Search results for "hot spot"

showing 10 items of 15 documents

Hot spots and gluon field fluctuations as causes of eccentricity in small systems

2021

We calculate eccentricities in high energy proton-nucleus collisions, by calculating correlation functions of the energy density field of the Glasma immediately after the collision event at proper time tau = 0. We separately consider the effects of color charge and geometrical hot spot fluctuations, analytically performing the averages over both in a dilute-dense limit. We show that geometric fluctuations of hot spots inside the proton are the dominant source of eccentricity whereas color charge fluctuations only give a negligible correction. The size and number of hot spots are the most important parameters characterizing the eccentricities.

Nuclear TheoryField (physics)ProtonAZIMUTHAL ANISOTROPIESFLOWmedia_common.quotation_subjectFOS: Physical sciencesHot spot (veterinary medicine)hiukkasfysiikka114 Physical sciences01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesProper timeEccentricity (behavior)LONG-RANGEHARMONICSNuclear Experiment010306 general physicsPLUS PB COLLISIONSGluon fieldmedia_commonPROTON-LEAD COLLISIONSPhysics010308 nuclear & particles physicskvarkki-gluoniplasmaANGULAR-CORRELATIONSComputational physicsHigh Energy Physics - PhenomenologyNEAR-SIDEAstrophysics::Earth and Planetary AstrophysicsHIGH TRANSVERSE-MOMENTUMPPBEvent (particle physics)Color chargePhysical Review D
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Convolutional Neural Network for Dust and Hotspot Classification in PV Modules

2020

20th IEEE International Conference on Environment and Electrical Engineering, EEEIC 2020, online, 9 Jun 2020 - 12 Jun 2020; Energies : open-access journal of related scientific research, technology development and studies in policy and management 13(23), 6357 (2020). doi:10.3390/en13236357 special issue: "Special Issue "Selected Papers from 20 IEEE International Conference on Environment and Electrical Engineering (EEEIC 2020)" / Special Issue Editor: Prof. Dr. Rodolfo Araneo, Guest Editor"

Control and OptimizationComputer science020209 energyReal-time computingEnergy Engineering and Power Technologydiagnosticconvolutional neural network02 engineering and technology010501 environmental sciencesSettore ING-IND/32 - Convertitori Macchine E Azionamenti Elettricilcsh:Technology01 natural sciencesConvolutional neural networkphotovoltaic energyhot spotHotspot (geology)diagnostics0202 electrical engineering electronic engineering information engineeringenergy efficientElectrical and Electronic EngineeringEngineering (miscellaneous)0105 earth and related environmental sciencesSettore ING-IND/11 - Fisica Tecnica Ambientalelcsh:TRenewable Energy Sustainability and the Environmentbusiness.industryPhotovoltaic systemDirtartificial intelligencerenewable energy620Renewable energyElectricity generationinfrared thermographydustddc:620businessEnergy (miscellaneous)Efficient energy use
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The early B-type star Rho Oph A is an X-ray lighthouse

2017

We present the results of a 140 ks XMM-Newton observation of the B2 star $\rho$ Ophiuchi A. The star has exhibited strong X-ray variability: a cusp-shaped increase of rate, similar to that which we partially observed in 2013, and a bright flare. These events are separated in time by about 104 ks, which likely corresponds to the rotational period of the star (1.2 days). Time resolved spectroscopy of the X-ray spectra shows that the first event is caused by an increase of the plasma emission measure, while the second increase of rate is a major flare with temperatures in excess of 60 MK ($kT\sim5$ keV). From the analysis of its rise, we infer a magnetic field of $\ge300$ G and a size of the f…

Rotation periodStars: activity010504 meteorology & atmospheric sciencesMagnetismAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesHot spot (veterinary medicine)Astrophysics01 natural sciencesSpectral linelaw.inventionStars: early-typelaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsX-rays: star010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Stars: magnetic fieldStarspotStars: individual: Rho OphiuchiInstitut für Physik und AstronomieAstronomy and AstrophysicsRadiusAstronomy and AstrophysicAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceStarspotAstrophysics::Earth and Planetary AstrophysicsLow MassAstrophysics - High Energy Astrophysical PhenomenaFlare
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Assessing land condition as a first step to achieving land degradation neutrality : A case study of the Republic of Srpska

2018

Abstract Land Degradation Neutrality (LDN) is a key voluntary and aspirational target of Sustainable Development Goal (SDG) 15 which urges countries to protect, restore and promote sustainable use of terrestrial ecosystems, sustainably manage forests, combat desertification, and halt and reverse land degradation and halt biodiversity loss. A first and critical important step in the implementation of LDN is assessing the current land condition using not only active restoration of degraded land, but also targeting land degradation drivers behind the land degradation process. In a first step to achieve these goals, countries were provided a global dataset for three sub-indicators of land degra…

Resource (biology)010504 meteorology & atmospheric sciencesSòls Erosiómedia_common.quotation_subjectGeography Planning and DevelopmentLand cover010501 environmental sciencesManagement Monitoring Policy and Law01 natural sciencesOpportunitiesUrbanizationIndicatorsHot spotsChallenges0105 earth and related environmental sciencesmedia_commonSustainable developmentLand usebusiness.industryEnvironmental resource managementPE&RCGeographyDesertificationSustainabilityLand degradationTrendsbusinessLDN target
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First measurements of magmatic gas composition and fluxes during an eruption (October 2010) of Piton de la Fournaise hot spot volcano, La reunion isl…

