Search results for "Low frequency"

showing 10 items of 97 documents

Laser Speckle Size And Temporal Transfer Function In Human Vision

1988

Using a blue laser stimulus we measured TMTF with speckle sizes of 19.1 µm, 3.3 µm and absence of speckle. Our results indicate, if we compare the TMTF curves obtained for different speckle sizes, a gain of modulation due fundamentally to the presence of the spec kle; in the low frequency region this gain of modulation can be explained in terms of inhibitory effects. On the other hand, we observe by using the diffusion-inhibition model, that the presence of speckle in the test-field produces a delay of 12 ms and a reduction of the height of the response, with respect to that obtained in the uniform test (with absence of speckle).

PhysicsBlue laserSpeckle patternOpticsbusiness.industryLow frequencybusinessTransfer functionSPIE Proceedings
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Study of the Temporal Behavior of 4U 1728−34 as a Function of Its Position in the Color‐Color Diagram

2001

We study the timing properties of the bursting atoll source 4U 1728-34 as a function of its position in the X-ray color-color diagram. In the island part of the color-color diagram (corresponding to the hardest energy spectra), the power spectrum of 4U 1728-34 shows several features such as a band-limited noise component present up to a few tens of Hz, a low-frequency quasi-periodic oscillation (LFQPO) at frequencies between 20 and 40 Hz, a peaked noise component around 100 Hz, and one or two QPOs at kHz frequencies. In addition to these, in the lower banana (corresponding to softer energy spectra) we also find a very low frequency noise (VLFN) component below ∼1 Hz. In the upper banana (co…

PhysicsCiencias AstronómicasOscillationAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)DiagramFOS: Physical sciencesSpectral densityX-rays: starsneutron [Stars]Astronomy and AstrophysicsColor–color diagramAstrophysicsAccretion accretion disksLow frequencyAstrophysicsStars: neutronSpectral lineSpace and Planetary ScienceStars: individual (4U 1728-34)Very low frequencyindividual (4U 1728-34) [Stars]Noise (radio)stars [X-rays]The Astrophysical Journal
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Microwave induced co-tunneling in single electron tunneling transistors

2002

Abstract The influence of microwaves on the co-tunneling in single electron tunneling transistors has been investigated as function of frequency and power in the temperature range from 150 to 500 mK. All 20 low frequency connections and the RF line were filtered, and the whole cryostat was suspended on rubber bellows. Cross-talk was minimized by using individual coaxial lines between the sample and the room temperature electronics. The co-tunneling experiments were performed at zero DC bias current by measuring the voltage response to a very small amplitude 2 Hz current modulation with the gate voltage fixed at maximum Coulomb blockade. With the microwave signal applied to one side of the t…

PhysicsCryostatCondensed matter physicsbusiness.industryTransistorEnergy Engineering and Power TechnologyCoulomb blockadeLow frequencyCondensed Matter::Mesoscopic Systems and Quantum Hall EffectCondensed Matter PhysicsElectronic Optical and Magnetic Materialslaw.inventionlawModulationOptoelectronicsElectrical and Electronic EngineeringbusinessQuantum tunnellingMicrowaveDC biasPhysica C: Superconductivity
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The nature of the extreme X-ray variability in the NLS1 1H 0707-495

2021

We examine archival XMM-Newton data on the extremely variable narrow-line Seyfert 1 (NLS1) active galactic nucleus (AGN) 1H 0707-495. We construct fractional excess variance (Fvar) spectra for each epoch, including the recent 2019 observation taken simultaneously with eROSITA. We explore both intrinsic and environmental absorption origins for the variability in different epochs, and examine the effect of the photoionised emission lines from outflowing gas. In particular, we show that the unusual soft variability first detected by eROSITA in 2019 is due to a combination of an obscuration event and strong suppression of the variance at 1 keV by photoionised emission, which makes the variance …

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Active galactic nucleusAccretion (meteorology)Astrophysics::High Energy Astrophysical PhenomenaX-rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLow frequencySpectral lineAmplitudeSpace and Planetary ScienceEmission spectrumAbsorption (electromagnetic radiation)Astrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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A finite difference time domain model for the Titan ionosphere Schumann resonances

2007

[1] This paper presents a numerical approach to model the electrical properties of Titan's atmosphere. The finite difference time domain technique is applied to model the atmosphere of Saturn's satellite in order to determine Schumann resonant frequencies and electromagnetic field distributions at the extremely low frequency range. Spherical coordinates are employed, and periodic boundary conditions are implemented in order to exploit the symmetry in rotation of the celestial body. Results are compared with a previous model using the transmission line matrix method up to 180 km altitude. For the first time a numerical FDTD model up to 800 km altitude is carried out, and we report lower freq…

