580 resultados para V1
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See README.TXT file for more details. Unpack and move resulting folder into your Minecraft 'saves' folder.
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Resumen tomado de la publicación
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QUAGMIRE is a quasi-geostrophic numerical model for performing fast, high-resolution simulations of multi-layer rotating annulus laboratory experiments on a desktop personal computer. The model uses a hybrid finite-difference/spectral approach to numerically integrate the coupled nonlinear partial differential equations of motion in cylindrical geometry in each layer. Version 1.3 implements the special case of two fluid layers of equal resting depths. The flow is forced either by a differentially rotating lid, or by relaxation to specified streamfunction or potential vorticity fields, or both. Dissipation is achieved through Ekman layer pumping and suction at the horizontal boundaries, including the internal interface. The effects of weak interfacial tension are included, as well as the linear topographic beta-effect and the quadratic centripetal beta-effect. Stochastic forcing may optionally be activated, to represent approximately the effects of random unresolved features. A leapfrog time stepping scheme is used, with a Robert filter. Flows simulated by the model agree well with those observed in the corresponding laboratory experiments.
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The Fourier-transform spectrum of CH3F from 2800 to 3100 cm−1, obtained by Guelachvili in Orsay at a resolution of about 0.003 cm−1, was analyzed. The effective Hamiltonian used contained all symmetry allowed interactions up to second order in the Amat-Nielsen classification, together with selected third-order terms, amongst the set of nine vibrational basis functions represented by the states ν1(A1), ν4(E), 2ν2(A1), ν2 + ν5(E), 2ν50(A1), and 2ν5±2(E). A number of strong Fermi and Coriolis resonances are involved. The vibrational Hamiltonian matrix was not factorized beyond the requirements of symmetry. A total of 59 molecular parameters were refined in a simultaneous least-squares analysis to over 1500 upper-state energy levels for J ≤ 20 with a standard deviation of 0.013 cm−1. Although the standard deviation remains an order of magnitude greater than the precision of the measurements, this work breaks new ground in the simultaneous analysis of interacting symmetric top vibrational levels, in terms of the number of interacting vibrational states and the number of parameters in the Hamiltonian.
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We describe a FORTRAN-90 program that computes scattering t-matrices for a molecule. These can be used in a Low-Energy Electron Diffraction program to solve the molecular structural problem very efficiently. The intramolecular multiple scattering is computed within a Dyson-like approach, using free space Green propagators in a basis of spherical waves. The advantage of this approach is related to exploiting the chemical identity of the molecule, and to the simplicity to translate and rotate these t-matrices without performing a new multiple-scattering calculation for each configuration. FORTRAN-90 routines for rotating the resulting t-matrices using Wigner matrices are also provided.
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We describe a FORTRAN-90 program to compute low-energy electron diffraction I(V) curves. Plane-waves and layer doubling are used to compute the inter-layer multiple-scattering, while the intra-layer multiple-scattering is computed in the standard way expanding the wavefield on a basis of spherical waves. The program is kept as general as possible, in order to allow testing different parts of multiple-scattering calculations. In particular, it can handle non-diagonal t-matrices describing the scattering of non-spherical potentials, anisotropic vibrations, anharmonicity, etc. The program does not use old FORTRAN flavours, and has been written keeping in mind the advantage for parallelism brought forward by FORTRAN-90.
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In addition to CO2, the climate impact of aviation is strongly influenced by non-CO2 emissions, such as nitrogen oxides, influencing ozone and methane, and water vapour, which can lead to the formation of persistent contrails in ice-supersaturated regions. Because these non-CO2 emission effects are characterised by a short lifetime, their climate impact largely depends on emission location and time; that is to say, emissions in certain locations (or times) can lead to a greater climate impact (even on the global average) than the same emission in other locations (or times). Avoiding these climate-sensitive regions might thus be beneficial to climate. Here, we describe a modelling chain for investigating this climate impact mitigation option. This modelling chain forms a multi-step modelling approach, starting with the simulation of the fate of emissions released at a certain location and time (time-region grid points). This is performed with the chemistry–climate model EMAC, extended via the two submodels AIRTRAC (V1.0) and CONTRAIL (V1.0), which describe the contribution of emissions to the composition of the atmosphere and to contrail formation, respectively. The impact of emissions from the large number of time-region grid points is efficiently calculated by applying a Lagrangian scheme. EMAC also includes the calculation of radiative impacts, which are, in a second step, the input to climate metric formulas describing the global climate impact of the emission at each time-region grid point. The result of the modelling chain comprises a four-dimensional data set in space and time, which we call climate cost functions and which describes the global climate impact of an emission at each grid point and each point in time. In a third step, these climate cost functions are used in an air traffic simulator (SAAM) coupled to an emission tool (AEM) to optimise aircraft trajectories for the North Atlantic region. Here, we describe the details of this new modelling approach and show some example results. A number of sensitivity analyses are performed to motivate the settings of individual parameters. A stepwise sanity check of the results of the modelling chain is undertaken to demonstrate the plausibility of the climate cost functions.
