Search results for "prominence"

showing 7 items of 7 documents

Prominence vs. aboutness in sequencing: a functional distinction within the left inferior frontal gyrus

2009

Prior research on the neural bases of syntactic comprehension suggests that activation in the left inferior frontal gyrus (lIFG) correlates with the processing of word order variations. However, there are inconsistencies with respect to the specific subregion within the IFG that is implicated by these findings: the pars opercularisor the pars triangularis. Here, we examined the hypothesis that the dissociation between parsopercularis and pars triangularis activation may reflect functional differences between clause-medial and clause-initial word order permutations, respectively. To this end, we directly compared clause-medial and clause-initial object-before-subject orders in German in a wi…

AdultMaleLinguistics and LanguageDissociation (neuropsychology)Cognitive NeuroscienceExperimental and Cognitive Psychologyleft inferior frontal gyrusLeft inferior frontal gyrusFunctional LateralityLanguage and LinguisticsSpeech and HearingSuperior temporal gyrusHumansPrefrontal cortexaboutnessinformation structureLanguageBrain MappingLanguage TestsfMRICognitionsequencingGermanword orderMagnetic Resonance ImagingFrontal Lobesyntactic processingAboutnesssuperior temporal gyrusprominenceFemaleNerve NetComprehensionPsychologySentenceWord orderCognitive psychology
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Discovering prominence and its role in language processing: an individual (differences) approach

2015

Abstract It has been suggested that, during real time language comprehension, the human language processing system attempts to identify the argument primarily responsible for the state of affairs (the “actor”) as quickly and unambiguously as possible. However, previous work on a prominence (e.g. animacy, definiteness, case marking) based heuristic for actor identification has suffered from underspecification of the relationship between different cue hierarchies. Qualitative work has yielded a partial ordering of many features (e.g. MacWhinney et al. 1984), but a precise quantification has remained elusive due to difficulties in exploring the full feature space in a particular language. Feat…

Linguistics and Languagecomputational modelactor identificationAmbiguity resolutionambiguity resolutionprominencelanguage processingemergencePsychologyindividual differencesLanguage and LinguisticsLinguistics
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In Situ Generation of Transverse Magnetohydrodynamic Waves from Colliding Flows in the Solar Corona

2018

This research has received funding from the UK Science and Technology Facilities Council (Consolidated Grant ST/K000950/1) and the European Union Horizon 2020 Research and Innovation Programme (grant agreement No. 647214). V.M.N. acknowledges the support of the BK21 plus program through the National Research Foundation funded by the Ministry of Education of Korea. Transverse magnetohydrodynamic (MHD) waves permeate the solar atmosphere and are a candidate for coronal heating. However, the origin of these waves is still unclear. In this Letter, we analyze coordinated observations from Hinode/Solar Optical Telescope (SOT) and Interface Region Imaging Spectrograph (IRIS) of a prominence/corona…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesF300NDASEnergy fluxF500magnetohydrodynamics (MHD)01 natural sciencesSolar prominenceSun: activity0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsCoronal rainwavesactivity [Sun]Magnetohydrodynamic drive010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsSun: coronaoscillations [Sun]Sun:oscillationsAstronomy and AstrophysicsPlasmaSun: filaments prominencesMagnetic fieldComputational physicsTransverse planeQC PhysicsSpace and Planetary SciencePhysics::Space PhysicsWavesfilaments prominences [Sun]MagnetohydrodynamicsThe Astrophysical Journal
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Simulating AIA observations of a flux rope ejection

2014

D.H.M. would like to thank STFC, the Leverhulme Trust and the European Commission’s Seventh Framework Programme (FP7/2007-2013) for their financial support. P.P. would like to thank the European Commission’s Seventh Framework Programme (FP7/2007-2013) under grant agreement SWIFF (project 263340, http://www.swiff.eu) and STFC for financial support. These results were obtained in the framework of the projects GOA/2009-009 (KU Leuven), G.0729.11 (FWO-Vlaanderen) and C 90347 (ESA Prodex 9). The research leading to these results has also received funding from the European Commission’s Seventh Framework Programme (FP7/2007-2013) under the grant agreements SOLSPANET (project No. 269299, http:// ww…

