Search results for "Planetary Science"

showing 10 items of 4367 documents

SCOPE-Based Emulators for Fast Generation of Synthetic Canopy Reflectance and Sun-Induced Fluorescence Spectra

2017

Progress in advanced radiative transfer models (RTMs) led to an improved understanding of reflectance (R) and sun-induced chlorophyll fluorescence (SIF) emission throughout the leaf and canopy. Among advanced canopy RTMs that have been recently modified to deliver SIF spectral outputs are the energy balance model SCOPE and the 3D models DART and FLIGHT. The downside of these RTMs is that they are computationally expensive, which makes them impractical in routine processing, such as scene generation and retrieval applications. To bypass their computational burden, a computationally effective technique has been proposed by only using a limited number of model runs, called emulation. The idea …

spectroscopy010504 meteorology & atmospheric sciencesComputer sciencesun-induced fluorescence0211 other engineering and technologiesEnergy balanceemulation02 engineering and technology01 natural scienceschemistry.chemical_compoundradiative transfer modellingSCOPERadiative transferlcsh:Sciencescene generationChlorophyll fluorescence021101 geological & geomatics engineering0105 earth and related environmental sciencesEmulationArtificial neural networkFluorescencemachine learningLatin hypercube samplingchemistryChlorophyllGeneral Earth and Planetary Scienceslcsh:QAlgorithmRemote Sensing
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A Decade of GRB Follow-Up by BOOTES in Spain (2003–2013)

2016

This article covers ten years of GRB follow-ups by the Spanish BOOTES stations: 71 follow-ups providing 23 detections. Follow-ups by BOOTES-1B from 2005 to 2008 were given in a previous article and are here reviewed and updated, and additional detection data points are included as the former article merely stated their existence. The all-sky cameras CASSANDRA have not yet detected any GRB optical afterglows, but limits are reported where available.

spectroscopyArticle Subjectlcsh:Astronomy100418AFOS: Physical sciencesgamma-ray burst02 engineering and technology01 natural scienceslcsh:QB1-991emission0103 physical sciences0202 electrical engineering electronic engineering information engineeringpanchromatic observations010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsshooterenergy injectionAstronomyAstronomy and AstrophysicsBOOTEShost-galaxySpace and Planetary Science28 February 1997020201 artificial intelligence & image processingAstrophysics - High Energy Astrophysical PhenomenaafterglowGamma-ray burstAdvances in Astronomy
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Remote Sensing of 3-D Geometry and Surface Moisture of a Peat Production Area Using Hyperspectral Frame Cameras in Visible to Short-Wave Infrared Spe…

2016

Miniaturized hyperspectral imaging sensors are becoming available to small unmanned airborne vehicle (UAV) platforms. Imaging concepts based on frame format offer an attractive alternative to conventional hyperspectral pushbroom scanners because they enable enhanced processing and interpretation potential by allowing for acquisition of the 3-D geometry of the object and multiple object views together with the hyperspectral reflectance signatures. The objective of this investigation was to study the performance of novel visible and near-infrared (VNIR) and short-wave infrared (SWIR) hyperspectral frame cameras based on a tunable Fabry–Pérot interferometer (FPI) in measuring a 3-D digital sur…

spectroscopygeometry010504 meteorology & atmospheric sciencesInfraredspektroskopiata11710211 other engineering and technologiesGeometryradiometry02 engineering and technologyremotely piloted aircraft01 natural scienceskalibrointiremote sensingCalibrationgeographic information systemComputer visionElectrical and Electronic Engineeringta218021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingta113ta213Contextual image classificationbusiness.industryHyperspectral imagingOtaNanocalibrationstereo visionVNIRInterferometryGeneral Earth and Planetary SciencesRGB color modelEnvironmental scienceRadiometrygeometriakaukokartoitusArtificial intelligencebusinessimage classificationIEEE Transactions on Geoscience and Remote Sensing
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Impact of Structural, Photochemical and Instrumental Effects on Leaf and Canopy Reflectance Variability in the 500–600 nm Range

2021

Current rapid technological improvement in optical radiometric instrumentation provides an opportunity to develop innovative measurements protocols where the remote quantification of the plant physiological status can be determined with higher accuracy. In this study, the leaf and canopy reflectance variability in the PRI spectral region (i.e., 500–600 nm) is quantified using different laboratory protocols that consider both instrumental and experimental set-up aspects, as well as canopy structural effects and vegetation photoprotection dynamics. First, we studied how an incorrect characterization of the at-target incoming radiance translated into an erroneous vegetation reflectance spectru…

spectroscopyreflectanceproximal sensing; spectroscopy; protocols; irradiance; reflectance; vegetation index; sun-/shade-adapted leaves; xanthophyll cycleirradianceScienceQGeneral Earth and Planetary Sciencesprotocolsproximal sensingvegetation indexRemote Sensing
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A Long Journey into the Investigation of the Structure–Dynamics–Function Paradigm in Proteins through the Activities of the Palermo Biophysics Group

2022

An overview of the biophysics activity at the Department of Physics and Chemistry Emilio Segrè of the University of Palermo is given. For forty years, the focus of the research has been on the protein structure–dynamics–function paradigm, with the aim of understanding the molecular basis of the relevant mechanisms and the key role of solvent. At least three research lines are identified; the main results obtained in collaboration with other groups in Italy and abroad are presented. This review is dedicated to the memory of Professors Massimo Ugo Palma, Maria Beatrice Palma Vittorelli, and Lorenzo Cordone, which were the founders of the Palermo School of Biophysics. We all have been, directl…

spectroscopywateraggregationGeneral Earth and Planetary SciencesamyloidsimulationsaccharidesSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)General Environmental Science
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Urban Heat Island Monitoring and Impacts on Citizen's General Health Status in Isfahan Metropolis: A Remote Sensing and Field Survey Approach.

