Vincent E. Larson
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Vincent E. Larson has a total of 366 co-authors. Here are the top co-authors by number of shared publications:
- Philip J. Rasch
Department of Atmospheric and Climate Science, University of Washington, Seattle, WA, USA
17 shared publications - Colin M. Zarzycki
Department of Meteorology and Atmospheric Science Pennsylvania State University State College PA USA
16 shared publications - Hui Wan
Pacific Northwest National Laboratory, Richland, Washington, United States
16 shared publications - Jean-Christophe Golaz
Lawrence Livermore National Laboratory Livermore CA USA
15 shared publications - Po-Lun Ma
Atmospheric, Climate, and Earth Sciences Division, Pacific Northwest National Laboratory, Richland, WA, USA
12 shared publications - Shixuan Zhang
Pacific Northwest National Laboratory Richland WA USA
12 shared publications
Latest Publications
- Open Access
- 26 September 2026
- Published by American Geophysical Union (AGU) in Journal of Advances in Modeling Earth Systems
- Vol. 18 (9)
The Coriolis Effects in Parameterization of Atmospheric Turbulence and Convection
The Coriolis effect can deflect turbulent momentum flux and anisotropy of turbulent kinetic energy. This Coriolis turbulent deflection is usually omitted in parameterizations of atmospheric turbulence and convection. However, previous large‐eddy simulations (LES) found that the nontraditional Coriolis terms (NCTs) can enhance vertical velocity variance with easterly flow and suppress it with westerly flow. To parameterize this effect in the atmosphere, this study introduces the Coriolis terms to the Cloud Layers Unified By Binormals (CLUBB) parameterization of clouds and turbulence. We design three single‐column benchmarks to test the implementation of the NCTs in CLUBB. First, assuming that all except the Coriolis terms vanish on the right‐hand side of the prognostic equations of the second‐order moments of velocity, we derive an analytical solution in which the anisotropy of the moments rotates back to the initial state with a certain period. Our CLUBB results match this analytic benchmark. Second, assuming dry and neutrally stratified atmosphere with constant geostrophic winds, our CLUBB and LES results suggest that the NCTs make the Ekman layer deeper with geostrophic easterlies but shallower with westerlies. Third, under realistic conditions for trade‐wind shallow convection, our CLUBB results show that the cloud layer becomes shallower if we omit the NCTs or flip the geostrophic winds from easterly to westerly. These benchmarks not only validate the Coriolis terms in CLUBB but also form a model hierarchy that aids our understanding of the effects of the NCTs on turbulence and convection.
- 26 September 2026
- Published by American Geophysical Union (AGU) in Journal of Advances in Modeling Earth Systems
- Vol. 18 (9)
Open AccessThe Coriolis Effects in Parameterization of Atmospheric Turbulence and Convection
The Coriolis effect can deflect turbulent momentum flux and anisotropy of turbulent kinetic energy. This Coriolis turbulent deflection is usually omitted in parameterizations of atmospheric turbulence and convection. However, previous large‐eddy simulations (LES) found that the nontraditional Coriolis terms (NCTs) can enhance vertical velocity variance with easterly flow and suppress it with westerly flow. To parameterize this effect in the atmosphere, this study introduces the Coriolis terms to the Cloud Layers Unified By Binormals (CLUBB) parameterization of clouds and turbulence. We design three single‐column benchmarks to test the implementation of the NCTs in CLUBB. First, assuming that all except the Coriolis terms vanish on the right‐hand side of the prognostic equations of the second‐order moments of velocity, we derive an analytical solution in which the anisotropy of the moments rotates back to the initial state with a certain period. Our CLUBB results match this analytic benchmark. Second, assuming dry and neutrally stratified atmosphere with constant geostrophic winds, our CLUBB and LES results suggest that the NCTs make the Ekman layer deeper with geostrophic easterlies but shallower with westerlies. Third, under realistic conditions for trade‐wind shallow convection, our CLUBB results show that the cloud layer becomes shallower if we omit the NCTs or flip the geostrophic winds from easterly to westerly. These benchmarks not only validate the Coriolis terms in CLUBB but also form a model hierarchy that aids our understanding of the effects of the NCTs on turbulence and convection.
