Search results for "Dual"

showing 10 items of 2547 documents

Quantification of LAI interannual anomalies by adjusting climatological patterns

2011

International audience; Scaling variations and shifts in the timing of seasonal phenology are central features of global change research. In this study, we propose a novel climatology fitting approach to quantify inter-annual anomalies in LAI seasonality. A consistent archive of daily LAI estimates was first derived from historical AVHRR satellite data for the 1981-2000 period over a globally representative sample of sites. The climatology values were then computed by averaging multi-year LAI profiles, gap filling and smoothing to eliminate possible high temporal frequency residual artifacts. The inter-annual variations in LAI were finally quantified by scaling and shifting the seasonal cli…

AVHRR010504 meteorology & atmospheric sciencesPhenology0211 other engineering and technologiesGlobal change02 engineering and technologyAtmospheric modelVegetationclimatology fittingSeasonalityResidualmedicine.disease01 natural sciencesLAIClimatology[SDE]Environmental SciencesmedicineEnvironmental scienceIndex Terms— inter-annual anomaliesTime seriesSmoothing021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensing
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The soil as a reservoir for antagonists to plant diseases

2007

The soil is often considered the milieu providing support for plant roots, water and nutrients for plant growth. But it is also considered a hostile environment harbouring plant pathogenic nematodes, bacteria and fungi. The most common attitude is to try to eliminate the plant pathogenic organisms by biocidal treatments such as methyl bromide fumigation, which are dangerous for man and the environment. Beside this pathogen eradication strategy, another approach to control soil-borne plant diseases consists in studying the plant-pathogen interactions at the cellular and molecular level to create new resistant cultivars or to develop new plant protection products based on elicitation of plant…

Abiotic componentbusiness.industryfungiBiological pest controlFumigationfood and beveragesBiologycomplex mixturesPlant diseaseBiotechnology[SDV.MP]Life Sciences [q-bio]/Microbiology and ParasitologyNutrientAgronomySusceptible individualpathogen eradication strategysoil borne pathogensSoil waterplant pathogenicbusinessPathogen[SDV.MP] Life Sciences [q-bio]/Microbiology and Parasitology
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Progetti di lessicografia onomastica dell’Atlante Linguistico della Sicilia

2022

L’Atlante Linguistico della Sicilia ha adottato, già una decina di anni fa, lo strumento del dizionario-atlante. Quando si è cominciato ad indagare il ricco universo onomastico, se ne è valutata la spendibilità anche su tre diversi corpora orali: uno relativo alle forme popolari del patrimonio toponomastico (DAToS, Dizionario-atlante toponomastico della Sicilia), uno riguardante l’inventario plurale dei soprannomi etnici (DASES, Dizionario-atlante dei soprannomi etnici in Sicilia), l’ultimo afferente al patrimonio antroponomastico popolare, individuale e familiare (DASS, Dizionario-atlante dei soprannomi di/in Sicilia). Il contributo fornisce lo stato dell’arte dei tre progetti e ne descriv…

About ten years ago the Linguistic Atlas of Sicily (ALS) adopted the dictionary-atlas tool. When the rich onomastic universe began to be investigated its use was also evaluated on three different oral corpora: one relating to the popular forms of the toponymic heritage (DAToS Dictionary-toponymic atlas of Sicily) one concerning the plural inventory of ethnic nicknames (DASES Dictionary-atlas of ethnic nicknames in Sicily) the latest afferent to the popular individual and family anthroponomastic heritage (DASS Dictionary-atlas of the nicknames of / in Sicily). The contribution provides the state of the art of the three projects and describes their methods objectives and dissemination tools.Settore L-FIL-LET/12 - Linguistica Italiana
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The large trans-Neptunian object 2002 TC 302 from combined stellar occultation, photometry, and astrometry data

