Search results for "Clouds"

showing 10 items of 95 documents

CNN-based People Detection in Voxel Space using Intensity Measurements and Point Cluster Flattening

2021

In this paper real-time people detection is demonstrated in a relatively large indoor industrial robot cell as well as in an outdoor environment. Six depth sensors mounted at the ceiling are used to generate a merged point cloud of the cell. The merged point cloud is segmented into clusters and flattened into gray-scale 2D images in the xy and xz planes. These images are then used as input to a classifier based on convolutional neural networks (CNNs). The final output is the 3D position (x,y,z) and bounding box representing the human. The system is able to detect and track multiple humans in real-time, both indoors and outdoors. The positional accuracy of the proposed method has been verifi…

Physicsbusiness.industryPoint clusterComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONconvolutional neural networkQA75.5-76.95Space (mathematics)computer.software_genrehuman detectionFlatteningComputer Science ApplicationsIntensity (physics)flatteningControl and Systems EngineeringVoxelModeling and SimulationElectronic computers. Computer sciencepoint cloudsComputer visionArtificial intelligencebusinesscomputerSoftwareModeling, Identification and Control
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Sensitivity of low-level clouds and precipitation to anthropogenic aerosol emission in southern West Africa: a DACCIWA case study

2021

Abstract. During the West African summer monsoon, pollutants emitted in urbanized coastal areas modify cloud cover and precipitation patterns. The Dynamics-Aerosol-Chemistry-Cloud-Interactions in West Africa (DACCIWA) field campaign provided numerous aircraft-based and ground-based observations, which are used here to evaluate two experiments made with the coupled WRF-CHIMERE model, integrating both the direct and indirect aerosol effect on meteorology. During one well-documented week (1–7 July 2016), the impacts of anthropogenic aerosols on the diurnal cycle of low-level clouds and precipitation are analyzed in detail using high and moderate intensity of anthropogenic emissions in the expe…

PollutionAtmospheric Scienceaerosolmedia_common.quotation_subjectCloud covercloudsMonsoonAtmospheric sciencescomplex mixturesWest africaDiurnal cycleaerosol emissionddc:550DACCIWAPrecipitationlow-level cloudsmedia_commonPollutant[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]AerosolEarth sciences13. Climate action[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology[SDE]Environmental SciencesEnvironmental sciencesummer monsoonDynamics-Aerosol-Chemistry-Cloud Interactions in West Africaanthropogenic aerosol emission
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X-raying the interstellar medium: the study of SNR shells at the OAPa

2006

SM: clouds ISM: general ISM: individual objects: Vela Supernova Remnant ISM: structure ISM: supernova remnants X-rays: ISM
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X-ray emission from supernova remnants interacting with interstellar clouds

2009

SNRmolecular clouds
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Quantifying unpredictability: A multiple-model approach based on satellite imagery data from Mediterranean ponds.

2017

Fluctuations in environmental parameters are increasingly being recognized as essential features of any habitat. The quantification of whether environmental fluctuations are prevalently predictable or unpredictable is remarkably relevant to understanding the evolutionary responses of organisms. However, when characterizing the relevant features of natural habitats, ecologists typically face two problems: (1) gathering long-term data and (2) handling the hard-won data. This paper takes advantage of the free access to long-term recordings of remote sensing data (27 years, Landsat TM/ETM+) to assess a set of environmental models for estimating environmental predictability. The case study inclu…

Satellite ImageryAtmospheric ScienceTeledetecció010504 meteorology & atmospheric sciences0208 environmental biotechnologyMarine and Aquatic Scienceslcsh:Medicine02 engineering and technologycomputer.software_genre01 natural sciencesRemote SensingLimnologyEnvironmental monitoringRange (statistics)Satellite imageryAdditive modellcsh:ScienceFreshwater EcologyMultidisciplinaryEcologyMediterranean RegionApplied MathematicsSimulation and ModelingHabitatsVariable (computer science)Physical SciencesMetric (mathematics)Engineering and TechnologyData miningAlgorithmsResearch ArticleFreshwater EnvironmentsEnvironmental MonitoringResearch and Analysis MethodsClustering AlgorithmsMeteorologySurface WaterCloudsPredictabilityPondsDivergence (statistics)Ecosystem0105 earth and related environmental sciencesEcology and Environmental Scienceslcsh:RBiology and Life SciencesAquatic EnvironmentsBodies of WaterModels TheoreticalEcologia aquàtica020801 environmental engineeringLakesRemote Sensing TechnologyEarth SciencesEnvironmental sciencelcsh:QHydrologycomputerMathematicsPLoS ONE
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Energy Efficient Resource Allocation for Wireless Power Transfer Enabled Collaborative Mobile Clouds

2016

In order to fully enjoy high rate broadband multimedia services, prolonging the battery lifetime of user equipment is critical for mobile users, especially for smartphone users. In this paper, the problem of distributing cellular data via a wireless power transfer enabled collaborative mobile cloud (WeCMC) in an energy efficient manner is investigated. WeCMC is formed by a group of users who have both functionalities of information decoding and energy harvesting, and are interested for cooperating in downloading content from the operators. Through device-to-device communications, the users inside WeCMC are able to cooperate during the downloading procedure and offload data from the base sta…

