Search results for "Amplitude"

showing 10 items of 1169 documents

Numerical Simulations of the Thermal Instability Collapse in Radiation Pressure Dominated Disks

2005

We show that accretion disks, both in the subcritical and supercritical accretion rate regime, may exhibit significant amplitude luminosity oscillations. The luminosity time behavior has been obtained by performing a set of time‐dependent 2D SPH simulations of accretion disks with different values of α and accretion rate. An explanation of this luminosity behavior is proposed in terms of limit‐cycle instability: the disk oscillates between a radiation pressure dominated configuration (with a high luminosity value) and a gas pressure dominated one (with a low luminosity value). The origin of this instability is the difference between the heat produced by viscosity and the energy emitted as r…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaQuasarAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRadiationInstabilityLuminosityViscosityAmplitudeRadiation pressureMagnetorotational instabilityAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy Astrophysics
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Local Finite-Amplitude Wave Activity as a Diagnostic for Rossby Wave Packets

2018

AbstractUpper-tropospheric Rossby wave packets (RWPs) are important dynamical features, because they are often associated with weather systems and sometimes act as precursors to high-impact weather. The present work introduces a novel diagnostic to identify RWPs and to quantify their amplitude. It is based on the local finite-amplitude wave activity (LWA) of Huang and Nakamura, which is generalized to the primitive equations in isentropic coordinates. The new diagnostic is applied to a specific episode containing large-amplitude RWPs and compared with a more traditional diagnostic based on the envelope of the meridional wind. In this case, LWA provides a more coherent picture of the RWPs an…

PhysicsAtmospheric Science010504 meteorology & atmospheric sciencesNetwork packetRossby waveBreaking waveMechanics01 natural sciencesFinite amplitude010305 fluids & plasmasWaveletPotential vorticity0103 physical sciences0105 earth and related environmental sciencesMonthly Weather Review
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A Budget Equation for the Amplitude of Rossby Wave Packets Based on Finite-Amplitude Local Wave Activity

2020

AbstractRecently, the authors proposed a novel diagnostic to quantify the amplitude of Rossby wave packets. This diagnostic extends the local finite-amplitude wave activity (LWA) of N. Nakamura and collaborators to the primitive-equations framework and combines it with a zonal filter to remove the phase dependence. In the present work, this diagnostic is used to investigate the dynamics of upper-tropospheric Rossby wave packets, with a particular focus on distinguishing between conservative dynamics and nonconservative processes. For this purpose, a budget equation for filtered LWA is derived and its utility is tested in a hierarchy of models. Idealized simulations with a barotropic and a d…

PhysicsAtmospheric ScienceAmplitudeNetwork packetPotential vorticityQuantum electrodynamicsRossby wavePhysics::Atmospheric and Oceanic PhysicsFinite amplitudeJournal of the Atmospheric Sciences
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Drop Shapes and Axis Ratio Distributions: Comparison between 2D Video Disdrometer and Wind-Tunnel Measurements

2009

Abstract Comparisons of drop shapes between measurements made using 2D video disdrometer (2DVD) and wind-tunnel experiments are presented. Comparisons are made in terms of the mean drop shapes and the axis ratio distributions. Very close agreement of the mean shapes is seen between the two sets of measurements; the same applies to the mean axis ratio versus drop diameter. Also, in both sets of measurements, an increase in the oscillation amplitudes with increasing drop diameter is observed. In the case of the 2DVD, a small increase in the skewness was also detected. Given that the two sets of measurements were conducted in very different conditions, the agreement between the two sets of dat…

PhysicsAtmospheric ScienceCloud microphysicsAmplitudeDisdrometerSkewnessOscillationDrop (liquid)Ocean EngineeringGeometrySurface layerWind tunnelRemote sensingJournal of Atmospheric and Oceanic Technology
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A fully manipulable damped driven harmonic oscillator using optical levitation

2020

We implement an experimental system based on optical levitation of a silicone oil droplet to demonstrate a damped driven harmonic oscillator. The apparatus allows us to control all the parameters present in the differential equation that theoretically describes such motion. The damping coefficient and driving force can be manipulated in situ by changing the pressure in the apparatus and by applying a variable electric field. We present two different experimental procedures. First, a transition from the overdamped to underdamped regimes is demonstrated by gradually lowering the air pressure. The characteristic resonance associated with an underdamped driven harmonic oscillator is observed by…

PhysicsAtmospheric pressureOscillationDifferential equationOptical levitation05 social sciences050301 educationGeneral Physics and AstronomyResonanceMechanics01 natural sciencesAmplitudeElectric field0103 physical sciences010306 general physics0503 educationHarmonic oscillatorAmerican Journal of Physics
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The UWB-OFDM Channel Analysis in Frequency

2009

In this paper, the ultra-wideband channel with orthogonal frequency division multiplexing (UWB-OFDM) is analyzed in the frequency domain. For UWB-OFDM channels with log-normal fading in the time domain, we show that the amplitude of each subcarrier can be approximated by a Nakagami-m random variable, where the fading parameter, the mean power and the correlation coefficient are expressed in terms of the following parameters: time arrival of the clusters, inter-arrival time of rays inside clusters, and power decay constants of rays and clusters.

