Search results for " format"

showing 10 items of 2156 documents

Identity Development in Adulthood: Introduction

2016

In line with Erikson’s suggestions, increasing empirical evidence substantiates that considerable identity development takes place over the course of adulthood. What then does identity development during adulthood entail? The key findings of adult identity formation from four culturally different countries, and the challenges of analyzing the complex concept of identity are discussed. Although a wide array of identity measures are available, they have not been sufficiently validated for use with middle-aged or older adults. Additionally, different measures may yield results that are not comparable across studies. More studies are needed on adult identity development in populations represent…

adulthoodSociology and Political ScienceCultural identity05 social sciencesEthnic groupIdentity (social science)Erikson's stages of psychosocial development050109 social psychologyidentity developmentSocial identity approachDevelopmental psychologycross-culturalaikuisuusidentity measuresCross-cultural0501 psychology and cognitive sciencesPsychology (miscellaneous)Empirical evidencePsychologySocial psychologyIdentity formationta515050104 developmental & child psychologyIdentity
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Microscopic Insights Into the Formation of Methanesulfonic Acid–Methylamine–Ammonia Particles Under Acid-Rich Conditions

2022

Understanding the microscopic mechanisms of new particle formation under acid-rich conditions is of significance in atmospheric science. Using quantum chemistry calculations, we investigated the microscopic formation mechanism of methanesulfonic acid (MSA)–methylamine (MA)–ammonia (NH3) clusters. We focused on the binary (MSA)2n-(MA)n and ternary (MSA)3n-(MA)n-(NH3)n, (n = 1–4) systems which contain more acid than base molecules. We found that the lowest-energy isomers in each system possess considerable thermodynamic and dynamic stabilities. In studied cluster structures, all bases are protonated, and they form stable ion pairs with MSA, which contribute to the charge transfer and the stab…

aerosolitbase ratio [acid]proton transferEcologyammoniakkipienhiukkasetilmakemiahappamuusklusteritnew particle formationrikkiyhdisteetacid-rich conditiontyppiyhdisteetmethanesulfonic acid–methylamine–ammonia particlesEcology Evolution Behavior and SystematicsFrontiers in Ecology and Evolution
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Identity Processes in Adulthood: Diverging Domains

2005

Patterns of identity formation were analyzed in a longitudinal framework, from ages 27 to 36 and then to 42 years of age. Information from all 3 ages was available for 197 participants (100 women, 97 men). A variation of Marcia’s (1966) Identity Status Interview included 5 domains: religious beliefs, political identity, occupational career, intimate relationships, and lifestyle. Great variability in identity status assessments was found across the domains at each age level. The domains representing work and family (occupation, relationships, and lifestyle) were more salient for middle- aged adults than were ideological domains (religion and politics). Development along the hypothesized sequ…

aikuisikäSociology and Political ScienceCultural identitymedia_common.quotation_subjectPolitical science of religionsalienceIdentity (social science)osa-alueetasema (yhteiskunnalliset ominaisuudet)Religious identityDevelopmental psychologyPoliticsIdentityfollow-upidentiteettidevelopmentstatusdomainsmedia_commoncongruenceVariation (linguistics)Psychology (miscellaneous)IdeologykehitysPsychologyIdentity formationSocial psychologyIdentity
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Field-Specific Educational Practices as a Source for Students' Vocational Identity Formation

2008

Although work-related identity research has undergone considerable expansion in recent years, vocational identity among students remains a neglected area. However, initial vocational education plays a crucial role in the process of lifelong learning. Accordingly, this chapter discusses students' vocational identity formation during their vocational education and training. As recent findings on vocational or professional identity emphasise its context-based or sociocultural construction, [the authors] examined students' vocational identity formation in two different fields: one) technology and transport, and two) social services and health care. [The authors'] quantitative data indicate that…

ammatillinen koulutusLifelong learningProfessional developmentIdentity (social science)Qualitative propertyammattiosaamisen näytötammatillinen identiteettiAdult educationVocational educationPedagogytyössäoppiminenworkplace learningSociologySociocultural evolutionIdentity formationvocational identityvocational skills demonstrations
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Double-application of platelet-rich plasma on bone healing in rabbits

