Search results for "LINE"

showing 10 items of 31271 documents

Eco-Friendly Estimation of Heavy Metal Contents in Grapevine Foliage Using In-Field Hyperspectral Data and Multivariate Analysis

2019

Heavy metal monitoring in food-producing ecosystems can play an important role in human health safety. Since they are able to interfere with plants’ physiochemical characteristics, which influence the optical properties of leaves, they can be measured by in-field spectroscopy. In this study, the predictive power of spectroscopic data is examined. Five treatments of heavy metal stress (Cu, Zn, Pb, Cr, and Cd) were applied to grapevine seedlings and hyperspectral data (350−2500 nm), and heavy metal contents were collected based on in-field and laboratory experiments. The partial least squares (PLS) method was used as a feature selection technique, and multiple linear regressions (…

010504 meteorology & atmospheric sciencesScience010501 environmental sciences01 natural sciencesMetalHuman healthLinear regressionPartial least squares regressionSpectroscopyheavy metals0105 earth and related environmental sciencesChemistrysvmQfungifield spectroscopy; hyperspectral; heavy metals; grapevine; PLS; SVM; MLRHyperspectral imagingfood and beveragesHeavy metalsplsEnvironmentally friendlyfield spectroscopygrapevinemlrhyperspectralvisual_artEnvironmental chemistryvisual_art.visual_art_mediumGeneral Earth and Planetary SciencesRemote Sensing; Volume 11; Issue 23; Pages: 2731
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An Integrated Multiscale Method for the Characterisation of Active Faults in Offshore Areas. The Case of Sant’Eufemia Gulf (Offshore Calabria, Italy)

2021

Diagnostic morphological features (e.g., rectilinear seafloor scarps) and lateral offsets of the Upper Quaternary deposits are used to infer active faults in offshore areas. Although they deform a significant seafloor region, the active faults are not necessarily capable of producing large earthquakes as they correspond to shallow structures formed in response to local stresses. We present a multiscale approach to reconstruct the structural pattern in offshore areas and distinguish between shallow, non-seismogenic, active faults, and deep blind faults, potentially associated with large seismic moment release. The approach is based on the interpretation of marine seismic reflection data and …

010504 meteorology & atmospheric sciencesSettore GEO/02 - Geologia Stratigrafica E SedimentologicaScienceSettore GEO/03 - Geologia StrutturaleInversion (geology)Active faultSlab-tear faultLate MioceneCalabrian arc (Italy)010502 geochemistry & geophysicsFault scarp01 natural sciencesPaleontologymorphotectonic analysiMorphotectonic analysisHigh-resolution seismic dataBathymetry0105 earth and related environmental sciencesActive tectonicsactive tectonicQAnticlineSeafloor spreadingTectonicsGeneral Earth and Planetary SciencesGeologySouthern tyrrhenian sea
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How Offshore Groundwater Shapes the Seafloor

2018

The MARCAN project, launched last January, is working to fill a gap in our knowledge of how freshwater flowing underground shapes and alters the continental margins.

010504 meteorology & atmospheric sciencesSettore GEO/04 - Geografia Fisica E Geomorfologia010502 geochemistry & geophysics01 natural sciencesSeafloor spreadingOceanographyContinental margin13. Climate actioncontinental marginGeneral Earth and Planetary SciencesSubmarine pipelineGroundwaterGroundwaterGeology0105 earth and related environmental sciencesEos
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Evidence of active fluid seepage (AFS) in the southern region of the central Mediterranean Sea

2018

Abstract Active fluid seepage (AFS) at the seafloor is a global phenomenon associated with seafloor morphologies in different geodynamic contexts. Advanced geophysical techniques have allowed geoscientists to characterise pockmarks, mounds and flares associated with AFS. We present a range of new marine geological data acquired in the southern region of the central Mediterranean Sea (northern Sicily continental margin, northwestern Sicily Channel and offshore of the Maltese Islands), which allow us to identify AFSs. AFSs are spatially distributed as clusters, aligned or isolated at different depths, ranging from few decametres offshore of the Maltese Islands; up to 400 m offshore of norther…

