Search results for "METEOROLOGY"

showing 10 items of 4531 documents

New orbital ephemerides for the dipping source 4U 1323-619: Constraining the distance to the source

2016

4U 1323-619 is a low mass X-ray binary system that shows type I X-ray bursts and dips. The most accurate estimation of the orbital period is 2.941923(36) hrs and a distance from the source that is lower than 11 kpc has been proposed. We aim to obtain the orbital ephemeris, the orbital period of the system, as well as its derivative to compare the observed luminosity with that predicted by the theory of secular evolution. We took the advantage of about 26 years of X-ray data and grouped the selected observations when close in time. We folded the light curves and used the timing technique, obtaining 12 dip arrival times. We fit the delays of the dip arrival times both with a linear and a quad…

neutron X-rays: binaries X-rays: stars ephemerides stars: individual: 4U 1323-619 [stars]010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEphemeris01 natural sciencesLuminositySettore FIS/05 - Astronomia E Astrofisica0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)stars: neutron X-rays: binaries X-rays: stars ephemerides stars: individual: 4U 1323-619Astronomy and AstrophysicsLight curveOrbital periodGalaxyNeutron starSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsLow MassAstrophysics - High Energy Astrophysical Phenomena
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Timing an Accreting Millisecond Pulsar: Measuring the Accretion Torque in IGR J00291+5934

2006

We performed a timing analysis of the fastest accreting millisecond pulsar IGR J00291+5934 using RXTE data taken during the outburst of December 2004. We corrected the arrival times of all the events for the orbital (Doppler) effects and performed a timing analysis of the resulting phase delays. In this way we have the possibility to study, for the first time in this class of sources, the spin-up of a millisecond pulsar as a consequence of accretion torques during the X-ray outburst. The accretion torque gives us for the first time an independent estimate of the mass accretion rate onto the neutron star, which can be compared with the observed X-ray luminosity. We also report a revised valu…

neutron; stars : magnetic fields; pulsars : general; pulsars : individual : IGR J00291+5934; X-ray : binaries [accretion accretion disks; stars]X-rays : binariesAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstrophysicsaccretion accretion diskAstrophysicsX-ray : binariesBinary pulsarLuminositypulsars : individual : IGR J00291+5934symbols.namesakePulsarMillisecond pulsarAstrophysics::Solar and Stellar Astrophysicspulsars : individual (IGR J00291+5934)PhysicsAccretion (meteorology)general; pulsars : individual (IGR J00291+5934); stars : magnetic fields; stars : neutron; X-rays : binaries [pulsars]Astrophysics (astro-ph)pulsars : generalStatic timing analysisAstronomystars : magnetic fieldAstronomy and Astrophysicsstars : neutronNeutron starSpace and Planetary SciencesymbolsAstrophysics::Earth and Planetary AstrophysicsDoppler effectX-ray pulsar
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Noise Reduction and Gap Filling of fAPAR Time Series Using an Adapted Local Regression Filter

2014

Time series of remotely sensed data are an important source of information for understanding land cover dynamics. In particular, the fraction of absorbed photosynthetic active radiation (fAPAR) is a key variable in the assessment of vegetation primary production over time. However, the fAPAR series derived from polar orbit satellites are not continuous and consistent in space and time. Filtering methods are thus required to fill in gaps and produce high-quality time series. This study proposes an adapted (iteratively reweighted) local regression filter (LOESS) and performs a benchmarking intercomparison with four popular and generally applicable smoothing methods: Double Logistic (DLOG), sm…

noise010504 meteorology & atmospheric sciencesRemote sensing applicationComputer scienceNoise reduction0211 other engineering and technologies02 engineering and technologyLand cover01 natural sciencesfAPAR; noise; MODIS; time series; filtering; interpolation; LOESSSmoothing splineLoessLOESSlcsh:Science021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingLocal regressionFilter (signal processing)Vegetation15. Life on landfilteringSnowinterpolationNoiseMODISfAPARGeneral Earth and Planetary Scienceslcsh:Qtime seriesSmoothingInterpolationRemote Sensing
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Diurnal Cycle Relationships between Passive Fluorescence, PRI and NPQ of Vegetation in a Controlled Stress Experiment