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The atmospheric carbon dioxide concentration plays a crucial role in the radiative balance and as such has a strong influence on the evolution of climate. Because of the numerous interactions between climate and the carbon cycle, it is necessary to include a model of the carbon cycle within a climate model to understand and simulate past and future changes of the carbon cycle. In particular, natural variations of atmospheric CO2 have happened in the past, while anthropogenic carbon emissions are likely to continue in the future. To study changes of the carbon cycle and climate on timescales of a few hundred to a few thousand years, we have included a simple carbon cycle model into the iLOVECLIM Earth System Model. In this study, we describe the ocean and terrestrial biosphere carbon cycle models and their performance relative to observational data. We focus on the main carbon cycle variables including the carbon isotope ratios δ13C and the Δ14C. We show that the model results are in good agreement with modern observations both at the surface and in the deep ocean for the main variables, in particular phosphates, dissolved inorganic carbon and the carbon isotopes.
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The Open Provenance Model is a model of provenance that is designed to meet the following requirements: (1) To allow provenance information to be exchanged between systems, by means of a compatibility layer based on a shared provenance model. (2) To allow developers to build and share tools that operate on such a provenance model. (3) To define provenance in a precise, technology-agnostic manner. (4) To support a digital representation of provenance for any 'thing', whether produced by computer systems or not. (5) To allow multiple levels of description to coexist. (6) To define a core set of rules that identify the valid inferences that can be made on provenance representation. This document contains the specification of the Open Provenance Model (v1.1) resulting from a community-effort to achieve inter-operability in the Provenance Challenge series.
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In the present investigation we mapped the primary visual area of the South American diurnal rodent, Dasyprocta aguti, by standardized electrophysiological mapping techniques. In particular, we performed a series of mapping experiments of the visual streak in the primary visual cortex. We found that the representation of the visual streak in V1 is greatly expanded, the nasal 10 degrees of the visual streak representation occupies ten times more cortical area than equivalent areas in the central or temporal representation. Comparison of these data with those on the density of ganglion cells in the retina at corresponding locations in the visual field reveal a significant mismatch between these two variables. The nasal representation is greatly expanded along the horizontal meridian in V1 as compared to the central and temporal regions whereas the density of ganglion cells decreases with progression along the visual streak from central region towards the nasal or temporal visual field. A review of the available data reveals that all lateral-eyed mammals exhibit a similar mismatch between the retinal and cortical representation of the visual field, and this mismatches is greater in those species with well defined visual streaks such as rabbit and agouti.
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In questa tesi viene presentata un’analisi dettagliata sulla struttura di profili recettori di neuroni coinvolti nell’elaborazione visiva, con particolare attenzione per le cellule appartenenti alla corteccia visiva primaria (V1). Dopo aver illustrato brevemente il percorso effettuato dall’informazione visiva, costituito da retina, nucleo genicolato laterale e V1, vengono descritte la struttura e le principali caratteristiche di profili recettori dei neuroni appartenenti ad ognuno di questi livelli di elaborazione. Per modellare i profili recettori di cellule corticali in V1 si è deciso di utilizzare filtri bidimensionali realizzati mediante funzioni di Gabor nel dominio spaziale. Questo modello ha, infatti, il grande vantaggio di possedere alcune tra le maggiori proprietà dei profili recettori di neuroni appartenenti a V1: struttura del profilo recettore nello spazio (x,y), selettività in orientazione e in frequenza spaziale, indipendenza dalla fase dello stimolo. Viene successivamente presentato il concetto di campo di associazione visivo, mediante il quale sono determinate le caratteristiche principali (posizione spaziale ed orientazione) che diversi oggetti devono possedere per essere percepiti non come unità singole, ma come un unico elemento. I campi di associazione possono essere modellati mediante l’utilizzo del sistema di equazioni differenziali proposto da Citti-Sarti, le cui soluzioni sono curve integrali adatte a ricostruire la struttura dei campi di associazione, come proposti da Field, Hayes ed Hess. Diverse ipotesi sono state presentate su come cellule appartenenti a V1 siano in grado di realizzare simili campi di associazione, ed in particolare, da dove queste possano prendere le informazioni necessarie per farlo. Una di queste è quella sostenuta dai dati di Bosking et al., secondo i quali le connessioni intracorticali più fitte sono quelle tra neuroni non adiacenti tra loro, i cui profili recettori