Search results for " Spectra"

showing 10 items of 709 documents

Study of the effects of nuclear motion on High Harmonic Generation in simple molecules

2009

Settore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciNuclear motion harmonic spectraSettore FIS/03 - Fisica Della Materia
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Spectral Analysis of LMC-X2 with XMM/Newton

2008

We present the results of the analisys of an archival observation of LMC X-2 performed with XMM/Newton. The spectra of this source has never been analyzed with a high precision instrument before. The spectrum of the source can be fitted with a blackbody with a temperature 1.5 keV plus a disk blackbody at 0.8 keV. We argue that the emission of this source can be straightforwardly interpreted as a sum of the emission from a boundary layer between the NS and the disc and a blackbody component coming from the disc itself. The detection of the O VIII emission line (and the lack of detection of lines in the iron region) can be due to the fact that the source lies in the Large Magellanic Cloud.

Settore FIS/05 - Astronomia E AstrofisicaX-rays: spectral analysis
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Synthetic and natural chromium bearing spinels: an optical spectroscopy study

2014

Four samples of synthetic chromium-bearing spinels of (Mg, Fe2+)(Cr, Fe3+)2O4 composition and four samples of natural spinels of predominantly (Mg, Fe2+)(Al, Cr)2O4 composition were studied at ambient conditions by means of optical absorption spectroscopy. Synthetic end-member MgCr2O4 spinel was also studied at pressures up to ca. 10 GPa. In both synthetic and natural samples, chromium is present predominantly as octahedral Cr3+ seen in the spectra as two broad intense absorption bands in the visible range caused by the electronic spin-allowed 4A2g → 4T2g and 4A2g → 4T1g transitions (U- and Y-band, respectively). A distinct doublet structure of the Y-band in both synthetic and natural spine…

Settore GEO/06 - MineralogiaOptical absorption spectraAbsorption spectroscopyTrivalent chromiumInorganic chemistrySpinelSpinelInfrared spectroscopychemistry.chemical_elementRacah parameterengineering.materialPressure effectChromiumCrystallographySpinel; Trivalent chromium; Optical absorption spectra; Pressure effectAbsorption edgechemistryOctahedronGeochemistry and PetrologyengineeringGeneral Materials ScienceSpectroscopySettore CHIM/02 - Chimica Fisica
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Indoor lighting quality: Effects of different wall colours

2016

This paper reports the results of measurements performed in a test room to investigate the impact of using different wall colours and light scenes on indoor lighting quality. Eye level spectral irradiances were measured for a user located inside the room and seated at a desk. These measurements allow the use of the Irradiance Toolbox, which makes it possible to calculate equivalent illuminances for the photopigments in the human eye. Moreover, the CIECAM02 colour appearance model was used to investigate the variations in hue and chroma values of the different wall colours when changing the light scene. The results demonstrate that there are significant variations in eye level spectral irra…

Settore ING-IND/11 - Fisica Tecnica Ambientalebusiness.industryComputer science0211 other engineering and technologiesIrradianceCIECAM0202 engineering and technology03 medical and health sciences0302 clinical medicineOpticsQuality (physics)021105 building & constructionTest roomElectrical and Electronic EngineeringbusinessIndoor lighting CIECAM02 Colour appearance models Photopigments Spectral irradianceNon visual effects of light colour perception030217 neurology & neurosurgery
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Input for baroreflex analysis: which blood pressure signal should be used?

2022

The baroreflex (BR) is an important physiological regulatory mechanism which reacts to blood pressure perturbations with reflex changes of target variables such as the heart period (electrocardiogram derived RR interval) or the peripheral vascular resistance (PVR). Evaluation of cardiac chronotropic (RR as a target variable) and vascular resistance (target PVR) BR arms was in previous studies mainly based on the use of the spontaneous variability of the systolic or diastolic blood pressure (SBP, DBP), respectively, as the input signals. The use of other blood pressure measures such as the mean blood pressure (MBP) as an input signal for BR analysis is still under investigation. Making the a…

