waveprop 0.0.10

Functions and scripts to simulate free-space optical wave propagation.

waveprop: Diffraction-based wave propagation simulator with PyTorch support

Python simulator for optical wave propagation based on scalar diffraction theory. Multiple propagation models are supported, with the desired propagation distance / complexity determining which one may be best. PyTorch support enables GPU acceleration and end-to-end training of arbitrary apertures.

Features

• Multiple scalar diffraction models: Fraunhofer, Fresnel, angular spectrum method, direct integration.
• Polychromatic through CIE color matching functions.
• Off-axis propagation and rescaling.
• PyTorch support (for GPU acceleration and end-to-end training).
• Arbitrary amplitude or phase masks.
• Spatial light modulator (SLM) simulator which incorporates deadspace and color filter.

Installation

pip install waveprop

To develop locally and/or play with examples, we recommend the following steps:

# create virtual environment
conda create -n waveprop python=3.9
conda activate waveprop

# install
pip install -e .

# for CUDA, check docs for appropriate command: https://pytorch.org/
conda install pytorch torchvision cudatoolkit=11.3 -c pytorch

# for some examples (e.g. holography.py)
pip install joblib imageio click

# run tests
pytest tests/

New release and upload to PyPi

From master branch of original repo, and using the appropriate value for X.X.X:

# Update version in setup.py

# Create tag and upload
git tag -a vX.X.X -m "Description."
git push origin vX.X.X

# Change version number in setup.py
python setup.py sdist

# Create package and upload to Pypi
twine upload dist/waveprop-X.X.X.tar.gz   

You will need a username and password for uploading to PyPi.

Finally, on GitHub set the new tag as the latest release by pressing the three dots to the right and selecting "Edit release, at top right selecting "Edit tag", and then publishing it!

Examples

In the [examples] folder are various scripts demonstrating the features of waveprop. It is recommended to run them from the repository root, as shown below.

Comparing propagation models

Polychromatic simulation

Off-axis and rescaling

PyTorch support

Spatial light modulator

Holography

The above GIF showing the propagation of a holography pattern was generated with the following command:

python examples/holography.py --target data/lcav.png --invert

The file path can be set to any local path, however the target will be reshaped to a square.

If only interested in the holography pattern at a single distance, e.g. the focal plane, the following command can be run, which will produce a GIF with a single image

python examples/holography.py --target data/lcav.png --invert --f_lens 0.5 --z_start 0.5 --nz 1

Scripts and functions to simulate free-space optical propagation.

In the examples folder:

• holography.py: determing phase pattern for holography and propagating over distances with angular spectrum method.
• adafruit_slm.py: polychromatric simulation of amplitude SLM with or without deadspace.
• adafruit_slm_mono_pytorch.py: monochromatric simulation of amplitude SLM with PyTorch support.
• square_ap_video.py: to compare various propagation approaches while varying the distance.
• square_ap_poly_video.py: polychromatic simulation of square aperture while varying the distance.
• circ_ap_fraunhofer.py: simulate circular aperture in the Fraunhofer regime.
• square_ap_fresnel.py: simulate square aperture in the Fresnel regime.
• bandlimiting_angular_spectrum.py: show benefit of band-limiting angular spectrum method.
• off_axis.py: comparing off-axis simulation with Fresnel, angular spectrum, and direct integration.
• rescale.py: comparing off-axis, rescaled simulation with Fresnel and angular spectrum.
• circ_ap_lab.py: simulate circular aperture with command-line defined arguments. Default is our lab setup.
• rect_ap_lab.py: simulate rectangular aperture with command-line defined arguments. Default is our lab setup.
• single_slit_lab.py (WIP): simulate single-slit with command-line defined arguments. Default is our lab setup.

NB: click is required for some scripts for parsing command-line arguments.

Following propagation models are implemented. All make use of FFT unless otherwise noted.

• Fraunhofer.
• Fresnel (one-step, two-step, multi-step, angular spectrum).
• Angular spectrum, with evanescent waves and option to bandlimit.
• Direct integration (no FFT), "brute force" numerical integration.
• FFT-DI, linearizes circular convolution of direction integration in DFT domain.
• Shifted Fresnel, uses three-FFT to model propagation off of optical axis with arbitrary input and output sampling.

Note that dimensions y corresponds to the first dimension (rows) while x corresponds to the second dimension (columns).

Literature and references

Fraunhofer and Fresnel numerical approaches come from the textbook "Numerical Simulation of Optical Wave Propagation with Examples in MATLAB" (2010). It is a very nicely-written book with code examples that are easy to follow.

