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Proceedings Paper

Numerical design analysis techniques for phased-array wide field-of-view imaging
Author(s): Burton D. O'Neil; Carol E. Hines; Christopher R. DeHainaut
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Paper Abstract

The process of simulating the optical performance of the phased array optical telescope has given us new insight on the role of the array and subaperture chief rays, array aberrations (global) and subaperture (individual telescopes) aberrations. The seven 3rd order Siedel surface aberration paraxial equations are reformulated in terms of phased array and includes a numerical example. In addition, a design method of combining each telescope chief ray to determine the vertex of the reference sphere is described. A theoretical calculation of subaperture piston resulting from array (global) 3rd order aberrations with numerical examples is presented.

Paper Details

Date Published: 1 June 1992
PDF: 14 pages
Proc. SPIE 1625, Design, Modeling, and Control of Laser Beam Optics, (1 June 1992); doi: 10.1117/12.58945
Show Author Affiliations
Burton D. O'Neil, Logicon R&D Associates (United States)
Carol E. Hines, Logicon R&D Associates (United States)
Christopher R. DeHainaut, Phillips Lab. (United States)

Published in SPIE Proceedings Vol. 1625:
Design, Modeling, and Control of Laser Beam Optics
Youssef Kohanzadeh; George N. Lawrence; John G. McCoy; Hugo Weichel, Editor(s)

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