Search results for "signal processing"

showing 10 items of 2451 documents

Whole mirror duplication-random loss model and pattern avoiding permutations

2010

International audience; In this paper we study the problem of the whole mirror duplication-random loss model in terms of pattern avoiding permutations. We prove that the class of permutations obtained with this model after a given number p of duplications of the identity is the class of permutations avoiding the alternating permutations of length p2+1. We also compute the number of duplications necessary and sufficient to obtain any permutation of length n. We provide two efficient algorithms to reconstitute a possible scenario of whole mirror duplications from identity to any permutation of length n. One of them uses the well-known binary reflected Gray code (Gray, 1953). Other relative mo…

[INFO.INFO-CC]Computer Science [cs]/Computational Complexity [cs.CC]Class (set theory)0206 medical engineeringBinary number0102 computer and information sciences02 engineering and technology[ MATH.MATH-CO ] Mathematics [math]/Combinatorics [math.CO]01 natural sciencesIdentity (music)Combinatorial problemsTheoretical Computer ScienceGray codeCombinatoricsPermutation[ INFO.INFO-BI ] Computer Science [cs]/Bioinformatics [q-bio.QM]Gene duplicationRandom loss[MATH.MATH-CO]Mathematics [math]/Combinatorics [math.CO]Pattern avoiding permutationGenerating algorithmComputingMilieux_MISCELLANEOUSMathematicsDiscrete mathematicsWhole duplication-random loss modelMathematics::CombinatoricsGenomeParity of a permutationComputer Science Applications[MATH.MATH-CO] Mathematics [math]/Combinatorics [math.CO][ INFO.INFO-CC ] Computer Science [cs]/Computational Complexity [cs.CC]Binary reflected Gray code010201 computation theory & mathematicsSignal Processing[INFO.INFO-BI]Computer Science [cs]/Bioinformatics [q-bio.QM]020602 bioinformaticsAlgorithmsInformation Systems
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The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory

2011

We present a comprehensive study of the influence of the geomagnetic field on the energy estimation of extensive air showers with a zenith angle smaller than $60^\circ$, detected at the Pierre Auger Observatory. The geomagnetic field induces an azimuthal modulation of the estimated energy of cosmic rays up to the ~2% level at large zenith angles. We present a method to account for this modulation of the reconstructed energy. We analyse the effect of the modulation on large scale anisotropy searches in the arrival direction distributions of cosmic rays. At a given energy, the geomagnetic effect is shown to induce a pseudo-dipolar pattern at the percent level in the declination distribution t…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencescosmic ray experimentCosmic rayAstrophysicsultra high energy cosmic raysEXTENSIVE AIR-SHOWERS01 natural sciencesDeclinationultra high energy cosmic ray0103 physical sciencescosmic rays detectors; cosmic ray experiments; ultra high energy cosmic rayscosmic rays detectorAnisotropyInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsZenithParticle detectors.Pierre Auger ObservatoryPhysics010308 nuclear & particles physicsPhysicsOBSERVATÓRIOSAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AzimuthMODELEarth's magnetic fieldPhysics::Space PhysicsLarge detector systems for particle and astroparticle physicARRAYFísica nuclearcosmic rays detectorscosmic ray experimentsAstrophysics - Instrumentation and Methods for AstrophysicsEnergy (signal processing)Cherenkov detectorJournal of Cosmology and Astroparticle Physics
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Parabolic pulse generation through passive reshaping of gaussian pulses in a normally dispersive fiber

2007

We numerically and experimentally demonstrate that a Gaussian pulse can be reshaped into a pulse with a stable parabolic intensity profile during propagation in normally dispersive nonlinear fibers.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Materials scienceGaussianPhysics::Optics02 engineering and technology01 natural sciences010309 opticssymbols.namesake020210 optoelectronics & photonicsOpticsFiber Bragg grating0103 physical sciences0202 electrical engineering electronic engineering information engineeringFiberGaussian processComputer Science::DatabasesComputingMilieux_MISCELLANEOUS[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Pulse (signal processing)business.industrySecond-harmonic generationNonlinear opticsPulse shapingsymbolsbusiness
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All-Optical Measurement of Background, Amplitude and Timing Jitter for high speed pulse trains or prbs sequences using autocorrelation function

2006

We present a simple method for all-optical measurements of background, amplitude- and timing-jitter of ultra high speed pulse trains or prbs sequences using the jitter dependences of the intercorrelation-peak shape.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Optical fiber02 engineering and technology01 natural sciencesPseudorandom binary sequencelaw.invention010309 optics020210 optoelectronics & photonicsOpticsHardware_GENERALlawComputer Science::Multimedia0103 physical sciencesHardware_INTEGRATEDCIRCUITS0202 electrical engineering electronic engineering information engineeringComputingMilieux_MISCELLANEOUSJitterPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Pulse (signal processing)business.industryAutocorrelationComputer Science::PerformanceAmplitudePhysics::Accelerator PhysicsTrainbusinessDegradation (telecommunications)
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Nonlinear spectral compression in optical fiber: A new tool for processing degraded signals

