Paper
16 July 2018 WFIRST coronagraph: digging dark-holes with partially corrected pupil phase
Erkin Sidick, John Krist, Ilya Poberezhskiy
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Abstract
The WFIRST coronagraph employs two sequential deformable mirrors to compensate for phase and amplitude errors in the coronagraph optical system. In such a system the actuators of the deformable mirrors would be used for two purposes: To flatten the overall wavefront errors at a system pupil, and to create "dark-holes". The actuators have limited stroke ranges. Therefore, if the pupil phase errors are relatively large, flattening them completely could use up a significant portion of the actuator stroke, sometimes leaving insufficient stroke for creating the dark-holes. We have investigated the impact of partially-corrected pupil phase errors on a Hybrid Lyot Coronagraph (HLC) broadband contrast performance. The predicted broadband contrast floor agrees well with those measured on the HLC testbed.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Erkin Sidick, John Krist, and Ilya Poberezhskiy "WFIRST coronagraph: digging dark-holes with partially corrected pupil phase", Proc. SPIE 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, 106986W (16 July 2018); https://doi.org/10.1117/12.2313520
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CITATIONS
Cited by 1 scholarly publication.
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KEYWORDS
Coronagraphy

Actuators

Deformable mirrors

Exoplanets

Performance modeling

Space telescopes

Stars

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