Search results for "Ala"

showing 10 items of 18976 documents

Highly Anisotropic Rhenium(IV) Complexes: New Examples of Mononuclear Single-Molecule Magnets

2013

The rhenium(IV) complex (NBu4)2[ReBr4(ox)] (1) (ox = oxalate and NBu4(+) = tetra-n-butylammonium cation) has been prepared and its crystal structure determined by X-ray diffraction. The structure is made up of discrete [ReBr4(ox)](2-) anions and bulky NBu4(+) cations. Each [ReBr4(ox)](2-) anion is surrounded by six NBu4(+) cations, which preclude any significant intermolecular contact between the anionic entities, the shortest rhenium···rhenium distance being 9.373(1) Å. Variable temperature dc and ac magnetic susceptibility measurements and field-dependent magnetization experiments on polycrystalline samples of 1 reveal the occurrence of highly anisotropic magnetically isolated Re(IV) cent…

010405 organic chemistryRelaxation (NMR)Inorganic chemistrychemistry.chemical_elementGeneral ChemistryCrystal structureRhenium010402 general chemistry01 natural sciencesBiochemistryMagnetic susceptibilityCatalysisOxalate3. Good health0104 chemical sciencesMagnetizationchemistry.chemical_compoundCrystallographyColloid and Surface ChemistrychemistryMolecule[PHYS.COND.CM-SCE]Physics [physics]/Condensed Matter [cond-mat]/Strongly Correlated Electrons [cond-mat.str-el]IsostructuralComputingMilieux_MISCELLANEOUSJournal of the American Chemical Society
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Synthesis, crystal structure and magnetic properties of two oxalato-bridged dimetallic trinuclear complexes combined with a polar cation

2010

Two isostructural heterometallic trinuclear oxalato-bridged complexes of formula C(4)[MCr(2)(ox)(6)(H(2)O)(2)]·nH(2)O (C(+) = 4-aminopyridinium; ox(2-) = oxalate dianion; M(2+) = Mn(2+), n = 3, 1; M(2+) = Co(2+), n = 3.25, 2) have been synthesized by using direct self-assembly methods combining C(3)[Cr(ox)(3)] and the chloride salts of the corresponding metal ion. The crystal structures of both compounds have been resolved by single-crystal X-ray diffraction. They crystallize in the C2/c space group [a = 11.5113(15) Å, b = 20.250(3) Å, c = 21.810(4) Å, beta = 100.447(10) degrees, V = 5161.6(3) Å(3), and Z = 4 for 1, and a = 11.4334(16) Å, b = 20.243(2) Å, c = 21.805(3) Å, beta = 101.113(9) …

010405 organic chemistryStereochemistryHydrogen bondCrystal structure010402 general chemistry01 natural sciencesMagnetic susceptibilityOxalate0104 chemical sciencesInorganic ChemistryMetalchemistry.chemical_compoundCrystallographychemistryvisual_artvisual_art.visual_art_mediumMolecule[CHIM]Chemical SciencesPyridiniumIsostructuralComputingMilieux_MISCELLANEOUS
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Cobalt Clusters with Cubane-Type Topologies Based on Trivacant Polyoxometalate Ligands.

2016

Four novel cobalt-substituted polyoxometalates having cobalt cores exhibiting cubane or dicubane topologies have been synthesized and characterized by IR, elemental analysis, electrochemistry, UV-vis spectroscopy, X-ray single-crystal analysis, and magnetic studies. The tetracobalt(II)-substituted polyoxometalate [Co4(OH)3(H2O)6(PW9O34)](4-) (1) consists of a trilacunary [B-α-PW9O34](9-) unit which accommodates a cubane-like {Co(II)4O4} core. In the heptacobalt(II,III)-containing polyoxometalates [Co7(OH)6(H2O)6(PW9O34)2](9-) (2), [Co7(OH)6(H2O)4(PW9O34)2]n(9n-) (3), and [Co7(OH)6(H2O)6(P2W15O56)2](15-) (4), dicubane-like {Co(II)6Co(III)O8} cores are encapsulated between two heptadentate [B…

010405 organic chemistrychemistry.chemical_elementNanotechnologyType (model theory)010402 general chemistryElectrochemistry01 natural sciences0104 chemical sciencesInorganic Chemistrychemistry.chemical_compoundCrystallographychemistryCubanePolyoxometalatePhysical and Theoretical ChemistrySpectroscopyCobaltExchange modelInorganic chemistry
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Dimensionless Stage-Discharge Relationship for a Non-Linear Water Reservoir: Theory and Experiments

