Search results for " method"

showing 10 items of 10455 documents

A classification of motivation and behavior change techniques used in self-determination theory-based interventions in health contexts

2020

While evidence suggests that interventions based on self-determination theory have efficacy in motivating adoption and maintenance of health-related behaviors, and in promoting adaptive psychological outcomes, the motivational techniques that comprise the content of these interventions have not been comprehensively identified or described. The aim of the present study was to develop a classification system of the techniques that comprise self-determination theory interventions, with satisfaction of psychological needs as an organizing principle. Candidate techniques were identified through a comprehensive review of self-determination theory interventions and nomination by experts. The study…

need satisfactionitsemäärääminenOrganizing principleComputer scienceHealth Toxicology and MutagenesisPsychological interventionSocial Sciences050109 social psychology/dk/atira/pure/core/keywords/exercise_nutrition_and_health_sciencesNEEDS0302 clinical medicineMedicine and Health SciencesDevelopmental and Educational PsychologyApplied PsychologyAutonomy supportmedia_commonmotivaatioManagement science05 social sciencesBehavior changeBehavior change methodsSCIENCEautonomous motivationautonomy supportmotivational techniqueNominationPHYSICAL-EDUCATION TEACHERSAutonomyNeed satisfactionINTRINSIC MOTIVATIONEnvironmental EngineeringSelf-determination theory interventionsmedia_common.quotation_subjectself-determination theory interventionsMotivational technique03 medical and health sciencesmotivaatiopsykologia0501 psychology and cognitive sciencesCompetence (human resources)Self-determination theorySUPPORT STUDENTS AUTONOMY030229 sport sciencesTAXONOMYGOALAutonomous motivationRELATEDNESS SUPPORTterveyskäyttäytyminenINTERNALIZATIONSPS Exercise Nutrition and Health SciencesCONSENSUS
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Technical and economical comparison between NdFeB and hard ferrites linear electrical generators from sea waves

2015

In this paper the authors perform a technical-economic comparison of two different Tubular Permanent Magnet Linear Machines for sea waves generation by using finite elements analysis. The first configuration includes ferrite rings while the second configuration includes neodymium-iron-boron rings. In order to compare the two types in economic and technical terms, a detailed analysis of the main figures of merit of the two configurations has been carried out. In particular, significant data such as flux distribution, rated voltage and current, axial force, electric power, realization cost and maintenance cost have been compared.

neodymium-iron-boronpermanent magnets linear machineComputer sciencebusiness.industryRenewable Energy Sustainability and the EnvironmentElectrical engineeringMechanical engineeringElectric generatorEnergy Engineering and Power TechnologySettore ING-IND/32 - Convertitori Macchine E Azionamenti ElettriciMagnetic fluxFinite element methodlaw.inventionferriteNeodymium magnetlawMagnetFigure of meritsea wave generatorElectric powerbusinessSettore ING-INF/07 - Misure Elettriche E ElettronicheVoltage
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Evaluation of Innovation Statistics Data Quality Dimensions.

2017

Promocijas darbā analizēta praktiskā situācija statistikas par inovācijām vākšanas un apstrādes procesā Latvijā, tiek apskatīta statistikas par inovācijām metodoloģija un tās pielietošanas prakse Latvijā, īpašu uzmanību pievēršot Latvijas inovāciju sistēmas īpatnībām. Pētījumā izstrādātās Latvijas inovāciju vadības un informācijas plūsmas sistēmas ietvaros tiek pamatots informatīvā atbalsta nozīmīgums lēmumu pieņemšanā. Balstoties uz Datu kvalitātes dimensiju novērtēšanas metodiku, veikts inovāciju statistikas datu kvalitātes novērtējums Latvijā. Ir izstrādāta un aprobēta Iteratīvā metode neraksturīgo punktu ietekmes mazināšanai. Pētījuma ietvaros tiek aplūkoti statistikas par inovācijām kv…

neraksturīgie punktistatistikas datu vākšanas un apstrādes metodoloģijaquality of statistical dataquality of methodologyEconomicsdatu kvalitātes dimensijasStatisticsEkonomikaStatistikadata quality dimensionsoutlying data pointsstatistikas datu kvalitāte
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Astrophysical muon neutrino flux in the northern sky with 2 years of IceCube data

2015

Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern Hemisphere data set consisting primarily of νe and ντ charged-current and neutral-current (cascade) neutrino interactions. Additionally, a fit for an astrophysical flux with an arbitrary spectral index is performed.

