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Erwan Pannier edited this page Feb 14, 2021
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Welcome to the radis wiki!
We're still working on crafting our development plan. In the meantime see :
-
Extension to non-Voigt profiles / line-mixing. These are particularly important at high pressure. See for instance Alberti 2015
(news 2021) RADIS now has a Development Plan draft. Have a look on our 💬 Slack #roadmap
- Have a look at the Astropy Development Workflow. We should use something very similar here.
Radis participates in GSoC as part of the OpenAstronomy organization.
- GSoC Guidelines - read this first and follow the instructions!
The RADIS team is currently writing some 💡 GSOC 2021 project proposals. Some ideas :
- Optimize which Lineshape engine to use (LDM/historical) depending on the spectrum type : https://github.com/radis/radis-benchmark/issues/5
- GPU for nonequilibrium. See GPU Roadmap https://github.com/radis/radis/issues/144
- Automatic differentiation for tuning uncertain molecular data and/or computing exact Jacobian spectra. https://github.com/radis/radis/issues/153
- Performance: reduce Memory usage https://github.com/radis/radis/issues/118
- Read more line databases, in particular interface to ExoMol and ChiantiPy : https://github.com/radis/radis/issues/34
- RADIS for Big Data : switch to lazy database librairies like Vaex, stream the database to spectra "on-the-fly"
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GSoC 2020 Project Ideas (then search for
radis
projects)
Proposals :