sono co-orientati (con la stessa orientazione preferenziale) e co-assiali (disposti lungo un asse del campo visivo che corrisponde all’orientazione preferenziale). L’analisi effettuata in questa tesi ha come obbiettivo proprio quello di ottenere informazioni utili su come cellule corticali siano legate alla fenomenologia dei campi di associazione. Come già detto, un filtro di Gabor bidimensionale può essere considerato un buon modello per profili recettori di questo tipo di cellule e quindi è possibile definirlo in maniera astratta come l’unità fondamentale nel processo di elaborazione visiva. Per questo motivo viene effettuata un’analisi di cross-correlazione tra un filtro di Gabor con una determinata orientazione e una famiglia di filtri di Gabor aventi n orientazioni. I risultati ottenuti sono stati trattati utilizzando la tecnica di soppressione dei non massimi, in modo da estrarre per ogni punto dell’immagine l’orientazione per la quale si ottiene la risposta massima. Successivamente, dai dati è stato possibile calcolare delle curve integrali simili a quelle ottenute dal modello differenziale proposto da Citti-Sarti. I risultati ottenuti da questa analisi si sono rivelati utili per comprendere più nel dettaglio i processi di elaborazione dei neuroni corticali, ed in particolare, per capire in che modo le informazioni necessarie per la realizzazione di strutture complesse ed articolate come quelle dei campi di associazione, siano già contenute intrinsecamente all’interno di ogni cellula corticale, unità fondamentale dell’elaborazione visiva.
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Il progetto di ricerca che ho svolto in questi mesi si è focalizzato sull'integrazione dei risultati raggiunti grazie all'elaborazione di nuovi dati sperimentali. Questi sono stati prelevati dalla corteccia visiva di macachi, attraverso l'utilizzo di tecniche di registrazione elettro-fisiologiche mediante array di micro-elettrodi[25], durante la presentazionedi alcuni filmati (sequenze di immagini o frames). Attraverso la tecnica del clustering, dalle registrazioni degli esperimenti sono stati raggruppati gli spike appartenenti ad uno stesso neurone, sfruttando alcune caratteristiche come la forma del potenziale d'azione. Da questa elaborazione e stato possibile risalire a quali stimoli hanno prodotto una risposta neurale. I dati messi a disposizione da Ringach non potevano essere trattati direttamente con le tecniche della spike-triggered average e della spike-triggered covariance a causa di alcune loro caratteristiche. Utilizzando filtri di Gabor bidimensionali e l'energia di orientazione e stato pero possibile modellare la risposta di cellule complesse in corteccia visiva primaria. Applicare questi modelli su dati ad alta dimensionalita immagini molto grandi), sfruttando la tecnica di standardizzazione (Z-score), ha permesso di individuare la regione, la scala e l'orientazione all'interno del piano immagine dei profili recettivi delle cellule di cui era stata registrata l'attività neurale. Ritagliare tale regione e applicare la spike-triggered covariance su dati della giusta dimensionalita, permetterebbe di risalire ai profili recettivi delle cellule eccitate in un preciso momento, da una specifica immagine e ad una precisa scala e orientazione. Se queste ipotesi venissero confermate si potrebbe marcare e rafforzare la bontà del modello utilizzato per le cellule complesse in V1 e comprendere al meglio come avviene l'elaborazione delle immagini.
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We update the forcings for the PMIP3 experiments for the Last Millennium to include new assessments of historical land use changes and discuss new suggestions for calibrating solar activity proxies to total solar irradiance.
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Histological serial sections, three-dimensional reconstructions and morphometry served to study the postnatal development of V1 in tree shrews. The main objectives were to evaluate the expansion of V1, the implications of its growth on the occipital cortex and, vice versa, the effects of the expanding neocortex on the topography of V1. The future V1 was identified on postnatal day 1 by its granular layer IV, covering the superior surface of the occipital cortices including the poles. A subdivision of layer IV, distinctive for the binocular part, was evident in the central region. V1 expanded continuously with age into all directions succeeded by the maturation of layering. The monocular part was recognized from day 15 onward, after the binocular part had reached its medial border. In reference to the retinotopic map of V1, regions emerged in a coherent temporo-spatial sequence delineating the retinal topography in a central to peripheral gradient beginning with the visual streak representation. The growth of V1 was greatest until tree shrews open their eyes, culminated during adolescence, and completed after a subsequent decrease in the young adult. Simultaneous expansion of the neocortex induced a shifting of V1. Translation and elongation of V1 entailed that the occipital cortex covered the superior colliculi along with a downward rotation of the poles. The enlargement of the occipital part of the hemispheres was in addition associated with the formation of a small occipital horn in the lateral ventricles, indicating an incipient 'true' occipital lobe harbouring mainly cortices involved in visual functions.