Search results for "Aperture"

showing 10 items of 182 documents

In-situ diagnostic of ultrashort probes based on Kerr-index transient Bragg grating

2019

Pump-probe experiments are essential tools to investigate ultrafast dynamics of laser-matter interaction. We are particularly interested in the dynamics of transparent dielectrics under high numerical aperture focusing. Two main challenges arise for the weak probe pulse. First, we need a precise knowledge of the probe delay with respect to the pump pulse. Second, dispersion compensation of the ultrashort probe pulse generally requires a prism compressor, which can generate angular dispersion, and therefore incorrect interpretation of the pump­probe measurements.

Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryPhysics::Optics02 engineering and technologyDielectric021001 nanoscience & nanotechnology01 natural sciencesPrism compressorAngular dispersionPulse (physics)010309 opticsOpticsFiber Bragg grating0103 physical sciencesTransient (oscillation)High numerical aperture0210 nano-technologybusinessUltrashort pulseComputingMilieux_MISCELLANEOUS
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Resolution and field of view improvement in digital holography using a VCSEL source array

2011

We describe a new implementation capable to produce superresolution (SR) and object field of view (FOV) improvement in digital lensless Fourier holography. The method provides synthetic aperture (SA) generation using angular multiplexing incoming from a Vertical Cavity Surface Emitting Laser (VCSEL) source array. SR imaging in a single exposure is obtained after proper digital processing of a multiplexed hologram coming from the incoherent addition of multiple sub-holograms, each one corresponding with a different source of the VCSEL array. FOV improvement in addition with SR imaging is achieved by recording a set of individual holograms obtained by sequential activation of the VCSEL source…

Physicsbusiness.industryAperture synthesisHolographyField of viewHolographic interferometryMultiplexingVertical-cavity surface-emitting laserlaw.inventionOpticslawOptoelectronicsbusinessImage resolutionDigital holography2011 10th Euro-American Workshop on Information Optics
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Thin plastic shell x-ray optics: an update

2003

We present new results from a program to develop large area X-ray telescopes that are made from thin plastic shells. We use multi-shell cylindrical lenses in a point-to-point configuration to form full aperture images of the small focal spot in a an X-ray tube on a microchannel plate detector. The image data are analyzed to yield radial profiles and encircled energy curves. The derived parameters can be extrapolated to the case of a telescope that is a conical approximation to Wolter 1 optics. The plastic shells can be coated with suitable mono- or multilayers that allow for a wideband coverage of X-ray energies. Our current program is focused on the development of a large area, hard X-ray …

Physicsbusiness.industryApertureAstrophysics::High Energy Astrophysical PhenomenaPlastic shell X-ray opticAstrophysics::Instrumentation and Methods for AstrophysicsShell (structure)X-ray opticsX-ray telescopeConical surfaceCondensed Matter PhysicsEncircled energylaw.inventionTelescopePoint-to-point X-ray imagingOpticsApproximate X-ray opticlawMicrochannel plate detectorElectrical and Electronic EngineeringX-ray opticbusiness
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Single-step superresolution by interferometric imaging

2009

The use of vertical-cavity surface-emitting laser (VCSEL) arrays for implementation of incoherent source superresolution is presented. The method uses an interferometer setup to obtain superresolution in a single step. The novelty of the method relies on the use of a VCSEL array as the light source, which provides a set of coherent sources which are mutually incoherent. The technique accomplishes the transmission of several spatial frequency bands of the object's spectrum in parallel by use of spatial multiplexing that occurs because of the tilted illumination of the source array. The recording process is done by interference of each frequency band with a complementary set of reference plan…

Physicsbusiness.industryFrequency bandAperture synthesisHolographyPhysics::OpticsInterference (wave propagation)Atomic and Molecular Physics and Opticslaw.inventionVertical-cavity surface-emitting laserInterferometryOpticsModulationlawSpatial frequencybusinessOptics Express
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Chromatic compensation in the near-field region: shape and size tunability

2005

We report a diffractive-lens triplet with which to achieve wavelength compensation in the near field diffracted by any aperture. On the one hand, the all-diffractive triplet allows us to tune, in a sequential way, the Fresnel-irradiance shape to be achromatized by changing the focal length of one diffractive lens. On the other hand, we can adjust the scale of the chromatically compensated Fresnel diffraction field by shifting the aperture along the optical axis. Within this framework, we present an extremely flexible white-light Fresnel-plane array illuminator based on the kinoform sampling filter. A variable compression ratio and continuous selection of the output pitch are the most appeal…

Physicsbusiness.industryKinoformApertureMaterials Science (miscellaneous)Astrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsNear and far fieldDiffraction efficiencyIndustrial and Manufacturing EngineeringOptical axisOpticsFocal lengthChromatic scaleBusiness and International ManagementbusinessFresnel diffractionApplied Optics
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Transversal superresolution with noncontact axial movement of periodic structures

2007

We present an innovative approach that allows superresolved images to be obtained by axial moving of two gratings and time integrating in the detector plane. The two gratings do not have to be in contact with either the object or the detector, and both are positioned between the object and the image planes. One of the main applications for the proposed approach in contrast to previously discussed time multiplexing superresolving methods is that it may fit well to superresolved imaging of remote objects, since both gratings are not in contact with either the object or the detector planes.

