Search results for "PLANE"

showing 10 items of 6821 documents

The Gaia-ESO Survey: The inner disk, intermediate-age open cluster Trumpler 23

2017

Full list of authors: Overbeek, J. C.; Friel, E. D.; Donati, P.; Smiljanic, R.; Jacobson, H. R.; Hatzidimitriou, D.; Held, E. V.; Magrini, L.; Bragaglia, A.; Randich, S.; Vallenari, A.; Cantat-Gaudin, T.; Tautvaišienė, G.; Jiménez-Esteban, F.; Frasca, A.; Geisler, D.; Villanova, S.; Tang, B.; Muñoz, C.; Marconi, G. Carraro, G.; San Roman, I.; Drazdauskas, A.; Ženovienė, R.; Gilmore, G.; Jeffries, R. D.; Flaccomio, E.; Pancino, E.; Bayo, A.; Costado, M. T.; Damiani, F.; Jofré, P.; Monaco, L.; Prisinzano, L.; Sousa, S. G.; Zaggia, S.

open clusters and associations: individual: Trumpler 23stars: abundancesMetallicityFOS: Physical sciencesGalaxy: abundances; Galaxy: disk; Galaxy: formation; Open clusters and associations: individual: Trumpler 23; Stars: abundances; Astronomy and Astrophysics; Space and Planetary ScienceAstrophysics01 natural sciencesGalaxy: diskPhotometry (optics)0103 physical sciencesGalaxy formation and evolutionDisc010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QBPhysics010308 nuclear & particles physicsabundances [Galaxy]Astronomy and AstrophysicsGalactic planeAstrophysics - Astrophysics of GalaxiesRadial velocityStarsindividual: Trumpler 23 [Open clusters and associations]Astrophysics - Solar and Stellar Astrophysicsformation [Galaxy]Space and Planetary ScienceGalaxy: formationAstrophysics of Galaxies (astro-ph.GA)abundances [Stars]Galaxy: abundancesdisk [Galaxy]Open cluster
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Solar radiative effects of a Saharan dust plume observed during SAMUM assuming spheroidal model particles

2011

The solar optical properties of Saharan mineral dust observed during the Saharan Mineral Dust Experiment (SAMUM) were explored based on measured size-number distributions and chemical composition. The size-resolved complex refractive index of the dust was derived with real parts of 1.51–1.55 and imaginary parts of 0.0008–0.006 at 550 nm wavelength. At this spectral range a single scattering albedo ω o and an asymmetry parameter g of about 0.8 were derived. These values were largely determined by the presence of coarse particles. Backscatter coefficients and lidar ratios calculated with Mie theory (spherical particles) were not found to be in agreement with independently measured lidar data.…

optical propertiesAtmospheric Scienceradiative transfer simulationsMaterials sciencespectral radiative flux densities010504 meteorology & atmospheric sciencesSingle-scattering albedospheroidal aerosol particlesMie scatteringAtmosphärische SpurenstoffeMineralogy010501 environmental sciencesMineral dustAtmosphärenprozessoren01 natural sciencesComputational physicsSaharan mineral dustExtinction (optical mineralogy)Radiative transferParticlescattering databaseParticle sizeAstrophysics::Earth and Planetary AstrophysicsOptical depth0105 earth and related environmental sciencesTellus B
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Optimal Spectral Wavelengths for Discriminating Orchard Species Using Multivariate Statistical Techniques

2019

Sustainable management of orchard fields requires detailed information about the tree types, which is a main component of precision agriculture programs. To this end, hyperspectral imagery can play a major role in orchard tree species mapping. Efficient use of hyperspectral data in combination with field measurements requires the development of optimized band selection strategies to separate tree species. In this study, field spectroscopy (350 to 2500 nm) was performed through scanning 165 spectral leaf samples of dominant orchard tree species (almond, walnut, and grape) in Chaharmahal va Bakhtiyari province, Iran. Two multivariable methods were employed to identify the optimum wavelengths:…

optimal spectral wavelengths010504 meteorology & atmospheric sciences0211 other engineering and technologiesRed edge02 engineering and technologyfield spectroscopy; orchards species; ANOVA–RFC–PCA; PLS; optimal spectral wavelengths; discriminant analysis01 natural sciencesPartial least squares regressionlcsh:Science021101 geological & geomatics engineering0105 earth and related environmental sciencesMathematicsRemote sensinganova–rfc–pcaorchards speciesNear-infrared spectroscopyHyperspectral imaging15. Life on landplsLinear discriminant analysisdiscriminant analysisfield spectroscopyRandom forestTree (data structure)Principal component analysisGeneral Earth and Planetary Scienceslcsh:QRemote Sensing
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STUDIES OF VARIABILITY IN PROTO-PLANETARY NEBULAE. II. LIGHT AND VELOCITY CURVE ANALYSES OF IRAS 22272+5435 AND 22223+4327

2013

We have carried out a detailed observational study of the light, color, and velocity variations of two bright, carbon-rich proto-planetary nebulae, IRAS 22223+4327 and 22272+5435. The light curves are based upon our observations from 1994 to 2011, together with published data by Arkhipova and collaborators. They each display four significant periods, with primary periods for IRAS 22223+4327 and 22272+5435 being 90 and 132 days, respectively. For each of them, the ratio of secondary to primary period is 0.95, a value much different from that found in Cepheids, but which may be characteristic of post-asymptotic giant branch (AGB) stars. Fewer significant periods are found in the smaller radia…

oscillations [stars]Cepheid variableFOS: Physical sciencesAstrophysics01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsgeneral [planetary nebulae]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsGalaxy rotation curvePhysicsNebula010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveAGB and post-AGB [stars]Planetary nebulaRadial velocityStarsAmplitudeAstrophysics - Solar and Stellar Astrophysicsvariables: general [stars]Space and Planetary Scienceindividual (IRAS 22223+4327 IRAS 22272+5435) [stars]Astrophysics::Earth and Planetary AstrophysicsThe Astrophysical Journal
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Pulsating B and Be stars in the Small Magellanic Cloud

