HLT1 by linking throughput to GPU core count, clock frequency, memory bandwidth, and thermal design power.
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Progress in global helioseismology: a new light on the solar modelling problem and its implications for solar-like stars
Review of helioseismic inversions shows the solar modelling problem remains unsolved with broad implications for stellar seismology and fields relying on precise stellar parameters.
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