neutrino astronomyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for Astrophysics
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Search for contained neutrino events at energies above 30 TeV in 2 years of data

2013

Neutrino observations are a unique probe of the universe's highest energy phenomena: neutrinos are able to escape from dense environments that photons cannot and are unambiguous tracers of hadronic interaction processes, in particular the acceleration of cosmic rays. We report on results of an all-sky search for these neutrinos at energies above 30 TeV in the cubic kilometer antarctic IceCube observatory 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.

neutrino astronomyAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsHigh Energy Physics::Experiment
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Search for contained neutrino events at energies greater than 1 TeV in 2 years of data

2015

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. Here we present the results of a search for neutrino interactions inside IceCube's instrumented volume between 1 TeV and 1 PeV in 641 days of data taken from 2010--2012. From these data we derive new constraints on the diffuse astrophysical neutrino spectrum,as well as the strongest upper limit yet on the flux of neutrinos from charmed-meson decay in the atmosphere.

neutrino astronomyPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsHigh Energy Physics::Experiment
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Search for sterile neutrinos with one year of IceCube data

2016

The IceCube neutrino telescope at the South Pole has measured the atmospheric muon neutrino spectrum as a function of zenith angle and energy to search for the oscillation signatures of light sterile neutrinos. The primary result of this search derives from the first year of data, taken during 2011, of the full 86-string IceCube configuration.

neutrino astronomyPhysics::Instrumentation and Detectorssterile neutrinosAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsHigh Energy Physics::Experiment
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Search for a diffuse flux of high-energy ¿µ with the ANTARES neutrino telescope

2011

A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A $(0.83\times 2\pi)$ sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an $E^{-2}$ flux spectrum, a 90% c.l. upper limit on the diffuse $\nu_\mu$ flux of $E^2\Phi_{90%} = 5.3 \times 10^{-8} \ \mathrm{GeV\ cm^{-2}\ s^{-1}\ sr^{-1}} $ in the energy range 20 TeV - 2.5 PeV is obtained. Other signal models with differ…

neutrino telescope; antares; diffuse muon neutrino fluxNuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFluxAstrophysicsNeutrino telescope01 natural sciences7. Clean energySpectral lineMUONSLIMITS0103 physical sciencesNeutrins010306 general physicsDETECTORmedia_commonPhysicsRange (particle radiation)MuonsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsMuon Collaboration[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODELDiffuse muon neutrino fluxSky:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]High Energy Physics::ExperimentFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)
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The advanced Virgo longitudinal control system for the O2 observing run

2020

Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During …

neutron star: binaryPhysics::Instrumentation and DetectorsAstronomycavity: opticalSuspended optical cavities01 natural sciencesGravitational wave detectorsoff-lineGravitational wave detectors; Interferometer; Suspended optical cavities; Control loopsControl loopSuspended optical cavitieLIGOInterferometer010303 astronomy & astrophysicsdetectorsSettore FIS/01Physics[PHYS]Physics [physics]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsGravitational wave detectors Interferometer Suspended optical cavities Control loopsGravitational wave detectorUpgrade[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]upgradecontrol systemGravitational wavelongitudinalAstrophysics::High Energy Astrophysical PhenomenainterferometerAstrophysics::Cosmology and Extragalactic Astrophysicscontrol loops; gravitational wave detectors; interferometer; suspended optical cavitiesgravitational radiation: direct detectionGeneral Relativity and Quantum CosmologySettore FIS/05 - Astronomia e AstrofisicaBinary black holebinary: coalescence0103 physical sciencesControl loops[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and AstrophysicssensitivityLIGOgravitational radiation detectordetector: sensitivityNeutron star* Automatic Keywords *VIRGOblack hole: binaryControl systemgravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Synthesis and Rearrangement of 2-(N-Methyl-N-nitroamino)-4-phenylthiazole

2007

2-(N-Methyl-N-nitroamino)-4-phenylthiazole (5) was prepared and rearranged in aqueous dioxane under influence of sulphuric acid of various concentrations. 2-(N-Methylamino)- 5-nitro-4-phenylthiazole (6) was the only product up to 50% acid concentration. At higher acidities, significant amounts of nitro derivatives 3b and3c, substituted in benzene ring, were also formed. The result indicates that migration of the N-nitro group occurs on the intramolecular path, however, in concentrated sulphuric acid, formation of nitronium ion and ring nitration also takes place.

nitramine rearrangementmechanism of migrationAngeli methodHantzsch synthesisPolish Journal of Chemistry
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