Physicsmedicine.diagnostic_testPlane (geometry)business.industryAperture synthesismedia_common.quotation_subjectDetectorImage processingAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsOpticsOptical coherence tomographyOptical transfer functionmedicineContrast (vision)Computer Vision and Pattern RecognitionbusinessImage resolutionmedia_commonJournal of the Optical Society of America A
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Inverse photonic-crystal-fiber design through geometrical and material scalings

2020

Geometrical and material - i.e., external and internal - scaling symmetries are exploited to obtain approximated analytical expressions for the mode effective index, group index, and chromatic dispersion of a scaled fiber. Our results include material refractive index scaling that changes the numerical aperture. First, the analytical expressions are successfully tested with a conventional step index fiber in a broadband range of wavelengths, from 1 to 2 mu m. Then, we establish a procedure to adapt the analytical expressions to photonic crystal fibers (PCFs) and illustrate its application in a triangular PCF with circular holes. These adapted analytical expressions show good agreement with …

Physicsoptical fiberOptical fiberMathematical analysisUNESCO::FÍSICAPhysics::OpticsSoliton (optics)Atomic and Molecular Physics and Opticsdesigning toolsElectronic Optical and Magnetic MaterialsNumerical aperturelaw.inventionlaw:FÍSICA [UNESCO]Dispersion (optics)EFFECTIVE-INDEX METHOD; SUPERCONTINUUM GENERATION; CHROMATIC DISPERSION; SOLITON; OCTAVEElectrical and Electronic EngineeringStep-index profilephotonic crystal fiberRefractive indexScalingPhotonic-crystal fiber
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Development of a MeV ion beam lithography system in Jyväskylä

2007

A lithographic facility for writing patterns with ion beams from cyclotron beams is under development for the Jyväskylä cyclotron. Instead of focusing and deflecting the beam with electrostatic and magnetic fields a different approach is used. Here a small rectangular beam spot is defined by the shadow of a computer-controlled variable aperture in close proximity to the sample. This allows parallel exposure of rectangular pattern elements of 5–500 μm side with protons up to 6 MeV and heavy ions (20Ne, 85Kr) up to few 100 MeV. Here we present a short overview of the system under construction and development of the aperture design, which is a critical aspect for all ion beam lithography syste…

Physics::Plasma PhysicsPhysics::Accelerator Physicsproton beam writingcyclotronproximity apertureMeV ion beam lithography
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INTEGRAL/SPI ground calibration

2003

Three calibration campaigns of the spectrometer SPI have been performed before launch in order to determine the instrument characteristics, such as the effective detection area, the spectral resolution and the angular resolution. Absolute determination of the effective area has been obtained from simulations and measurements. At 1 MeV, the effective area is 65 cm^2 for a point source on the optical axis, the spectral resolution ~2.3 keV. The angular resolution is better than 2.5 deg and the source separation capability about 1 deg. Some temperature dependant parameters will require permanent in-flight calibration.

Point source[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesInstrumentation ; Detectors ; Spectrographs ; Space vehicles ; Gamma rays ; ObservationsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]OpticsSpectrographs0103 physical sciencesCalibrationSource separationAngular resolutionSpectral resolutionspace vehicles: instrumentsInstrumentation010303 astronomy & astrophysicsObservations:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]instrumentation: spectrographsPhysicsSpectrometer[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryinstrumentation: detectorsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaGamma raysAntenna apertureAstrophysics (astro-ph)DetectorsSpace vehiclesAstronomy and AstrophysicsOptical axisSpace and Planetary Sciencebusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]gamma rays: observations
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The INTEGRAL IBIS/ISGRI System Point Spread Function and Source Location Accuracy

2003

The imager on board INTEGRAL (IBIS) presently provides the most detailed sky images ever obtained at energies above 30 keV. The telescope is based on a coded aperture imaging system which allows to obtain sky images in a large field of view 29deg x 29deg with an angular resolution of 12'. The System Point Spread Function of the telescope and its detailed characteristics are here described along with the specific analysis algorithms used to derive the accurate point-like source locations. The derived location accuracy is studied using the first in-flight calibration data on strong sources for the IBIS/ISGRI system. The dependence of the calibrated location accuracy with the signal to noise r…

Point spread functionAstrophysics::High Energy Astrophysical PhenomenaData analysisFOS: Physical sciencesImage processingField of viewAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAlaw.inventionTelescopeHigh angular resolutionSignal-to-noise ratioImage processinglawData analysis ; Image processing ; High angular resolutionAngular resolutionCoded aperture:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]Remote sensingIbisPhysicsbiologyUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsbiology.organism_classificationSpace and Planetary Science:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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