Phased array optical telescope

Optical: systems and elements – Compound lens system – Telescope

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359618, G02B 2300, G02B 2302

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active

051132842

ABSTRACT:
A phased array telescope in which the output field angle of each afocal subtelescope is equal to the arcsin of the product of the magnification and the sine of the input field angle. The resultant subtelescope distortion reduces piston error at the input to the beam combining telescope to increase resolution by reducing piston error otherwise caused by distortion-free subtelescopes. The phased array telescope uses only reflecting surfaces in order to operate over a wide spectral band. Optically powered primary, secondary and tertiary reflecting surfaces are combined with an aspheric folding mirror before the image that would have been formed by the secondary mirror to control the distortion of each subtelescope to exactly follow the arcsin rule provided.

REFERENCES:
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patent: 4981354 (1991-01-01), DeHainaut et al.
Hege et al., "Multiple Mirror Telescope as a Phased Array Telescope", Applied Optics, 15 Aug. 1985, vol. 24, No. 16, pp. 2565-2576.
Stulinger, Tilman W., "All-Reflective Phased Array Telescopes", International Lens Design Conference, 11-14 Jun. 1990, Proc. SPIE, 1354, (pp. 438-446).
Traub, Wesley A., "Combining Beams from Separated Telescopes", Applied Optics, vol. 24, No. 4, Feb. 15, 1986 (pp. 528-531).
Beckers, Jacques M., "The VLT Interferometer, III. Factors Affecting Wide Filed-of -View Operations", Proc. SPIA, 1236, 1990 (11 pages).
Weaver et al., "Design Consideration for Multiple Telescope Imaging Arrays", submitted for publication in Optical Engineering, Sep. 1988, vol. 27, No. 9 (pp. 730-735).
Lampkin et al., "Optical and Mechanical Design Aspects of a Four-Telescope Array for Combined Imaging", submitted for publication in Optical Engineering, Sep. 1988, vol. 27, No. 9 (pp. 749-754).

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