Search results for "MAGNITUDE"

showing 10 items of 501 documents

Fukushima, or the Black Swan of Nuclear Energy

2012

By its own merits, the great earthquake that hit Japan on 11 March 2011 would have qualified as one of the worse disasters of recent times. With a magnitude of 9.0 MW, it was the most powerful known earthquake ever to have hit Japan, and one of the most powerful in history. It released a surface energy 2 × 1017 Joule. Enough, if harnessed, to power a city the size of Los Angeles for an entire year.

Nuclear reactor coreNuclear engineeringEnvironmental scienceBoiling water reactorMagnitude (mathematics)JouleBlack swan theorySurface energyEnergy (signal processing)Power (physics)
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Individual Differences in Working Memory Capacity Are Unrelated to the Magnitude of Benefits from Object- and Dimension-Based Retro-Cues

2021

OphthalmologyDimension (vector space)Computer scienceWorking memorybusiness.industryMagnitude (mathematics)Computer visionArtificial intelligenceObject (computer science)businessSensory SystemsJournal of Vision
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Absolute frequency and isotope shift measurements of mercury 1S0–3P1 transition

2019

We report the measurement of the absolute frequencies of the 6s2 1S0−6s6p 3P1 transition (253.7 nm) and the relevant isotope shifts in five mercury isotopes  198Hg,  199Hg,  200Hg,  202Hg, and  204Hg. The Doppler-free saturated absorption measurements were performed in an atomic vapour cell at room temperature with a four-harmonic generated (FHG) continuous-wave (cw) laser digitally locked to the atomic transition. It was referenced with a femtosecond optical frequency comb synchronized to the frequency of local representation of the International Atomic Time to provide traceability to the SI second by the 330 km-long stabilized fibre optical link. The transition frequencies and isotope shi…

Optical fiberMaterials scienceIsotopeInternational Atomic Timebusiness.industryOptical linkchemistry.chemical_element02 engineering and technology021001 nanoscience & nanotechnologyLaser01 natural sciencesAtomic and Molecular Physics and Opticslaw.inventionMercury (element)010309 opticsOpticschemistrylaw0103 physical sciencesFemtosecondAtomic physics0210 nano-technologybusinessOrder of magnitudeOptics Express
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Improved orbital parameters of accreting millisecond pulsar SAX J1808.4-3658

2006

Abstract We analyze the three outbursts of the X-ray millisecond pulsar SAX J1808.4-3658 that occurred in 1998, 2000, and 2002 observed with RXTE. With a technique based on epoch folding search we find an unique orbital solution valid over the five years of high temporal resolution data available. We revise the estimate of the orbital period, P orb  = 7249.1569(1) s and of its error, which we decrease by one order of magnitude. We also give the first constraint on the orbital period derivative, - 6.6 × 10 - 12 P ˙ orb + 0.8 × 10 - 12 s s - 1 . We find that in 2002 the pulse profile shape is clearly asymmetric, showing a secondary peak at about 145° from the main pulse, which is different fr…

Orbital elementsPhysicsAtmospheric ScienceEpoch (astronomy)Aerospace EngineeringAstronomyAstronomy and AstrophysicsAstrophysicsOrbital periodPulse (physics)Orb (astrology)GeophysicsSpace and Planetary ScienceMillisecond pulsarGeneral Earth and Planetary SciencesHigh temporal resolutionOrder of magnitudeAdvances in Space Research
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Precise determination of orbital parameters in system with slowly drifting phases: application to the case of XTE J1807-294

2007

We describe a timing technique that allows to obtain precise orbital parameters of an accreting millisecond pulsar in those cases in which intrinsic variations of the phase delays (caused e.g. by proper variation of the spin frequency) with characteristic timescale longer than the orbital period do not allow to fit the orbital parameters over a long observation (tens of days). We show under which conditions this method can be applied and show the results obtained applying this method to the 2003 outburst observed by RXTE of the accreting millisecond pulsar XTE J1807-294 which shows in its phase delays a non-negligible erratic behavior. We refined the orbital parameters of XTE J1807-294 usin…

Orbital elementsPhysicspulsars : individualAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Phase (waves)pulsars : generalFOS: Physical sciencesstars : magnetic fieldAstronomy and AstrophysicsAstrophysicsOrbital periodAstrophysicsstars : neutronX-ray : binariesXTE J1807-294Space and Planetary ScienceMillisecond pulsarAstrophysics::Earth and Planetary AstrophysicsSpin (physics)Variation (astronomy)magnetic fields; stars : neutron; pulsars : general; pulsars : individual; XTE J1807-294; X-ray : binaries [stars]Order of magnitude
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Excitation of plasmonic nanoantennas by nonresonant and resonant electron tunnelling.

