Zernike-like systems in polygons and polygonal facets

Zernike polynomials are commonly used to represent the wavefront phase on circular optical apertures, since they form a complete and orthonormal basis on the unit disk. In [Diaz et all, 2014] we introduced a new Zernike basis for elliptic and annular optical apertures based on an appropriate diffeom...

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Autores: Ferreira González, Chelo, López García, José Luis, Navarro, Rafael, Pérez Sinusía, Ester
Tipo de recurso: artículo
Estado:Versión aceptada para publicación
Fecha de publicación:2015
País:España
Institución:Universidad San Jorge (USJ)
Repositorio:Academica-e. Repositorio Institucional de la Universidad Pública de Navarra
OAI Identifier:oai:academica-e.unavarra.es:2454/31769
Acceso en línea:https://hdl.handle.net/2454/31769
Access Level:acceso abierto
Palabra clave:Zernike polynomials
Orthonormal systems
Polygonal facets
Segmented mirror telescopes
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spelling Zernike-like systems in polygons and polygonal facetsFerreira González, CheloLópez García, José LuisNavarro, RafaelPérez Sinusía, EsterZernike polynomialsOrthonormal systemsPolygonal facetsSegmented mirror telescopesZernike polynomials are commonly used to represent the wavefront phase on circular optical apertures, since they form a complete and orthonormal basis on the unit disk. In [Diaz et all, 2014] we introduced a new Zernike basis for elliptic and annular optical apertures based on an appropriate diffeomorphism between the unit disk and the ellipse and the annulus. Here, we present a generalization of this Zernike basis for a variety of important optical apertures, paying special attention to polygons and the polygonal facets present in segmented mirror telescopes. On the contrary to ad hoc solutions, most of them based on the Gram-Smith orthonormalization method, here we consider a piece-wise diffeomorphism that transforms the unit disk into the polygon under consideration. We use this mapping to define a Zernike-like orthonormal system over the polygon. We also consider ensembles of polygonal facets that are essential in the design of segmented mirror telescopes. This generalization, based on in-plane warping of the basis functions, provides a unique solution, and what is more important, it guarantees a reasonable level of invariance of the mathematical properties and the physical meaning of the initial basis functions. Both, the general form and the explicit expressions for a typical example of telescope optical aperture are provided.This research was supported by the Spanish Ministry of Economía y Competitividad and the European Union, grant FIS2011-22496, and by the Government of Aragón, research group E99. The financial support of the State University of Navarra is also acknowledged.Optical Society of AmericaIngeniería Matemática e InformáticaMatematika eta Informatika IngeniaritzaUniversidad Pública de Navarra / Nafarroako Unibertsitate Publikoa2015info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionapplication/pdfhttps://hdl.handle.net/2454/31769reponame:Academica-e. Repositorio Institucional de la Universidad Pública de Navarrainstname:Universidad San Jorge (USJ)Inglésinfo:eu-repo/grantAgreement/MICINN//FIS2011-22496© 2015 Optical Society of America. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modifications of the content of this paper are prohibited.info:eu-repo/semantics/openAccessoai:academica-e.unavarra.es:2454/317692026-06-17T12:41:47Z
dc.title.none.fl_str_mv Zernike-like systems in polygons and polygonal facets
title Zernike-like systems in polygons and polygonal facets
spellingShingle Zernike-like systems in polygons and polygonal facets
Ferreira González, Chelo
Zernike polynomials
Orthonormal systems
Polygonal facets
Segmented mirror telescopes
title_short Zernike-like systems in polygons and polygonal facets
title_full Zernike-like systems in polygons and polygonal facets
title_fullStr Zernike-like systems in polygons and polygonal facets
title_full_unstemmed Zernike-like systems in polygons and polygonal facets
title_sort Zernike-like systems in polygons and polygonal facets
dc.creator.none.fl_str_mv Ferreira González, Chelo
López García, José Luis
Navarro, Rafael
Pérez Sinusía, Ester
author Ferreira González, Chelo
author_facet Ferreira González, Chelo
López García, José Luis
Navarro, Rafael
Pérez Sinusía, Ester
author_role author
author2 López García, José Luis
Navarro, Rafael
Pérez Sinusía, Ester
author2_role author
author
author
dc.contributor.none.fl_str_mv Ingeniería Matemática e Informática
Matematika eta Informatika Ingeniaritza
Universidad Pública de Navarra / Nafarroako Unibertsitate Publikoa
dc.subject.none.fl_str_mv Zernike polynomials
Orthonormal systems
Polygonal facets
Segmented mirror telescopes
topic Zernike polynomials
Orthonormal systems
Polygonal facets
Segmented mirror telescopes
description Zernike polynomials are commonly used to represent the wavefront phase on circular optical apertures, since they form a complete and orthonormal basis on the unit disk. In [Diaz et all, 2014] we introduced a new Zernike basis for elliptic and annular optical apertures based on an appropriate diffeomorphism between the unit disk and the ellipse and the annulus. Here, we present a generalization of this Zernike basis for a variety of important optical apertures, paying special attention to polygons and the polygonal facets present in segmented mirror telescopes. On the contrary to ad hoc solutions, most of them based on the Gram-Smith orthonormalization method, here we consider a piece-wise diffeomorphism that transforms the unit disk into the polygon under consideration. We use this mapping to define a Zernike-like orthonormal system over the polygon. We also consider ensembles of polygonal facets that are essential in the design of segmented mirror telescopes. This generalization, based on in-plane warping of the basis functions, provides a unique solution, and what is more important, it guarantees a reasonable level of invariance of the mathematical properties and the physical meaning of the initial basis functions. Both, the general form and the explicit expressions for a typical example of telescope optical aperture are provided.
publishDate 2015
dc.date.none.fl_str_mv 2015
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/acceptedVersion
format article
status_str acceptedVersion
dc.identifier.none.fl_str_mv https://hdl.handle.net/2454/31769
url https://hdl.handle.net/2454/31769
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv info:eu-repo/grantAgreement/MICINN//FIS2011-22496
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Optical Society of America
publisher.none.fl_str_mv Optical Society of America
dc.source.none.fl_str_mv reponame:Academica-e. Repositorio Institucional de la Universidad Pública de Navarra
instname:Universidad San Jorge (USJ)
instname_str Universidad San Jorge (USJ)
reponame_str Academica-e. Repositorio Institucional de la Universidad Pública de Navarra
collection Academica-e. Repositorio Institucional de la Universidad Pública de Navarra
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