2017

International audience; We propose two new applications of the spectral focusing by self-phase modulation that occurs in a nonlinear optical fiber. We numerically show the possibility of using nonlinear spectral compression to improve the optical signal to noise ratio and mitigate the amplitude jitter of the signal pulses. We also demonstrate experimentally that use of spectral focusing in a combination with an external sinusoidal phase modulation achieves efficient suppression of coherent spectral background.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Polarization-maintaining optical fiber02 engineering and technologyOptical modulation amplitudeOptical time-domain reflectometer01 natural sciencesSignallaw.invention010309 optics020210 optoelectronics & photonicsSignal-to-noise ratioOpticslawNonlinear fiber optics0103 physical sciences0202 electrical engineering electronic engineering information engineeringsignal processingJitterPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryspectral compressionbusinessPhase modulationOptical attenuator
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All-fibered high-quality 28-GHz to 112 GHz pulse sources based on nonlinear compression of optical temporal besselons

2021

The generation of high quality pulse trains at repetition rates of several tens of GHz remains a crucial step for optical telecommunications, optical sampling or component testing applications. Unfortunately, the current bandwidth limitations of optoelectronic devices do not allow the direct generation of well-defined optical pulse trains with low duty cycles. An attractive solution is based on a direct temporal phase modulation that is then converted into an intensity modulation thanks to a dispersive element that imprints a spectral quadratic phase. Picosecond pulses at repetition rates of several tens of GHz have been successfully demonstrated [1] . However, this approach suffers from a …

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Materials scienceExtinction ratiobusiness.industryBandwidth (signal processing)Nonlinear opticsPulse (physics)Quality (physics)OpticsPicosecondbusinessIntensity modulationPhase modulationComputingMilieux_MISCELLANEOUS
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Pulse transition to similaritons in normally dispersive fibre amplifiers

2013

selected by the editors of Journal of Optics as a Highlight of 2013a video linked to the experiments can be seen at : http://youtu.be/thbXaW91D5g; International audience; A detailed experimental characterization of the transition process of an initially Gaussian pulse to the asymptotic self-similar parabolic solution in optical fibre amplifiers operating in the normal dispersion regime is performed.

[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Materials science[ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Pulse (signal processing)business.industryAmplifier02 engineering and technology01 natural sciencesComputer Science::Digital LibrariesAtomic and Molecular Physics and OpticsOptical fibre amplifiersElectronic Optical and Magnetic Materials010309 optics020210 optoelectronics & photonicsOptics0103 physical sciencesDispersion (optics)0202 electrical engineering electronic engineering information engineeringbusiness
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Observation of the suppression of the flux of cosmic rays above 4x10^19eV

2008

The energy spectrum of cosmic rays above 2.5 × 10¹⁸ eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index γ of the particle flux, J ∝ E-γ, at energies between 4 × 10¹⁸ eV and 4 × 10¹⁹ eV is 2.69 ± 0.02(stat) ± 0.06(syst), steepening to 4.2 ± 0.4(stat) ± 0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz'min.

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::High Energy Astrophysical Phenomenaenergy spectrumFOS: Physical sciencesGeneral Physics and AstronomyFluxOsservatorio Pierre Augerspectral indexCosmic rayparticle fluxAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEXTENSIVE AIR-SHOWERSAstrophysicsUPPER LIMIT01 natural sciencesPower lawAugerNuclear physicsENERGY[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmicicosmic rays0103 physical sciencesddc:550Particle flux010303 astronomy & astrophysicsCiencias ExactasPhysicsPierre Auger ObservatorySpectral indexSPECTRUM[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaARRAYHigh Energy Physics::ExperimentSciami atmosferici estesiEnergy (signal processing)
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Prise en compte de la technologie dans la quantification des biomarqueurs

2016

International audience; Part de la variance technologique dans la quantification des biomarqueurs. Exemple en protéomique avec la technologie MALDI-TOF

[SDV] Life Sciences [q-bio][SDV.BIO]Life Sciences [q-bio]/Biotechnology[SDV]Life Sciences [q-bio]bioinformatics spectrum analysis signal processing mass spectrometry MALDI[SDV.BIO] Life Sciences [q-bio]/Biotechnology
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Equivalence of Open-Loop and Closed-Loop Operation of SAW Resonators and Delay Lines

2019

International audience; Surface acoustic wave (SAW) sensors in the form of two-port resonators or delay lines are widely used in various fields of application. The readout of such sensors is achieved by electronic systems operating either in an open-loop or in a closed-loop configuration. The mode of operation of the sensor system is usually chosen based on requirements like, e.g., bandwidth, dynamic range, linearity, costs, and immunity against environmental influences. Because the limit of detection (LOD) at the output of a sensor system is often one of the most important figures of merit, both readout structures, i.e., open-loop and closed-loop systems, are analyzed in terms of the minim…

[SPI.OTHER]Engineering Sciences [physics]/OtherPhysics - Instrumentation and DetectorsComputer scienceddc:621.3ResonatorPhase NoiseFOS: Physical sciencesSAW sensorslcsh:Chemical technology01 natural sciencesBiochemistryArticleAnalytical Chemistryfrequency detectionResonator0103 physical sciencesPhase noiseElectronic engineeringreadout systemsFigure of meritddc:6lcsh:TP1-1185[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Electrical and Electronic EngineeringReadout Systems010301 acousticsInstrumentationDelay LineDynamic rangeFrequency Detection010401 analytical chemistryBandwidth (signal processing)Surface acoustic waveOpen-loop controllerarticlePhase DetectionLinearityInstrumentation and Detectors (physics.ins-det)Open-loop Vs. Closed-loopdelay lineAtomic and Molecular Physics and Opticsphase noise0104 chemical sciencesSaw Sensorsopen-loop vs. closed-loopresonatorPhase-sensitive Sensorsphase detectionphase-sensitive sensors
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