2010

Objective: Platelet-rich plasma (PRP) is considered to enhance bone formation especially at early stages of wound healing, depending on the limited and short life-span of platelets and growth factors. The aim of this study was to evaluate efficacy of double-application of PRP (DA-PRP) on bone healing in a rabbit calvarial defect model. Study design: Twenty-eight rabbits, each had two surgically prepared calvarial bone defects (10mm diameter), were included in this study and randomly divided into six groups. Defects (n=56) were treated with single-application of PRP (SA-PRP)(n=10), SA-PRP and beta-tricalciumphosphate (SA-PRP+TCP)(n=10), DA-PRP (n=8), DA-PRP and beta-tricalciumphosphate (DA-P…

animal diseasesDentistryBone healingBone and BonesAndrologyOsteogenesisStatistical analysesAnimalsBone formationPlateletGeneral DentistryWound HealingCalvarial defectPlatelet-Rich PlasmaChemistrybusiness.industrySignificant differenceClinical and Experimental dentistry:CIENCIAS MÉDICAS [UNESCO]nervous system diseasesOtorhinolaryngologyPlatelet-rich plasmaUNESCO::CIENCIAS MÉDICASFemaleResearch-ArticleSurgeryRabbitsbusinessWound healing
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Oxidation Processes in Sicilian Olive Oils Investigated by a Combination of Optical and EPR Spectroscopy

2012

:  Extra virgin olive oil (EVOO) is recognized as one of the healthiest foods for its high content of antioxidants, which forestall and slow down radical formation. Free radical-initiated oxidation is considered one of the main causes of rancidity in fats and oils. As a consequence, reliable protocols for the investigation of oil oxidation based on selective, noninvasive, and fast methods are highly desirable. Here we report an experimental approach based on UV-Vis absorbance, steady-state fluorescence, and electron paramagnetic resonance (EPR) spectroscopy for studying oxidation processes induced by temperature for a period up to 35 d on Sicilian EVOO samples. We followed the decrease in β…

antioxidantAntioxidantmedicine.medical_treatmentAnalytical chemistryTocopherolsextra virgin olive oilAntioxidantslaw.inventionAbsorbancechemistry.chemical_compoundlawmedicinePlant OilsUV-Vis fluorescenceSpectroscopyElectron paramagnetic resonanceOlive OilFree Radical FormationChromatographyChemistryElectron Spin Resonance SpectroscopyTemperaturePolyphenolsbeta Caroteneelectron paramagnetic resonanceVegetable oilPolyphenolChlorophyllUV-Vis absorbanceOxidation-ReductionFood ScienceJournal of Food Science
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Il corpo e l'arte come risorsa formativa all'Università:un percorso attraverso la danza-movimento terapia per futuri formatori

2015

The body and the Art as formative resources at University: a path through the dance-movement therapy for future educators Based on a personal experience of workshop with university master's students for over ten years, the article shows how a dance-movement therapy course can quickly open up new existential perspectives, enabling new narrative about one’s relationship with the world and increasing reflexive capacity and self-awareness. The students seem to find a way for integrating different parts of themselves, for accepting their difficulties and weaknesses, for reflecting and developing deep contacts, overcoming insecurity and discovering their value and their own creative abilities.

arte e formazione creativitàdanza-movimento terapiaformazione di formatoriformazione universitariaintegrazione mente corpo emozioniSettore M-PED/01 - Pedagogia Generale E Sociale
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The Gaia-ESO Survey: The origin and evolution of s-process elements

