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Geoscientific Model Development An interactive open-access journal of the European Geosciences Union
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Volume 10, issue 8
Geosci. Model Dev., 10, 3145-3165, 2017
https://doi.org/10.5194/gmd-10-3145-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
Geosci. Model Dev., 10, 3145-3165, 2017
https://doi.org/10.5194/gmd-10-3145-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.

Model description paper 28 Aug 2017

Model description paper | 28 Aug 2017

MicroHH 1.0: a computational fluid dynamics code for direct numerical simulation and large-eddy simulation of atmospheric boundary layer flows

Chiel C. van Heerwaarden1,2, Bart J. H. van Stratum1,2, Thijs Heus3, Jeremy A. Gibbs4, Evgeni Fedorovich5, and Juan Pedro Mellado2 Chiel C. van Heerwaarden et al.
  • 1Meteorology and Air Quality Group, Wageningen University, Wageningen, the Netherlands
  • 2Max Planck Institute for Meteorology, Hamburg, Germany
  • 3Cleveland State University, Cleveland, OH, USA
  • 4Department of Mechanical Engineering, University of Utah, Salt Lake City, UT, USA
  • 5University of Oklahoma, Norman, OK, USA

Abstract. This paper describes MicroHH 1.0, a new and open-source (www.microhh.org) computational fluid dynamics code for the simulation of turbulent flows in the atmosphere. It is primarily made for direct numerical simulation but also supports large-eddy simulation (LES). The paper covers the description of the governing equations, their numerical implementation, and the parameterizations included in the code. Furthermore, the paper presents the validation of the dynamical core in the form of convergence and conservation tests, and comparison of simulations of channel flows and slope flows against well-established test cases. The full numerical model, including the associated parameterizations for LES, has been tested for a set of cases under stable and unstable conditions, under the Boussinesq and anelastic approximations, and with dry and moist convection under stationary and time-varying boundary conditions. The paper presents performance tests showing good scaling from 256 to 32768 processes. The graphical processing unit (GPU)-enabled version of the code can reach a speedup of more than an order of magnitude for simulations that fit in the memory of a single GPU.

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MicroHH (www.microhh.org) is a new and open-source computational fluid dynamics code for the simulation of turbulent flows in the atmosphere. It is made to simulate atmospheric flows up to the finest detail levels at very high resolution. It has been designed from scratch in C++ in order to use a modern design that allows the code to run on more than 10 000 cores, as well as on a graphical processing unit.
MicroHH (www.microhh.org) is a new and open-source computational fluid dynamics code for the...
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