2008

Context: Stellar pulsations in main-sequence B-type stars are driven by the kappa-mechanism due to the Fe-group opacity bump. The current models do not predict the presence of instability strips in the B spectral domain at very low metallicities. As the metallicity of the SMC is lower than Z=0.005, it constitutes a very suitable object to test these predictions. Aims: The main objective is to investigate the existence of B-type pulsators at low metallicities, searching for short-term periodic variability in absorption-line B and Be stars in the SMC. The analysis has been performed in a sample of 313 B and Be stars with fundamental astrophysical parameters accurately determined from high-res…

oscillations [stars]statistics [Stars]Be starHertzsprung–Russell diagramMetallicityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesStars : emission-line Be; stars : oscillations; Stars : early-type; Stars : statistics; Galaxies : Magellanic Cloudssymbols.namesakeMagellanic Clouds [Galaxies]early-type [Stars]0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstrophysics (astro-ph)Astronomy and AstrophysicsLight curveGalaxy:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Stars13. Climate actionSpace and Planetary Scienceemission-line Be [Stars]symbolsSmall Magellanic CloudAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasInstability strip:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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Fixed Angle Inverse Scattering for Almost Symmetric or Controlled Perturbations

2020

We consider the fixed angle inverse scattering problem and show that a compactly supported potential is uniquely determined by its scattering amplitude for two opposite fixed angles. We also show that almost symmetric or horizontally controlled potentials are uniquely determined by their fixed angle scattering data. This is done by establishing an equivalence between the frequency domain and the time domain formulations of the problem, and by solving the time domain problem by extending the methods of [RS19] which adapts the ideas introduced in [BK81] and [IY01] on the use of Carleman estimates for inverse problems.

osittaisdifferentiaaliyhtälötApplied MathematicsMathematical analysisscattering amplitudePlane waveFOS: Physical sciencesplane waveMathematical Physics (math-ph)fixed angleinverse scattering01 natural sciencesinversio-ongelmat010101 applied mathematicsScattering amplitudeComputational MathematicsFixed angleMathematics - Analysis of PDEsInverse scattering problemFOS: Mathematics0101 mathematicsAnalysisMathematical PhysicsMathematicsAnalysis of PDEs (math.AP)
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Uniqueness of positive solutions to some Nonlinear Neumann Problems

2017

Using the moving plane method, we obtain a Liouville type theorem for nonnegative solutions of the Neumann problem ⎧ ⎨ ⎩ div (ya∇u(x, y)) = 0, x ∈ Rn,y > 0, lim y→0+yauy(x, y) = −f(u(x, 0)), x ∈ Rn, under general nonlinearity assumptions on the function f : R → R for any constant a ∈ (−1, 1). peerReviewed

osittaisdifferentiaaliyhtälötLiouville type theoremNeumann problemmoving plane method
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Stationary sets and asymptotic behavior of the mean curvature flow with forcing in the plane

2020

We consider the flat flow solutions of the mean curvature equation with a forcing term in the plane. We prove that for every constant forcing term the stationary sets are given by a finite union of disks with equal radii and disjoint closures. On the other hand for every bounded forcing term tangent disks are never stationary. Finally in the case of an asymptotically constant forcing term we show that the only possible long time limit sets are given by disjoint unions of disks with equal radii and possibly tangent. peerReviewed

osittaisdifferentiaaliyhtälötMathematics - Analysis of PDEsforced mean curvature flowFOS: Mathematicsstationary setscritical setsGeometry and TopologyAstrophysics::Earth and Planetary Astrophysicslarge time behaviorAnalysis of PDEs (math.AP)
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Nonlinear Liouville Problems in a Quarter Plane

2016

We answer affirmatively the open problem proposed by Cabr\'e and Tan in their paper "Positive solutions of nonlinear problems involving the square root of the Laplacian" (see Adv. Math. {\bf 224} (2010), no. 5, 2052-2093).

osittaisdifferentiaaliyhtälötPlane (geometry)General MathematicsOpen problemta111010102 general mathematicsMathematical analysis35B09 35B53 35J60Quarter (United States coin)01 natural sciencesNonlinear systemMathematics - Analysis of PDEsSquare root0103 physical sciencesFOS: Mathematicspartial differential equations010307 mathematical physics0101 mathematicsLaplace operatorAnalysis of PDEs (math.AP)MathematicsInternational Mathematics Research Notices
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Natural Halogen Emissions to the Atmosphere: Sources, Flux, and Environmental Impact

2022

Understanding the atmospheric geochemical cycle of both natural and anthropogenic halogens is important because of the detrimental effect halogens have on the environment, notably on tropospheric and stratospheric ozone. Oceans are the primary natural source for atmospheric Cl, F, Br, and I, but anthropogenic emissions are still important, especially for Cl. While emissions of human-made halocarbons (e.g., chlorofluorocarbons or CFCs) are expected to continue to decrease allowing progressive stratospheric ozone recovery, volcanic activity (e.g., clusters of mid-scale explosive eruptions or large-scale explosive eruptions) might disturb this recovery over the next decades. This review provid…

ozone depletionmethyl halidesvolcanic gasesGeochemistry and Petrologybrominevery-short lived substancesEarth and Planetary Sciences (miscellaneous)oceansElements
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