Articles | Volume 8, issue 10
Geosci. Model Dev., 8, 3131–3150, 2015
https://doi.org/10.5194/gmd-8-3131-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Special issue: Isaac Newton Institute programme on multiscale numerics for...
Model description paper 07 Oct 2015
Model description paper | 07 Oct 2015
DYNAMICO-1.0, an icosahedral hydrostatic dynamical core designed for consistency and versatility
T. Dubos et al.
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- Application of the Synchronized B-Grid Staggering for Solution of the Shallow-Water Equations on the Spherical Icosahedral Grid H. Miura 10.1175/MWR-D-18-0304.1
- DCMIP2016: a review of non-hydrostatic dynamical core design and intercomparison of participating models P. Ullrich et al. 10.5194/gmd-10-4477-2017
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- Impact and importance of hyperdiffusion on the spectral element method: A linear dispersion analysis P. Ullrich et al. 10.1016/j.jcp.2018.06.035
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- The Global Methane Budget 2000–2017 M. Saunois et al. 10.5194/essd-12-1561-2020
- A variational formulation of geophysical fluid motion in non-Eulerian coordinates T. Dubos 10.1002/qj.2942
- ORCHIDEE-ROUTING: revising the river routing scheme using a high-resolution hydrological database T. Nguyen-Quang et al. 10.5194/gmd-11-4965-2018
- Total energy and potential enstrophy conserving schemes for the shallow water equations using Hamiltonian methods – Part 1: Derivation and properties C. Eldred & D. Randall 10.5194/gmd-10-791-2017
- Accuracy analysis of mimetic finite volume operators on geodesic grids and a consistent alternative P. Peixoto 10.1016/j.jcp.2015.12.058
- Global climate modeling of Saturn's atmosphere. Part II: Multi-annual high-resolution dynamical simulations A. Spiga et al. 10.1016/j.icarus.2019.07.011
- A mixed mimetic spectral element model of the 3D compressible Euler equations on the cubed sphere D. Lee & A. Palha 10.1016/j.jcp.2019.108993
- An Energy Consistent Discretization of the Nonhydrostatic Equations in Primitive Variables M. Taylor et al. 10.1029/2019MS001783
- Global climate modeling of Saturn’s atmosphere. Part IV: Stratospheric equatorial oscillation D. Bardet et al. 10.1016/j.icarus.2020.114042
- Global climate modeling of Saturn's atmosphere. Part III: Global statistical picture of zonostrophic turbulence in high-resolution 3D-turbulent simulations S. Cabanes et al. 10.1016/j.icarus.2020.113705
- WAVETRISK-1.0: an adaptive wavelet hydrostatic dynamical core N. Kevlahan & T. Dubos 10.5194/gmd-12-4901-2019
- Simulation of the performance and scalability of message passing interface (MPI) communications of atmospheric models running on exascale supercomputers Y. Zheng & P. Marguinaud 10.5194/gmd-11-3409-2018
- Revealing the Intensity of Turbulent Energy Transfer in Planetary Atmospheres S. Cabanes et al. 10.1029/2020GL088685
- Idealised simulations of the deep atmosphere of hot Jupiters F. Sainsbury-Martinez et al. 10.1051/0004-6361/201936445
- Discretization of generalized Coriolis and friction terms on the deformed hexagonal C-grid A. Gassmann 10.1002/qj.3294
- Covariant Structure of Models of Geophysical Fluid Motion T. Dubos 10.1103/PhysRevLett.120.034501
- Numerical instabilities of spherical shallow-water models considering small equivalent depths P. Peixoto et al. 10.1002/qj.3191
- A quasi-Hamiltonian discretization of the thermal shallow water equations C. Eldred et al. 10.1016/j.jcp.2018.10.038
- A Layer‐Averaged Nonhydrostatic Dynamical Framework on an Unstructured Mesh for Global and Regional Atmospheric Modeling: Model Description, Baseline Evaluation, and Sensitivity Exploration Y. Zhang et al. 10.1029/2018MS001539
- NCAR Release of CAM‐SE in CESM2.0: A Reformulation of the Spectral Element Dynamical Core in Dry‐Mass Vertical Coordinates With Comprehensive Treatment of Condensates and Energy P. Lauritzen et al. 10.1029/2017MS001257
- Latitudinal variation of clouds’ structure responsible for Venus’ cold collar I. Garate-Lopez & S. Lebonnois 10.1016/j.icarus.2018.05.011
1 citations as recorded by crossref.
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Short summary
The design of the icosahedral atmospheric dynamical core DYNAMICO is presented. The key contribution is to combine a strict separatation of kinematics from dynamics to a Hamiltonian formulation of the equations of motion in a non-Eulerian vertical coordinate to achieve energetic consistency. This approach allows for a unified treatment of various equations of motion: multi-layer shallow-water equations and hydrostatic primitive equations.
The design of the icosahedral atmospheric dynamical core DYNAMICO is presented. The key...