2020

In the field of hydrology, stage&ndash

010504 meteorology & atmospheric sciences0207 environmental engineering02 engineering and technologyOceanography01 natural sciencesWater balanceWater reservoirSettore AGR/08 - Idraulica Agraria E Sistemazioni Idraulico-Forestali020701 environmental engineeringlcsh:ScienceWaste Management and Disposal0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and TechnologyMathematicsConservation of energyMechanicsDischarge coefficientstage-discharge relationshipanalytical solutionNonlinear systemexperimental testContinuity equationlcsh:Qnon-linear reservoirDimensionless quantity
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Budyko’s Based Method for Annual Runoff Characterization across Different Climatic Areas: an Application to United States

2018

Runoff data knowledge is of fundamental importance for a wide range of hydrological, ecological, and socioeconomic applications. The reconstruction of annual runoff is a fundamental task for several activities related to water resources management, especially for ungauged basins. At catchment scales, the Budyko's framework provides an extremely useful and, in some cases, accurate estimation of the long-term partitioning of precipitation into evapotranspiration and runoff as a function of the prevailing climatic conditions. Recently the same long-term partitioning rules have been successfully used to describe water partitioning also at the annual scale and calculate the annual runoff distrib…

010504 meteorology & atmospheric sciences0208 environmental biotechnologyDrainage basin02 engineering and technologyStructural basinWater resources assessment01 natural sciencesBudyko's curveEvapotranspirationRange (statistics)Precipitation0105 earth and related environmental sciencesWater Science and TechnologyCivil and Structural EngineeringSubdivisionHydrologygeographygeography.geographical_feature_categorybusiness.industrySettore ICAR/02 - Costruzioni Idrauliche E Marittime E IdrologiaMOPEX data020801 environmental engineeringWater resourcesEnvironmental scienceAnnual water balanceAnnual runoff distributionSurface runoffbusiness
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Geographic and temporal variations in turbulent heat loss from lakes : A global analysis across 45 lakes

2018

Heat fluxes at the lake surface play an integral part in determining the energy budget and thermal structure in lakes, including regulating how lakes respond to climate change. We explore patterns in turbulent heat fluxes, which vary across temporal and spatial scales, using in situ high-frequency monitoring data from 45 glob- ally distributed lakes. Our analysis demonstrates that some of the lakes studied follow a marked seasonal cycle in their turbulent surface fluxes and that turbulent heat loss is highest in larger lakes and those situated at low latitude. The Bowen ratio, which is the ratio of mean sensible to mean latent heat fluxes, is smaller at low lati- tudes and, in turn, the rel…

010504 meteorology & atmospheric sciences0208 environmental biotechnologyta1172ta1171Climate change02 engineering and technologyAquatic ScienceOceanographyAtmospheric sciences01 natural sciencesjärvetLatitudeWater balanceheat fluxesLatent heatparasitic diseaseslakesBowen ratioturbulent heat loss0105 earth and related environmental sciencesthermal structurelake surface15. Life on landilmastonmuutoksetEnergy budget020801 environmental engineeringclimate change13. Climate actionHeat transferarticlesEnvironmental scienceSpatial variabilitylämpötilaenergy budgetlämpöhäviöLimnology and Oceanography
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Using scintillometry to assess reference evapotranspiration methods and their impact on the water balance of olive groves

2016

Abstract Reference evapotranspiration (ET 0 ) is widely used for irrigation scheduling, to promote an efficient use of water resources for a sustainable agro-ecosystem productivity, as well as to manage water quality and to face other environmental concerns. As suggested by ASCE-EWRI and FAO, standard Penman–Monteith methods are generally applied for an accurate estimation of ET 0 from hourly to daily scale. In absence of detailed meteorological information several simplified equations, using a limited number of variables, have been proposed as alternative. In this paper, the performance of different reference evapotranspiration methods, at hourly (Penman–Monteith, Pristley–Taylor, Makkink …

010504 meteorology & atmospheric sciencesASCE and FAO-56 papers0208 environmental biotechnologySoil Science02 engineering and technologyET Radiation based models01 natural scienceslaw.inventionWater balancelawScintillometerEvapotranspirationSettore AGR/08 - Idraulica Agraria E Sistemazioni Idraulico-ForestaliReference evapotranspiration; ASCE and FAO-56 papers; Scintillometer; ET Radiation based modelsReference evapotranspirationPenman–Monteith equation0105 earth and related environmental sciencesWater Science and TechnologyEarth-Surface ProcessesHydrologyEvapotranspirationSettore ICAR/02 - Costruzioni Idrauliche E Marittime E IdrologiaIrrigation schedulingMicrometeorology020801 environmental engineeringWater resourcesScintillometerEnvironmental scienceWater qualityMediterranean climateScale (map)Agronomy and Crop Science
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Cosmic-Ray Anisotropies in Right Ascension Measured by the Pierre Auger Observatory

