Search results for "SPECTRA"

showing 10 items of 3542 documents

How does environmental variation translate into biological processes?

2001

Birth and death rates, as so many other biological processes, are usually not linearly related to environmental variation. Common examples of non-linear response forms include unimodal ‘‘optimum-type’’ responses and various saturating responses. These responses filter the signal coming from the environment to a corresponding biological process. We explored how different types of environmental signal may be transformed to a biological process. We were interested in the effect of the filter on modulation of (1) the variance of the signal, on (2) the variance-covariance structure between the signal and the filtered signal, and on (3) the match between the power spectra of the signal and the fi…

Physicseducation.field_of_studyColors of noiseModulationPopulationSpectral densityFilter (signal processing)Biological systemeducationSignalEcology Evolution Behavior and SystematicsBirth–death processPower (physics)Oikos
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Coherent population oscillations with nitrogen-vacancy color centers in diamond

2015

We present results of our research on two-field (two-frequency) microwave spectroscopy in nitrogen-vacancy (NV-) color centers in a diamond. Both fields are tuned to transitions between the spin sublevels of the NV- ensemble in the 3A2 ground state (one field has a fixed frequency while the second one is scanned). Particular attention is focused on the case where two microwaves fields drive the same transition between two NV- ground state sublevels (ms=0 -> ms=+1). In this case, the observed spectra exhibit a complex narrow structure composed of three Lorentzian resonances positioned at the pump-field frequency. The resonance widths and amplitudes depend on the lifetimes of the levels in…

Physicseducation.field_of_studyField (physics)Atomic Physics (physics.atom-ph)PopulationRelaxation (NMR)ResonanceFOS: Physical sciences02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesSpectral linePhysics - Atomic Physics0103 physical sciencesRotational spectroscopyAtomic physics010306 general physics0210 nano-technologyGround stateeducationSpin (physics)
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NaK Λ doubling and permanent electric dipoles in low-lying1Πstates: Experiment and theory

1998

The paper presents \ensuremath{\Lambda} splittings and q factors in the NaK $D{}^{1}\ensuremath{\Pi}$ state, directly measured from the electric radio-frequency-optical double resonance (RF-ODR) in laser-induced fluorescence (LIF) for a number of vibrational states $v=1--22$ with definite rotational levels J between 7 and 46. Permanent electric dipole moment values (d) have been obtained by measuring in LIF spectra the relative intensities of ``forbidden'' lines caused by dc Stark effect induced $e/f$ mixing in the ${}^{1}\ensuremath{\Pi}$ state, with their subsequent processing, which allowed us to obtain the $q/d$ ratio. A possible influence of the hyperfine structure on the RF-ODR signal…

Physicseducation.field_of_studyPopulationAtomic and Molecular Physics and OpticsSpectral linePseudopotentialElectric dipole momentsymbols.namesakeStark effectsymbolsAtomic physicsGround stateeducationWave functionHyperfine structurePhysical Review A
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Observation of an Intense Quasicontinuum of Superdeformed Rotational Transitions inEu143

1996

Quasicontinuum spectra in coincidence with transitions belonging to the different potential wells of {sup 143}Eu are studied with an increasing number of coincidence folds. An intense bump of rotationally correlated transitions is observed to develop in the high spin region. Fold distributions, angular anisotropies, moment of inertia determinations, and lower limits of lifetimes as a function of the rotational frequency show that the bump originates from highly collective rotationally damped {ital E}2 transitions generated by superdeformed states. {copyright} {ital 1996 The American Physical Society.}

Physicseducation.field_of_studyPopulationGeneral Physics and AstronomyMoment of inertiaAtomic physicsAnisotropyeducationRotational frequencyCoincidenceSpectral linePhysical Review Letters
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SPECTROSCOPY AND NON-EQUILIBRIUM DISTRIBUTION OF VIBRATIONALLY EXCITED METHANE IN A SUPERSONIC JET

1998

Abstract High-resolution spectra of supersonic jets of vibrationally excited methane have been recorded by diode laser in the 8 μm region. A formalism for the description of energy distribution is proposed. It allows to estimate populations of vibrational polyads. Under these non-equilibrium conditions, translational temperature is also measured from line profiles. For relaxation, it is shown that vibrational relaxation between polyads is negligible whereas strong redistribution of population arises inside each polyad. Spectroscopically, observed lines involving the first four excited polyads allows cross-checked tests for energy level analysis.

