Search results for "PLANE"

showing 10 items of 6821 documents

El reto de la competitividad y sostenibilidad para los destinos turísticos

2015

Desde la segunda mitad del siglo pasado, la actividad turística ha ido ganando peso entre las actividades productivas de países y regiones a escala mundial. Aunque tradicionalmente se ha identificado el crecimiento económico con la expansión de la industria, ya en las últimas décadas del siglo XX la actividad turística se consolidó como un sector productivo más, con capacidad para generar empleo y renta. Las características de esta actividad permiten que se desarrolle, con mayor o menos intensidad y éxito, en áreas excluidas de la expansión de la actividad industrial. Es más, se ha convertido en una oportunidad para áreas castigadas por la desindustrialización y en una actividad complementa…

General Earth and Planetary SciencesTurismolcsh:H1-99Competitividadlcsh:Social sciences (General)SostenibilidadGeneral Environmental ScienceESPACIO I+D: Innovación más Desarrollo
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Revising midlatitude summer temperatures back to A.D. 600 based on a wood density network

2015

Annually resolved and millennium-long reconstructions of large-scale temperature variability are primarily composed of tree ring width (TRW) chronologies. Changes in ring width, however, have recently been shown to bias the ratio between low- and high-frequency signals. To overcome limitations in capturing the full spectrum of past temperature variability, we present a network of 15 maximum latewood density (MXD) chronologies distributed across the Northern Hemisphere extratropics. Independent subsets of continental-scale records consistently reveal high MXD before 1580 and after 1910, with below average values between these periods. Reconstructed extratropical summer temperatures reflect n…

Northern HemisphereTree ringsClimate changeG Geography (General)Dendroclimatology3rd-DASAtmospheric sciencesAtmosphereMaximum latewood densityVolcanic coolingGeophysicsMillennial reconstructionMiddle latitudesClimatologyPaleoclimatologyG1Extratropical cycloneDendrochronologyLittle Ice AgeGeneral Earth and Planetary SciencesBeta valueGeology
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Comparison of Crop Trait Retrieval Strategies Using UAV-Based VNIR Hyperspectral Imaging.

2021

Hyperspectral cameras onboard unmanned aerial vehicles (UAVs) have recently emerged for monitoring crop traits at the sub-field scale. Different physical, statistical, and hybrid methods for crop trait retrieval have been developed. However, spectra collected from UAVs can be confounded by various issues, including illumination variation throughout the crop growing season, the effect of which on the retrieval performance is not well understood at present. In this study, four retrieval methods are compared, in terms of retrieving the leaf area index (LAI), fractional vegetation cover (fCover), and canopy chlorophyll content (CCC) of potato plants over an agricultural field for six dates duri…

Canopystatistical method010504 meteorology & atmospheric sciencesScience0211 other engineering and technologiesGrowing season02 engineering and technologyLUT-based inversion; hybrid method; statistical method; leaf area index; fractional vegetation cover; canopy chlorophyll content01 natural sciencesLUT-based inversionhybrid methodLeaf area index021101 geological & geomatics engineering0105 earth and related environmental sciencesMathematicsRemote sensingfractional vegetation coverleaf area indexQHyperspectral imagingcanopy chlorophyll contentStatistical modelRandom forestVNIRGeneral Earth and Planetary SciencesScale (map)Remote sensing
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Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe–Metis/Solar Orbiter Observations

2022

Abstract The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in combination with the remote-sensing observation of the coronal source region provided by the METIS coronagraph aboard Solar Orbiter. The coronal outflows observed near the ecliptic by Metis on 2021 January 17 at 16:30 UT, between 3.5 and 6.3 R ⊙ above the eastern solar limb, can be associated with the streams sampled by PSP at 0.11 and 0.26 au from the Sun, in two time intervals almost 5 days apart. The two plasma flows come from two distinct source regions, characterized by different magnetic field polarity and intensity at the coronal base. It follows that both the global and local p…

Magnetohydrodynamics (694)Settore FIS/05 - Astronomia E AstrofisicaAstronomi astrofysik och kosmologiSpace and Planetary ScienceSolar corona (1483)Space plasmas (1544)Solar wind (1534)Interplanetary turbulence (830)Astronomy Astrophysics and CosmologyAstronomy and AstrophysicsAlfven waves (23)Heliosphere (711)
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Pressure Shift and Gravitational Red Shift of Balmer Lines in White Dwarfs. Rediscussion

2015

The Stark-induced shift and asymmetry, the so-called pressure shift (PS) of $H_\alpha$ and $H_\beta$ Balmer lines in spectra of DA white dwarfs (WDs), as masking effects in measurements of the gravitational red shift in WDs, have been examined in detail. The results are compared with our earlier ones from before a quarter of a century (Grabowski et al. 1987, hereafter ApJ'87; Madej and Grabowski 1990). In these earlier papers, as a dominant constituent of the Balmer-line-profiles, the standard, symmetrical Stark line profiles, shifted as the whole by PS-effect, were applied to all spectrally active layers of the WD atmosphere. At present, in each of the WD layers, the Stark-line-profiles (e…

Physicsatomic processes; line: formation; line: profiles; plasmas; white dwarfsmedia_common.quotation_subjectFOS: Physical sciencesBalmer seriesWhite dwarfAstronomy and AstrophysicsAstrophysicsPlasmaAsymmetrySpectral linesymbols.namesakeStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencesymbolsSolar and Stellar Astrophysics (astro-ph.SR)Line (formation)media_commonGravitational redshift
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Effects of tilling methods on soil penetration resistance, organic carbon and water stable aggregates in a vineyard of semiarid Mediterranean environ…

