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Optical simulation of the Simons Observatory Large Aperture Telescope and accompanying holography measurements.

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solat-optics

Code style: black Imports: isort

Near- and Far-field optical simulation of the Simons Observatory Large Aperture Telescope. This is the repository associated with the publication: The Simons Observatory: Characterizing the Large Aperture Telescope Receiver with Radio Holography.

Author: Grace E. Chesmore

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Installation Instructions:

  1. git clone [email protected]:McMahonCosmologyGroup/solat-optics.git
  2. cd solat_optics/
  3. pip3 install .

Tutorials

Three tutorials are available as Jupyter notebooks:

  1. Near-field
  2. Far-field
  3. Quantifying Optical Systematics

Near-field

Part 1 of the tutorial builds the surfaces of the optics tube which will eventually be used in the near-field simulation of the optics tube. First ray-trace from the focal plane out through the window. This toy-model is useful for predicting the beam path and size based on the receiver's position of the focal plane, however this will provide no diffraction information. The user can drag / zoom / and hover over the ray-trace to see the labelled optics tube surfaces.

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Part 2 ray-traces from both the source and the receiver positions to the Lyot stop, located near the center of the optics tube, yielding the source and receiver electric fields $E_{\text{source}}$ and $E_{\text{rec}}$. The Lyot stop defines the size of the beam and therefor we integrate the receiver and source electric fields over the area of the Lyot stop (where the pink and blue rays meet in the middle of the optics tube).

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Part 3 demonstrates how to run the simulation from the command line, and how to do so in parallel to speed up the simulation. Doing so will save the simulation to a .txt file. Lastly, the simulated near-field power and phase are read out from the text file and plotted.

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Far-field

Part 1 outlines the simulation where the optics tube simulated field is propagated through the two Large Aperture Telescope (LAT) mirrors. To do this, a ray-trace from a far-field point source through the LAT and to the LATR focal plane builds the electric field $E_{\text{source}}$. The simulated optics tube field is used as our receiver electric field $E_{\text{rec}}$.

Part 2 demonstrates how to run the simulation from the command line, and how to do so in parallel to speed up the simulation. Doing so will save the simulation to a .txt file. Lastly, the simulated far-field power and phase are read out from the text file and the amplitude of the far-field beam is plotted.

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Quantifying Optical Systematics

Contributions

If you have write access to this repository, please:

  • create a new branch
  • push your changes to that branch
  • merge or rebase to get in sync with main
  • submit a pull request on github
  • If you do not have write access, create a fork of this repository and proceed as described above. For more details, see Contributing.

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Optical simulation of the Simons Observatory Large Aperture Telescope and accompanying holography measurements.

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