2013
DOI: 10.1007/s12567-013-0041-x
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Large deployable telescopes—also for μm-wavelengths?

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(1 citation statement)
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“…This effectively ensures that the spot size at α -Centauri is 100 km in diameter. Modular parabolic shells of carbon-fibre reinforced flexible silicone of ~10–20 m diameter have been proposed for large-aperture astronomical reflectors (Baier et al ., 2013). Another option for a ~10–20 m diameter Fresnel module is the planar photon sieve comprising a flat membrane filled with ~10 7 concentrically distributed ~ μ -sized holes similar to a Fresnel zone plate in which the holes diffract light rather than grooves refracting light (Anderson, 2005).…”
Section: Beamed Propulsionmentioning
confidence: 99%
“…This effectively ensures that the spot size at α -Centauri is 100 km in diameter. Modular parabolic shells of carbon-fibre reinforced flexible silicone of ~10–20 m diameter have been proposed for large-aperture astronomical reflectors (Baier et al ., 2013). Another option for a ~10–20 m diameter Fresnel module is the planar photon sieve comprising a flat membrane filled with ~10 7 concentrically distributed ~ μ -sized holes similar to a Fresnel zone plate in which the holes diffract light rather than grooves refracting light (Anderson, 2005).…”
Section: Beamed Propulsionmentioning
confidence: 99%