code-saturne / code-saturne/code_saturne
Subgrid flux model for scalars
- Dominant language
- C++
- Stars
- 307
- Forks
- 102
- PR merge metrics
- No merged PRs in 30d
Description
Currently, for Large Eddy Simulations, subgrid flux of scalars are obtained using a constant subgrid Prandtl number (default value is 1). It would be interesting to have more options as scalar fluctuations are not always similar to velocity fluctuations.
(transferred from Mantis bug tracker issue 215, opened by Mathtrack).
Contributor guide
Research direction
The issue concerns scalar subgrid fluxes in Large Eddy Simulations, but it names no source files, tests, or entry points. First locate the existing constant subgrid-Prandtl implementation and related validation cases; done should mean additional scalar-flux options are supported and verified against appropriate simulation results.
Written by the indexing model from the issue text.
Assessment
- Domain
- hpc
- Issue type
- Feature
- Difficulty
- 5/5
- Estimated time
- Over a week
- Activity status
- Stale
- Clarity
- Needs clarification
- Newbie friendliness
- 25/100