22 August 2017 Ground to on-orbit alignment study of the WFIRST wide-field channel and resulting changes in the telescope architecture
Author Affiliations +
The Wide-Field Infrared Survey Telescope (WFIRST) mission[1] is the top-ranked large space mission in the New Worlds, New Horizon (NWNH) Decadal Survey of Astronomy and Astrophysics. WFIRST will settle essential questions in both exoplanet and dark energy research and will advance topics ranging from galaxy evolution to the study of objects within the galaxy. The WFIRST mission uses a repurposed 2.4-m Forward Optical Telescope assembly (FOA), which, when completed with new aft optics will be an Integrated Optical Assembly (IOA). WFIRST is equipped with a Wide Field Instrument (WFI) and a Coronagraph Instrument (CGI). An Instrument Carrier (IC) meters these payload elements together and to the spacecraft bus (S/C). A distributed ground system receives the data, uploads commands and software updates, and processes the data. After transition from the study phase, Pre-Phase-A (a.k.a., “Cycle 6”) design to NASA Phase A formulation, a significant change to the IOA was initiated; including moving the tertiary mirror from the instrument package to a unified three-mirror anastigmat (TMA) placement, that provides a wide 0.28-sq° instrumented field of view to the Wide Field Instrument (WFI). In addition, separate relays from the primary and secondary mirror feed the Wide Field Instrument (WFI) and Coronagraph Instrument (CGI). During commissioning the telescope is aligned using wavefront sensing with the WFI[2]. A parametric and Monte-Carlo analysis was performed, which determined that alignment compensation with the secondary mirror alone degraded performance in the other instruments. This led to the addition of a second compensator in the WFI optical train to alleviate this concern. This paper discusses the trades and analyses that were performed and resulting changes to the WFIRST telescope architecture.
Conference Presentation
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
John Hagopian, John Hagopian, Nerses Armani, Nerses Armani, Lisa Bartusek, Lisa Bartusek, Tom Casey, Tom Casey, Dave Content, Dave Content, Yves Conturie, Yves Conturie, Guangjun Gao, Guangjun Gao, Alden Jurling, Alden Jurling, Cathy Marx, Cathy Marx, Joe Marzouk, Joe Marzouk, Bert Pasquale, Bert Pasquale, J. Scott Smith, J. Scott Smith, Hong Tang, Hong Tang, Arthur Whipple, Arthur Whipple, } "Ground to on-orbit alignment study of the WFIRST wide-field channel and resulting changes in the telescope architecture", Proc. SPIE 10377, Optical System Alignment, Tolerancing, and Verification XI, 103770E (22 August 2017); doi: 10.1117/12.2280333; https://doi.org/10.1117/12.2280333


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