- Open Access
- 14 September 2026
- Published by Wiley
The Coriolis effects in parameterization of atmospheric turbulence and convection
The Coriolis effect can deflect turbulent momentum flux and anisotropy of turbulent kinetic energy. This Coriolis turbulent deflection is usually omitted in parameterizations of atmospheric turbulence and convection. However, previous large-eddy simulations (LES) found that the nontraditional Coriolis terms (NCTs) can enhance vertical velocity variance with easterly flow and suppress it with westerly flow. To parameterize this effect in the atmosphere, this study introduces the Coriolis terms to the Cloud Layers Unified By Binormals (CLUBB) parameterization of clouds and turbulence. We design three single-column benchmarks to test the implementation of the NCTs in CLUBB. First, assuming that all except the Coriolis terms vanish on the right-hand side of the prognostic equations of the second-order moments of velocity, we derive an analytical solution in which the anisotropy of the moments rotates back to the initial state with a certain period. Our CLUBB results match this analytic benchmark. Second, assuming dry and neutrally stratified atmosphere with constant geostrophic winds, our CLUBB and LES results suggest that the NCTs make the Ekman layer deeper with geostrophic easterlies but shallower with westerlies. Third, under realistic conditions for trade-wind shallow convection, our CLUBB results show that the cloud layer becomes shallower if we omit the NCTs or flip the geostrophic winds from easterly to westerly. These benchmarks not only validate the Coriolis terms in CLUBB but also form a model hierarchy that aids our understanding of the effects of the NCTs on turbulence and convection.
- 14 September 2026
- Published by Wiley
Open AccessThe Coriolis effects in parameterization of atmospheric turbulence and convection
The Coriolis effect can deflect turbulent momentum flux and anisotropy of turbulent kinetic energy. This Coriolis turbulent deflection is usually omitted in parameterizations of atmospheric turbulence and convection. However, previous large-eddy simulations (LES) found that the nontraditional Coriolis terms (NCTs) can enhance vertical velocity variance with easterly flow and suppress it with westerly flow. To parameterize this effect in the atmosphere, this study introduces the Coriolis terms to the Cloud Layers Unified By Binormals (CLUBB) parameterization of clouds and turbulence. We design three single-column benchmarks to test the implementation of the NCTs in CLUBB. First, assuming that all except the Coriolis terms vanish on the right-hand side of the prognostic equations of the second-order moments of velocity, we derive an analytical solution in which the anisotropy of the moments rotates back to the initial state with a certain period. Our CLUBB results match this analytic benchmark. Second, assuming dry and neutrally stratified atmosphere with constant geostrophic winds, our CLUBB and LES results suggest that the NCTs make the Ekman layer deeper with geostrophic easterlies but shallower with westerlies. Third, under realistic conditions for trade-wind shallow convection, our CLUBB results show that the cloud layer becomes shallower if we omit the NCTs or flip the geostrophic winds from easterly to westerly. These benchmarks not only validate the Coriolis terms in CLUBB but also form a model hierarchy that aids our understanding of the effects of the NCTs on turbulence and convection.
- Open Access
- 11 June 2026
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 53 (12)
Assessing the Impact of Countergradient Fluxes on the General Circulation in the Community Atmosphere Model
Parameterizing boundary layer turbulence in Earth System Models (ESMs) introduces a key source of uncertainty. Here, we explore the impact of implementing a prognostic formulation (PMF) for momentum flux, which permits countergradient (CG) fluxes. We implement PMF in the turbulence parameterization in the Community Atmosphere Model version 6 (CAM6). CG fluxes in PMF reduce globally‐integrated momentum flux in CAM6. A similar response in globally‐integrated momentum flux is observed when reducing a tunable diffusivity parameter in the existing diagnostic formulation for momentum flux (DMF). Both methods of reducing effective eddy diffusivity produce qualitatively similar responses in the modeled general circulation, namely an enhanced upward branch of the Hadley cell, increased equatorward low‐level flow, and strengthened meridional temperature and moisture gradients. However, the reduction in effective eddy diffusivity from CG fluxes in PMF produces a higher‐magnitude response in the general circulation compared to reducing the diffusivity parameter in DMF.
- 11 June 2026
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 53 (12)
Open AccessAssessing the Impact of Countergradient Fluxes on the General Circulation in the Community Atmosphere Model
Parameterizing boundary layer turbulence in Earth System Models (ESMs) introduces a key source of uncertainty. Here, we explore the impact of implementing a prognostic formulation (PMF) for momentum flux, which permits countergradient (CG) fluxes. We implement PMF in the turbulence parameterization in the Community Atmosphere Model version 6 (CAM6). CG fluxes in PMF reduce globally‐integrated momentum flux in CAM6. A similar response in globally‐integrated momentum flux is observed when reducing a tunable diffusivity parameter in the existing diagnostic formulation for momentum flux (DMF). Both methods of reducing effective eddy diffusivity produce qualitatively similar responses in the modeled general circulation, namely an enhanced upward branch of the Hadley cell, increased equatorward low‐level flow, and strengthened meridional temperature and moisture gradients. However, the reduction in effective eddy diffusivity from CG fluxes in PMF produces a higher‐magnitude response in the general circulation compared to reducing the diffusivity parameter in DMF.