2020

All authors: Ortiz, J. L.; Santos-Sanz, P.; Sicardy, B.; Benedetti-Rossi, G.; Duffard, R.; Morales, N.; Braga-Ribas, F.; Fernández-Valenzuela, E.; Nascimbeni, V.; Nardiello, D.; Carbognani, A.; Buzzi, L.; Aletti, A.; Bacci, P.; Maestripieri, M.; Mazzei, L.; Mikuz, H.; Skvarc, J.; Ciabattari, F.; Lavalade, F. Scarfi, G.; Mari, J. M.; Conjat, M.; Sposetti, S.; Bachini, M.; Succi, G.; Mancini, F.; Alighieri, M.; Dal Canto, E.; Masucci, M.; Vara-Lubiano, M.; Gutiérrez, P. J.; Desmars, J.; Lecacheux, J.; Vieira-Martins, R.; Camargo, J. I. B.; Assafin, M.; Colas, F.; Beisker, W.; Behrend, R.; Mueller, T. G.; Meza, E.; Gomes-Junior, A. R.; Roques, F.; Vachier, F.; Mottola, S.; Hellmich, S.; Campo …

Absolute magnitude010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysicsKuiper belt objects: individual: 2002 TC30201 natural sciencesOccultationlaw.inventionTelescopePhotometry (optics)lawGeometric albedoFísica Aplicada0103 physical sciencesTrans-Neptunian object010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Earth and Planetary Astrophysics (astro-ph.EP)photometric [Techniques]Astronomy and Astrophysicsgeneral [Kuiper belt]Astrometryindividual: 2002 TC302 [Kuiper belt objects]AstrometryAstrometry; Kuiper belt objects: individual: 2002 TC302; Kuiper belt: general; Occultations; Techniques: photometricLight curveSpace and Planetary Science[SDU]Sciences of the Universe [physics]Kuiper belt: generalOccultations[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Techniques: photometricAstrophysics - Earth and Planetary AstrophysicsAstronomy & Astrophysics
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A parametric description of the 3D structure of the Galactic bar/bulge using the VVV survey

2017

We study the structure of the inner Milky Way using the latest data release of the Vista Variables in Via Lactea (VVV) survey. The VVV is a deep near-infrared, multi-colour photometric survey with a coverage of 300 square degrees towards the Bulge/Bar. We use Red Clump (RC) stars to produce a high-resolution dust map of the VVV's field of view. From de-reddened colour-magnitude diagrams we select Red Giant Branch stars to investigate their 3D density distribution within the central 4 kpc. We demonstrate that our best-fit parametric model of the Bulge density provides a good description of the VVV data, with a median percentage residual of 5$\%$ over the fitted region. The strongest of the o…

Absolute magnitudeInitial mass functionastro-ph.GAMilky WayFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: bulgeBulge0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsRed clumpGalaxy: structureAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSLuminosity function (astronomy)Physics010308 nuclear & particles physicsGalactic CenterAstronomyAstronomy and AstrophysicsGalaxy: fundamental parametersAstrophysics - Astrophysics of GalaxiesGalaxy: centregalaxies: individual: Milky WayRed-giant branchSpace and Planetary ScienceGalaxy: formationAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Detection of deuterated molecules, but not of lithium hydride, in the z = 0.89 absorber toward PKS 1830−211

2020

Deuterium and lithium are light elements of high cosmological and astrophysical importance. In this work we report the first detection of deuterated molecules and a search for lithium hydride, 7LiH, at redshift z=0.89 in the spiral galaxy intercepting the line of sight to the quasar PKS1830-211. We used ALMA to observe several submillimeter lines of ND, NH2D, and HDO, and their related isotopomers NH2, NH3, and H2^18O, in absorption against the southwest image of the quasar, allowing us to derive XD/XH abundance ratios. The absorption spectra mainly consist of two distinct narrow velocity components for which we find remarkable differences. One velocity component shows XD/XH abundances that…

Absorption spectroscopyquasarsFOS: Physical scienceschemistry.chemical_elementAstrophysics01 natural scienceschemistry.chemical_compound0103 physical sciencesISM -galaxiesgalaxiesindividual010303 astronomy & astrophysicsLine (formation)Physics[PHYS]Physics [physics]Spiral galaxy010308 nuclear & particles physicsmolecules -radio linesAstronomy and AstrophysicsQuasarAstrophysics - Astrophysics of GalaxiesRedshift3. Good healthPKS 1830−211 -galaxiesabundances -ISMDeuteriumchemistry13. Climate actionSpace and Planetary ScienceLithium hydride[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)Lithium[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorption lines -quasars
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Toward adjustment profiles for lower secondary student-athletes in the Finnish dual career context: A mixed-methods approach

