Search results for "Instrumentation"

showing 10 items of 4914 documents

IPHAS-selected classical Be stars

2016

We present a semi-automatic procedure to obtain fundamental physical parameters and distances of classical Be (CBe) stars, based on the Barbier-Chalonge-Divan (BCD) spectrophotometric system. Our aim is to apply this procedure to a large sample of CBe stars detected by the IPHAS photometric survey, to determine their fundamental physical parameters and to explore their suitability as galactic structure tracers. In this paper we describe the methodology used and the validation of the procedure by comparing our results with those obtained from different independent astrophysical techniques for subsamples of stars in common with other studies. We also present a test case study of the galactic …

Early type starsAstrophysics and AstronomyPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsStellar distanceAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science::Digital Librariesobservational astronomyStellar AstronomyEarly-type starsBe starsAstrophysics::Solar and Stellar AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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Be stars in the exofield of CoRoT. II.

2018

The class of Be stars are the epitome of rapid rotators in the main sequence. These stars are privileged candidates for studying the incidence of rotation on the stellar internal structure and on non-radial pulsations. Pulsations are considered possible mechanisms to trigger mass-ejection phenomena required to build up the circumstellar disks of Be stars. Time series analyses of the light curves of 15 faint Be stars observed with the CoRoT satellite were performed to obtain the distribution of non-radial pulsation (NRP) frequencies in their power spectra at epochs with and without light outbursts and to discriminate pulsations from rotation-related photometric variations. Standard Fourier t…

Early type starsAstrophysics and AstronomyStellar AstronomyEarly-type starsBe starsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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Système distribué d'alerte de la qualité de l'eau pour la rivière Mudan basé sur l'EFDC et les SIG

2016

Simulation and Early Warning System (SEWS) is a powerful tool for river water quality monitoring. Mudan River, an important river in northeastern cold regions of China, can run out of China into Russia. Thus, the water quality of Mudan River is highly concerned not only locally andregionally but also internationally. Objective of this study is to establish an excellent SEWS of water quality so that the spatio-temporal distribution of water quality in both open-water and ice-covered periods can be accurately simulated and visualized to understand the spatial variation of pollutants along the river course. The dissertation is structured into 7 chapters, chapter 1 outlines the background of th…

Early warningModèle hydrodynamiquePréavis d'alerteCalcul distribuéGISSIGScenario analysisWater qualityAnalyse de scénariosTwo-dimensional simulationSimulation bidimensionnelleDistributed computationHydrodynamic modelQualité de l'eau[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det][SDU.STU.HY]Sciences of the Universe [physics]/Earth Sciences/Hydrology
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Walking on exoplanets: Is Star Wars right?

2016

As the number of detected extrasolar planets increases, exoplanet databases become a valuable resource, confirming some details about planetary formation, but also challenging our theories with new unexpected properties.

Earth and Planetary Astrophysics (astro-ph.EP)010504 meteorology & atmospheric sciencesExtraterrestrial EnvironmentComputer scienceMotion PicturesAstrophysics::Instrumentation and Methods for AstrophysicsPlanetsFOS: Physical sciencesWalkingStar (graph theory)01 natural sciencesAgricultural and Biological Sciences (miscellaneous)ExoplanetAstrobiologySpace and Planetary Science0103 physical sciencesExobiologyAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysics0105 earth and related environmental sciencesGravitationAstrophysics - Earth and Planetary Astrophysics
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Hiding in plain sight: observing planet-starspot crossings with the James Webb Space Telescope

2021

Transiting exoplanets orbiting active stars frequently occult starspots and faculae on the visible stellar disc. Such occultations are often rejected from spectrophotometric transits, as it is assumed they do not contain relevant information for the study of exoplanet atmopsheres. However, they can provide useful constraints to retrieve the temperature of active features and their effect on transmission spectra. We analyse the capabilities of the James Webb Space Telescope in the determination of the spectra of occulted starspots, despite its lack of optical wavelength instruments on board. Focusing on K and M spectral types, we simulate starspots with different temperatures and in differen…

Earth and Planetary Astrophysics (astro-ph.EP)PhysicsJames Webb Space TelescopeStarspotAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsStellar classificationExoplanetStarsWavelengthAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePlanetAstrophysics::Solar and Stellar AstrophysicsPrismAstrophysics::Earth and Planetary AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstrophysics - Earth and Planetary Astrophysics
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A network of precision gravimeters as a detector of matter with feeble nongravitational coupling

2019

Hidden matter that interacts only gravitationally would oscillate at characteristic frequencies when trapped inside of Earth. For small oscillations near the center of the Earth, these frequencies are around 300 $\mu$Hz. Additionally, signatures at higher harmonics would appear because of the non-uniformity of Earth's density. In this work, we use data from a global network of gravimeters of the International Geodynamics and Earth Tide Service (IGETS) to look for these hypothetical trapped objects. We find no evidence for such objects with masses on the order of 10$^{14}$ kg or greater with an oscillation amplitude of 0.1 $r_e$. It may be possible to improve the sensitivity of the search by…