2011

Piton de la Fournaise (PdF), in the western Indian Ocean, is a very active hot spot basaltic volcano, with 1-2 fissure eruptions per year on average. Its magmas have been widely studied and its eruptions are well anticipated by the local seismic-geodetic monitoring network. However, no datum was yet available for its magmatic gas emissions (restricted to only eruptive phases and hardly accessible). Here we report on the first measurements of the chemical composition and mass flux of magmatic gases emitted during a PdF eruption in October 2010. Hot gases arising from different eruptive vents were remotely measured with OP-FTIR spectroscopy, using molten lava fragments as IR radiation source,…

Piton de la Fournaise volcano hot spot magmatic gasSettore GEO/08 - Geochimica E Vulcanologia
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Capability assessment of the SEVIRI/MSG GPP product for the detection of areas affected by water stress

2020

[ES] Se presenta el nuevo producto de producción primaria bruta (GPP) de EUMETSAT derivado a partir de datos del satélite geoestacionario SEVIRI/MSG (MGPP LSA-411) y se evalúa su potencial para detectar zonas afectadas por estrés hídrico (hot spots). El producto GPP se basa en la aproximación de Monteith, que modela la GPP de la vegetación como el producto de la radiación fotosintéticamente activa (PAR) incidente, la fracción de PAR absorbida (fAPAR) y un factor de eficiencia de uso de la radiación (ε). El potencial del producto MGPP para detectar hot spots se evalúa, utilizando un periodo corto de tres años, a escala local y regional, comparando con datos in situ derivados de medidas en to…

010504 meteorology & atmospheric sciencesWater stressGeography Planning and Development0211 other engineering and technologieslcsh:G1-92202 engineering and technology01 natural sciencesMonteithDetectionEstrés hídricoMGPPEarth and Planetary Sciences (miscellaneous)Hot spotsMSGlcsh:Geography (General)021101 geological & geomatics engineering0105 earth and related environmental sciences
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Enhanced volcanic hot-spot detection using MODIS IR data: results from the MIROVA system

2015

geographygeography.geographical_feature_category010504 meteorology & atmospheric sciencesMeteorologyGeologyOcean EngineeringHot spot (veterinary medicine)010502 geochemistry & geophysics01 natural sciencesVolcanoGeology0105 earth and related environmental sciencesWater Science and TechnologyRemote sensingGeological Society, London, Special Publications
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INTEGRAL and RXTE observations of accreting millisecond pulsar IGR J00291+5934 in outburst

2005

Simultaneous observations of the accretion-powered millisecond pulsar IGR J00291+5934 by International Gamma-Ray Astrophysics Laboratory and Rossi X-ray Timing Explorer during the 2004 December outburst are analysed. The average spectrum is well described by thermal Comptonization with an electron temperature of 50 keV and Thomson optical depth tau_T ~ 1 in a slab geometry. The spectral shape is almost constant during the outburst. We detect a spin-up of the pulsar with nudot=8.4x10E-13 Hz/s. The ISGRI data reveal the pulsation of X-rays at a period of 1.67 milliseconds up to ~150 keV. The pulsed fraction is shown to increase from 6 per cent at 6 keV to 12--20 per cent at 100 keV. This is n…

Spectral shape analysisAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesHot spot (veterinary medicine)Astrophysicsaccretion accretion discs binaries: close stars: individual: IGR J00291+5934 stars: neutron X-rays: binariesAstrophysics01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]symbols.namesakestars: neutronPulsaraccretionMillisecond pulsar0103 physical sciencesOptical depth (astrophysics)010306 general physics010303 astronomy & astrophysicsPhysicsMillisecondbinaries: close[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Astrophysics (astro-ph)Astronomy and Astrophysicsaccretion discspulsars: individual (IGR J00291+5934)13. Climate actionSpace and Planetary SciencesymbolsElectron temperatureDoppler effectX-ray: binaries
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Correlated gluonic hot spots meet symmetric cumulants data at LHC energies

2019

We present a systematic study on the influence of spatial correlations between the proton constituents, in our case gluonic hot spots, their size and their number on the symmetric cumulant SC(2, 3), at the eccentricity level, within a Monte Carlo Glauber framework [1]. When modeling the proton as composed by 3 gluonic hot spots, the most common assumption in the literature, we find that the inclusion of spatial correlations is indispensable to reproduce the negative sign of SC(2, 3) in the highest centrality bins as dictated by data. Further, the subtle interplay between the different scales of the problem is discussed. To conclude, the possibility of feeding a 2+1D viscous hydrodynamic sim…

COLLISIONSNuclear and High Energy PhysicsParticle physicsNuclear TheoryFLOWMonte Carlo methodFOS: Physical sciencesSmall systemshiukkasfysiikka114 Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)correlations0103 physical sciencesEntropy (information theory)ddc:530initial state010306 general physicsCumulantPhysicsLarge Hadron Colliderta114010308 nuclear & particles physicselliptic flowElliptic flowhot spotsHigh Energy Physics - Phenomenologysmall systemsSubstructureGlauberNuclear Physics A
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Airborne measurement of hot spot reflectance signatures

2004

The so-called hot spot is a fine directional signature of the surface reflectance observed for phase angles close to zero. In this paper, we analyze and discuss several such signatures acquired from the airborne POLDER and HyMap instruments during the DAISEX'99 campaign over agricultural crops. The observed signatures are very similar to those acquired from space at a resolution of several tens of kilometers [J. Geophys. Res. 107 (2002)], which provides further evidence that the hot spot is a scale-free feature. The hot spots can be fitted by a two-parameter function (amplitude and width) of the phase angle derived from canopy radiative transfer modeling. The model predicts that the amplitu…

Canopy[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere010504 meteorology & atmospheric sciencesInstrumentationPhase angleResolution (electron density)0211 other engineering and technologiesSoil ScienceGeologyHot spot (veterinary medicine)02 engineering and technology01 natural sciencesAmplitudeRange (statistics)Computers in Earth Sciences[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentGeologyHyMapComputingMilieux_MISCELLANEOUS021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensing
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