2022

Engagement, burnout, and experiences are central concepts for understanding student-athlete adjustment in a dual career (DC) environment. As part of a larger 3-year, lower secondary sports schools pilot project, the aim of this study was to examine student-athletes’ DC adjustment in Finnish lower secondary sports schools at the end of the second academic year. By combining quantitative and qualitative methods, we sought to (a) identify adjustment profiles among student-athletes based on measures of engagement and burnout in school and sport and (b) to extract experiences that describe the distribution of student-athletes in the profiles. A latent profile analysis using questionnaire data fr…

Academic yearburnoutpragmatismmixed methodsyläkoululaiseteducationSample (statistics)Context (language use)sitoutuminenBurnoutuupumusDual (category theory)Developmental psychologySkills managementurheilu-uranuoretopiskeluTime managementexperiencesPsychologyApplied PsychologyengagementajanhallintaurheilijatQualitative researchPsychology of Sport and Exercise
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Pulsating in Unison at Optical and X-Ray Energies: Simultaneous High Time Resolution Observations of the Transitional Millisecond Pulsar PSR J1023+00…

2019

PSR J1023+0038 is the first millisecond pulsar discovered to pulsate in the visible band; such a detection took place when the pulsar was surrounded by an accretion disk and also showed X-ray pulsations. We report on the first high time resolution observational campaign of this transitional pulsar in the disk state, using simultaneous observations in the optical (TNG, NOT, TJO), X-ray (XMM-Newton, NuSTAR, NICER), infrared (GTC) and UV (Swift) bands. Optical and X-ray pulsations were detected simultaneously in the X-ray high intensity mode in which the source spends $\sim$ 70% of the time, and both disappeared in the low mode, indicating a common underlying physical mechanism. In addition, o…

AccretionAccretion disks-pulsars: Individual (psr j1023+0038)-stars: Neutron-X-rays: Binaries010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaPulsarAccretion discMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsX-rayAstronomy and AstrophysicsTime resolutionAccretion (astrophysics)Space and Planetary ScienceVisible bandAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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UV variability and accretion dynamics in the young open cluster NGC 2264

2015

We explore UV and optical variability signatures for several hundred members of NGC 2264 (3 Myr). We performed simultaneous u- and r-band monitoring over two full weeks with CFHT/MegaCam. About 750 young stars are probed; 40% of them are accreting. Statistically distinct variability properties are observed for accreting and non-accreting cluster members. The accretors exhibit a significantly higher level of variability than the non-accretors, especially in the UV. The amount of u-band variability correlates statistically with UV excess in disk-bearing objects, which suggests that accretion and star-disk interaction are the main sources of variability. Cool magnetic spots, several hundred de…

AccretionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSettore FIS/05 - Astronomia E AstrofisicaStars: low-maAstrophysics::Solar and Stellar Astrophysicsaccretion diskAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Stars: variables: T TauriPhysicsPhotosphereHerbig Ae/BeAstronomy and AstrophysicsAstronomy and AstrophysicUltraviolet: starAccretion (astrophysics)StarsWavelengthAmplitudeAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceOpen clusters and associations: individual: NGC 2264Stars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsOpen cluster
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Broad-band spectral analysis of the accreting millisecond X-ray pulsar SAX J1748.9-2021

2016

We analyzed a 115 ks XMM-Newton observation and the stacking of 8 days of INTEGRAL observations, taken during the raise of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021. The source showed numerous type-I burst episodes during the XMM-Newton observation, and for this reason we studied separately the persistent and burst epochs. We described the persistent emission with a combination of two soft thermal components, a cold thermal Comptonization component (~2 keV) and an additional hard X-ray emission described by a power-law (photon index ~2.3). The continuum components can be associated with an accretion disc, the neutron star (NS) surface and a thermal Compton…

AccretionBinaries - X-rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesIndividualAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicaPulsarSAX J1748.9-2021Millisecond pulsarAccretion discs -X-ray0103 physical sciencesAccretion; Accretion discs -X-rays; Binaries - X-rays; Galaxies -X-rays; Individual; SAX J1748.9-2021; Space and Planetary Science; Astronomy and Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSolar massMillisecondAstronomyAstronomy and AstrophysicsAccretion (astrophysics)Neutron starSpace and Planetary ScienceGalaxies -X-rayEddington luminositysymbolsAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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