Earth and Planetary Astrophysics (astro-ph.EP)Physics::Space PhysicsFOS: Physical sciencesAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics - Earth and Planetary AstrophysicsPhysics::Geophysics
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A Survey on Gaussian Processes for Earth-Observation Data Analysis: A Comprehensive Investigation

2016

Gaussian processes (GPs) have experienced tremendous success in biogeophysical parameter retrieval in the last few years. GPs constitute a solid Bayesian framework to consistently formulate many function approximation problems. This article reviews the main theoretical GP developments in the field, considering new algorithms that respect signal and noise characteristics, extract knowledge via automatic relevance kernels to yield feature rankings automatically, and allow applicability of associated uncertainty intervals to transport GP models in space and time that can be used to uncover causal relations between variables and can encode physically meaningful prior knowledge via radiative tra…

Earth observation010504 meteorology & atmospheric sciencesGeneral Computer Science0211 other engineering and technologies02 engineering and technologycomputer.software_genre01 natural sciencesField (computer science)Kernel (linear algebra)symbols.namesakeAtmospheric radiative transfer codesElectrical and Electronic EngineeringInstrumentationGaussian process021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingbusiness.industryHyperspectral imagingFunction approximationsymbolsGlobal Positioning SystemGeneral Earth and Planetary SciencesData miningbusinesscomputerIEEE Geoscience and Remote Sensing Magazine
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Soil Water Content Assessment: Critical Issues Concerning the Operational Application of the Triangle Method

2015

Knowledge of soil water content plays a key role in water management efforts to improve irrigation efficiency. Among the indirect estimation methods of soil water content via Earth Observation data is the triangle method, used to analyze optical and thermal features because these are primarily controlled by water content within the near-surface evaporation layer and root zone in bare and vegetated soils. Although the soil-vegetation-atmosphere transfer theory describes the ongoing processes, theoretical models reveal limits for operational use. When applying simplified empirical formulations, meteorological forcing could be replaced with alternative variables when the above-canopy temperatu…

Earth observationIrrigationAtomic and Molecular Physics and OpticComputer scienceEvaporationAirborne remote sensing; Soil moisture; Triangle method; Electrical and Electronic Engineering; Atomic and Molecular Physics and Optics; Analytical Chemistry; BiochemistrySoil sciencelcsh:Chemical technologyBiochemistryVineyardArticleAnalytical Chemistrytriangle methodStatisticsThermallcsh:TP1-1185Electrical and Electronic EngineeringInstrumentationWater contentSettore ICAR/02 - Costruzioni Idrauliche E Marittime E IdrologiaAerodynamicsAtomic and Molecular Physics and Opticsairborne remote sensingSoil watersoil moistureSettore ICAR/06 - Topografia E CartografiaSensors
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Irradiation-induced damage in porous low-k materials during low-energy heavy-ion elastic recoil detection analysis

2006

Abstract With the implementation of time-of-flight elastic recoil detection (ToF-ERD) for the analysis of thin films with high depth resolution using a standard ‘low-energy’ accelerator, routine application of ERD in semiconductor technology becomes possible. In case of irradiation-sensitive materials, like organosilicate low- k films, the energetic incident beam damages the sample during the measurement, resulting in loss of the lighter elements and, as a consequence, altering the sample composition. The ion beam induced damage is investigated for 19 F, 35 Cl, 63 Cu, 79 Br and 127 I beams at energies of 6–16 MeV and typical fluences for ERD analysis. By means of Fourier transform infrared …

Elastic recoil detectionNuclear and High Energy PhysicsIon beamInfraredChemistryAnalytical chemistryIrradiationFourier transform infrared spectroscopyThin filmSpectroscopyInstrumentationBeam (structure)Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Considerations about multiple and plural scattering in heavy-ion low-energy ERDA

2009

Abstract Low-energy heavy-ion Elastic Recoil Detection Analysis (ERDA) is becoming a mature technique for high-resolution characterization of thin films, i.e. below 50 nm thickness. In combination with a small tandem accelerator (∼2 MV terminal voltage) and beam energies below 20 MeV, it is suitable for routine analysis of key materials in semiconductor technology. At low-energies, however, small angle multiple scattering and large angle plural scattering of ions play a significant role, starting from the first nanometers. Multiple and plural scattering dominate the depth resolution deterioration with increasing depth and, when glancing angles are used, introduce long tails in the elemental…

Elastic recoil detectionNuclear and High Energy PhysicsRecoilScatteringChemistryMonte Carlo methodThin filmAtomic physicsInstrumentationBeam (structure)Characterization (materials science)IonNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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