Magnetohydrodynamics (MHD)corona [Sun]Sun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysicsmagnetohydrodynamics (MHD)7. Clean energyProminencesObservatoryRadiative transferQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsQASun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)QBPhysicsUV radiation [Sun]Line-of-sightSun: coronaAstronomy and AstrophysicsPlasmaSun: UV radiationCoronacoronal mass ejections (CMEs) [Sun]Magnetic fluxSun: filamentsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]13. Climate actionSpace and Planetary ScienceExtreme ultravioletPhysics::Space Physicsfilaments prominences [Sun]Rope
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Future capabilities of CME polarimetric 3D reconstructions with the METIS instrument: A numerical test

2015

D.H.M. would like to thank STFC and the Leverhulme Trust for their financial support. P.P. would like to thank STFC and the Leverhulme Trust. The computational work for this paper was carried out on the joint STFC and SFC (SRIF) funded cluster at the University of St Andrews (Scotland, UK). Context. Understanding the 3D structure of coronal mass ejections (CMEs) is crucial for understanding the nature and origin of solar eruptions. However, owing to the optical thinness of the solar corona we can only observe the line of sight integrated emission. As a consequence the resulting projection effects hide the true 3D structure of CMEs. To derive information on the 3D structure of CMEs from whit…

Magnetohydrodynamics (MHD)corona [Sun]Sun: coronal mass ejections (CMEs)Sun: filaments prominencesNDASFOS: Physical sciencesLibrary scienceAstrophysicspolarimetric [Techniques]MetisQB AstronomyAstrophysics::Solar and Stellar AstrophysicsNumerical testsQCSolar and Stellar Astrophysics (astro-ph.SR)QBPhysicsSun: coronaTechniques: polarimetricAstronomy and Astrophysicscoronal mass ejections (CMEs) [Sun]QC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space Physicsfilaments prominences [Sun]
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PROMINENCE PLASMA DIAGNOSTICS THROUGH EXTREME-ULTRAVIOLET ABSORPTION

2013

In this paper we introduce a new diagnostic technique that uses prominence EUV and UV absorption to determine the prominence plasma electron temperature and column emission measure, as well as He/H relative abundance; if a realistic assumption on the geometry of the absorbing plasma can be made, this technique can also yield the absorbing plasma electron density. This technique capitalizes on the absorption properties of Hydrogen and Helium at different wavelength ranges and temperature regimes. Several cases where this technique can be successfully applied are described. This technique works best when prominence plasmas are hotter than 15,000 K and thus it is ideally suited for rapidly hea…

Physics010308 nuclear & particles physicsExtreme ultraviolet lithographySolar Physicschemistry.chemical_elementAstronomy and AstrophysicsAstrophysicsPlasma7. Clean energy01 natural sciencesSolar prominenceComputational physicsAstrophysicWavelengthSettore FIS/05 - Astronomia E AstrofisicachemistrySpace and Planetary Science0103 physical sciencesCoronal mass ejectionPlasma diagnosticsAstrophysics; Solar PhysicsAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsHelium
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Marcatge posicional i prominència en el vocalisme àton

2008

It has long been noticed that more perceptible elements tend to associate to positions that are structurally stronger to the end that several prominent features converge in the same site; and vice versa: elements of low perceptibility prototypically associate to less prominent positions ("positional markedness"). The main aim of this paper is to present the effects of positional markedness in the a-tonic vowel system of Catalan through the analysis of two cases that have not been studied in depth, i.e. the occurrence of different epenthetic vowels according to the position in which they appear in Alghero and western Catalan, and the presence of different patterns of vowel reduction in weste…

lcsh:Language and LiteratureFonologiaCatalan languageUNESCO::CIENCIAS DE LAS ARTES Y LAS LETRASLingüísticaPositional markedness; prominence; epenthesis; vowel reductionFilologíasVocalsmusculoskeletal neural and ocular physiologyPositional markednessepenthesisPhonologybehavioral disciplines and activitiesCatalà parlatlcsh:Philology. LinguisticsCatalàprominencelcsh:P1-1091:CIENCIAS DE LAS ARTES Y LAS LETRAS [UNESCO]mental disorderslcsh:Pvowel reductionVowelspsychological phenomena and processes
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