A more rigorous treatment and derivation of Fraunhofer and Fresnel approximations analytic expressions, and conditions can be found in the following textbooks (we reference the following versions in the docstrings):

• "Introduction to Fourier Optics" by Goodman (Second Edition).
• "Fundamentals of Photonics" by Saleh and Teich (Third Edition).
• "Principles of Optics" by Born and Wolf (Seventh Edition).

A description of the Direct Integration (DI) method and its FFT version can be found in "Fast-Fourier-transform based numerical integration method for the Rayleigh–Sommerfeld diffraction formula" (2006). This serves as a good baseline as it is an approximation of the Rayleigh-Sommerfeld diffraction integral via a Riemann sum (Eq 9). Main drawbacks are computational load, as DI directly performs the discrete convolution and FFT-DI requires three FFTs. Moreover, FFT-DI is only practical for small output windows.

The angular spectrum (AS) approach is another well-known formulation that is directly derived from the Rayleigh-Sommerfeld equation. However, it tends to have issues outside of the scenarios of small apertures and in the near-field. "Band-Limited Angular Spectrum Method for Numerical Simulation of Free-Space Propagation in Far and Near Fields" offers a solution to this problem by limiting the bandwidth of the propagation field. An implementation of this approach has been largely replicated from the code of "Neural holography with camera-in-the-loop training". Their index-to-frequency mapping and FFT shifting seemed to be off, and they did not include evanescent waves; both of which were modified for the implementation found here.

Shifted Fresnel allows for the simulation off of the optical-axis and for arbitrary input and output sampling. A description of this approach can be found in "Shifted Fresnel diffraction for computational holography".

TODO

Propagation models:

• Interpolation of angular spectrum with FS coefficients (ours).
• Rectangular tiling, Section 4 of "Shifted Fresnel diffraction for computational holography".
• Circ aperture and single slit exp from "Fast-Fourier-transform based numerical integration method for the Rayleigh–Sommerfeld diffraction formula"

Examples:

• For single slit, something terribly wrong. Compare with following results:
  • https://core.ac.uk/download/pdf/233057112.pdf
  • https://www.osapublishing.org/josa/fulltext.cfm?uri=josa-59-3-293&id=53644
  • https://www.osapublishing.org/josa/fulltext.cfm?uri=josa-59-3-293&id=53644
• Double slit

Analytic forms of (see Born book):

• Fresnel circular aperture
• Fresnel rectangular aperture
• Circular aperture from "Fast-Fourier-transform based numerical integration method for the Rayleigh–Sommerfeld diffraction formula", Eq 36

Compare / mention complexity of different approaches

Other libraries

• Diffractio: https://diffractio.readthedocs.io/en/latest/readme.html
  • Cite "Applied Optics" vol 45 num 6 pp. 1102-1110 (2006) for Rayleigh Sommerfeld propagation.
• LightPipes: https://opticspy.github.io/lightpipes/manual.html#free-space-propagation
• AOtools: https://aotools.readthedocs.io/en/v1.0.1/opticalpropagation.html
  • Ported scripts from "Numerical Simulation of Optical Wave Propagation with Examples in MATLAB".
• PyOptica: https://gitlab.com/pyoptica/pyoptica
  • Free-space propagation: https://gitlab.com/pyoptica/pyoptica/-/blob/master/pyoptica/optical_elements/free_space.py
  • Gerschberg-Saxton: https://gitlab.com/pyoptica/pyoptica/-/blob/master/notebooks/gerchberg_saxton.ipynb
• DeepOptics: https://github.com/vsitzmann/deepoptics
  • Differentiable free-space propagation: https://github.com/vsitzmann/deepoptics/blob/defbb975309a6a3f3d2a86b92e82d02156ab213e/src/layers/optics.py#L386
• Angular Spectum: https://github.com/rafael-fuente/Diffraction-Simulations--Angular-Spectrum-Method
  • Monochromatic: https://github.com/rafael-fuente/Diffraction-Simulations--Angular-Spectrum-Method/blob/5b3610643b97ab6b81c80ef4c8aa5b0d9501f314/diffractsim/monochromatic_simulator.py#L191
  • Polychromatic: https://github.com/rafael-fuente/Diffraction-Simulations--Angular-Spectrum-Method/blob/5b3610643b97ab6b81c80ef4c8aa5b0d9501f314/diffractsim/polychromatic_simulator.py#L190

License

MIT