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Proceedings Paper

Wavefront coding applied to a two-mirror telescope
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Paper Abstract

A wave-front coded imaging system is an optical-digital method for aberration control. Wave-front coding technology incorporates an aspheric element in the optical system in order to capture a coded image and by digital processing decode it to obtain the final image. The WFC system is very insensitive to defocus-like aberrations and thereby becomes a tool in the aberration balancing for telescope systems. We propose WFC technology to be implemented in a two spherical mirror telescope. In this work we present the design and simulation of the proposed telescope, trade-offs encountered in the design process and aspects of the image restoration.

Paper Details

Date Published: 22 July 2014
PDF: 7 pages
Proc. SPIE 9145, Ground-based and Airborne Telescopes V, 91453N (22 July 2014); doi: 10.1117/12.2055355
Show Author Affiliations
Jose A. Araiza-Duran, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
Esteban Luna, Instituto de Astronomía, Univ. Nacional Autónoma de México (Mexico)
Alejandro Cornejo, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
Joel Herrera, Univ. Nacional Autónoma de México (Mexico)


Published in SPIE Proceedings Vol. 9145:
Ground-based and Airborne Telescopes V
Larry M. Stepp; Roberto Gilmozzi; Helen J. Hall, Editor(s)

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