Geoscientific model development· 2026Q1
Towards high-fidelity simulations of coastal submesoscale baroclinic instabilities with MPAS-O (vE3SM3.0.0) – Part 1: Idealized experiments
- 1citations
- Q1SCImago
- 2026year
Short summary
MPAS-O (vE3S3.0.0) accurately simulates coastal submesoscale baroclinic instabilities, with performance primarily dependent on spatial grid resolution (down to 100m) rather than model choice, showing similar results to ROMS.
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Key points
- MPAS-O's simulation of coastal submesoscale baroclinic instabilities is highly similar across horizontal resolutions from 10 km to 100 m.
- Spatial grid resolution has a greater impact on simulation fidelity than the choice between MPAS-O and ROMS.
- MPAS-O exhibits less numerical mixing and more physical mixing compared to ROMS across all tested resolutions.
- Differences in numerical mixing are attributed to MPAS-O's flux-corrected transport tracer advection scheme and ROMS' MPDATA scheme.
AI-generated from the title and abstract; the full text is not read.
Abstract
Abstract. Rapid advances in computational power over the past decade have enabled global, kilometer-scale simulations that realistically represent open-ocean submesoscale dynamics. However, the ability of global ocean models to represent coastal submesoscale dynamics—where flows are more heterogeneous and strongly shaped by coastlines, bathymetry, and buoyancy inputs—remains largely unexplored. This study is the first of two companion papers assessing coastal submesoscale processes in MPAS-O, an unstructured global ocean model. Here, we present the first idealized evaluation of MPAS-O’s representation of coastal submesoscale dynamics using observed conditions in the Mississippi–Atchafalaya (M-A) River plume as a template for initial conditions, and with the previously validated structured-grid regional model ROMS serving as a benchmark. We compare statistical metrics based on flow invariants—total strain, relative vorticity, and divergence—as well as velocity gradients in frontal coordinates, across horizontal resolutions ranging from 10 km to 100 m within an idealized model domain. We find that the representation of submesoscale baroclinic instabilities is highly similar across all resolutions such that the impact of model choice is smaller than the choice of spatial grid resolution. We also compare numerical and physical mixing between models using online diagnostics based on discrete variance decay. We find that ROMS generally has more numerical mixing and less physical mixing than MPAS-O across all resolutions. Trends in numerical mixing likely arise from MPAS-O's flux-corrected transport tracer advection scheme, which is shown to be anti-diffusive relative to the MPDATA scheme used in the ROMS simulations. Trends in physical mixing likely arise from differences in each model’s configuration of the vertical mixing scheme (the K-Profile Parameterization). A companion paper extends this idealized model-model comparison to realistic simulations of the M-A River plume.
The authors' abstract, as published at the source. Geoscientific model development, 2026 · DOI ↗
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OceanographyEarth and Planetary Sciences