2018

Tillage, especially in semiarid Mediterranean environment, enhances the mineralization process of soil organic matter (SOM) and, in turn, decreases aggregate stability. Furthermore, continuous tillage leads to the formation of plough pan beneath the tilled layer. In the present study, we investigated the effect of an innovative self-propelled machine (spading machine, SM) for shallow tillage on SOM, water stable aggregates (WSA) and soil penetration resistance (PR). Such effects were compared to those of chisel plough (CP), rotary tiller (RT) and no tillage (NT). Each tilling method was applied up to a depth of 15 cm, whereas in NT only a brush cutter was used for weed control. Soil analyse…

business.product_categorySettore AGR/13 - Chimica AgrariaSoil Science010501 environmental sciences01 natural sciencesVineyardPloughChisel· Spading machine&nbspEnvironmental ChemistryWater content0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and TechnologyTotal organic carbonGlobal and Planetary ChangeSoil organic matter· Plough pan&nbspSettore AGR/09 - Meccanica AgrariaGeology04 agricultural and veterinary sciencesMineralization (soil science)PollutionTillageAgronomy· Water content040103 agronomy & agriculture0401 agriculture forestry and fisheriesTilling method&nbspbusiness
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MICROLENSING OF QUASAR ULTRAVIOLET IRON EMISSION

2013

We measure the differential microlensing of the UV Fe II and Fe III emission line blends between 14 quasar image pairs in 13 gravitational lenses. We find that the UV iron emission is strongly microlensed in four cases with amplitudes comparable to that of the continuum. Statistically modeling the magnifications, we infer a typical size of r{sub s}∼4√(M/M{sub ⊙}) light-days for the Fe line-emitting regions, which is comparable to the size of the region generating the UV continuum (∼3-7 light-days). This may indicate that a significant part of the UV Fe II and Fe III emission originates in the quasar accretion disk.

PhysicsAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)Astronomy and AstrophysicsQuasarAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsmedicine.disease_causeGravitational microlensing01 natural sciencesGravitationAmplitudeAccretion discSpace and Planetary Science0103 physical sciencesmedicineEmission spectrum010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsUltravioletThe Astrophysical Journal
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Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave

2017

Multiwavelength monitoring of Be/X-ray binaries is crucial to understand the mechanisms producing their outbursts. H 1145-619 is one of these systems, which has recently displayed X-ray activity. We investigate the correlation between the optical emission and the X-ray activity to predict the occurrence of new X-ray outbursts from the inferred state of the circumstellar disc. We have performed a multiwavelength study of H 1145-619 from 1973 to 2017 and present here a global analysis of its variability over the last 40 years. We have used optical spectra from the SAAO, SMARTS and SALT telescopes and optical photometry from INTEGRAL/OMC and ASAS. We also used X-ray observations from INTEGRAL/…

BrightnessBe starAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectX-ray binarystars: emission-lineFOS: Physical sciencesAstrophysics01 natural sciencesSpectral lineDensity wave theoryPhotometry (optics)X-rays: binariesstars: neutrontechniques: photometric0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsBeAstronomy and AstrophysicsLight curvestars: emission-line BeAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceSkyAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenatechniques: spectroscopicAstronomy & Astrophysics
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Joule heating and the thermal evolution of old neutron stars

1998

We consider Joule heating caused by dissipation of the magnetic field in the neutron star crust. This mechanism may be efficient in maintaining a relatively high surface temperature in very old neutron stars. Calculations of the thermal evolution show that, at the late evolutionary stage ($t \geq 10$ Myr), the luminosity of the neutron star is approximately equal to the energy released due to the field dissipation and is practically independent of the atmosphere models. At this stage, the surface temperature can be of the order of $3 \times 10^{4} - 10^{5}$K. Joule heating can maintain this high temperature during extremely long time ($\geq 100$ Myr), comparable with the decay time of the m…

PhysicsField (physics)Astrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsDissipationAstrophysicsLuminosityMagnetic fieldNeutron starSpace and Planetary ScienceThermalAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsMagnetohydrodynamicsJoule heatingAstrophysics::Galaxy Astrophysics
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The Gaia-ESO Survey: The origin and evolution of s-process elements

2018

Context. Several works have found an increase of the abundances of the s-process neutron-capture elements in the youngest Galactic stellar populations. These trends provide important constraints on stellar and Galactic evolution and they need to be confirmed with large and statistically significant samples of stars spanning wide age and distance intervals. Aims. We aim to trace the abundance patterns and the time evolution of five s-process elements - two belonging to the first peak, Y and Zr, and three belonging to the second peak, Ba, La, and Ce - using the Gaia-ESO IDR5 results for open clusters and disc stars. Methods. From the UVES spectra of cluster member stars, we determined the ave…

astro-ph.GAMetallicityFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: diskAstronomi astrofysik och kosmologiAbundance (ecology)QB4600103 physical sciencesAstronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar AstrophysicsDisc010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsgeneral [Open clusters and associations][SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsOpen clusters and associations: generalAstrophysics - Astrophysics of GalaxiesStarsAbundances [Galaxy][SDU]Sciences of the Universe [physics]13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesAstrophysics::Earth and Planetary AstrophysicsDisk [Galaxy]s-processOpen cluster
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