- Open Access
- 5 June 2026
- Published by Wiley
Effectiveness of observable constraints on the worst-case uncertainty of a global atmospheric model
- 5 June 2026
- Published by Wiley
Open AccessEffectiveness of observable constraints on the worst-case uncertainty of a global atmospheric model
- Open Access
- 18 May 2026
- Published by American Geophysical Union (AGU) in Journal of Advances in Modeling Earth Systems
- Vol. 18 (5)
Enhancing Great Plains Nocturnal Precipitation and Low‐Level Jets in AM4 With an Extended CLUBB Closure
In this study, we extend the Cloud Layers Unified by Binormals (CLUBB) turbulence scheme within the GFDL atmospheric model (AM4) by implementing direct momentum‐flux prognosis and a multiscale turbulent lengthscale, to improve the simulation of nocturnal precipitation and associated Low‐Level Jets (LLJs) over the Great Plains (GP). Toward this aim, we set up four AM4‐CLUBB configurations: diagnosed momentum flux, prognosed momentum flux, diagnosed momentum flux with a multiscale turbulent lengthscale, and prognosed momentum flux with a multiscale turbulent lengthscale. Simulations are evaluated against the AM4 control, the Integrated Multi‐satellitE Retrievals for GPM (IMERG), and the Doppler wind radar profiles from the Atmospheric Radiation Measurement program. Results show that all AM4‐CLUBB configurations improve the precipitation timing from the unrealistic midday peak seen in the AM4 control simulation toward the satellite‐observed nocturnal maximum. The configuration that prognoses momentum flux and uses a multi‐scale turbulent lengthscale, best matches the timing and intensity of GP precipitation rate. This configuration is also that which more accurately simulates the ARM‐observed nocturnal LLJ wind profiles, while increasing the frequency of counter‐gradient momentum fluxes near the LLJ core compared to prognosing momentum fluxes with the original AM4‐CLUBB turbulent lengthscale. Momentum budget analysis attributes this increase to a nearly fivefold enhancement in the buoyancy production term when using the multiscale formulation, and leads to stronger nocturnal convective activity, as diagnosed from the greater vertical velocity skewness and plume asymmetry.
- 18 May 2026
- Published by American Geophysical Union (AGU) in Journal of Advances in Modeling Earth Systems
- Vol. 18 (5)
Open AccessEnhancing Great Plains Nocturnal Precipitation and Low‐Level Jets in AM4 With an Extended CLUBB Closure
In this study, we extend the Cloud Layers Unified by Binormals (CLUBB) turbulence scheme within the GFDL atmospheric model (AM4) by implementing direct momentum‐flux prognosis and a multiscale turbulent lengthscale, to improve the simulation of nocturnal precipitation and associated Low‐Level Jets (LLJs) over the Great Plains (GP). Toward this aim, we set up four AM4‐CLUBB configurations: diagnosed momentum flux, prognosed momentum flux, diagnosed momentum flux with a multiscale turbulent lengthscale, and prognosed momentum flux with a multiscale turbulent lengthscale. Simulations are evaluated against the AM4 control, the Integrated Multi‐satellitE Retrievals for GPM (IMERG), and the Doppler wind radar profiles from the Atmospheric Radiation Measurement program. Results show that all AM4‐CLUBB configurations improve the precipitation timing from the unrealistic midday peak seen in the AM4 control simulation toward the satellite‐observed nocturnal maximum. The configuration that prognoses momentum flux and uses a multi‐scale turbulent lengthscale, best matches the timing and intensity of GP precipitation rate. This configuration is also that which more accurately simulates the ARM‐observed nocturnal LLJ wind profiles, while increasing the frequency of counter‐gradient momentum fluxes near the LLJ core compared to prognosing momentum fluxes with the original AM4‐CLUBB turbulent lengthscale. Momentum budget analysis attributes this increase to a nearly fivefold enhancement in the buoyancy production term when using the multiscale formulation, and leads to stronger nocturnal convective activity, as diagnosed from the greater vertical velocity skewness and plume asymmetry.
