902 resultados para Richards Cabin


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This paper presents the swelling behaviour of clayey materials under controlled suction imposed both by a Richards chamber and by controlling the relative humidity with concentrated saline solutions. Soil-water characteristic curves (matrix and total) were determined by the filter paper method. The materials under study belong to the Guabirotuba Formation, of Pleistocene age, in the Curitiba Basin in the state of Parana, southern Brazil. Materials under several stages of suction of 5000-40 000 kPa were subjected to swelling tests in an oedometer press. The results indicated that the greater the suction the higher the swelling pressure. However, when swelling tests were carried out with suction variation controlled by relative humidity, in which the increase in moisture was very slow, the samples showed no swelling.

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Patients with rare and complex diseases such as congenital adrenal hyperplasia (CAH) often receive fragmented and inadequate care unless efforts are coordinated among providers. Translating the concepts of the medical home and comprehensive health care for individuals with CAH offers many benefits for the affected individuals and their families. This manuscript represents the recommendations of a 1.5 day meeting held in September 2009 to discuss the ideal goals for comprehensive care centers for newborns, infants, children, adolescents, and adults with CAH. Participants included pediatric endocrinologists, internal medicine and reproductive endocrinologists, pediatric urologists, pediatric surgeons, psychologists, and pediatric endocrine nurse educators. One unique aspect of this meeting was the active participation of individuals personally affected by CAH as patients or parents of patients. Representatives of Health Research and Services Administration (HRSA), New York-Mid-Atlantic Consortium for Genetics and Newborn Screening Services (NYMAC), and National Newborn Screening and Genetics Resource Center (NNSGRC) also participated. Thus, this document should serve as a "roadmap" for the development phases of comprehensive care centers (CCC) for individuals and families affected by CAH.

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Review paper and Proceedings of the Inaugural Meeting of the Head and Neck Optical Diagnostics Society (HNODS) on March 14th 2009 at University College London.

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The complete surgical removal of disease is a desirable outcome particularly in oncology. Unfortunately much disease is microscopic and difficult to detect causing a liability to recurrence and worsened overall prognosis with attendant costs in terms of morbidity and mortality. It is hoped that by advances in optical diagnostic technology we could better define our surgical margin and so increase the rate of truly negative margins on the one hand and on the other hand to take out only the necessary amount of tissue and leave more unaffected non-diseased areas so preserving function of vital structures. The task has not been easy but progress is being made as exemplified by the presentations at the 2nd Scientific Meeting of the Head and Neck Optical Diagnostics Society (HNODS) in San Francisco in January 2010. We review the salient advances in the field and propose further directions of investigation.

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While histopathology of excised tissue remains the gold standard for diagnosis, several new, non-invasive diagnostic techniques are being developed. They rely on physical and biochemical changes that precede and mirror malignant change within tissue. The basic principle involves simple optical techniques of tissue interrogation. Their accuracy, expressed as sensitivity and specificity, are reported in a number of studies suggests that they have a potential for cost effective, real-time, in situ diagnosis.

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Epithelial cells are mainly responsible for the formation of tissues that cover the external and internal surfaces of organs like skin, lining of the lungs and intestines. The cells must adhere to substrates and to each other in compliance with certain stimulus. In this way, adhesion properties can be regulated by the cell which simultaneously senses the chemical and mechanical properties of its environment. Their adhesion and growth on biomaterials depends on substrate properties such as surface wettability, topography and chemistry. The aim of this study is to investigate cell-surface interactions using several materials and different surfaces.