PhysicsAutomatización y sistemas de controlOrthogonal frequency-division multiplexingTecnologíaNakagami distributionTopologyBanda anchaAutomation Command and control systemSubcarrierComputer Science::OtherSystems engineeringComputer Science::PerformanceIntersymbol interferenceAmplitudeFrequency domainComunicación inalámbricaElectronic engineeringComputer Science::Networking and Internet ArchitectureSistemas de comunicación inalámbricaFadingTime domainIngeniería de sistemas y comunicacionesComputer Science::Information Theory
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Next-to-leading order Balitsky-Kovchegov equation beyond large Nc

2020

We calculate finite-Nc corrections to the next-to-leading order (NLO) Balitsky-Kovchegov (BK) equation. We find analytical expressions for the necessary correlators of six Wilson lines in terms of the two-point function using the Gaussian approximation. In a suitable basis, the problem reduces from the diagonalization of a six-by-six matrix to the diagonalization of a three-by-three matrix, which can easily be done analytically. We study numerically the effects of these finite-Nc corrections on the NLO BK equation. In general, we find that the finite-Nc corrections are smaller than the expected 1/Nc2∼10%. The corrections may be large for individual correlators, but have less of an influence…

PhysicsBasis (linear algebra)010308 nuclear & particles physicsFunction (mathematics)114 Physical sciences01 natural sciencesComputer Science::Digital LibrariesGaussian approximationMatrix (mathematics)DipoleAmplitude0103 physical sciencesOrder (group theory)Rapidity010306 general physicsMathematical physicsPhysical Review
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The B0.5IVe CoRoT target HD 49330. I. Photometric analysis from CoRoT data

2009

International audience; Context: Be stars undergo outbursts producing a circumstellar disk from the ejected material. The beating of non-radial pulsations has been put forward as a possible mechanism of ejection. Aims: We analyze the pulsational behavior of the early B0.5IVe star HD 49330 observed during the first CoRoT long run towards the Galactical anticenter (LRA1). This Be star is located close to the lower edge of the beta Cephei instability strip in the HR diagram and showed a 0.03 mag outburst during the CoRoT observations. It is thus an ideal case for testing the aforementioned hypothesis. Methods: We analyze the CoRoT light curve of HD 49330 using Fourier methods and non-linear le…

PhysicsBe starHertzsprung–Russell diagramAstrophysics::High Energy Astrophysical PhenomenaAstronomyAstronomy and AstrophysicsContext (language use)AstrophysicsLight curveStarssymbols.namesakeAmplitudeSpace and Planetary Science[SDU]Sciences of the Universe [physics]symbolsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsEmission spectrumInstability strip[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics::Galaxy Astrophysics
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Teleportation-induced correlated quantum channels.

2009

Quantum teleportation of a n-qubit state performed using as entangled resource a general bipartite state of 2n qubits instead of n Bell states is equivalent to a correlated Pauli channel. This provides a new characterization of such channels in terms of many-body correlation functions of the teleporting media. Our model is then generalized to the Continuous Variable case. We show that this new representation provides a relatively simple method for determining whether a correlated quantum channel is able to reliably convey quantum messages by studying the entanglement properties of the teleportation mediating system.

PhysicsBell stateQuantum PhysicsFOS: Physical sciencesGeneral Physics and AstronomyQuantum entanglementQuantum channelQuantum capacityQuantum Physics01 natural sciences010305 fluids & plasmasComputer Science::Emerging TechnologiesQuantum mechanicsQubit0103 physical sciencesquantum information theoryquantum channelsQuantum informationQuantum Physics (quant-ph)010306 general physicsAmplitude damping channelQuantum teleportationPhysical review letters
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Critical Dynamics in a Binary Fluid: Simulations and Finite-Size Scaling

2006

We report comprehensive simulations of the critical dynamics of a symmetric binary Lennard-Jones mixture near its consolute point. The self-diffusion coefficient exhibits no detectable anomaly. The data for the shear viscosity and the mutual-diffusion coefficient are fully consistent with the asymptotic power laws and amplitudes predicted by renormalization-group and mode-coupling theories {\it provided} finite-size effects and the background contribution to the relevant Onsager coefficient are suitably accounted for. This resolves a controversy raised by recent molecular simulations.

PhysicsBinary fluidStatistical Mechanics (cond-mat.stat-mech)Shear viscosityDynamics (mechanics)FOS: Physical sciencesGeneral Physics and AstronomyBinary numberAmplitudePoint (geometry)Statistical physicsAnomaly (physics)ScalingCondensed Matter - Statistical MechanicsPhysical Review Letters
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