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spelling todo:paper_0277786X_v7102_n_p_Hild2023-10-03T15:16:39Z Test images of a sector star versus radial and axial merit functions Hild, R. Campos, J. Yzuel, M. Iemmi, C. Escalera, J.C. Diffractive optics Optical imaging theory Optical merit functions Optical system design Spatial light modulators Diffractive optics Digital image storage Functions Imaging systems Light Light modulation Liquid membranes Modulation Modulators Optical filters Optical image storage Optical systems Optical transfer function Optoelectronic devices Phase shift Photolithography Probability density function Three dimensional Wave filters Axial points D lines Degree of coherences In dependences Merit functions Modulation Transfer functions Optical imaging systems Optical imaging theory Optical merit functions Optical system design Optimum filters Phase only filters Phase shifting Phase variations Spatial light modulators Spread functions Test images Light modulators The radial and axial point spread function (PSF) and the 3D modulation transfer function (MTF) were calculated to demonstrate the influence of phase only filters in classical optical imaging systems. The 3D line spread function (LSF) makes it possible to discuss the influence of the degree of coherence in the optical imaging system with the phase only filter as well. First, the phase only filter under discussion was divided in five equally area annuli. The phase variations are either linearly increasing or decreasing with the annulus number or alternating between 0 and π. Second we have used a filter that consists on one phase annulus with a phase shift of π in different positions over the pupil. Numerical and experimental results are shown in this paper. A spatial light modulator (SLM) was used to obtain experimentally the influence of the different phase only filters on the image of a sector star. The merit functions for filters with a phase shift of π in one annulus are also studied. These filters produce a wide variety of responses in dependence of the position of the phase shifting annulus. By studying the merit functions, a clear prediction of the imaging behaviour of an optical system is possible as well. The conclusion of our work has been that it is necessary to study the influence of the filter on the different merit functions in order to design an optimum filter for a given application. © 2008 SPIE. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0277786X_v7102_n_p_Hild
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Diffractive optics
Optical imaging theory
Optical merit functions
Optical system design
Spatial light modulators
Diffractive optics
Digital image storage
Functions
Imaging systems
Light
Light modulation
Liquid membranes
Modulation
Modulators
Optical filters
Optical image storage
Optical systems
Optical transfer function
Optoelectronic devices
Phase shift
Photolithography
Probability density function
Three dimensional
Wave filters
Axial points
D lines
Degree of coherences
In dependences
Merit functions
Modulation Transfer functions
Optical imaging systems
Optical imaging theory
Optical merit functions
Optical system design
Optimum filters
Phase only filters
Phase shifting
Phase variations
Spatial light modulators
Spread functions
Test images
Light modulators
spellingShingle Diffractive optics
Optical imaging theory
Optical merit functions
Optical system design
Spatial light modulators
Diffractive optics
Digital image storage
Functions
Imaging systems
Light
Light modulation
Liquid membranes
Modulation
Modulators
Optical filters
Optical image storage
Optical systems
Optical transfer function
Optoelectronic devices
Phase shift
Photolithography
Probability density function
Three dimensional
Wave filters
Axial points
D lines
Degree of coherences
In dependences
Merit functions
Modulation Transfer functions
Optical imaging systems
Optical imaging theory
Optical merit functions
Optical system design
Optimum filters
Phase only filters
Phase shifting
Phase variations
Spatial light modulators
Spread functions
Test images
Light modulators
Hild, R.
Campos, J.
Yzuel, M.
Iemmi, C.
Escalera, J.C.
Test images of a sector star versus radial and axial merit functions
topic_facet Diffractive optics
Optical imaging theory
Optical merit functions
Optical system design
Spatial light modulators
Diffractive optics
Digital image storage
Functions
Imaging systems
Light
Light modulation
Liquid membranes
Modulation
Modulators
Optical filters
Optical image storage
Optical systems
Optical transfer function
Optoelectronic devices
Phase shift
Photolithography
Probability density function
Three dimensional
Wave filters
Axial points
D lines
Degree of coherences
In dependences
Merit functions
Modulation Transfer functions
Optical imaging systems
Optical imaging theory
Optical merit functions
Optical system design
Optimum filters
Phase only filters
Phase shifting
Phase variations
Spatial light modulators
Spread functions
Test images
Light modulators
description The radial and axial point spread function (PSF) and the 3D modulation transfer function (MTF) were calculated to demonstrate the influence of phase only filters in classical optical imaging systems. The 3D line spread function (LSF) makes it possible to discuss the influence of the degree of coherence in the optical imaging system with the phase only filter as well. First, the phase only filter under discussion was divided in five equally area annuli. The phase variations are either linearly increasing or decreasing with the annulus number or alternating between 0 and π. Second we have used a filter that consists on one phase annulus with a phase shift of π in different positions over the pupil. Numerical and experimental results are shown in this paper. A spatial light modulator (SLM) was used to obtain experimentally the influence of the different phase only filters on the image of a sector star. The merit functions for filters with a phase shift of π in one annulus are also studied. These filters produce a wide variety of responses in dependence of the position of the phase shifting annulus. By studying the merit functions, a clear prediction of the imaging behaviour of an optical system is possible as well. The conclusion of our work has been that it is necessary to study the influence of the filter on the different merit functions in order to design an optimum filter for a given application. © 2008 SPIE.
format CONF
author Hild, R.
Campos, J.
Yzuel, M.
Iemmi, C.
Escalera, J.C.
author_facet Hild, R.
Campos, J.
Yzuel, M.
Iemmi, C.
Escalera, J.C.
author_sort Hild, R.
title Test images of a sector star versus radial and axial merit functions
title_short Test images of a sector star versus radial and axial merit functions
title_full Test images of a sector star versus radial and axial merit functions
title_fullStr Test images of a sector star versus radial and axial merit functions
title_full_unstemmed Test images of a sector star versus radial and axial merit functions
title_sort test images of a sector star versus radial and axial merit functions
url http://hdl.handle.net/20.500.12110/paper_0277786X_v7102_n_p_Hild
work_keys_str_mv AT hildr testimagesofasectorstarversusradialandaxialmeritfunctions
AT camposj testimagesofasectorstarversusradialandaxialmeritfunctions
AT yzuelm testimagesofasectorstarversusradialandaxialmeritfunctions
AT iemmic testimagesofasectorstarversusradialandaxialmeritfunctions
AT escalerajc testimagesofasectorstarversusradialandaxialmeritfunctions
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