Search results for "Planet"

showing 10 items of 5662 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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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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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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Reliability of Frail and Barthel Tests for Detecting Frailty in Palliative Oncological Patients in a Home Hospitalization Unit: A Comparative Study.

2022

Cancer is a condition that can increase the risk of frailty. In addition, palliative oncological patients in home hospitalization can find their activities of daily living affected. The main objective was to measure the degree of frailty in the oncological population in home hospitalization comparing Barthel and Frail-VIG Indexes. This is a descriptive cross-sectional study. A sample of oncological patients in home hospitalization (n = 50) that included 27 men and 23 women were recruited, and disability due to frailty was measured using the VIG frailty index and the Barthel scale for Activities of Daily Living (ADLs). Spearman’s correlation coefficients were categorized as weak (rs &l…

palliative carePaliative careFrailtyHospitalització domiciliàriafrailty; palliative care; cancer; home care; frail-VIG indexPaleontologyCáncerCuidados en casaCuidados paliativosHome careGeneral Biochemistry Genetics and Molecular BiologyOncologíaSpace and Planetary ScienceFrail-VIG indexTractament pal·liatiuÍndice VIG de vulnerabilidadEnfermeríaCàncer Pacientshuman activitiesVulnerabilidadEcology Evolution Behavior and SystematicsCancerLife (Basel, Switzerland)
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The Palliative Care in the Metastatic Spinal Tumors. A Systematic Review on the Radiotherapy and Surgical Perspective

2022

Spine represents the most common site for metastatic disease involvement. Due to the close relationship between the spinal cord and critical structures, therapeutic management of spinal metastases remains challenging. Spinal localization can lead to neurological sequelae, which can significantly affect the quality of life in patients with a limited life expectancy. The authors conducted a systematic literature review according to PRISMA guidelines in order to determine the impact of the most updated palliative care on spinal metastases. The initial literature search retrieved 2526 articles, manually screened based on detailed exclusion criteria. Finally, 65 studies met the inclusion criteri…

palliative carequality of lifespinal metastasisSpace and Planetary Sciencespinal cord stimulationSettore MED/27 - NeurochirurgiaPaleontologyradiofrequency ablationGeneral Biochemistry Genetics and Molecular BiologyEcology Evolution Behavior and Systematicsradiotherapyvertebral augmentation
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Gravity-derived Moho map for Latvia

2020

A precise understanding of crustal structure is essential to the fields of geodynamics, seismology and certain branches of geophysics. A boundary between the crust and the mantle is known as the MohoroviÄiÄ discontinuity, simply referred to as the âMohoâ. Moho geometry and depth have been extensively studied in Europe, but there are still regions with little information about it. One such area is the northern Baltics, Latvia in particular. So far, only one seismic refraction profile, spanning from Sovetsk (Kaliningrad) to Kohtla-Järve (Estonia), has been used to study the deep structure of the Earth in Latvia. We propose gravity inversion (ParkerâOldenburg algorithm) to gain more insight i…

parker–oldenburg inversionGravity (chemistry)biologyMoholcsh:QE1-996.5mohorovičić discontinuitylatviaGeodesybiology.organism_classificationcrustal thickness.lcsh:Geologygravity dataGeneral Earth and Planetary SciencesGeologyWater Science and TechnologyEstonian Journal of Earth Sciences
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