Settore ING-INF/06 - Bioingegneria Elettronica E InformaticaArterial baroreflex blood pressure cardiovascular variability spectral analysis transfer function head-up tilt mental arithmetic task muscle sympathetic nerve activity
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Quantifying High-Order Interactions in Cardiovascular and Cerebrovascular Networks

2022

We present a method to analyze the dynamics of physiological networks beyond the framework of pairwise interactions. Our method defines the so-called O-information rate (OIR) as a measure of the higher-order interaction among several physiological variables. The OIR measure is computed from the vector autoregressive representation of multiple time series, and is applied to the network formed by heart period, systolic and diastolic arterial pressure, respiration and cerebral blood flow variability series measured in healthy subjects at rest and after head-up tilt. Our results document that cardiovascular, cerebrovascular and respiratory interactions are highly redundant, and that redundancy …

Settore ING-INF/06 - Bioingegneria Elettronica e InformaticaInformation dynamics spectral analysis Granger causality time series analysis network physiology2022 12th Conference of the European Study Group on Cardiovascular Oscillations (ESGCO)
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On the spectral properties of some classes of operators

2010

This article concerns the spectral properties of some classes of operators defined by means some inequelities

Settore MAT/05 - Analisi MatematicaLocal spectral theory and Fredholm theory
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Weyl's and Browder's theorems through the quasi-nilpotent part

2006

Weyl and Browder type theorems are characterized by means the quasi-nilpotent part

Settore MAT/05 - Analisi MatematicaQuasi-nilpotent part local spectral theory Weyl type theorems
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Accretion shock on CTTSs and its X-ray emission

2009

High spectral resolution X-ray observations of classical T Tauri stars (CTTSs) demonstrate the presence of plasma at T~2-3×10^6 K and ne~10^11-10^13 cm-3. Stationary models suggest that this emission is due to shock-heated accreting material. We address this issue by a 1-D hydrodynamic model of the impact of the accretion flow onto a chromosphere of a CTTS with the aim of investigating the stability of accretion shock and the role of the chromosphere. Our simulations include the effects of gravity, radiative losses from optically thin plasma, the thermal conduction and a detailed modeling of the stellar chromosphere. Here we present the results of a simulation based on the parameters of the…

Shock wavePhysicsPlanetary bow shocksAstrophysics::High Energy Astrophysical Phenomenainterplanetary shocksPlasmaAstrophysicsNumerical approximation and analysisThermal conductionAccretion (astrophysics)T Tauri starSettore FIS/05 - Astronomia E AstrofisicaX-ray emission spectra and fluorescenceRadiative transferHydrodynamicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsSpectral resolutionChromosphereAstrophysics::Galaxy Astrophysics
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Probing the radio emission from air showers with polarization measurements

2014

The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple setups. The direction of the electric field induced by this emission process depends only on the local magnetic field vector and on the incoming direction of the air shower. We report on measurements of the electric field vector where, in addition to this geomagnetic component, another component has been observed which cannot be described by the geomagnetic emission process. The data provide strong evidence that the other electric field component is polarized radially wit…

SignalsAstronomy01 natural sciencesElectric fieldComputational physicsCosmic-raysComposition energy spectra and interactionscosmic rayRadio wavePhysicsEarth's magnetic fieldHigh Energy Astrophysical Phenomena (astro-ph.HE)Radiation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsPolarization (waves)Polarization (waves)BolometersThunderstormsMagnetic fieldComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCAMPO MAGNÉTICOradio emissionRadio waveNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerComposition energy spectra and interactions; Solar electromagnetic emission; BolometersAstrophysics::High Energy Astrophysical Phenomenainfrared submillimeter wave microwave and radiowave receivers and detectorsFieldFOS: Physical sciencesPierre Auger Observatory ; air shower ; radio emissionRadiationMonte-carlo SimulationsOpticsElectric field0103 physical sciencesddc:530Pierre auger observatory010306 general physicsPulsesInstrumentation and Methods for Astrophysics (astro-ph.IM)Pierre Auger Observatory010308 nuclear & particles physicsbusiness.industrySolar electromagnetic emissionFísicaOpticsDetectorComputational physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerEarth's magnetic fieldMagnetic fieldExperimental High Energy PhysicsbusinessCodalema
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