Search results for "Measurements"

showing 10 items of 720 documents

Preparation methods to optimize the performance of sensor discs for fast chemiluminescence ozone analyzers.

2013

Fast ozone (O(3)) measurements (1-50 Hz) in the atmosphere are required for airborne studies and for the measurement of ground-based O(3) fluxes by the eddy covariance technique. Fast response analyzers, based on heterogeneous chemiluminescence, need dye coated sensor discs on which the chemiluminescence is generated. In this study, we present three new preparation methods for those sensor discs. Currently available sensor discs exhibit a fast temporal decay of sensitivity, resulting in short duty times which is troublesome for many field applications. To produce sensor discs that provide more stable signals over time, three dyes and nine energy transfer reagents were tested (as well as dif…

OzoneLuminescent MeasurementsChemistryAnalytical chemistryGeneral Chemistrylaw.inventionPreparation methodMatrix (chemical analysis)chemistry.chemical_compoundAdsorptionOzoneEnergy TransferlawReagentLuminescent MeasurementsEnvironmental ChemistrySensitivity (control systems)Coloring AgentsChemiluminescenceEnvironmental sciencetechnology
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Serum 25-hydroxyvitamin D levels in patients with cutaneous lupus erythematosus in a Mediterranean region

2010

Low vitamin D levels have been found in patients with autoimmune diseases, including type I diabetes, rheumatoid arthritis, multiple sclerosis and systemic lupus erythematosus. The main source of vitamin D is exposure to sunlight, but the same solar radiation is known to exacerbate lupus erythematosus. We investigated the prevalence of vitamin D insufficiency in patients with cutaneous lupus erythematosus (CLE). We designed a cross-sectional study including 55 patients with CLE to measure their serum 25-hydroxyvitamin D (25(OH)D) by chemiluminescence immunoassay and compare it with a control group consisting of 37 healthy sex and age-matched subjects recruited from the patients' relatives a…

PaperAdultMaleVitaminmedicine.medical_specialtySubacute Lupus ErythematosusParathyroid hormoneSystemic Lupus ErythematosusGastroenterologyvitamin D deficiencyYoung Adultchemistry.chemical_compoundRheumatologyInternal medicineLupus Erythematosus CutaneousPrevalencemedicineVitamin D and neurologyHumansVitamin DAgedAged 80 and overLupus erythematosusSystemic lupus erythematosusMediterranean Regionbusiness.industryfungiCase-control studyMiddle AgedVitamin D Deficiencymedicine.diseaseCross-Sectional StudiesEndocrinologychemistryParathyroid HormoneCase-Control StudiesRheumatoid arthritisLuminescent MeasurementsCutaneous LupusFemalebusinessLupus
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Synthesis, structure and magnetic properties of the one-dimensional chain compound {K[Fe(1,3,5-triazine-2,4,6-tricarboxylate)(H2O)2]·2H2O}∞

2002

The one-dimensional chain compound {[Fe(1,3,5-triazine-2,4,6-tricarboxylate)(H2O)2]}n−n was obtained from a reaction of 1,3,5-triazine-2,4,6-tricarboxylate with Fe(II) in water at room temperature. The high-spin Fe(II) centers adopt a pentagonal bipyramid geometry with unusual ligand binding modes. Magnetic measurements revealed weak magnetic interactions between paramagnetic centers; these were modeled with both axial and rhombic distortions.

Paramagnetismchemistry.chemical_compoundCrystallographyMagnetic measurementsPentagonal bipyramidal molecular geometryChain (algebraic topology)135-TriazineChemistryCompound KGeneral ChemistryTricarboxylateJournal of the Chemical Society, Dalton Transactions
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The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector

2010

The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2 - 200 TeV. The result is compared to different atmospheric neutrino models and it is compatible with the atmospheric neutrinos from pion and kaon decays. No significant contribution from charm hadron decays or extraterrestrial neutrinos is detected. The capabilities to improve the measurement of the neutrino spectrum with the successor experiment IceCube are discussed.

Particle physicsAMANDA[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Solar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAMANDA; Atmospheric neutrinos; Cherenkov radiation; Neural net; Unfoldingneural netFOS: Physical sciencesAetiology screening and detection [ONCOL 5]01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsunfoldingPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cherenkov radiationHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsSolar neutrino problematmospheric neutrinosCosmic neutrino backgroundNeutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

2013

We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to approximately 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the twenty-eight events at the $4\sigma$ level. These twenty-eight events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General Science & TechnologyPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2AstrophysicsIceCube Collaboration01 natural sciences7. Clean energyHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - Experiment (hep-ex)MD Multidisciplinary0103 physical sciences010303 astronomy & astrophysicsastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Multidisciplinaryhep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyneutrinosSolar neutrino problemKM3NeTNeutrino detector13. Climate actionastro-ph.COMeasurements of neutrino speedHigh Energy Physics::Experimentddc:500NeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsScience
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Precise measurement of the neutrino mixing parameter θ23 from muon neutrino disappearance in an off-axis beam

2014

New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter theta_{23}. Using an off-axis neutrino beam with a peak energy of 0.6 GeV and a data set corresponding to 6.57 x 10^{20} protons on target, T2K has fit the energy-dependent nu_mu oscillation probability to determine oscillation parameters. Marginalizing over the values of other oscillation parameters yields sin^2 (theta_{23}) = 0.514 +0.055/-0.056 (0.511 +- 0.055), assuming normal (inverted) mass hierarchy. The best-fit mass-squared splitting for normal hierarchy is Delta m^2_{32} = (2.51 +- 0.10) x 10^{-3} eV^2/c^4 (inverted hierarchy: Delta m^2_{13} = (2.48 +- 0.10) …