2020

We present measurements of the large-scale cosmic-ray anisotropies in right ascension, using data collected by the surface detector array of the Pierre Auger Observatory over more than 14 years. We determine the equatorial dipole component, ~d⊥, through a Fourier analysis in right ascension that includes weights for each event so as to account for the main detector-induced systematic effects. For the energies at which the trigger efficiency of the array is small, the “East-West” method is employed. Besides using the data from the array with detectors separated by 1500 m, we also include data from the smaller but denser sub-array of detectors with 750 m separation, which allows us to extend …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsAstrophysicsanisotropy [cosmic radiation]Amplitude01 natural sciencessurface [detector]010303 astronomy & astrophysicsRight ascensionastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSGalactic CenterAstrophysics::Instrumentation and Methods for AstrophysicsCosmic RaysAugerobservatoryAmplitudePhysics::Space PhysicsAstrophysics - High Energy Astrophysical PhenomenaExtragalactic cosmic rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raycosmic radiation: anisotropyExtragalactic cosmic rayGalactic center0103 physical sciencesHigh Energy PhysicsPierre auger observatory0105 earth and related environmental sciencesPierre Auger Observatorydetector: surfaceFísicaAstronomy and AstrophysicsCosmic rayefficiency [trigger]GalaxyDipole* Automatic Keywords *Space and Planetary ScienceExperimental High Energy Physicstrigger: efficiencyddc:520galaxyDipoleObservatoryEnergy (signal processing)anisotropiesRight ascension[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)dipoleThe Astrophysical Journal
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Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

2021

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsEP/ T017325/101 natural sciencesrotationGeneral Relativity and Quantum CosmologyPSR J0537−6910neutron starsLuminosityGravitatational Waves PSR J0537−6910 LIGO VirgoHISTORYLIGOSupernova remnantneutron star010303 astronomy & astrophysicsgravitational waveQCQBpulsarPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/03N157BPhysics/dk/atira/pure/sustainabledevelopmentgoals/partnershipsGravitational waves neutron stars pulsarEPSRCPhysical Sciencesmoment: multipole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodPSR J0537-6910Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsEphemeris1ST SEARCHGravitational wavesX-raySDG 17 - Partnerships for the GoalsPulsar0103 physical sciences/dk/atira/pure/subjectarea/asjc/1900/1912X-ray: emissiongravitational waves; pulsars; PSR J0537-6910; neutron starsSTFCAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyNeutron Star Interior Composition ExplorerR-MODEGravitational waveVirgopulsar: rotationRCUKAstronomy and AstrophysicsLIGONeutron starVIRGOSUPERNOVA REMNANTSpace and Planetary Sciencegravitational radiation: emissionpulsars/dk/atira/pure/subjectarea/asjc/3100/3103Gravitatational Waves[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory

2020

Results of a search for ultra-high-energy neutrinos with the Pierre Auger Observatory from the direction of the blazar TXS 0506+056 are presented. They were obtained as part of the follow-up that stemmed from the detection of high-energy neutrinos and gamma rays with IceCube, Fermi-LAT, MAGIC, and other detectors of electromagnetic radiation in several bands. The Pierre Auger Observatory is sensitive to neutrinos in the energy range from 100 PeV to 100 EeV and in the zenith-angle range from θ = 60° to θ = 95°, where the zenith angle is measured from the vertical direction. No neutrinos from the direction of TXS 0506+056 have been found. The results were analyzed in three periods: One of 6 m…

010504 meteorology & atmospheric sciencesAstronomyAstrophysicspower spectrum7. Clean energy01 natural sciencesIceCubeObservatoryMAGIC (telescope)UHE Cosmic Rays010303 astronomy & astrophysicsHigh energy astrophysics Neutrino astrony Blazars Transient sources Active galaxiesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEOBSERVATÓRIOSAstrophysics::Instrumentation and Methods for Astrophysicsneutrino: UHEUHE [neutrino]AugerobservatoryHigh energy astrophysics; Neutrino astronomy; Blazars; Transient sources; Active galaxiesNeutrino detectorNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHigh energy astrophysicsradiation: electromagneticHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGLASTblazar0103 physical sciencesNeutrinoHigh Energy PhysicsZenithAstrophysique0105 earth and related environmental sciencesPierre Auger ObservatoryFísicaAstronomy and AstrophysicsAstronomiesensitivityMAGICTransient sourcesSciences de l'espaceelectromagnetic [radiation]13. Climate actionSpace and Planetary Sciencegamma rayExperimental High Energy PhysicsActive galaxiesddc:520spectralNeutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Blazars
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