Paper
26 August 2005 Optical design of the Terrestrial Planet Finder Coronagraph starlight suppression system
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Abstract
A baseline design for NASA's Terrestrial Planet Finder Coronagraph (TPFC) starlight suppression system (SSS) is described. The design is based on a 8x3.5m elliptical aperture telescope leading to terrestrial planet detection at a minimum angle of ~4λ/D. The design accommodates classical Lyot coronagraph as well as shaped pupil approaches and includes separate optical paths for two polarizations each with its own deformable mirror control. Critical design challenges and trades are described.
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Pantazis Mouroulis and Stuart B. Shaklan "Optical design of the Terrestrial Planet Finder Coronagraph starlight suppression system", Proc. SPIE 5874, Current Developments in Lens Design and Optical Engineering VI, 58740J (26 August 2005); https://doi.org/10.1117/12.613794
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CITATIONS
Cited by 4 scholarly publications.
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KEYWORDS
Coronagraphy

Beam splitters

Telescopes

Mirrors

Polarization

Planets

Wavefronts

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