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Bart J. H. van Stratum

Publications and source records attributed to Bart J. H. van Stratum.

2 recordsLinked to original sources

Comparing the dynamics of idealized squall lines between NWP and LES models

Both Numerical Weather Prediction (NWP) models and Large-Eddy Simulation (LES) models are used to simulate convective systems, such as squall lines, but with different purposes. NWP models aim for the most accurate weather forecasts, whereas LES models are typically used to advance our understanding of physical processes. Therefore, these types of models differ in their design. With increasing computer power, the domain sizes and resolutions of these models converge, which raises the question if the model results also converge. We investigated an idealized squall line with the NWP model ICON (ICOsahedral Non-hydrostatic) and the LES model MicroHH. These models differ in their design, mainly because ICON solves the compressible equations on a triangular grid, while MicroHH solves the anelastic equations on a regular grid. The case setup, including resolution, domain size, boundary conditions, and microphysics scheme, is aligned between the models. The models simulate the same squall-line structure and circulation pattern in simulations with both warm and ice microphysics. However, there are quantitative differences with MicroHH having a more intense squall-line circulation than ICON at all resolutions (1 km, 500 m, and 250 m), mainly because MicroHH has less numerical diffusion. The magnitude of the differences is sensitive to the advection scheme and the resolution and less sensitive to the formulation of turbulent diffusion. The quantitative differences between the models across resolutions highlight the importance of model physics and numerics, whereas the good qualitative agreement gives confidence that insights from LES can be applied in NWP.

physics.ao-ph↗

Shallow cumulus convection over land in cloud-resolving simulations with a coupled ray tracer

We present simulations of cumulus convection over land with shortwave radiation computed by a Monte Carlo ray tracer coupled to the flow solver. Ray tracing delivers very realistic in-cloud heating rates and global horizontal irradiance fields. The necessary performance of the ray tracer has been enabled by the raw power of GPU computing and from techniques for accelerating data lookup and ray tracer convergence. We used a case study over a grassland in the Netherlands to compare simulations with a coupled ray tracer to those with a conventional two-stream solver, and to test ray tracer convergence. We demonstrate that the simulated cloud evolution is insensitive across a wide range of samples sizes in the ray tracer. Furthermore, simulations with a coupled ray tracer produce surface irradiance patterns that resemble observations and that strongly feed back to the evolution of clouds via locally enhanced surface heat fluxes.

physics.ao-ph↗