Search results for "COST Action"

showing 10 items of 26 documents

Development of a big data bank for PV monitoring data, analysis and simulation in COST Action 'PEARL PV'

2019

COST Action entitled PEARL PV aims at analyzing data of monitored PV systems installed all over Europe to quantitatively evaluate the long-term performance and reliability of these PV systems. For this purpose, a data bank is being implemented that can contain vast amounts of data, which will enable systematic performance analyses in combination with simulations. This paper presents the development process of this data bank.

Computer scienceProcess (engineering)business.industryReliability (computer networking)Performance05 social sciencesPhotovoltaic systemBig dataData analysis050301 educationReliability7. Clean energyReliability engineeringPV systemsPEARL (programming language)Monitoring data0502 economics and businessData bankCost actionbusiness0503 educationcomputer050203 business & managementData monitoringcomputer.programming_language
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Medico-legal implications of sleep apnoea syndrome: driving license regulations in Europe.

2008

Background: Sleep apnoea syndrome (SAS), one of the main medical causes of excessive daytime sleepiness, has been shown to be a risk factor for traffic accidents. Treating SAS results in a normalized rate of traffic accidents. As part of the COST Action B-26, we looked at driving license regulations, and especially at its medical aspects in the European region. Methods: We obtained data from Transport Authorities in 25 countries (Austria, AT; Belgium, BE; Czech Republic, CZ; Denmark, DK; Estonia, EE; Finland, FI; France, FR; Germany, DE; Greece, GR; Hungary, HU; Ireland, IE; Italy, IT; Lithuania, LT; Luxembourg, LU; Malta, MT; Netherlands, NL; Norway, EC; Poland, PL; Portugal, PT; Slovakia,…

Cross-Cultural Comparisonmedicine.medical_specialtyPediatricsAutomobile DrivingSleep ApneaDriving license regulationsExcessive daytime sleepinessPoison controlDisorders of Excessive SomnolenceSettore MED/10 - Malattie Dell'Apparato RespiratorioOccupational safety and healthRisk FactorsInjury preventionmedicineHumansPsychiatryLicenseSleep Apnea ObstructiveTraffic/legislation & jurisprudencebusiness.industryAccidents TrafficSleep apneaDisorders of Excessive Somnolence/complicationsGeneral MedicineSleep Apnea Obstructive/complicationsmedicine.diseaseEuropeObstructive sleep apnoeaAccidents Traffic/legislation & jurisprudenceAccidentsCost action sleep apneaMedical certificateObstructive/complicationsmedicine.symptombusinessAutomobile Driving/legislation & jurisprudenceNarcolepsySleep medicine
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Biomineralix (COST action TD0903), 2009-2014: an overview.

2015

Biomineralization is the process by which living systems produce minerals. At theEuropean scale, this particular scientific field associates researchers of diverse horizons,ranging from zoology, mineralogy, palaeontology, and environmental sciences to materialssciences, dentistry and bone surgery. In this context, the COST Action TD0903, also referredas Biomineralix, was set up in November 2009 under the auspices of the COST Office inBrussels. This scientific network was active during four and half years, until May 2014. Itassociated 17 European countries, and a total of 29 laboratories. Its main objectives weremultiple: 1. To promote biochemical and proteomic research on the biomineralisat…

Engineeringbusiness.industryProcess (engineering)Mechanical EngineeringScale (chemistry)Environmental resource managementNanotechnologyContext (language use)[ SDV.IB.BIO ] Life Sciences [q-bio]/Bioengineering/BiomaterialsNatural (archaeology)Living systems[SDV.IB.BIO] Life Sciences [q-bio]/Bioengineering/BiomaterialsMechanics of Materials[ SDV.BBM.GTP ] Life Sciences [q-bio]/Biochemistry Molecular Biology/Genomics [q-bio.GN]Bone surgery[SDV.BBM.GTP] Life Sciences [q-bio]/Biochemistry Molecular Biology/Genomics [q-bio.GN]General Materials ScienceMarine ecosystemCost actionbusinessComputingMilieux_MISCELLANEOUS
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Network for blood pressure research in children and adolescents (COST Action CA 19115)

2021

High blood pressure is a clearly established modifiable risk factor for cardiovascular and renal disease. Although most of its adverse effects develop in adulthood, it has become clear that high BP is a lifelong problem that can manifest early in life. While few would dispute the importance of taking effective steps to identify and manage this condition in middle-aged and elderly individuals, relatively little attention has been paid to the problem of high BP in children and adolescents.Therefore, the development of actions focused on early childhood, childhood and adolescence and the investigation of the underlying causes of this epidemic are of utmost importance. There is a pressing need …

GerontologyAdultAdolescentRisk factors in diseasesmedia_common.quotation_subjectCOST ActionBlood PressureDiseaseAdolescentsPediatricsRisk AssessmentTeenagersRJ1-570Scarcity03 medical and health sciences0302 clinical medicineMultidisciplinary approachRisk Factors030225 pediatricsManagement of Technology and InnovationMedicineHumansCost actionEarly childhoodChildNiñosAdolescentesChildrenmedia_commonAgedPresión arterialbusiness.industryFactors de risc en les malaltiesRisk factor (computing)Middle AgedEuropeBlood pressureAction (philosophy)Child PreschoolHypertensionHipertensióbusinessInfants
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Crust-magnetosphere coupling during magnetar evolution and implications for the surface temperature

