Search results for "Point spread function"

showing 5 items of 75 documents

Evaluation of the performance of multifocal intraocular lenses image quality: analysis of the standard methods

2007

Purpose: To analyze the standard methods used to describe intraocular lenses (IOL) and to suggest some improvements to make them applicable for multifocal IOLs. Methods: The EN-ISO standards and the standards of the American National Standards Institute (ANSI) for the evaluation of the performance of IOLs are tested for multifocal IOLs. The MTF of the one refractive multifocal IOL and two hybrid refractive-diffractive multifocal IOLs is measured for both distance focus and near focus and using different pupil sizes. Results: The average modulation (AM) from 0 to 100 c/mm of multifocal IOLs (for the distance focus) is about 40-50% lower than the AM of monofocal IOLs, for all pupil sizes stud…

Point spread functionbusiness.industryPupil sizeMultifocal intraocular lensStandard methodsPupilOphthalmologyOpticsImage quality analysisIntraocular lensesOptometryMultifocal IOLsMedicinebusinessActa Ophthalmologica Scandinavica
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2021

Abstract We propose a signal deconvolution procedure for imaging spectrometer data, where a measured point spread function (PSF) is deconvolved itself before being used for deconvolution of the signal. We evaluate the effectiveness of our procedure for improvement of the spatio-spectral signal, as well as our target application, i.e. estimation of sun-induced fluorescence (SIF). Imaging spectrometers are well established instruments for remote sensing. When used for scientific purposes these instruments are usually calibrated on a regular basis. In our case the point spread function of the optics is measured in an elaborate procedure with a tunable monochromator point light source. PSFs are…

Point spread functionmedicine.medical_specialtyComputer scienceWiener filterAstrophysics::Instrumentation and Methods for AstrophysicsImaging spectrometerSoil ScienceHyperspectral imagingGeologyPeak signal-to-noise ratioSpectral imagingsymbols.namesakesymbolsmedicineDeconvolutionComputers in Earth SciencesImage sensorAlgorithmRemote sensingRemote Sensing of Environment
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Experimental validation of a customized phase mask designed to enable efficient computational optical sectioning microscopy through wavefront encodin…

2017

In this paper, wavefront-encoded (WFE) computational optical sectioning microscopy (COSM) using a fabricated square cubic (SQUBIC) phase mask, designed to render the system less sensitive to depth-induced aberration, is investigated. The WFE-COSM system is characterized by a point spread function (PSF) that does not vary as rapidly with imaging depth compared to the conventional system. Thus, in WFE-COSM, image restoration from large volumes can be achieved using computationally efficient space-invariant (SI) algorithms, thereby avoiding the use of depth-variant algorithms. The fabricated SQUBIC phase mask was first evaluated and found to have a 75% fidelity compared to the theoretical desi…

WavefrontPoint spread functionMicroscopeMaterials scienceOptical sectioningImage qualitybusiness.industryMaterials Science (miscellaneous)Experimental data02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesIndustrial and Manufacturing Engineeringlaw.invention010309 opticsOpticslaw0103 physical sciencesMicroscopyBusiness and International Management0210 nano-technologybusinessImage restorationApplied optics
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Development of Slewing Mirror Telescope Optical System for the UFFO-pathfinder

2013

The Slewing Mirror Telescope (SMT) is the UV/optical telescope of UFFO-pathfinder. The SMT optical system is a Ritchey-Chretien (RC) telescope of 100 mm diameter pointed by means of a gimbal-mounted flat mirror in front of the telescope. The RC telescope has a 17 × 17arcmin2 in Field of View and 4.3 arcsec resolution (full width half maximum of the point spread function) The beam-steering mirror enables the SMT to access a 35 × 35degree region and point and settle within 1 sec. All mirrors were fabricated to about 0.02 wavelengths RMS in wave front error (WFE) and 84.7% average reflectivity over 200 nm ~ 650 nm. The RC telescope was aligned to 0.05 wavelengths RMS in WFE (test wavelength 63…

WavefrontPoint spread functionPhysicsbusiness.industryGeneral EngineeringAstronomy and AstrophysicsField of viewAstrophysicsOptical telescopelaw.inventionTelescopeWavelengthFull width at half maximumOpticsPathfinderSpace and Planetary Sciencelawbusiness
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Interocular differences in visual quality due to ocular aberrations and scattering in a patient with post-traumatic anisocoria: A case report

2012

AbstractA 41-year-old patient with visual disturbances after an ocular trauma in right eye three years before was carefully analyzed and discussed. No corneal or intraocular sequelae were present. Only a significant anisocoria could be observed. Right eye (RE) achieved a best spectacle-corrected visual acuity (BSCVA) of 0.05 LogMAR with a refraction of +0.50 sphere and −1.25 cylinder. Left eye (LE) achieved a BSCVA of 0.0 LogMAR with a refraction of +0.75 sphere and −1.00 cylinder. In photopic conditions pupil diameter was 4.96mm for RE and 3.02mm for LE whereas in scotopic conditions, these values were 7.45mm and 6.71mm, respectively. More significant levels of higher-order corneal and ocu…

medicine.medical_specialtyVisual acuitygenetic structuresCase ReportPupilScatteringlcsh:OphthalmologyOphthalmologymedicinelcsh:QC350-467AberraciónScotopic visionPupilaAnisocoriabusiness.industryFunción de dispersión del puntoPupil sizePupilRefractionAnisocoriaPoint spread functioneye diseasesDispersiónlcsh:RE1-994Visual DisturbanceOptometrysense organsmedicine.symptombusinessAberrationlcsh:Optics. LightPhotopic visionOptometryJournal of Optometry
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