Search results for "Oise"

showing 10 items of 1967 documents

Puhe pullataikinassa : toiminnallinen S2-opetus ja opettajuudet kotoutumista tukevassa ammatillisessa koulutuksessa

2017

Maisterintutkielmassani tarkastelen suomi toisena kielenä opetusta sitä urallaan ensi kertaa toteuttaneiden opettajien näkökulmasta. Opetus tapahtui ammattiopistossa kotoutumista tukevassa sekä opiskelu- ja työelämävalmiuksia lisäävässä koulutuksessa, joka oli suunnattu läheisessä vastaanottokeskuksessa asuneille aikuisille turvapaikanhakijoille. Kielenopetus järjestettiin pääasiassa integroituna ammatillisiin opintoihin ja sitä toteuttivat niin S2-opettaja kuin ammatinopettajatkin. Tutkimuksen tavoitteet ovat kuvata toiminnallista kielenopetusta ammatillisessa kontekstissa sekä tarkastella opettajien kielentämiä kokemuksia omassa ammatillisessa identiteetissään narratiivisten opettajuuksie…

narratiivinen analyysiintegroitu opetuskieltenopettajatammatillinen koulutusetnografiasuomi toisena kielenä opetusopettajuuskieletopetusmenetelmätsuomi toisena kielenäopetusturvapaikanhakijattoiminnalliset menetelmät
researchProduct

Halla-ahon ahdistus ja ironia : ulossulkeva suomalaisuus ja ahdas nationalismi Scripta-blogissa

2020

nationalismitunteetHalla-aho Jussiironiakansallinen identiteettiviholliskuvattoiseussuomalaisuusretoriikkablogitaffektitoikeistoliikkeetpopulismi
researchProduct

Ecological impacts of invasive signal crayfish in large boreal lakes

2012

native fishkalakannattulokaslajitmacroinvertebratestäplärapuparasitesselkärangattomatravinnonkäyttöinvasive speciesPacifastacus leniusculuspohjaeläimistöloisetmonimuotoisuushabitat connectivityvieraslajit
researchProduct

Noise effect in a FitzHugh-Nagumo circuit driven by a bichromatic signal

2013

We analyze the response of a nonlinear circuit exactly ruled by the FitzHugh-Nagumo equations. This circuit is submitted to a bichromatic signal including a high frequency and a low frequency. In absence of noise, we show that for an appropriate amplitude of the high frequency driving, the response of the circuit estimated at the low frequency can be optimized via the phenomenon of vibrational resonance. Next, we show that under certain conditions, noise can contribute to the effect of vibrational resonance. Colored noise is also considered. Our experimental results are confirmed by a numerical analysis.

neural networkStochastic resonance[PHYS.PHYS.PHYS-BIO-PH]Physics [physics]/Physics [physics]/Biological Physics [physics.bio-ph]Acoustics01 natural sciencesNoise (electronics)010305 fluids & plasmas[NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]Noise generator[ PHYS.PHYS.PHYS-BIO-PH ] Physics [physics]/Physics [physics]/Biological Physics [physics.bio-ph][NLIN.NLIN-PS] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]0103 physical sciencesPhase noise[ NLIN.NLIN-PS ] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.PHYS.PHYS-BIO-PH] Physics [physics]/Physics [physics]/Biological Physics [physics.bio-ph]Noise spectral densityQuantum noiseNoise floor[SPI.TRON] Engineering Sciences [physics]/Electronics[ SPI.TRON ] Engineering Sciences [physics]/Electronics[SPI.TRON]Engineering Sciences [physics]/ElectronicsBurst noiseQuantum electrodynamicsnonlinear circuitStochastic resonance2013 22nd International Conference on Noise and Fluctuations (ICNF)
researchProduct

Increasing the Astrophysical Reach of the Advanced Virgo Detector via the Application of Squeezed Vacuum States of Light

2019

Current interferometric gravitational-wave detectors are limited by quantum noise over a wide range of their measurement bandwidth. One method to overcome the quantum limit is the injection of squeezed vacuum states of light into the interferometer's dark port. Here, we report on the successful application of this quantum technology to improve the shot noise limited sensitivity of the Advanced Virgo gravitational-wave detector. A sensitivity enhancement of up to 3.2±0.1 dB beyond the shot noise limit is achieved. This nonclassical improvement corresponds to a 5%-8% increase of the binary neutron star horizon. The squeezing injection was fully automated and over the first 5 months of the thi…

neutron star: binaryGravitational waves detectionGeneral Physics and Astronomy01 natural sciencesvacuum stateNOISEinterferometric detectorLIGOnoise: quantumgravitational waves; squeezing; vacuumSettore FIS/01PhysicsQuantum opticsPhysicsQuantum limitQuantum noiseDetectorPhysical Sciencesgravitational waves squeezed lightinterferometric detectorsGravitational waveSqueezed coherent statePhysics Multidisciplinarysqueezed stateGravitation and AstrophysicshorizonGravitational wavesGeneral Relativity and Quantum CosmologyOpticsSettore FIS/05 - Astronomia e Astrofisica0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]SDG 7 - Affordable and Clean Energy010306 general physicsenhancementAstrophysiqueScience & Technology/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energybusiness.industryShot noisegravitational radiationgravitational waves thermal noisesensitivityLIGOdetector: sensitivityQuantum technology* Automatic Keywords *VIRGOinjectionPhysics and Astronomygravitational radiation detector: interferometerGravitational waves; interferometric detectors; noiseWAVEbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]gravitational waves nonlinear optics quantum opticsPhysical Review Letters
researchProduct