- Open Access
- 8 May 2026
- Published by Copernicus GmbH in Geoscientific Model Development
- Vol. 19 (9) , 3783-3800
Actionable reporting of CPU-GPU performance comparisons: insights from a CLUBB case study
Graphics Processing Units (GPUs) are becoming increasingly central to high-performance computing (HPC), but fair comparison with central processing units (CPUs) remains challenging, particularly for applications that can be subdivided into smaller workloads. Traditional metrics such as speedup ratios can overstate GPU advantages and obscure the conditions under which CPUs are competitive, as they depend strongly on workload choice. We introduce two peak-based performance metrics, the Peak Ratio Crossover (PRC) and the Peak-to-Peak Ratio (PPR), which provide clearer comparisons by accounting for the best achievable performance of each device. Using the performance of the Cloud Layers Unified by Binormals (CLUBB) standalone model as a case study, we demonstrate these metrics in practice, show how they can guide execution strategy, and examine how they shift under factors that affect workload. We further analyze how implementation choices and code structure influence these metrics, showing how they enable performance comparisons to be expressed in a concise and actionable way, while also helping identify which optimization efforts should be prioritized to meet different performance goals.
- 8 May 2026
- Published by Copernicus GmbH in Geoscientific Model Development
- Vol. 19 (9) , 3783-3800
Open AccessActionable reporting of CPU-GPU performance comparisons: insights from a CLUBB case study
Graphics Processing Units (GPUs) are becoming increasingly central to high-performance computing (HPC), but fair comparison with central processing units (CPUs) remains challenging, particularly for applications that can be subdivided into smaller workloads. Traditional metrics such as speedup ratios can overstate GPU advantages and obscure the conditions under which CPUs are competitive, as they depend strongly on workload choice. We introduce two peak-based performance metrics, the Peak Ratio Crossover (PRC) and the Peak-to-Peak Ratio (PPR), which provide clearer comparisons by accounting for the best achievable performance of each device. Using the performance of the Cloud Layers Unified by Binormals (CLUBB) standalone model as a case study, we demonstrate these metrics in practice, show how they can guide execution strategy, and examine how they shift under factors that affect workload. We further analyze how implementation choices and code structure influence these metrics, showing how they enable performance comparisons to be expressed in a concise and actionable way, while also helping identify which optimization efforts should be prioritized to meet different performance goals.
- Open Access
- 14 March 2026
- Published by Copernicus GmbH
Enhancing Great Plains Nocturnal Precipitation and Low-Level Jets in AM4 with an Extended CLUBB Closure
We extend the Cloud Layers Unified by Binormals (CLUBB) turbulence scheme within the GFDL atmospheric model (AM4) by implementing direct momentum-flux prognosis and a multiscale turbulent length scale, to improve the simulation of nocturnal precipitation and associated Low-Level Jets (LLJs) over the Great Plains (GP). Towards this aim, we set up four AM4-CLUBB configurations: diagnosed momentum flux, prognosed momentum flux, diagnosed momentum flux with a multiscale turbulent lengtshcale, and prognosed momentum flux with a multiscale turbulent lengtshcale. Simulations are evaluated against the AM4 control, the Integrated Multi-satellitE Retrievals for GPM (IMERG), and the Doppler wind radar profiles from the Atmospheric Radiation Measurement (ARM) program. Results show that all AM4-CLUBB configurations improve the precipitation timing from the unrealistic midday peak seen in the AM4 control simulation toward the satellite-observed nocturnal maximum. The configuration that prognoses momentum flux and uses a multi-scale turbulent length scale, best matches the timing and intensity of GP precipitation rate. This configuration is also that which more accurately simulates the ARM-observed nocturnal LLJ wind profiles, while increasing the frequency of counter-gradient momentum fluxes near the LLJ core compared to prognosing momentum fluxes with the original AM4-CLUBB turbulent lengthscale. Momentum budget analysis attributes this increase to a nearly fivefold enhancement in the buoyancy production term when using the multiscale formulation, and leads to stronger nocturnal convective activity, as diagnosed from the greater vertical velocity skewness and plume asymmetry.