Physicseducation.field_of_studyRadiationPopulationLaserAtomic and Molecular Physics and OpticsMethaneSpectral linelaw.inventionMathematics::Logicchemistry.chemical_compoundchemistrylawExcited stateVibrational energy relaxationSupersonic speedPhysics::Chemical PhysicsAtomic physicseducationSpectroscopySpectroscopyJournal of Quantitative Spectroscopy and Radiative Transfer
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On coronal structures and their variability in active stars: The case of Capella observed with Chandra/LETGS

2003

In this paper we present a detailed analysis of two X-ray spectra of Capella, taken eleven months apart with the Low Energy Transmission Grating Spectrometer (LETGS) of the Chandra Observatory. We have studied variability of the coronal emission over different time scales, both in the whole X-ray band and in narrow temperature ranges identified by lines. The comparison of the two observations shows that the whole coronal emission of Capella in March 2000 was 3% higher than in February 2001; there also appears to be a tendency, albeit a marginal one, for the hottest lines to show the largest changes between the two observations. A detailed search for short-term variability (on time scales ra…

Physicseducation.field_of_studySpectrometerAstrophysics::High Energy Astrophysical PhenomenaPopulationMonte Carlo methodAstronomyAstronomy and AstrophysicsPlasmaAstrophysicsSpectral lineIonStarsSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceObservatoryX-rays: stars techniques: spectroscopic stars: activity stars: coronae stars: individual: Capellaeducation
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The stellar population of the Rosat North Ecliptic Pole survey. II. Spectral analysis

2008

X-ray surveys allow to identify young, main-sequence stars in the solar neighborhood. Young, stellar samples, selected according to their activity, can be used to determine the stellar birthrate in the last billion years. The ROSAT North Ecliptic Pole survey (NEP), with its moderately deep sensitivity (fluxes ~10^(-14) erg cm^(-2) sec^(-1)), is the best survey, to date, able to sample the intermediate-age (10^8 - 10^9 years) nearby population. The identification process of NEP X-ray sources resulted in 144 X-ray sources having a normal stellar counterpart, with an excess of yellow stars with respect to model predictions. We want to determine if these X-ray active stars are young or intermed…

Physicseducation.field_of_studyStellar populationPopulationAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsEcliptic poleAstrophysicsAstrophysicsBillion yearsStarsSpace and Planetary ScienceROSATSpectral analysiseducationLine (formation)
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Compact dielectric reflective elements II Multichannel filter of closely spaced spectral bands

1994

The optical design of an interference wedge filter providing the simultaneous separation of a number of closely spaced spectral bands is studied. Multiple reflections of the incident collimated beam within the wedge are initiated, each of them characterized by a different angle of incidence and consequently by specific spectral parameters of the transmitted band. Model calculations based on the measured angular dependences of filter transmission parameters have been performed. The design is proposed for applications in optical communications (wavelength division demultiplexing), analytical spectroscopy (minipolychromators), color analysis, and similar areas.

Physicseducation.field_of_studybusiness.industryMaterials Science (miscellaneous)Physics::OpticsWedge filterSpectral bandsWedge (geometry)Industrial and Manufacturing EngineeringCollimated lightlaw.inventionWavelengthOpticslawAngle of incidence (optics)Filter (video)Business and International ManagementeducationbusinessBeam splitterApplied Optics
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The optical blocking filter for the ATHENA wide field imager: Ongoing activities towards the conceptual design

2015

ATHENA is the L2 mission selected by ESA to pursue the science theme "Hot and Energetic Universe" (launch scheduled in 2028). One of the key instruments of ATHENA is the Wide Field Imager (WFI) which will provide imaging in the 0.1-15 keV band over a 40'x40' large field of view, together with spectrally and time-resolved photon counting. The WFI camera, based on arrays of DEPFET active pixel sensors, is also sensitive to UV/Vis photons. Optically generated electron-hole pairs may degrade the spectral resolution as well as change the energy scale by introducing a signal offset. For this reason, the use of an X-ray transparent optical blocking filter is needed to allow the observation of all …

PhysicsfilterOffset (computer science)PhotonPixelbusiness.industryElectronic Optical and Magnetic MaterialApplied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicPhoton countingATHENAVibrationInstrumentation for AstrophysicX-rayOpticsConceptual designWFIField-effect transistorSpectral resolutionElectrical and Electronic Engineeringbusiness
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Multiband Photometry of the Blazar PKS 0537-441: A Major Active State in December 2004 - March 2005

2005

Multiband VRIJHK photometry of the Blazar PKS 0537-441 obtained with the REM telescope from December 2004 to March 2005 is presented. A major period of activity is found with more than four magnitudes variability in the V filter in 50 days and of 2.5 in 10 days. In intensity and duration the activity is similar to that of 1972 reported by Eggen (1973), but it is much better documented. No clear evidence of variability on time-scale of minutes is found. The spectral energy distribution is roughly described by a power-law, with the weaker state being the softer.

Physicsgalaxies: active; galaxies: BL Lacertae objects: PKS 0537-441galaxies: activeAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicslaw.inventionTelescopePhotometry (astronomy)galaxies: BL Lacertae objects: PKS 0537-441Space and Planetary Sciencelawgalaxies: active ; galaxies: BL Lacertae objects: PKS 0537-441active [galaxies]Spectral energy distributionActive stateBlazarBL Lacertae objects: PKS 0537-441 [galaxies]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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