2018

Context. Several works have found an increase of the abundances of the s-process neutron-capture elements in the youngest Galactic stellar populations. These trends provide important constraints on stellar and Galactic evolution and they need to be confirmed with large and statistically significant samples of stars spanning wide age and distance intervals. Aims. We aim to trace the abundance patterns and the time evolution of five s-process elements - two belonging to the first peak, Y and Zr, and three belonging to the second peak, Ba, La, and Ce - using the Gaia-ESO IDR5 results for open clusters and disc stars. Methods. From the UVES spectra of cluster member stars, we determined the ave…

astro-ph.GAMetallicityFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: diskAstronomi astrofysik och kosmologiAbundance (ecology)QB4600103 physical sciencesAstronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar AstrophysicsDisc010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsgeneral [Open clusters and associations][SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsOpen clusters and associations: generalAstrophysics - Astrophysics of GalaxiesStarsAbundances [Galaxy][SDU]Sciences of the Universe [physics]13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesAstrophysics::Earth and Planetary AstrophysicsDisk [Galaxy]s-processOpen cluster
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The Gaia-ESO Survey : Probes of the inner disk abundance gradient

2016

The nature of the metallicity gradient inside the solar circle (R_GC < 8 kpc) is poorly understood, but studies of Cepheids and a small sample of open clusters suggest that it steepens in the inner disk. We investigate the metallicity gradient of the inner disk using a sample of inner disk open clusters that is three times larger than has previously been studied in the literature to better characterize the gradient in this part of the disk. We used the Gaia-ESO Survey (GES) [Fe/H] values and stellar parameters for stars in 12 open clusters in the inner disk from GES-UVES data. Cluster mean [Fe/H] values were determined based on a membership analysis for each cluster. Where necessary, dis…

astro-ph.SRField (physics)Cepheid variableRed giantastro-ph.GAMetallicityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: diskAstronomi astrofysik och kosmologiAbundance (ecology)0103 physical sciencesCluster (physics)Astrophysics::Solar and Stellar AstrophysicsAstronomy Astrophysics and Cosmology010303 astronomy & astrophysicsQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBPhysics010308 nuclear & particles physicsStars: abundancesabundances [Galaxy]Astronomy and AstrophysicsGalaxy: abundances; Galaxy: disk; Galaxy: formation; Stars: abundances; Astronomy and Astrophysics; Space and Planetary ScienceAstrophysics - Astrophysics of GalaxiesGalaxy: abundanceabundances [stars]StarsAstrophysics - Solar and Stellar Astrophysicsformation [Galaxy]Galaxy: formationSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesAstrophysics::Earth and Planetary Astrophysicsdisk [Galaxy]Open cluster
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Gaia-ESO Survey: Global properties of clusters Trumpler 14 and 16 in the Carina nebula

2017

Aims: We present the first extensive spectroscopic study of the global population in star clusters Trumpler 16, Trumpler 14, and Collinder 232 in the Carina nebula, using data from the Gaia-ESO Survey, down to solar-mass stars. Methods: In addition to the standard homogeneous survey data reduction, a special processing was applied here because of the bright nebulosity surrounding Carina stars. Results: We find about 400 good candidate members ranging from OB types down to slightly subsolar masses. About 100 heavily reddened early-type Carina members found here were previously unrecognized or poorly classified, including two candidate O stars and several candidate Herbig Ae/Be stars. Their l…

astro-ph.SROpen clusters and associations: individual: Carina nebulaastro-ph.GAExtinction (astronomy)PopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsOpen clusters and associations: individual: Trumpler 1401 natural sciencesindividual: Trumpler 16 [Open clusters and associations]Open clusters and associations: individual: Trumpler 16individual: Trumpler 14 [Open clusters and associations]Stars: early-typeearly-type [Stars]pre-main sequence [Stars]QB4600103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)O-type starLine (formation)[PHYS]Physics [physics]PhysicsNebulaeducation.field_of_studyOpen clusters and associations: Individual: Carina nebula; Open clusters and associations: Individual: Trumpler 14; Open clusters and associations: Individual: Trumpler 16; Stars: Early-type; Stars: Pre-main sequence; Astronomy and Astrophysics; Space and Planetary Science010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesStarsStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Stars: pre-main sequenceAstrophysics::Earth and Planetary Astrophysicsindividual: Carina nebula [Open clusters and associations][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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