Mr. Austin Nordman Profile

Austin Nordman

at Jet Propulsion Lab

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Proceedings Article | 30 September 2024 Presentation + Paper

Optical alignment of the Roman space telescope’s coronagraph instrument

Brian Monacelli, Jordan Rupp, Kris Tuason, David Aldrich, Caleb Baker, Brian Kern, Nathan Bush, Austin Nordman, Eric Ek, Sonny Gutierrez, Hong Tang

Proceedings Volume 13134, 131340E (2024) https://doi.org/10.1117/12.3030113

KEYWORDS: Optical alignment, Mirrors, Coronagraphy, Telescopes, Optical fabrication, Equipment, Twyman Green interferometers, Interferograms

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Optical alignment of the Coronagraph Instrument (CGI) was completed in time to begin its full-functional and environmental testing in late 2023 and its integration into the Roman Space Telescope (RST) in summer 2024. The optics of the CGI relay the optical pupil of the RST five times so that science operations, such as coronagraphy and wavefront control, can be conducted in the different internal pupil and image planes. Within the pupil relays, the CGI has multiple active optical assemblies, including a fast-steering mirror, a focus-control mirror, two deformable mirrors, and six precision alignment mechanisms that articulate different masks and apertures into the beam.

Initial alignment of the CGI optics was completed in the reverse direction, using a commercial dynamic Twyman-Green interferometer to measure the wavefront error through each relay as optics were added sequentially from back to front. The end-to-end wavefront error was initially verified using surrogate optics in place of the active optical assemblies, to allow their simultaneous development and test. Throughout alignment, pupil and image planes were referenced and coaligned optically using fiducials, including spherically mounted retroreflectors (SMRs) that were positioned by a laser tracker and measured by the interferometer camera.

Upon end-to-end alignment of the pupil-relay optics, the active optical assemblies were integrated and aligned individually, and the entire CGI alignment was then optimized. The CGI optical subsystem was also mapped to SMR fiducials, which will later be used to integrate CGI into the RST observatory and verify its alignment to the Telescope’s line of sight. This paper details the many alignment steps required to successfully achieve the performance criteria of the CGI.

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