2020

Urban heat islands (UHIs) are one of the urban management challenges, especially in metropolises, which can affect citizens’ health and well-being. This study used a combination of remote sensing techniques with field survey to investigate systematically the effects of UHI on citizens’ health in Isfahan metropolis, Iran. For this purpose, the land surface temperature (LST) over a three-year period was monitored by Landsat-8 satellite imagery based on the split window algorithm. Then, the areas where UHI and urban cold island (UCI) phenomena occurred were identified and a general health questionnaire-28 (GHQ-28) was applied to evaluate the health status of 800 citizens in terms o…

split window algorithm010504 meteorology & atmospheric sciencesLand surface temperatureScienceQgeneral health questionnaire-28land surface temperatureurban heat island010501 environmental sciencesField survey01 natural sciencesGeography13. Climate actionRemote sensing (archaeology)Social function11. SustainabilityGeneral Earth and Planetary Sciencesurban heat island; land surface temperature; split window algorithm; general health questionnaire-28; Isfahan metropolisGeneral healthUrban heat islandIsfahan metropolisUrban management0105 earth and related environmental sciencesSocial functioningRemote sensingRemote sensing
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The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

2007

(abridged:) The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) surveys the most populated ~5 square degrees of the Taurus star formation region, using the XMM-Newton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association. Many targets are also studied in the optical, and high-resolution X-ray grating spectroscopy has been obtained for selected bright sources. The X-ray spectra have been coherently analyzed with two different thermal models (2-component thermal model, and a continuous emission measure distribution model). We present ov…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaBrown dwarfFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Observatory0103 physical sciencesProtostarAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsstars : formationStar formationMolecular cloudAstrophysics (astro-ph)Astronomy and AstrophysicsAccretion (astrophysics)Starsgravitational waves13. Climate actionSpace and Planetary ScienceX-rays : star
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Spectral properties of X-ray bright variable sources in the Taurus Molecular Cloud

2006

We analyze 19 bright variable X-ray sources detected in the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), in order to characterize the variations with time of their coronal properties and to derive informations on the X-ray emitting structures. We performed time-resolved spectroscopy of the EPIC PN and MOS spectra of the XEST sources, using a model with one or two thermal components, and we used the time evolution of the temperatures and emission measures during the decay phase of flares to derive the size of the flaring loops. The light curves of the selected sources show different types of variability: flares, long-lasting decay or rise through the whole observation, sl…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaX-rays : starsFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciences7. Clean energySpectral linelaw.inventionlaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSpectroscopy010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsMolecular cloudAstrophysics (astro-ph)Astronomy and Astrophysicsstars : late-typeRadiusPlasmaLight curve13. Climate actionSpace and Planetary Sciencestars : coronaeFlare
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Stochastic gravito-inertial modes discovered by CoRoT in the hot Be star HD 51452

2012

International audience; Context. Be stars are rapidly rotating stars with a circumstellar decretion disk. They usually undergo pressure and/or gravity pulsation modes excited by the κ-mechanism, i.e. an effect of the opacity of iron-peak elements in the envelope of the star. In the Milky Way, p-modes are observed in stars that are hotter than or equal to the B3 spectral type, while g-modes are observed at the B2 spectral type and cooler. Aims. We observed a B0IVe star, HD 51452, with the high-precision, high-cadence photometric CoRoT satellite and high-resolution, ground-based HARPS and SOPHIE spectrographs to study its pulsations in great detail. We also used the lower resolution spectra a…

starsBe -stars010504 meteorology & atmospheric sciencesBe starK-type main-sequence staroscillations -starsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsrotation01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsStellar structureindividual010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences[PHYS]Physics [physics]PhysicsASTROFÍSICA ESTELARStellar rotationFlare starAstronomyAstronomy and AstrophysicsLight curveESPECTROSCOPIAHD 51452 -starsStarsT Tauri star13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsemission-line[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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High Energy Emission and its Variability in Young Stellar Objects

2019

Young stars show a variety of highly energetic phenomena, from accretion and outflow processes to hot coronal plasmas confined in their outer atmosphere, all regulated by the intense stellar magnetic fields. Many aspects on each of these phenomena are debated, but, most notably, their complex mutual interaction remains obscure. In this work I report how these phenomena are simultaneously responsible for the high-energy emission from young stars, with a special focus on the expected and observed variability in the X-ray band. Investigating variations in the X-ray emission from young stars allows us to pose constraints on flare and coronal plasma properties, coronal heating, accretion stream …

starsYoung stellar objectAstrophysics::High Energy Astrophysical PhenomenaMagnetosphereFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionX-raySettore FIS/05 - Astronomia E Astrofisicaaccretionstarlaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicspremain sequenceSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsactivityAstronomy and AstrophysicsPlasmaAccretion (astrophysics)StarsT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceT Tauri starOutflowAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFlare
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