Open Access Presentation + Paper
6 July 2018 Diffraction analysis of large segmented mirror concepts for exoplanet exploration
Author Affiliations +
Abstract
Diffraction effects of large segmented mirror gaps and secondary mirror support struts produce diffraction peaks or flares that are a detriment to exoplanet detection. In this paper we present detailed parametric diffraction analyses of an innovative “Pinwheel Pupil” segmented mirror concept utilizing curved segment gaps and secondary support struts that can potentially eliminate these diffraction flares that can obscure a faint exoplanet image. The resulting numerical diffraction performance predictions are quantitatively compared to that of both ideal monolithic circular pupils and classical annular pupils with straight secondary mirror struts. We utilize performance – based merit functions consisting of both radial and azimuthal profiles of the resulting telescope point spread function.
Conference Presentation
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
James E. Harvey, Ryan G. Irvin, Karlton Crabtree, Richard N. Pfisterer, and James B. Breckinridge "Diffraction analysis of large segmented mirror concepts for exoplanet exploration", Proc. SPIE 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, 106981Q (6 July 2018); https://doi.org/10.1117/12.2313999
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Diffraction

Mirrors

Point spread functions

Segmented mirrors

Telescopes

Exoplanets

Space telescopes

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