Overview of MPAS Atmosphere


The atmospheric component of MPAS, as with all MPAS components, uses an unstructured centroidal Voronoi mesh (grid, or tessellation) and C-grid staggering of the state variables as the basis for the horizontal discretization in the fluid-flow solver. The unstructured variable resolution meshes can be generated having smoothly-varying mesh transitions (see the figure to the right); we believe that this capability will ameliorate many issues associated with the traditional mesh refinement strategy of one-way and two-way grid nesting where the transitions are abrupt. Using the flexibility of the MPAS meshes, we are working towards applications in high-resolution numerical weather prediction (NWP) and regional climate, in addition to global uniform-resolution NWP and climate applications.

The MPAS atmosphere consists of an atmospheric fluid-flow solver (the dynamical core) and a subset of the Advanced Research WRF (ARW) model atmospheric physics. Work is underway to port the MPAS atmospheric dynamical core to the Community Atmosphere Model (CAM) in the Community Earth Systems Model (CESM), which will provide coupling between MPAS Ocean and MPAS Atmosphere and coupling to the CAM physics and other components of the CESM system. Work is also progressing on porting the National Centers for Environmental Prediction (NCEP) Global Forecast System (GFS) atmospheric physics to MPAS.

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Dynamical Core

The MPAS atmospheric dynamical core solves the fully compressible nonhydrostatic equations of motion. The horizontal Voronoi mesh, depicted to the right, uses a C-grid staggering of the state variables; the horizontal velocity u is defined as the normal velocity on Voronoi cell faces while the other state variables are defined at the cell centers. The dual of the Voronoi mesh is the triangular mesh shown in dashed lines in the figure. The variable resolution meshes a predominantly comprised of hexagons, but pentagons and septagons are occasionally present. The primary advances associated with the C-grid-staggered Voronoi mesh can be found in Thuburn et al, 2009 and Ringler et al, 2010.

A description of the compressible nonhydrostatic atmospheric solver can be found in Skamarock et al, 2012. The fully compressible nonhydrostatic equations are cast in terms of a geometric-height vertical coordinate, and the solver makes use of a split-explicit time integration scheme that is described in Klemp et al, 2007. The time-integration scheme employs a 3rd-order Runge-Kutta method, and large time step, for the meteorologically significant modes and a forward-backward method with smaller time steps for the acoustic modes (See Wicker and Skamarock, 2002). The numerical schemes used in the atmospheric component of MPAS are very similar to those employed in the Advanced Research WRF model. The major differences are that the ARW model uses rectangular meshes and a hydrostatic pressure (mass) vertical coordinate. Additionally, MPAS uses a vector-invariant form of the horizontal momentum equation and a more general version of the WRF transport scheme given in Skamarock and Gassmann, 2011.

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MPAS cross section through the Himalayas at 28 degrees N latitude for a 15 km (mean cell-center spacing) uniform mesh. The model top is at 30 km. The vertical coordinate in the MPAS-Atmosphere solver allows for both the traditional terrain following coordinate (left) and a general hybrid coordinate (right).



The MPAS-Atmosphere solver can use a traditional terrain-following height coordinate, where the horizontal coordinate surfaces are terrain following at the lowest level and relax to a constant height surface at the rigid-lid upper boundary. MPAS-A can also use a generalized hybrid coordinate that can be configured to relax to a constant height at an intermediate height below the lid and, additionally, preferentially filter the small wavelength topography features in the terrain-following component at higher levels. The formulation is described in Klemp, 2011.




Atmospheric Physics


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The MPAS-Atmosphere solver uses a physics suite taken from the Advanced Research WRF model focusing on the physics configurations used in the ARW Nested Regional Climate Model application (WRF-NRCM) and the tropical cyclone prediction experiments. The physics are described in the WRF-ARW Technical Note. The available physics packages are:


Surface Layer

module_sf_sfclay.F (Monin-Obukhov) as in WRF 4.5; MYNN as in WRF 3.6.1.

PBL

YSU as in WRF 4.5; MYNN as in WRF 3.6.1.

Land Surface Model

Noah (4-layers) as in WRF 4.5.

Gravity Wave Drag

YSU GWDO as in WRF 4.5.

Convection

Kain-Fritsch as in WRF 3.2.1; Tiedtke as in WRF 3.3.1; New Tiedtke as in WRF 4.5; modified version of scale-aware Grell-Freitas as in WRF 3.6.1.

Microphysics

WSM6 as in WRF 4.5; Thompson (non-aerosol aware) as in WRF 3.8.1; Kessler

Radiation

RRTMG sw as in WRF 3.8.1; RRTMG lw as in WRF 3.8.1; CAM radiation as in WRF 3.3.1, with some additions from WRF 3.5.

MPAS-Atmosphere will also be available as a CAM core in CESM. As such the MPAS dynamical core will have use of the full CAM physics suite as well as model coupling to other CESM components included the ocean cores MPAS and POP, the land model CLM, ice models, etc.




Further Information

More information on MPAS can be found on the MPAS home page. The atmospheric solver is being developed primarily at the National Center for Atmospheric Research (NCAR) in the Mesoscale and Microscale Meteorology (MMM) Division in NCAR’s Earth Systems Laboratory (NESL). For further information on the atmospheric solver contact Bill Skamarock at NSF NCAR.