2018

We study the coupling of the force-free magnetosphere to the long-term internal evolution of a magnetar. We allow the relation between the poloidal and toroidal stream functions - that characterizes the magnetosphere - to evolve freely without constraining its particular form. We find that, on time-scales of the order of kyr, the energy stored in the magnetosphere gradually increases, as the toroidal region grows and the field lines expand outwards. This continues until a critical point is reached beyond which force-free solutions for the magnetosphere can no longer be constructed, likely leading to some large-scale magnetospheric reorganization. The energy budget available for such events …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomyMagnetosphereAstronomy and AstrophysicsCrustneutron [Stars]Magnetar01 natural sciencesmagnetars [Stars]magnetic field [Stars]Space and Planetary ScienceMagnetic fields0103 physical sciencesCost action010306 general physicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsAstronomía y Astrofísica
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Long-term evolution of the force-free twisted magnetosphere of a magnetar

2017

We study the long-term quasi-steady evolution of the force-free magnetosphere of a magnetar coupled to its internal magnetic field. We find that magnetospheric currents can be maintained on long timescales of the order of thousands of years. Meanwhile, the energy, helicity and twist stored in the magnetosphere all gradually increase over the course of this evolution, until a critical point is reached, beyond which a force-free magnetosphere cannot be constructed. At this point, some large-scale magnetospheric rearrangement, possibly resulting in an outburst or a flare, must occur, releasing a large fraction of the stored energy, helicity and twist. After that, the quasi-steady evolution sho…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomyMagnetosphereAstronomy and Astrophysicsneutron [Stars]AstrophysicsMagnetar01 natural sciencesMagnetic fieldTerm (time)magnetars [Stars]Space and Planetary ScienceMagnetic fieldsPhysics::Space Physics0103 physical sciencesCost actionMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsAstronomía y Astrofísica
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The force-free twisted magnetosphere of a neutron star – II. Degeneracies of the Grad–Shafranov equation

2017

We extend our previous study of equilibrium solutions of non-rotating force-free magnetospheres of neutron stars. We show that multiple solutions exist for the same sets of parameters, implying that the solutions are degenerate. We are able to obtain configurations with disconnected field lines, however, in nearly all cases these correspond to degenerate higher energy solutions. We carry out a wide parametric search in order to understand the properties of the solutions. We confirm our previous results that the lower energy solutions have up to $\sim 25\%$ more energy than the vacuum case, helicity of the order of $\sim 5$ (in some defined units), maximum twist of $\sim 1.5$ rad, and a dipo…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsWork (thermodynamics)MHDFOS: Physical sciencesMagnetosphereneutron [Stars]Astronomy and Astrophysics01 natural sciencesMagnetic fieldmagnetars [Stars]magnetic field [Stars]Neutron starGrad–Shafranov equationClassical mechanicsSpace and Planetary ScienceMagnetic fieldsQuantum electrodynamics0103 physical sciencesCost actionMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsAstronomía y AstrofísicaMonthly Notices of the Royal Astronomical Society
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Instability of twisted magnetar magnetospheres

2019

We present three-dimensional force-free electrodynamics simulations of magnetar magnetospheres that demonstrate the instability of certain degenerate, high energy equilibrium solutions of the Grad-Shafranov equation. This result indicates the existence of an unstable branch of twisted magnetospheric solutions and allows to formulate an instability criterion. The rearrangement of magnetic field lines as a consequence of this instability triggers the dissipation of up to 30% of the magnetospheric energy on a thin layer above the magnetar surface. During this process, we predict an increase of the mechanical stresses onto the stellar crust, which can potentially result in a global mechanical f…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsnumerical [Methods]bursts [X-rays]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and Astrophysicsneutron [Stars]MagnetarInstabilitymagnetars [Stars]Theoretical physicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsCost actionAstrophysics - High Energy Astrophysical PhenomenaPartial supportSolar and Stellar Astrophysics (astro-ph.SR)Astronomía y Astrofísica
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The force-free twisted magnetosphere of a neutron star

2016

We present a detailed analysis of the properties of twisted, force-free magnetospheres of non-rotating neutron stars, which are of interest in the modelling of magnetar properties and evolution. In our models the magnetic field smoothly matches to a current-free (vacuum) solution at some large external radius, and they are specifically built to avoid pathological surface currents at any of the interfaces. By exploring a large range of parameters, we find a few remarkable general trends. We find that the total dipolar moment can be increased by up to $40\%$ with respect to a vacuum model with the same surface magnetic field, due to the contribution of magnetospheric currents to the global ma…

MHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesMagnetosphere7. Clean energy01 natural sciences010305 fluids & plasmasNuclear physicsmagnetars [Stars]0103 physical sciencesmedia_common.cataloged_instanceCost actionEuropean union010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)media_commonAstronomía y AstrofísicaHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and Astrophysicsneutron [Stars]Magnetic fieldNeutron starAstrophysics - Solar and Stellar AstrophysicsWork (electrical)Space and Planetary ScienceMagnetic fieldsMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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Vector boson scattering: Recent experimental and theory developments

2018

This document summarises the talks and discussions happened during the VBSCan Split17 workshop, the first general meeting of the VBSCan COST Action network. This collaboration is aiming at a consistent and coordinated study of vector-boson scattering from the phenomenological and experimental point of view, for the best exploitation of the data that will be delivered by existing and future particle colliders.

Particle physicsStandard ModelGeneral Physics and AstronomyFOS: Physical sciencesvector boson: scatteringEWSB (Electroweak symmetry breaking); HEP; LHC; Standard Model; VBSLHC VBS HEP Standard Model EWSB (Electroweak symmetry breaking)01 natural sciences114 Physical sciencesVector bosonHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Point (geometry)Cost actionVBS010306 general physicsactivity reportParticle Physics - PhenomenologyPhysics010308 nuclear & particles physicsScatteringhep-exhep-phlcsh:QC1-999HEPHigh Energy Physics - PhenomenologyEWSB (Electroweak symmetry breaking)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]networkLHClcsh:PhysicsParticle Physics - Experiment
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