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Quasars and AGN play an important role in many aspects of the modern cosmology. Of particular interest is the issue of the interplay between AGN activity and formation and evolution of galaxies and structures. Studies on nearby galaxies revealed that most (and possibly all) galaxy nuclei contain a super-massive black hole (SMBH) and that between a third and half of them are showing some evidence of activity (Kormendy and Richstone, 1995). The discovery of a tight relation between black holes mass and velocity dispersion of their host galaxy suggests that the evolution of the growth of SMBH and their host galaxy are linked together. In this context, studying the evolution of AGN, through the luminosity function (LF), is fundamental to constrain the theories of galaxy and SMBH formation and evolution. Recently, many theories have been developed to describe physical processes possibly responsible of a common formation scenario for galaxies and their central black hole (Volonteri et al., 2003; Springel et al., 2005a; Vittorini et al., 2005; Hopkins et al., 2006a) and an increasing number of observations in different bands are focused on collecting larger and larger quasar samples. Many issues remain however not yet fully understood. In the context of the VVDS (VIMOS-VLT Deep Survey), we collected and studied an unbiased sample of spectroscopically selected faint type-1 AGN with a unique and straightforward selection function. Indeed, the VVDS is a large, purely magnitude limited spectroscopic survey of faint objects, free of any morphological and/or color preselection. We studied the statistical properties of this sample and its evolution up to redshift z 4. Because of the contamination of the AGN light by their host galaxies at the faint magnitudes explored by our sample, we observed that a significant fraction of AGN in our sample would be missed by the UV excess and morphological criteria usually adopted for the pre-selection of optical QSO candidates. If not properly taken into account, this failure in selecting particular sub-classes of AGN could, in principle, affect some of the conclusions drawn from samples of AGN based on these selection criteria. The absence of any pre-selection in the VVDS leads us to have a very complete sample of AGN, including also objects with unusual colors and continuum shape. The VVDS AGN sample shows in fact redder colors than those expected by comparing it, for example, with the color track derived from the SDSS composite spectrum. In particular, the faintest objects have on average redder colors than the brightest ones. This can be attributed to both a large fraction of dust-reddened objects and a significant contamination from the host galaxy. We have tested these possibilities by examining the global spectral energy distribution of each object using, in addition to the U, B, V, R and I-band magnitudes, also the UV-Galex and the IR-Spitzer bands, and fitting it with a combination of AGN and galaxy emission, allowing also for the possibility of extinction of the AGN flux. We found that for 44% of our objects the contamination from the host galaxy is not negligible and this fraction decreases to 21% if we restrict the analysis to a bright subsample (M1450 <-22.15). Our estimated integral surface density at IAB < 24.0 is 500 AGN per square degree, which represents the highest surface density of a spectroscopically confirmed sample of optically selected AGN. We derived the luminosity function in B-band for 1.0 < z < 3.6 using the 1/Vmax estimator. Our data, more than one magnitude fainter than previous optical surveys, allow us to constrain the faint part of the luminosity function up to high redshift. A comparison of our data with the 2dF sample at low redshift (1 < z < 2.1) shows that the VDDS data can not be well fitted with the pure luminosity evolution (PLE) models derived by previous optically selected samples. Qualitatively, this appears to be due to the fact that our data suggest the presence of an excess of faint objects at low redshift (1.0 < z < 1.5) with respect to these models. By combining our faint VVDS sample with the large sample of bright AGN extracted from the SDSS DR3 (Richards et al., 2006b) and testing a number of different evolutionary models, we find that the model which better represents the combined luminosity functions, over a wide range of redshift and luminosity, is a luminosity dependent density evolution (LDDE) model, similar to those derived from the major Xsurveys. Such a parameterization allows the redshift of the AGN density peak to change as a function of luminosity, thus fitting the excess of faint AGN that we find at 1.0 < z < 1.5. On the basis of this model we find, for the first time from the analysis of optically selected samples, that the peak of the AGN space density shifts significantly towards lower redshift going to lower luminosity objects. The position of this peak moves from z 2.0 for MB <-26.0 to z 0.65 for -22< MB <-20. This result, already found in a number of X-ray selected samples of AGN, is consistent with a scenario of “AGN cosmic downsizing”, in which the density of more luminous AGN, possibly associated to more massive black holes, peaks earlier in the history of the Universe (i.e. at higher redshift), than that of low luminosity ones, which reaches its maximum later (i.e. at lower redshift). This behavior has since long been claimed to be present in elliptical galaxies and it is not easy to reproduce it in the hierarchical cosmogonic scenario, where more massive Dark Matter Halos (DMH) form on average later by merging of less massive halos.

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[ES] Las líneas generales de la larga y compleja historia volcánica de las islas Canarias son bien conocidas (IIartung, 1857; IIausen, 1956 a 1973; Fuster et d., 1968 a la actualidad; Rothe, 1974;Schmincke, 1976). Sin embargo, los depósitos marinos antiguos de abundante contenido fósil, conocidos y estudiados parcialmente desde el siglo pasado, se han interpretado incorrectamente (Crofts, 1967 ; Lecointre, Tinkler y Richards, 1967 ; Klug, 1968; Müller y Tietz, 1975). La cronologia geológica del archipiélago se basaba al principio sólo en los datos paleontol6gicos (Lyell, 1864; Rothpletz y Simonelli, 1890). Hoy, con las dataciones radiomPtricas y el estudio del paleornagnetismo (Abdel Monen et al., 1971, 1972; Rona y NorwaId, 1970; Lietz y Schemincke, 1975; Mac Dougall y Schmincke, 1977), se ha minusvalorado la paleontología, quizá por medir el tiempo con una precisión menos espectacular, aunque no siempre menos exacta.