010504 meteorology & atmospheric sciencesSicily ChannelSettore GEO/02 - Geologia Stratigrafica E SedimentologicaRange (biology)Settore GEO/03 - Geologia Strutturale010502 geochemistry & geophysics01 natural sciencesFluid seepagePaleontologyGas flaresMediterranean seaContinental marginElectrical and Electronic EngineeringInstrumentation0105 earth and related environmental sciencesMoundgeographyFluid seepage; Gas flares; Mound; Pockmark; Sicily Channel; Instrumentation; Electrical and Electronic Engineeringgeography.geographical_feature_categoryContinental shelfApplied MathematicsPockmarkFluid seepage; Gas flares; Mound; Pockmark; Sicily ChannelGas flareCondensed Matter PhysicsSeafloor spreadingPockmarkSubmarine pipelineGeologyChannel (geography)
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High‐resolution stimulated Raman spectroscopy and analysis of line positions and assignments for the ν 2 and ν 3 bands of 13 C 2 H 4

2016

High-resolution stimulated Raman spectra of13C2H4 in the regions of the ν2 and ν3 Raman active modes have been recorded at two temperatures (145 and 296 K) based on the quasi continuous-wave (cw) stimulated Raman spectrometer at Instituto de Estructura de la Materia IEM-CSIC in Madrid. A tensorial formalism adapted to X2Y4 planar asymmetric tops with D2h symmetry (developed in Dijon) and a program suite called D2hTDS (now part of the XTDS/SPVIEW spectroscopic software) were proposed to analyze and calculate the high-resolution spectra. A total of 103 and 51 lines corresponding to ν2 and ν3 Raman active modes have been assigned and fitted in wavenumber with a global root mean square deviatio…

010504 meteorology & atmospheric sciencesSpectrometerChemistryAnalytical chemistry02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesSpectral linesymbols.namesakePlanarsymbolsWavenumberGeneral Materials ScienceAtomic physics0210 nano-technologySpectroscopyRaman spectroscopyRoot-mean-square deviationSpectroscopyRaman scattering0105 earth and related environmental sciencesJournal of Raman Spectroscopy
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The tsunami phenomenon

2017

Abstract With human activity increasingly concentrating on coasts, tsunamis (from Japanese tsu = harbour, nami = wave) are a major natural hazard to today’s society. Stimulated by disastrous tsunami impacts in recent years, for instance in south-east Asia (2004) or in Japan (2011), tsunami science has significantly flourished, which has brought great advances in hazard assessment and mitigation plans. Based on tsunami research of the last decades, this paper provides a thorough treatise on the tsunami phenomenon from a geoscientific point of view. Starting with the wave features, tsunamis are introduced as long shallow water waves or wave trains crossing entire oceans without major energy l…

010504 meteorology & atmospheric sciencesSubmarineGeologyAquatic ScienceHazard analysis010502 geochemistry & geophysics01 natural sciencesWaves and shallow waterOceanographyWave shoalingNatural hazardSubmarine pipelineSedimentary rockTsunami earthquakeGeologySeismology0105 earth and related environmental sciencesProgress in Oceanography
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Impulsive coronal heating from large-scale magnetic rearrangements: from IRIS to SDO/AIA

2019

The Interface Region Imaging Spectrograph (IRIS) has observed bright spots at the transition region footpoints associated with heating in the overlying loops, as observed by coronal imagers. Some of these brightenings show significant blueshifts in the Si iv line at 1402.77 A (logT[K] = 4.9). Such blueshifts cannot be reproduced by coronal loop models assuming heating by thermal conduction only, but are consistent with electron beam heating, highlighting for the first time the possible importance of non-thermal electrons in the heating of non-flaring active regions. Here we report on the coronal counterparts of these brightenings observed in the hot channels of the Atmospheric Imaging Assem…

