Integrated Ray Tracing (IRT) simulation of SCOTS measurement of GMT fast steering mirror surface

Ji Nyeong Choi; Dongok Ryu; Sug-Whan Kim; Logan Graves; Peng Su; Run Huang; Dae Wook Kim

doi:10.1117/12.2188845

16 November 2015 Integrated Ray Tracing (IRT) simulation of SCOTS measurement of GMT fast steering mirror surface

Ji Nyeong Choi, Dongok Ryu, Sug-Whan Kim, Logan Graves, Peng Su, Run Huang, Dae Wook Kim

Proceedings Volume 9575, Optical Manufacturing and Testing XI; 957513 (2015) https://doi.org/10.1117/12.2188845
Event: SPIE Optical Engineering + Applications, 2015, San Diego, California, United States

Abstract

The Software Configurable Optical Testing System (SCOTS) is one of the newest testing methods for large mirror surfaces. The Integrated Ray Tracing (IRT) technique can be applicable to the SCOTS simulation by performing non-sequential ray tracing from the screen to the camera detector in the real scale. Therefore, the radiometry of distorted pattern images are numerically estimated by the IRT simulation module. In this study, we construct an IRT SCOTS simulation model for the Fast Steering Mirror Prototype (FSMP) surface of the Giant Magellan Telescope (GMT). GMT FSMP is an off-axis ellipsoidal concave mirror that is 1064 mm in diameter and has PV 3.1 mm in aspheric departure. The surface error requirement is less than 20 nm rms. The screen is modeled as an array of 1366 by 768 screen pixels of 0.227 mm in pitch size. The screen is considered as a Lambertian scattering surface. The screen and the camera are positioned around 4390 mm away from the mirror and separated by around 132 mm from each other. The light source are scanning lines and sinusoidal patterns generated by 616,050 rays per one screen pixel. Of the initially generated rays, 0.22 % are received by the camera’s detector and contribute to form distorted pattern images. These images are converted to the slope and height maps of the mirror surface. The final result for the height difference between input surface and reconstructed surface was 14.14 nm rms. Additionally, the simulated mirror pattern image was compared with the real SCOTS test for the GMT FSMP. This study shows applicability of using the IRT model to SCOTS simulation with nanometer level numerical accuracy.

Citation Download Citation

Ji Nyeong Choi, Dongok Ryu, Sug-Whan Kim, Logan Graves, Peng Su, Run Huang, and Dae Wook Kim "Integrated Ray Tracing (IRT) simulation of SCOTS measurement of GMT fast steering mirror surface", Proc. SPIE 9575, Optical Manufacturing and Testing XI, 957513 (16 November 2015); https://doi.org/10.1117/12.2188845

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