2017

In order to estimate vegetation photosynthesis from remote sensing observations; some critical parameters need to be quantified. From all absorbed light; the plant needs to release any excess that is not used for photosynthesis; by non-photochemical quenching; by fluorescence emission and unregulated thermal dissipation. Non-photochemical quenching (NPQ) processes are controlled photoprotective mechanisms which; once activated; strongly control the dynamics of photochemical efficiency. With illumination conditions increasing and decreasing during a diurnal cycle; photoprotection mechanisms needs to change accordingly. The goal of this work is to quantify dynamic NPQ; measured from active fl…

non-photochemical energy dissipation0106 biological sciencesPhotoinhibition010504 meteorology & atmospheric sciencesSciencedroughtsolar-induced fluorescence (SIF)PhotosynthesisPhotochemical Reflectance IndexAtmospheric sciencesFLuorescence EXplorer01 natural sciencesstressDiurnal cycle0105 earth and related environmental sciencesRemote sensingphotosynthesisQuenching (fluorescence)Chemistry(FLEX)Qdrought; stress; non-photochemical energy dissipation; solar-induced fluorescence (SIF); photosynthesis; non-photochemical quenching (NPQ); Photochemical Reflectance Index (PRI); FLuorescence EXplorer; (FLEX)15. Life on landFluorescencePhotochemical Reflectance Index (PRI)non-photochemical quenching (NPQ)Photosynthetically active radiationPhotoprotectionGeneral Earth and Planetary Sciences010606 plant biology & botanyRemote Sensing; Volume 9; Issue 8; Pages: 770
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Prenatal air pollution exposure and growth and cardio-metabolic risk in preschoolers

2020

Objectives: We investigated the association between outdoor air pollutants exposure in the first trimester of pregnancy, and growth and cardio-metabolic risk at four years of age, and evaluated the mediating role of birth weight. Methods: We included mother-child pairs (N = 1,724) from the Spanish INMA birth cohort established in 2003-2008. First trimester of pregnancy nitrogen dioxide (NO2) and fine particles (PM2.5) exposure levels were estimated. Height, weight, waist circumference, blood pressure, and lipids were measured at four years of age. Body mass index (BMI) trajectories from birth to four years were identified. Results: Increased PM2.5 exposure in the first trimester of pregnanc…

obesity010504 meteorology & atmospheric sciencesair pollutionprenatal exposureuse regression-models010501 environmental sciencesMalalties neonatals01 natural sciencesPregnancyInterquartile rangePrenatal exposureChildhood obesityChildlcsh:Environmental sciencesGeneral Environmental Sciencelcsh:GE1-3502. Zero hungerAir Pollutants*Childhood obesityObstetrics*Prenatal exposureChildhood growthhealthtraffic pollutionfetalPollutionMaternal ExposureChild PreschoolContaminaciómaternal smokingFemaleNeonatal diseaseschildhood obesitypregnant-womenmedicine.medical_specialtyWaistBirth weightNitrogen DioxideAir pollutioncomplex mixturesChildhood obesity*Air pollutionchildhood growthearly-childhoodmedicineHumansmediation analysis0105 earth and related environmental sciencesparticulate matterFetusPregnancybusiness.industrymedicine.disease*Particulate matterObesity*Childhood growthbusinessParticulate matterBody mass index
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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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A revision of the structure and stratigraphy of pre-Green Tuff ignimbrites at Pantelleria (Strait of Sicily)

