Poster + Paper
13 December 2020 An open-source Gaussian beamlet decomposition tool for modeling astronomical telescopes
Author Affiliations +
Conference Poster
Abstract
In the pursuit of directly imaging exoplanets, the high-contrast imaging community has developed a multitude of tools to simulate the performance of coronagraphs on segmented-aperture telescopes. As the scale of the telescope increases and science cases move toward shorter wavelengths, the required physical optics propagation to optimize high-contrast imaging instruments becomes computationally prohibitive. Gaussian Beamlet Decom- position (GBD) is an alternative method of physical optics propagation that decomposes an arbitrary wavefront into paraxial rays. These rays can be propagated expeditiously using ABCD matrices, and converted into their corresponding Gaussian beamlets to accurately model physical optics phenomena without the need of diffraction integrals. The GBD technique has seen recent development and implementation in commercial software (e.g. FRED, CODE V, ASAP)1-3 but appears to lack an open-source platform. We present a new GBD tool developed in Python to model physical optics phenomena, with the goal of alleviating the computational burden for modeling complex apertures, many-element systems, and introducing the capacity to model misalignment errors. This study demonstrates the synergy of the geometrical and physical regimes of optics utilized by the GBD technique, and is motivated by the need for advancing open-source physical optics propagators for segmented- aperture telescope coronagraph design and analysis. This work illustrates GBD with Poisson's spot calculations and show significant runtime advantage of GBD over Fresnel propagators for many-element systems.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jaren N. Ashcraft and Ewan S. Douglas "An open-source Gaussian beamlet decomposition tool for modeling astronomical telescopes", Proc. SPIE 11450, Modeling, Systems Engineering, and Project Management for Astronomy IX, 114501D (13 December 2020); https://doi.org/10.1117/12.2561921
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KEYWORDS
Telescopes

Image segmentation

Wave propagation

Systems modeling

Coronagraphy

Device simulation

Exoplanets

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