Articles | Volume 10, issue 8
https://doi.org/10.5194/gmd-10-3145-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/gmd-10-3145-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
MicroHH 1.0: a computational fluid dynamics code for direct numerical simulation and large-eddy simulation of atmospheric boundary layer flows
Chiel C. van Heerwaarden
CORRESPONDING AUTHOR
Meteorology and Air Quality Group, Wageningen University, Wageningen, the Netherlands
Max Planck Institute for Meteorology, Hamburg, Germany
Bart J. H. van Stratum
Meteorology and Air Quality Group, Wageningen University, Wageningen, the Netherlands
Max Planck Institute for Meteorology, Hamburg, Germany
Thijs Heus
Cleveland State University, Cleveland, OH, USA
Jeremy A. Gibbs
Department of Mechanical Engineering, University of Utah, Salt Lake City, UT, USA
Evgeni Fedorovich
University of Oklahoma, Norman, OK, USA
Juan Pedro Mellado
Max Planck Institute for Meteorology, Hamburg, Germany
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3 citations as recorded by crossref.
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- Role of large eddies in the breakdown of the Reynolds analogy in an idealized mildly unstable atmospheric surface layer K. McColl et al. 10.1002/qj.3077
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Discussed (preprint)
Latest update: 18 Mar 2024
Short summary
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...