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| Model Components of the Community Climate System Model (CCSM) |
For current and planned formulations of the CCSM, the Atmospheric dynamical core (dycore) will be the parallel bottleneck

Current operational dycores use Latitude-Longitude Grids: Well tested numerical methods, many good solutions to the “pole problem”, except these solutions all degrade parallel scalability
Petascale performance requires moving to quasi-uniform unstructured grids:![]() |
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Current SNL Focus: Integration and evaluation of cubed-sphere dycores into the CCSM.
- Initial dycore: Spectral Elements
- We developed a new locally conservative version based on compatibility (as opposed to flulx based local conservation)
- Motivated by DOE ASCR funded work on compatible differencing
- This will be the first dycore in CCSM to locally conserve both mass and energy
- Future dycores to be integrated and evaluated:
- GFDL Finite Volumes on the cubed-sphere
- NCAR Discontinuous Galerkin
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Maintained by Bernadette Watts