Particle physicsGeneral PhysicsPhysics MultidisciplinaryMODELSGeneral Physics and AstronomyFOS: Physical sciencesMASS01 natural sciences09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGMuon neutrino010306 general physicsNeutrino oscillationDETECTORMixing (physics)01 Mathematical SciencesPhysicsNeutronsScience & Technology02 Physical Sciences010308 nuclear & particles physicsScatteringOscillationhep-exPhysicsFísicaT2K CollaborationPhysical SciencesSYMMETRIESHigh Energy Physics::ExperimentNeutrinoHigh energy physics Mixing Parameter estimation Parameter extractionConfidence limit Energy dependent Neutrino oscillations Off-axis neutrino beam Oscillation parameters Oscillation probabilities Precise measurements Statistical uncertaintyBeam (structure)Energy (signal processing)
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On the flavor composition of the high-energy neutrino events in IceCube

2014

The IceCube experiment has recently reported the observation of 28 high-energy (> 30 TeV) neutrino events, separated into 21 showers and 7 muon tracks, consistent with an extraterrestrial origin. In this letter we compute the compatibility of such an observation with possible combinations of neutrino flavors with relative proportion (alpha_e:alpha_mu:alpha_tau). Although the 7:21 track-to-shower ratio is naively favored for the canonical (1:1:1) at Earth, this is not true once the atmospheric muon and neutrino backgrounds are properly accounted for. We find that, for an astrophysical neutrino E^(-2) energy spectrum, (1:1:1) at Earth is disfavored at 81% C.L. If this proportion does not c…

Particle physicsHigh energySolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEnergy spectrum010306 general physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Study of Beauty Hadron Decays into Pairs of Charm Hadrons

2014

First observations of the decays Λ[0 over b] → Λ[+ over c]D[− over (s)] are reported using data corresponding to an integrated luminosity of 3  fb[superscript −1] collected at 7 and 8 TeV center-of-mass energies in proton-proton collisions with the LHCb detector. In addition, the most precise measurement of the branching fraction B(B[0 over s] → D[superscript +]D[− over s]) is made and a search is performed for the decays B[0 over (s)] → Λ[+ over c]Λ[− over c]. The results obtained are B(Λ[0 over b] → Λ[+ over c]D[superscript −])/B(Λ[0 over b] → Λ[+ over c]D[− over s]) = 0.042 ± 0.003(stat) ± 0.003(syst), ⎡⎣B(Λ[0 over b] → Λ[+ over c]D[− over s]) over B([¯ over B[superscript 0] → D[superscr…

Particle physicsMesonHadronNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciencesLHCb - Abteilung Hofmann13.30.-aSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)precise measurements14.20.Mr[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]TOOLCharm (quantum number)MASSESNuclear ExperimentQCBARYONSPhysicsLuminosity (scattering theory)Branching fractioncenter-of-mass energiesintegrated luminositybaryons; masses; toolParticle physicsBaryonproton proton collisionsLHCbprecise measurements; center-of-mass energies; tellurium compounds; integrated luminosity; hadrons; branching fractions; proton proton collisionshadronsDecays of baryonbranching fractionsBottom baryons (|B|>0)Física nuclearHigh Energy Physics::ExperimentLHCFísica de partículesExperimentstellurium compoundsTellurium compoundsParticle Physics - Experiment
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Absence of a day-night asymmetry in the7Be solar neutrino rate in Borexino

2012

We report on a search for the day-night asymmetry of the Be-7 solar neutrino rate measured by Borexino at the Laboratori Nazionali del Gran Sasso (LNGS), Italy. The measured value, Adn=0.001 +- 0.012 (stat) +- 0.007 (syst), shows the absence of a significant asymmetry. This result alone rejects the so-called LOW solution at more than 8.5 sigma. Combined with the other solar neutrino data, it isolates the Large Mixing Angle (LMA) -- MSW solution at DeltaChi2 > 190 without relying on the assumption of CPT symmetry in the neutrino sector. We also show that including the day-night asymmetry, data from Borexino alone restricts the MSW neutrino oscillations to the LMA solution at 90% confidence l…

Particle physicsNuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectSolar neutrino01 natural sciencesAsymmetrySolar neutrinoNuclear physicsDay-night effect0103 physical sciences010306 general physicsNeutrino oscillationNuclear Experimentday–night effectBorexinomedia_commonPhysicsneutrino oscillations010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemNeutrino detectorsolar neutrinosMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoCPT violation
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Conditions for statistical determination of the neutrino mass spectrum in radiative emission of neutrino pairs in atoms

2016

The photon spectrum in macrocoherent atomic de-excitation via radiative emission of neutrino pairs (RENP) has been proposed as a sensitive probe of the neutrino mass spectrum, capable of competing with conventional neutrino experiments. In this paper we revisit this intriguing technique in order to quantify the requirements for statistical determination of some of the properties of the neutrino spectrum, in particular the neutrino mass scale and the mass ordering. Our results are sobering. We find that, even under ideal conditions, the determination of neutrino parameters needs experimental live times of the order of days to years for several laser frequencies, assuming a target of volume o…

Particle physicsPhotonNeutrino theory of lightPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesRadiative transferNeutrinsNeutrinos010306 general physicsNeutrino oscillationPhysicsPhotons010308 nuclear & particles physicsSolar neutrino problem3. Good healthFotonsHigh Energy Physics - PhenomenologyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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