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
researchProduct

Hulluksi nimetty Huttunen : kulttuurintutkimuksen näkökulmia hulluksinimeämiseen Arto Paasilinnan Ulvovassa myllärissä

2017

Tutkielma tarkastelee hulluuden nimeämistä ja nimeämisen syitä Arto Paasilinnan Ulvova mylläri -romaanin (1981) kuvaamassa maailmassa. Teoreettiselta viitekehykseltään ja menetelmiltään tutkielma on yhteiskunnallisesti ja monitieteisesti orientoitunutta kulttuurintutkimusta ja kulttuurista mielenterveystutkimusta. Keskeisimmät tutkimukselliset virikkeet ovat Stuart Hallin analyyseistä, jotka kiinnittävät huomiota erilaisuuksiin, eroihin ja toiseuksiin sekä niiden kulttuuris-yhteiskunnalliseen rakentumiseen. Keskiössä on myös Hallin ja Michel Foucault'n kautta määrittyvä näkemys vallan produktiivisesta ja kehämäisestä luonteesta. Tutkielma on artikkelimuotoinen ja koostuu johdanto- ja yhteen…

nimittelymielenterveyspoikkeavuusmielenterveyshäiriötvallankäyttöhulluuskirjallisuudentutkimuskaunokirjallisuustoiseusTapaustutkimusstereotypiatsosioekonomiset tekijätPaasilinna Arto
researchProduct

Noise Reduction and Gap Filling of fAPAR Time Series Using an Adapted Local Regression Filter

2014

Time series of remotely sensed data are an important source of information for understanding land cover dynamics. In particular, the fraction of absorbed photosynthetic active radiation (fAPAR) is a key variable in the assessment of vegetation primary production over time. However, the fAPAR series derived from polar orbit satellites are not continuous and consistent in space and time. Filtering methods are thus required to fill in gaps and produce high-quality time series. This study proposes an adapted (iteratively reweighted) local regression filter (LOESS) and performs a benchmarking intercomparison with four popular and generally applicable smoothing methods: Double Logistic (DLOG), sm…

noise010504 meteorology & atmospheric sciencesRemote sensing applicationComputer scienceNoise reduction0211 other engineering and technologies02 engineering and technologyLand cover01 natural sciencesfAPAR; noise; MODIS; time series; filtering; interpolation; LOESSSmoothing splineLoessLOESSlcsh:Science021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingLocal regressionFilter (signal processing)Vegetation15. Life on landfilteringSnowinterpolationNoiseMODISfAPARGeneral Earth and Planetary Scienceslcsh:Qtime seriesSmoothingInterpolationRemote Sensing
researchProduct

Noise effect in a sine-Gordon Lattice

2013

International audience; This paper is devoted to the influence of internal noise in a sine-Gordon chain exhibiting the well known nonlinear supratransmission phenomenon. It is shown that spatiotemporal noise can trigger breather modes with a given probability in a range of parameters where they do not occur without noise. A frequency analysis is carried out to quantify the degree of coherence of the emitted breather. It is shown that there exists an appropriate amount of noise which ensures the existence of breather modes with the best coherence.

noiseBreather[PHYS.PHYS.PHYS-BIO-PH]Physics [physics]/Physics [physics]/Biological Physics [physics.bio-ph]Degree of coherence01 natural sciences010305 fluids & plasmaslaw.invention[NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]law[ PHYS.PHYS.PHYS-BIO-PH ] Physics [physics]/Physics [physics]/Biological Physics [physics.bio-ph]Quantum mechanicsLattice (order)0103 physical sciencesPhase noise[NLIN.NLIN-PS] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS][ NLIN.NLIN-PS ] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]Statistical physics010306 general physicsNonlinear Sciences::Pattern Formation and SolitonsBreatherPhysicsFrequency analysis[PHYS.PHYS.PHYS-BIO-PH] Physics [physics]/Physics [physics]/Biological Physics [physics.bio-ph]Quantum noiseShot noisecoherence resonance[SPI.TRON] Engineering Sciences [physics]/Electronics[SPI.TRON]Engineering Sciences [physics]/Electronics[ SPI.TRON ] Engineering Sciences [physics]/ElectronicsNonlinear systemStochastic resonance
researchProduct

Thermal noise limit for ultra-high vacuum noncontact atomic force microscopy

2013

The noise of the frequency-shift signal Δf in noncontact atomic force microscopy (NC-AFM) consists of cantilever thermal noise, tip–surface-interaction noise and instrumental noise from the detection and signal processing systems. We investigate how the displacement-noise spectral density dz at the input of the frequency demodulator propagates to the frequency-shift-noise spectral density dΔf at the demodulator output in dependence of cantilever properties and settings of the signal processing electronics in the limit of a negligible tip–surface interaction and a measurement under ultrahigh-vacuum conditions. For a quantification of the noise figures, we calibrate the cantilever displacemen…

noiseCantilevernoncontact atomic force microscopyGeneral Physics and AstronomyNanotechnologyCantileverlcsh:Chemical technologyNoise (electronics)lcsh:Technology530Full Research PaperOpticsPhase noiseNanotechnologyGeneral Materials ScienceDetection theorylcsh:TP1-1185Electrical and Electronic Engineeringlcsh:SciencePhysicsNoise temperaturefilterbusiness.industrylcsh:TNoise spectral densityBandwidth (signal processing)Spectral density(NC-AFM)noncontact atomic force microscopy (NC-AFM)lcsh:QC1-999Nanosciencelcsh:Qfeedback loopbusinesslcsh:Physics
researchProduct