ScheduleenergiatehokkuusComputer Networks and CommunicationsComputer sciencewireless power transfer02 engineering and technology7. Clean energyBase station0203 mechanical engineeringresources allocation0202 electrical engineering electronic engineering information engineeringWirelessResource managementElectrical and Electronic Engineeringenergy efficiencyta113collaborative mobile cloudscontent distributionta213business.industryQuality of service020206 networking & telecommunications020302 automobile design & engineeringEnergy consumptionUser equipmentMobile telephonybusinessComputer networkEfficient energy useIEEE Journal on Selected Areas in Communications
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AE Aurigae: First detection of non-thermal X-ray emission from a bow shock produced by a runaway star

2012

Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow shocks have been detected in the mid-infrared for several high-mass runaway stars and in radio waves for one star. Theoretical models predict the production of high-energy photons by non-thermal radiative processes in a number sufficiently large to be detected in X-rays. To date, no stellar bow shock has been detected at such energies. We present the first detection of X-ray emission from a bow shock produced by a runaway star. The star is AE Aur, which was likely expelled from its birthplace due to the encounter of two massive binary systems and now is passing through the dense nebula IC 405…

Shock waveAstrofísicaCiencias Astronómicasstars: kinematics and dynamicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-rays: generalISM: cloudsmassive [stars]general [X-rays]Radiative transferISM: clouds radiation mechanisms: non-thermal stars: individual: AE Aur stars: kinematics and dynamics stars: massive X-rays: generalAstrophysics::Solar and Stellar AstrophysicsBow shock (aerodynamics)kinematics and dynamics [stars]Solar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsCosmic dustPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NebulaAstronomy and Astrophysicsradiation mechanisms: non-thermalnon-thermal [radiation mechanisms]Astrophysics - Astrophysics of GalaxiesInterstellar mediumAstronomíastars: individual (AE Aur)stars: massiveStarsindividual (AE Aur) [stars]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaclouds [ISM]Radio wave
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Crushing of interstellar gas clouds in supernova remnants. I. The role of thermal conduction and radiative losses

2005

We model the hydrodynamic interaction of a shock wave of an evolved supernova remnant with a small interstellar gas cloud like the ones observed in the Cygnus loop and in the Vela SNR. We investigate the interplay between radiative cooling and thermal conduction during cloud evolution and their effect on the mass and energy exchange between the cloud and the surrounding medium. Through the study of two cases characterized by different Mach numbers of the primary shock (M = 30 and 50, corresponding to a post-shock temperature $T\approx 1.7\times 10^6$ K and $\approx 4.7\times 10^6$ K, respectively), we explore two very different physical regimes: for M = 30, the radiative losses dominate the…

Shock wavePhysicsCygnus LoopRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsThermal conductionAstrophysicsCoronaSupernovaSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Sciencehydrodynamics shock waves ISM: clouds ISM: supernova remnantsRadiative transferSupernova remnantAstrophysics::Galaxy Astrophysicsclouds ISM: supernova remnants [hydrodynamics shock waves ISM]
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Crushing of interstellar gas clouds in supernova remnants II. X-ray emission

2006

AIMS. We study and discuss the time-dependent X-ray emission predicted by hydrodynamic modeling of the interaction of a SNR shock wave with an interstellar gas cloud. The scope includes: 1) to study the correspondence between modeled and X-ray emitting structures, 2) to explore two different physical regimes in which either thermal conduction or radiative cooling plays a dominant role, and 3) to investigate the effects of the physical processes at work on the emission of the shocked cloud in the two different regimes. METHODS. We use a detailed hydrodynamic model, including thermal conduction and radiation, and explore two cases characterized by different Mach numbers of the primary shock: …

Shock wavePhysicsRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and Astrophysicsshock wavesAstrophysicsRadiationThermal conductionAstrophysicsISM: cloudsCoronaX-rays: ISMShock (mechanics)Supernovasymbols.namesakeMach numberSpace and Planetary SciencehydrodynamicssymbolsAstrophysics::Galaxy AstrophysicsISM: supernova remnants
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Modeling lightning observations from space-based platforms (CloudScat.jl 1.0)

2020

This is an open access article. This work is distributed under the Creative Commons Attribution 4.0 License.

Source codeSoftware_OPERATINGSYSTEMS010504 meteorology & atmospheric sciencesComputer sciencemedia_common.quotation_subjectMultispectral imageReal-time computingCloud computingComputingMilieux_LEGALASPECTSOFCOMPUTINGclouds01 natural sciencesComponent (UML)0103 physical sciencesInternational Space Station010303 astronomy & astrophysics0105 earth and related environmental sciencesmedia_commonHardware_MEMORYSTRUCTURESbusiness.industrylcsh:QE1-996.5scatteringAtmosphärische SpurenstoffeModular designLightninglcsh:GeologySatellitebusinesslightning
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