- 14 March 2026
- Published by Copernicus GmbH
Open AccessEnhancing Great Plains Nocturnal Precipitation and Low-Level Jets in AM4 with an Extended CLUBB Closure
We extend the Cloud Layers Unified by Binormals (CLUBB) turbulence scheme within the GFDL atmospheric model (AM4) by implementing direct momentum-flux prognosis and a multiscale turbulent length scale, to improve the simulation of nocturnal precipitation and associated Low-Level Jets (LLJs) over the Great Plains (GP). Towards this aim, we set up four AM4-CLUBB configurations: diagnosed momentum flux, prognosed momentum flux, diagnosed momentum flux with a multiscale turbulent lengtshcale, and prognosed momentum flux with a multiscale turbulent lengtshcale. Simulations are evaluated against the AM4 control, the Integrated Multi-satellitE Retrievals for GPM (IMERG), and the Doppler wind radar profiles from the Atmospheric Radiation Measurement (ARM) program. Results show that all AM4-CLUBB configurations improve the precipitation timing from the unrealistic midday peak seen in the AM4 control simulation toward the satellite-observed nocturnal maximum. The configuration that prognoses momentum flux and uses a multi-scale turbulent length scale, best matches the timing and intensity of GP precipitation rate. This configuration is also that which more accurately simulates the ARM-observed nocturnal LLJ wind profiles, while increasing the frequency of counter-gradient momentum fluxes near the LLJ core compared to prognosing momentum fluxes with the original AM4-CLUBB turbulent lengthscale. Momentum budget analysis attributes this increase to a nearly fivefold enhancement in the buoyancy production term when using the multiscale formulation, and leads to stronger nocturnal convective activity, as diagnosed from the greater vertical velocity skewness and plume asymmetry.
- Open Access
- 13 March 2026
- Published by Copernicus GmbH
Tropical Cyclones in CAM7: Assessing the Impact of Prognostic Momentum Fluxes and Convective Parameterization at Global and Storm Scales
Accurately simulating tropical cyclones (TCs) in global climate models remains a key challenge due to not only multiscale interactions that govern storm genesis, intensity, and structure, but computational constraints that limit model grid spacing. Here we evaluate TC representation in a development version of the Community Atmosphere Model, version 7 (CAM7), which introduces several major updates, including higher vertical resolution, a revised Zhang-McFarlane deep convection scheme, and a new prognostic formulation for turbulent momentum fluxes in the boundary-layer scheme CLUBB. Using a suite of globally-uniform and variable-resolution simulations at 0.25deg grid spacing, we assess both large-scale statistics (global and basinwise TC frequency) and storm-scale characteristics (inflow angle, inflow depth, and wind structure).CAM7 with prognostic momentum fluxes produces improved spatial patterns of TC activity and more realistic intensity metrics compared to prior CAM generations. However, default configurations overproduce storms by roughly a factor of two. By increasing the parameterized CAPE consumption by deep convection during TC genesis, we achieve a ~40% reduction in global TC counts and improved agreement with observed basin distributions. At the storm scale, we reduce boundary-layer diffusivity, leading to stronger tangential winds, larger inflow angles, and shallower inflow layers, consistent with idealized f-plane sensitivity experiments and more in line with both observations and large-eddy simulations.These results demonstrate that targeted parameter tuning in deep convection and boundary-layer turbulence schemes can substantially improve both the frequency and structure of simulated TCs in CAM7, advancing its capability for high-resolution climate and weather prediction applications.
- 13 March 2026
- Published by Copernicus GmbH
Open AccessTropical Cyclones in CAM7: Assessing the Impact of Prognostic Momentum Fluxes and Convective Parameterization at Global and Storm Scales
Accurately simulating tropical cyclones (TCs) in global climate models remains a key challenge due to not only multiscale interactions that govern storm genesis, intensity, and structure, but computational constraints that limit model grid spacing. Here we evaluate TC representation in a development version of the Community Atmosphere Model, version 7 (CAM7), which introduces several major updates, including higher vertical resolution, a revised Zhang-McFarlane deep convection scheme, and a new prognostic formulation for turbulent momentum fluxes in the boundary-layer scheme CLUBB. Using a suite of globally-uniform and variable-resolution simulations at 0.25deg grid spacing, we assess both large-scale statistics (global and basinwise TC frequency) and storm-scale characteristics (inflow angle, inflow depth, and wind structure).CAM7 with prognostic momentum fluxes produces improved spatial patterns of TC activity and more realistic intensity metrics compared to prior CAM generations. However, default configurations overproduce storms by roughly a factor of two. By increasing the parameterized CAPE consumption by deep convection during TC genesis, we achieve a ~40% reduction in global TC counts and improved agreement with observed basin distributions. At the storm scale, we reduce boundary-layer diffusivity, leading to stronger tangential winds, larger inflow angles, and shallower inflow layers, consistent with idealized f-plane sensitivity experiments and more in line with both observations and large-eddy simulations.These results demonstrate that targeted parameter tuning in deep convection and boundary-layer turbulence schemes can substantially improve both the frequency and structure of simulated TCs in CAM7, advancing its capability for high-resolution climate and weather prediction applications.
