Version 16 (modified by 3 years ago) ( diff ) | ,
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Code we could consider deleting
- rifts
- tetras
- flowband models
- ice model coupling
- ADOLC support
- remove external packages we are not using (and old versions of MPI/PETSc etc)
- LA theta XTaylor Hood Uzawa Pressure etc
- we should have a discussion about long term support for multiple interfaces
- tao
- KML (MATLAB can do most of it natively https://www.mathworks.com/help/map/exporting-vector-data-to-kml.html)
Things to improve/address
- [Mathieu] too many memory allocations
- [Surendra] get rid of Esa solver, adapt newly developed solid Earth capabilities instead
- [Mathieu] make
model
a dynamic class (do not set all fields by default). This would help integrate new solutions that may not be ice oriented into ISSM (e.g. GIA, Kriging, etc) - [Mathieu] treat material like friction: create/call class on the fly instead of carrying it in a dataset
- [Mathieu] Fast SSA (with static array allocation P1/triangle etc), would require to delete coupling....
- [Surendra] Code Ivins GIA module in C++....
- [Nicole] Thermal solution in GEMB improvement in speed (possible use of solvers instead of explicit loop)
New capabilities
- [Mathieu] Julia interface? may not be mature enough for what we want to do
- [Nicole] Coupling of GEMB to the thermal model
- [Mathieu / Nicole] Age tracking / advection of the snow layer
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