PhysicsMeteorologySchumann resonancesFinite-difference time-domain methodSpherical coordinate systemTransmission-line matrix methodCondensed Matter PhysicsComputational physicssymbols.namesakePhysics::Space PhysicssymbolsGeneral Earth and Planetary SciencesPeriodic boundary conditionsExtremely low frequencyAstrophysics::Earth and Planetary AstrophysicsElectrical and Electronic EngineeringIonosphereTitan (rocket family)Radio Science
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Wave Modulations in the Nonlinear Biinductance Transmission Line

2001

Adding dissipative elements to a discrete biinductance transmission line which admits both low frequency (LF) and high frequency (HF) modes, dynamics of a weakly nonlinear modulated wave is investi...

PhysicsNonlinear systemModulational instabilityCondensed matter physicsComputer simulationWave propagationTransmission lineQuantum electrodynamicsDissipative systemGinzburg landau equationGeneral Physics and AstronomyLow frequencyJournal of the Physical Society of Japan
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On the correlation between phase-locking modes and Vibrational Resonance in a neuronal model

2018

International audience; We numerically and experimentally investigate the underlying mechanism leading to multiple resonances in the FitzHugh-Nagumo model driven by a bichromatic excitation. Using a FitzHugh-Nagumo circuit, we first analyze the number of spikes triggered by the system in response to a single sinusoidal wave forcing. We build an encoding diagram where different phase-locking modes are identified according to the amplitude and frequency of the sinusoidal excitation. Next, we consider the bichromatic driving which consists in a low frequency sinusoidal wave perturbed by an additive high frequency signal. Beside the classical Vibrational Resonance phenomenon, we show in real ex…

PhysicsNumerical AnalysisQuantitative Biology::Neurons and CognitionApplied MathematicsPerturbation (astronomy)phase locking modesLow frequencyneural networks01 natural sciences010305 fluids & plasmasComputational physicsCorrelationNonlinear systemnonlinear dynamicsSine waveAmplitude[NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]Control theoryModeling and Simulation0103 physical sciencesVibrational resonance[ NLIN.NLIN-PS ] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]010306 general physicsvibrational resonanceExcitation
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Control of multiphoton radiative recombination through the action of two low-frequency fields

2004

Interference effects caused by the simultaneous action of a two low frequency fields with commensurate frequencies during laser assisted radiative recombination (LARR) are investigated theoretically. Varying the relative phase of the two fields the following LARR features may be controlled: a) location of the maxima in the total emitted power; b) enhancement of the total emitted power; c) polar shape of the differential emitted power; d) shape of the emitted power spectra.

PhysicsPhysics and Astronomy (miscellaneous)Low frequencyLaserInterference (wave propagation)Spectral linerecombinationlaw.inventionlaserlawPolarSpontaneous emissionAtomic physicsMaximaInstrumentationcontrolRecombination
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<title>Low-frequency excitation of double quantum dots</title>

2008

We address theoretically adiabatic regime of charge transport for a model of two tunnel-coupled quantum dots connected in series. The energy levels of the two dots are harmonically modulated by an external potential with a constant phase shift between the two. Motivated by recent experiments with surface-acoustic-wave excitation, we consider two situations: (a) pure pumping in the absence of external voltage (also at finite temperature), and (b) adiabatic modulation of the current driven by large external bias. In both cases we derive results consistent with published experimental data. For the case (b) we explicitly derive the adiabatic limit of Tien-Gordon formula for photon-assisted tunn…

PhysicsQuantum dotQuantum mechanicsConductanceLow frequencyDouble quantumAdiabatic processExcitationQuantum tunnellingVoltageSPIE Proceedings
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Extremely low frequency band station for natural electromagnetic noise measurement

2015

A new permanent ELF measurement station has been deployed in Sierra Nevada, Spain. It is composed of two magnetometers, oriented NS and EW, respectively. At 10 Hz, their sensitivity is 19 μV/pT and the signal-to-noise ratio (SNR) is 28 dB for a time-varying signal of 1 pT, the expected field amplitude in Sierra Nevada. The station operates for frequencies below 24 Hz. The magnetometers, together with their corresponding electronics, have been specifically designed to achieve such an SNR for small signals. They are based on high-resolution search coils with ferromagnetic core and 106 turns, operating in limited geometry configuration. Different system noise sources are considered, and a stud…

PhysicsSchumann resonancesMagnetometerbusiness.industryCondensed Matter PhysicsSignallaw.inventionOpticsAmplitudelawGeneral Earth and Planetary SciencesSpectrogramExtremely low frequencyElectrical and Electronic EngineeringbusinessSensitivity (electronics)Noise (radio)Radio Science
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