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In der vorliegenden Arbeit werden zwei physikalischeFließexperimente an Vliesstoffen untersucht, die dazu dienensollen, unbekannte hydraulische Parameter des Materials, wiez. B. die Diffusivitäts- oder Leitfähigkeitsfunktion, ausMeßdaten zu identifizieren. Die physikalische undmathematische Modellierung dieser Experimente führt auf einCauchy-Dirichlet-Problem mit freiem Rand für die degeneriertparabolische Richardsgleichung in derSättigungsformulierung, das sogenannte direkte Problem. Ausder Kenntnis des freien Randes dieses Problems soll dernichtlineare Diffusivitätskoeffizient derDifferentialgleichung rekonstruiert werden. Für diesesinverse Problem stellen wir einOutput-Least-Squares-Funktional auf und verwenden zu dessenMinimierung iterative Regularisierungsverfahren wie dasLevenberg-Marquardt-Verfahren und die IRGN-Methode basierendauf einer Parametrisierung des Koeffizientenraumes durchquadratische B-Splines. Für das direkte Problem beweisen wirunter anderem Existenz und Eindeutigkeit der Lösung desCauchy-Dirichlet-Problems sowie die Existenz des freienRandes. Anschließend führen wir formal die Ableitung desfreien Randes nach dem Koeffizienten, die wir für dasnumerische Rekonstruktionsverfahren benötigen, auf einlinear degeneriert parabolisches Randwertproblem zurück.Wir erläutern die numerische Umsetzung und Implementierungunseres Rekonstruktionsverfahrens und stellen abschließendRekonstruktionsergebnisse bezüglich synthetischer Daten vor.

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Il fulcro tematico e concettuale della tesi consiste nel rapporto complesso, paradossale e spesso anche controverso esistente fra il teatro e la performance (art) – e cioè il rapporto fra i concetti di “teatralità” e di “performatività”. L’attenzione è posta su quelle correnti nelle arti performative contemporanee che tendono allo scioglimento delle nozioni di genere, disciplina, tecnica e autorialità e che mettono in questione lo status stesso dell’opera performativa (lo spettacolo) in quanto prodotto esclusivamente estetico, cioè spettacolare. Vengono esaminate – prelevando rispettivamente dal campo del teatro, della danza e della performance art – le pratiche di Jerzy Grotowski e Thomas Richards, Jérôme Bel e Marina Abramović. Quello che accomuna queste pratiche ben diverse tra loro non è soltanto la problematica del rapporto fra teatralità e performatività ma soprattutto l’aspetto particolarmente radicale e assiduo (e anche paradossale) del loro doppio sforzo, che consiste nello spingere la propria disciplina oltre ogni confine prestabilito e nello stesso tempo nel cercare di ri-definire i suoi codici fondanti e lo statuto ontologico che la distinguerebbero dalle altre discipline performative. Sono esaminate anche diverse teorizzazioni della performance con particolare attenzione a quei contributi che mettono in luce (e in questione) il delicato rapporto fra il teatro e la performance (art) attraverso una (ri)concettualizzazione e comparazione dei termini di teatralità e di performatività. La tesi esamina l’evoluzione della comprensione di quel rapporto all’interno del campo teorico-storico e artistico che inizialmente riflette la tendenza a percepire il rapporto in termini di opposizione e addirittura esclusione per approdare col tempo a una visione più riconciliante e complementare. Le radicali pratiche contemporanee fra il teatro e la performance rappresentano forse una nuova forma-processo performativa specifica e autonoma – che potrebbe essere definita tout court “performance” – e con cui viene definitivamente superato il progetto teatrale modernista?

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Nel 1932 Ernst Robert Curtius pubblica il pamphlet politico culturale Deutscher Geist in Gefahr nel quale chiarisce il suo pensiero di fronte alla grave crisi in cui versa la Germania. Egli si schiera contro le posizioni di destra del suo tempo, delle quali critica apertamente la boria nazionalista, il rozzo antisemitismo e la creazione di un mito nazionale elaborato come strumento di manipolazione dell’opinione pubblica. Ritiene inoltre inaccettabili le posizioni rivoluzionarie, tanto di destra quanto di sinistra, che vogliono liberarsi della tradizione umanistica europea e disprezzano la Zivilisation francese; allo stesso modo rifiuta l’ideale di un germanesimo eroico avulso dalla storia europea e respinge infine tutte le forme di nichilismo che si risolvono in un atteggiamento di indifferenza nei confronti della realtà, dei valori e della storia. Curtius accetta il sistema democratico come unica soluzione e ritiene che le decisioni politiche debbano mirare al bene di tutti i ceti sociali indipendentemente dagli interessi di partiti e di singoli gruppi. Rifiuta qualunque forma, anche culturale, di supremazia della Germania, aspira a un’Europa cosmopolita, le cui nazioni siano valorizzate nelle loro caratteristiche specifiche, ed è convinto che per la costruzione della pace gli europei debbano vivere, studiare e lavorare insieme imparando gli uni le lingue degli altri. Per Curtius l’Umanesimo della tradizione classica e la letteratura del Medioevo sono parte integrante della vita di ogni europeo e fonte di energie spirituali per affrontare in modo creativo il presente e il futuro.

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To evaluate the use of computer-assisted designed and manufactured (CAD/CAM) orbital wall and floor implants for late reconstruction of extensive orbital fractures.

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http://www.ncbi.nlm.nih.gov/pubmed/20014309