- Open Access
- 10 March 2026
- Published by Copernicus GmbH
- Vol. 2025, 1-28
Reply on RC2
Graphics Processing Units (GPUs) are becoming increasingly central to high-performance computing (HPC), but fair comparison with central processing units (CPUs) remains challenging, particularly for applications that can be subdivided into smaller workloads. Traditional metrics such as speedup ratios can overstate GPU advantages and obscure the conditions under which CPUs are competitive, as they depend strongly on workload choice. We introduce two peak-based performance metrics, the Peak Ratio Crossover (PRC) and the Peak-to-Peak Ratio (PPR) which provide clearer comparisons by accounting for the best achievable performance of each device. Using a case study into the performance of the Cloud Layers Unified by Binormals (CLUBB) standalone model, we demonstrate these metrics in practice, show how they can guide execution strategy, and examine how they shift under factors that affect workload. We further analyze how implementation choices and code structure influence these metrics, showing how they enable performance comparisons to be expressed in a concise and actionable way, while also helping identify which optimization efforts should be prioritized to meet different performance goals.
- 10 March 2026
- Published by Copernicus GmbH
- Vol. 2025, 1-28
Open AccessReply on RC2
Graphics Processing Units (GPUs) are becoming increasingly central to high-performance computing (HPC), but fair comparison with central processing units (CPUs) remains challenging, particularly for applications that can be subdivided into smaller workloads. Traditional metrics such as speedup ratios can overstate GPU advantages and obscure the conditions under which CPUs are competitive, as they depend strongly on workload choice. We introduce two peak-based performance metrics, the Peak Ratio Crossover (PRC) and the Peak-to-Peak Ratio (PPR) which provide clearer comparisons by accounting for the best achievable performance of each device. Using a case study into the performance of the Cloud Layers Unified by Binormals (CLUBB) standalone model, we demonstrate these metrics in practice, show how they can guide execution strategy, and examine how they shift under factors that affect workload. We further analyze how implementation choices and code structure influence these metrics, showing how they enable performance comparisons to be expressed in a concise and actionable way, while also helping identify which optimization efforts should be prioritized to meet different performance goals.
- Open Access
- 10 March 2026
- Published by Copernicus GmbH
- Vol. 2025, 1-28
Reply on RC1
Graphics Processing Units (GPUs) are becoming increasingly central to high-performance computing (HPC), but fair comparison with central processing units (CPUs) remains challenging, particularly for applications that can be subdivided into smaller workloads. Traditional metrics such as speedup ratios can overstate GPU advantages and obscure the conditions under which CPUs are competitive, as they depend strongly on workload choice. We introduce two peak-based performance metrics, the Peak Ratio Crossover (PRC) and the Peak-to-Peak Ratio (PPR) which provide clearer comparisons by accounting for the best achievable performance of each device. Using a case study into the performance of the Cloud Layers Unified by Binormals (CLUBB) standalone model, we demonstrate these metrics in practice, show how they can guide execution strategy, and examine how they shift under factors that affect workload. We further analyze how implementation choices and code structure influence these metrics, showing how they enable performance comparisons to be expressed in a concise and actionable way, while also helping identify which optimization efforts should be prioritized to meet different performance goals.
- 10 March 2026
- Published by Copernicus GmbH
- Vol. 2025, 1-28
Open AccessReply on RC1
Graphics Processing Units (GPUs) are becoming increasingly central to high-performance computing (HPC), but fair comparison with central processing units (CPUs) remains challenging, particularly for applications that can be subdivided into smaller workloads. Traditional metrics such as speedup ratios can overstate GPU advantages and obscure the conditions under which CPUs are competitive, as they depend strongly on workload choice. We introduce two peak-based performance metrics, the Peak Ratio Crossover (PRC) and the Peak-to-Peak Ratio (PPR) which provide clearer comparisons by accounting for the best achievable performance of each device. Using a case study into the performance of the Cloud Layers Unified by Binormals (CLUBB) standalone model, we demonstrate these metrics in practice, show how they can guide execution strategy, and examine how they shift under factors that affect workload. We further analyze how implementation choices and code structure influence these metrics, showing how they enable performance comparisons to be expressed in a concise and actionable way, while also helping identify which optimization efforts should be prioritized to meet different performance goals.