Prysm is a python 3.6+ library for numerical optics. It contains features that are a superset of POPPY or PROPER for physical optics, as well as thin lens, thin film, and detector modeling. There is also a submodule that can replace the software that comes with an interferometer for data analysis. On CPU, end-to-end calculation is more than 3x as fast as the above for like-for-like calculations. On GPU, prysm is more than 1,000x faster than its competition.
The library can be used for everything from forward modeling of optical systems from camera lenses to coronographs to reverse modeling and phase retrieval. Due to its composable structure, it plays well with others and can be substituted in or out of other code easily. For a list of features, see the documentation. Of special note is prysm's interchangeable backend system, which allows the user to freely exchange numpy for cupy, enabling use of a GPU for all computations, or other similar exchanges, such as pytorch for algorithmic differentiation.
prysm is on pypi:
pip install prysm
Prysm uses numpy for array operations or any compatible library. To use GPUs, you may install cupy and use it as the backend at runtime. Plotting uses matplotlib. Images are read and written with imageio. Some MTF utilities utilize pandas and seaborn. Reading of Zygo datx files requires h5py.
Some features may be missing from this list.
Several examples are provided in the documentation.
A guide for using the library is provided in the documentation.
If you find an issue with prysm, please open an issue or pull request. Prysm has some usage of f-strings, so any code contributed is only expected to work on python 3.6+, and is licensed under the MIT license. The library is most in need of contributions in the form of tests and documentation.
Here lies a short list of organizations or projects using prysm:
prysm was used to perform phase retrieval used to focus Nav and Hazcam, enhanced engineering cameras used to operate the Mars2020 Perserverence rover.
prysm is used to build the official model of LOWFS, the Low Order Wavefront Sensing (and Control) system for the Roman coronoagraph instrument. In this application, it has been used to validate dynamics of a hardware testbed to 35 picometers, or 0.08% of the injected dynamics.
prysm is used by several FFRDCs in the US, as well as their equivalent organizations abroad
prysm is used by multiple high and ultra precision optics manufactures as part of their metrology data processing workflow
prysm is used by multiple interferometer vendors to cross validate their own software offerings
prysm is used at multiple universities to model optics both in a generic capacity and laboratory systems
There are likely many more. These are key uses known to the authors.