010504 meteorology & atmospheric sciencesSun: activity Sun: corona Sun: UV radiation Astrophysics - Solar and Stellar AstrophysicsFOS: Physical sciencesAstrophysicsElectron01 natural sciences0103 physical sciencesmedicineAstrophysics::Solar and Stellar AstrophysicsIris (anatomy)010303 astronomy & astrophysicsSpectrographSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsAstronomy and AstrophysicsCoronal loopThermal conductionmedicine.anatomical_structureAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceCoronal planePhysics::Space PhysicsCathode rayAstrophysics::Earth and Planetary Astrophysics
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Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A

2019

We perform three-dimensional hydrodynamic simulations of aspherical core-collapse supernovae focusing on the matter mixing in SN 1987A. The impacts of four progenitor (pre-supernova) models and parameterized aspherical explosions are investigated. The four pre-supernova models include a blue supergiant (BSG) model based on a slow merger scenario developed recently for the progenitor of SN 1987A (Urushibata et al. 2018). The others are a BSG model based on a single star evolution and two red supergiant (RSG) models. Among the investigated explosion (simulation) models, a model with the binary merger progenitor model and with an asymmetric bipolar-like explosion, which invokes a jetlike explo…

010504 meteorology & atmospheric sciencesSupergiant starAstrophysics::High Energy Astrophysical PhenomenaBinary numberchemistry.chemical_elementNeutron starFOS: Physical sciencesHydrodynamical simulationAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesCore-collapse supernovaeAstrophysics::Solar and Stellar AstrophysicsRed supergiant010303 astronomy & astrophysicsMixing (physics)HeliumStellar evolutionary modelSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsSupernova dynamicSupernovaNeutron starchemistryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceExplosive nucleosynthesisSupergiantAstrophysics - High Energy Astrophysical Phenomena
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Deep X-ray view of the Class I YSO Elias 29 with XMM-Newton and NuSTAR

2019

[Abridged] We investigated the X-ray characteristics of the Class I YSO Elias 29 with joint XMM-Newton and NuSTAR observations of 300 ks and 450 ks, respectively. These are the first observations of a very young (<1 Myr) stellar object in a band encompassing simultaneously both soft and hard X-rays. In addition to the hot Fe complex at 6.7 keV, we observed fluorescent emission from Fe at $\sim6.4$ keV, confirming the previous findings. The line at 6.4 keV is detected during quiescent and flaring states and its flux is variable. The equivalent width is found varying in the $\approx 0.15--0.5$ keV range. These values make unrealistic a simple model with a centrally illuminated disk and sug…

010504 meteorology & atmospheric sciencesYoung stellar objectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_studyStar formationAstronomy and AstrophysicsCoronaAccretion (astrophysics)Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomenastars:activity–stars:coronae–stars:pre-mainsequence–stars:formation–stars:flareEquivalent widthFlare
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Nitrogen broadening of SF6 transitions in the nu3 band

2001

Abstract Nitrogen induced pressure-broadened halfwidths of a number of ν3 transitions of SF6 are calculated using the complex Robert–Bonamy (CRB) formalism. The calculations are made at 200, 250, 296 and 350 K and the temperature dependence of the halfwidths are determined. The intermolecular potential is taken as a sum of the leading electrostatic and Lennard-Jones [6] , [7] , [8] , [9] , [10] , [11] , [12] atom–atom components. The dynamics of the collision process are correct to second order in time. The calculated halfwidths are used to simulate the ν3 spectrum, which is compared to a simulation made using the HITRAN96 halfwidths and measurements made at the Universite Pierre et Marie C…

010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Organic Chemistrychemistry.chemical_elementSulfur hexafluoride01 natural sciencesNitrogenAnalytical ChemistryMarie curieInorganic ChemistrySulfur hexafluoridechemistry.chemical_compoundFormalism (philosophy of mathematics)chemistry[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesIntermolecular potentialTemperature dependence of the halfwidthHalfwidthsAtomic physicsLine broadening010306 general physicsSpectroscopy0105 earth and related environmental sciences
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