2013

International audience; At Pantelleria, peralkaline silicic magmas were erupted across a range of eruptive typologies and magnitudes: pyroclastic flows, Plinian to strombolian pumice fallout and lava flows. In this paper we focus on the intermediate cycle of eruptive activity which is bracketed by ignimbrite units slightly older than the two caldera collapses which marked the volcanological activity of the island. This age interval (180-85 ka) was punctuated by six ignimbrite-forming eruptions (silicic and variably peralkaline) for a cumulative erupted magma volume of approximately 6 km3 dense rock equivalent. Based on new 40Ar/39Ar (Na,K)-feldspar ages and petrographic data, we propose an …

pantellerite010504 meteorology & atmospheric sciencesLava[SDE.MCG]Environmental Sciences/Global ChangesGeochemistrySilicicPyroclastic rock010502 geochemistry & geophysics01 natural sciencesPeralkaline rock40Ar/39Ar datingGeochemistry and PetrologyPumiceperalkaline magma[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/VolcanologyCalderaPeralkaline magmasGeomorphology0105 earth and related environmental sciencesIgnimbritesSettore GEO/07 - Petrologia E PetrografiaStrombolian eruptionignimbriteGeophysicsDense-rock equivalentPantellerites40Ar/39Ar dating.GeologyPantelleria
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Guano-related phosphate-rich minerals in European caves

2019

International audience; Guano is a typical deposit found in caves derived from the excretions of bats and in minor cases of birds. These organic deposits decompose and form a series of acid fluids and gases that can interact with the minerals, sediments, and rocks present in the cave. Over sixty phosphates are known and described from caves, but guano decay also often leads to the formation of nitrates and sulfates. In this study twenty-two European caves were investigated for their guano-related secondary minerals. Using various analytical techniques, seventeen phosphates, along with one sulfate (gypsum), were recognized as secondary products of guano decay. Among those minerals, some are …

phosphatesGypsum010504 meteorology & atmospheric sciencesQH301-705.5Settore GEO/04 - Geografia Fisica E GeomorfologiaGeochemistrybat guanocave minerals phosphate bat guanoengineering.material010502 geochemistry & geophysics01 natural sciencessecondary cave mineralsApatitechemistry.chemical_compoundCavesecondary cave minerals phosphates minerogenesis limestone caves bat guanominerogenesisBiology (General)Sulfatelimestone cavephosphate0105 earth and related environmental sciencesEarth-Surface Processescave mineralsQE1-996.5geographygeography.geographical_feature_categoryMineralSettore GEO/07 - Petrologia E PetrografiaGeology15. Life on landPhosphatehumanitiessecondary cave mineralchemistryminerogenesivisual_artlimestone cavesGuanoengineeringvisual_art.visual_art_mediumPyrite[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
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A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251

2013

We present the analysis of the gravitational microlensing event OGLE-2011-BLG-0251. This anomalous event was observed by several survey and follow-up collaborations conducting microlensing observations towards the Galactic Bulge. Based on detailed modelling of the observed light curve, we find that the lens is composed of two masses with a mass ratio q=1.9 x 10^-3. Thanks to our detection of higher-order effects on the light curve due to the Earth's orbital motion and the finite size of source, we are able to measure the mass and distance to the lens unambiguously. We find that the lens is made up of a planet of mass 0.53 +- 0.21,M_Jup orbiting an M dwarf host star with a mass of 0.26 +- 0.…

planets and satellites: detection010504 meteorology & atmospheric sciencesSatellitesbulge [Galaxy]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsDiscoveryGravitational microlensing01 natural sciencesGalaxy: bulgeEinstein radiusLensgravitational lensing: weakSettore FIS/05 - Astronomia e AstrofisicaPlanetSnow0103 physical sciencesgravitational lensing; weak; planets and satellites; detection; planetary systems; Galaxy; bulgegravitational lensing: weak; planets and satellites: detection; planetary systems; Galaxy: bulgeBinaryQB Astronomy010303 astronomy & astrophysicsplanetary systemsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesQBPhysicsEarth and Planetary Astrophysics (astro-ph.EP)Giant planetSystemsSearchAstronomy and AstrophysicsRadiusFrequencyPlanetary systemMass ratioMassLight curveStarsAlgorithmdetection [Planets and satellites]Planetary systemsSpace and Planetary ScienceDwarfAstrophysics::Earth and Planetary Astrophysicsweak [Gravitational lensing]Astrophysics - Earth and Planetary AstrophysicsAstronomy and Astrophysics
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