AMUSE
Combine existing numerical codes in an easy to use Python framework. With AMUSE you can simulate objects such as star clusters, proto-planetary disks and galaxies.
Understanding the interaction between clouds and the large-scale circulation
Clouds and convection processes are important for the climate system, yet they are not explicitly resolved in global climate models due to computational limitations. The approximate parameterized representation of these processes is the main source of model uncertainty in climate models and has hampered progress in our understanding of the interaction between clouds and the large-scale circulation for decades.
We will pursue a new 3d-super-parameterization (3d-SP) approach to overcome this conundrum. This approach builds further on super-parameterization (SP) approach, proposed 15 years ago. We will nest 3-dimensional Large Eddy Simulation (LES) models into the grid columns of a Global Circulation Model.
This way, the parameterized descriptions of clouds, convection and turbulence with all their shortcomings will be replaced by a realistic 3-dimensional simulation technique for these processes.
Although computationally more expensive than traditional parameterizations and conventional super-parameterization, this approach is ideally suited to take full advantage of present-day parallel computers because of the minimal communication between the LES models and will be much more efficient than a direct simulation on the large scale at the resolution of the nested LES model.
This project team will use state-of-the-art high performance computing (HPC) technologies to make this approach feasible and within reach of modern supercomputers. Furthermore, the team plans to employ recently developed algorithmic approaches to further speed up computations.
The overarching goal is to develop and explore a computational tool that is able to realistically resolve the interaction between the large-scale atmospheric circulation and the smaller scale cloud and convective processes.
Reproducibility for digital-twin simulations in astrophysics
Using remote sensing to develop damage indicators across all Antarctic ice shelves
For future exascale climate and weather predictions
Coupling an implicit low-resolution model to an explicit high-resolution ocean model
The country below sea level
Handling data assimilation on a large scale
The evolution of embedded star clusters
Combine existing numerical codes in an easy to use Python framework. With AMUSE you can simulate objects such as star clusters, proto-planetary disks and galaxies.
A Python environment to interface and couple oceanographic and other earth system model codes.