2016

A rigorous theory of photon emission accompanied inelastic tunnelling inside the gap of plasmonic nanoantennas has been developed. The disappointingly low efficiency of the electrical excitation of surface plasmon polaritons in these structures can be increased by orders of magnitude when a resonant tunnelling structure is incorporated inside the gap. Resonant tunnelling assisted surface plasmon emitter may become a key element in future electrically-driven nanoplasmonic circuits.

Orders of magnitude (temperature)FOS: Physical sciencesPhysics::Optics02 engineering and technologyElectron01 natural sciences0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Physics::Atomic and Molecular ClustersGeneral Materials Science010306 general physicsQuantum tunnellingPlasmonCommon emitterPhysicsCondensed Matter - Mesoscale and Nanoscale Physicsbusiness.industrySurface plasmon021001 nanoscience & nanotechnologySurface plasmon polariton3. Good healthOptoelectronics0210 nano-technologybusinessExcitationOptics (physics.optics)Physics - OpticsNanoscale
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Comparison of computational and experimental saturation vapor pressures of α-pinene + O<sub>3</sub> oxidation products

2021

Abstract. Accurate information on gas-to-particle partitioning is needed to model secondary organic aerosol formation. However, determining reliable saturation vapor pressures of atmospherically relevant multifunctional organic compounds is extremely difficult. We estimated saturation vapor pressures of α-pinene ozonolysis derived secondary organic aerosol constituents using FIGAERO-CIMS experiments and COSMO-RS theory. We found a good agreement between experimental and computational saturation vapor pressures for molecules with molar masses around 190 g mol−1 and higher, most within a factor of 3 comparing the average of the experimental vapor pressures and the COSMO-RS estimate of the iso…

OzonolysisMaterials scienceMolar mass010504 meteorology & atmospheric sciencesThermal decompositionAnalytical chemistryThermal desorptioncomplex mixtures01 natural sciencesAerosolOrders of magnitude (specific energy)13. Climate actionMoleculeSaturation (chemistry)0105 earth and related environmental sciences
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A test of electric charge conservation with Borexino

2015

Borexino is a liquid scintillation detector located deep underground at the Laboratori Nazionali del Gran Sasso (LNGS, Italy). Thanks to the unmatched radio-purity of the scintillator, and to the well understood detector response at low energy, a new limit on the stability of the electron for decay into a neutrino and a single mono-energetic photon was obtained. This new bound, tau > 6.6 10**28 yr at 90 % C.L., is two orders of magnitude better than the previous limit.

Particle physicsPhysics - Instrumentation and DetectorsOrders of magnitude (temperature)Physics::Instrumentation and DetectorsGeneral Physics and AstronomyFOS: Physical sciencesElectronScintillatorElectric chargeHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)ddc:550Nuclear ExperimentBorexinoComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]Liquid scintillation countingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)High Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Comparison of Procedures to estimate Steady Flow Rate in Field Measurement of Saturated Hydraulic Conductivity by the Guelph Permeameter Method

1999

Abstract Different procedures for estimating steady flow rate during field application of the Guelph permeameter method were compared in terms of field-saturated hydraulic conductivity K fs and equilibration time t s estimates. The steady flow rate was evaluated by the slope of the linear portion of the cumulative drop in water level in the permeameter reservoir versus time plot (reference procedure) and by approximate procedures that use the first three or four consecutive values of the rate of fall of the water level equal or differing by less than a given percentage. The influence of the selected time interval between two successive readings ( Δt =2 or 10 min) at the permeameter was also…

Permeability (earth sciences)Infiltration (hydrology)Hydraulic conductivitySample size determinationDrop (liquid)Soil scienceGeotechnical engineeringAquatic ScienceOrder of magnitudeMathematicsVolumetric flow ratePermeameterJournal of Agricultural Engineering Research
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Symmetry-species conversion in CD3systems

1993

The rates for symmetry-species conversion of CD3 groups are calculated using a model in which the interaction between the quadrupolar moment of the deuterons with electric-field gradient at the site of the nucleus causes symmetry-changing transitions. Just the same phonons are considered for energy conservation as are used to describe the temperature dependence of inelastic neutron scattering experiments. For the conversion rate, a similar temperature dependence is found as has already been obtained for CH3. For temperatures around the tunnelling energy, a behaviour is predicted for CD3 that is different from the behaviour in protonated systems according to all theories known to the authors…

PhononChemistryCondensed Matter PhysicsResonance (particle physics)Inelastic neutron scatteringTunnel effectsymbols.namesakeDeuteriumOrders of magnitude (time)symbolsddc:530General Materials ScienceAtomic physicsRaman spectroscopyQuantum tunnellingJournal of Physics: Condensed Matter
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