969 resultados para HIGH-CONTRAST ELECTROCHROMISM


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The silicon-based gate-controlled lateral bipolar junction transistor (BJT) is a controllable four-terminal photodetector with very high responsivity at low-light intensities. It is a hybrid device composed of a MOSFET, a lateral BJT, and a vertical BJT. Using sufficient gate bias to operate the MOS transistor in inversion mode, the photodetector allows for increasing the photocurrent gain by 106 at low light intensities when the base-emitter voltage is smaller than 0.4 V, and BJT is off. Two operation modes, with constant voltage bias between gate and emitter/source terminals and between gate and base/body terminals, allow for tuning the photoresponse from sublinear to slightly above linear, satisfying the application requirements for wide dynamic range, high-contrast, or linear imaging. MOSFETs from a standard 0.18-μm triple-well complementary-metal oxide semiconductor technology with a width to length ratio of 8 μm /2 μm and a total area of ∼ 500μm2 are used. When using this area, the responsivities are 16-20 kA/W. © 2001-2012 IEEE.

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Neste trabalho são apresentadas expressões exatas e aproximações quadráticas das conhecidas equações de Knott-Zöeppritz, que calculam as amplitudes dos coeficientes Rpp e Rsp em termos dos contrastes médios relativos, bem como é procedida a inversão dos parâmetros de dados de AVO a partir destas aproximações quadráticas. Nesta inversão é utilizado o algoritmo de Levenberg-Marquardt, e são considerados apenas os eventos refletidos Rpp e convertidos Rsp, não associados. Nos estudos dos parâmetros físicos dos meios contrastes de impedância (δz), módulo de cisalhamento (δμ) e velocidade da onda p (δα), verificou-se quais desses parâmetros podem ser invertidos. Os resultados obtidos mostram que o contraste de impedância (δz) é muito bem resolvido estando ele relacionado com o contraste de velocidade da onda p (δα) ou com o contraste de cisalhamento (δμ), no caso de eventos refletidos considerando modelos de alto, moderado e baixo contrastes. Por outro lado ao se fixar o contraste de impedância e relacionar os outros dois parâmetros em consideração, os resultados mostram que esses são mal resolvidos, ou seja, a região de ambiguidade torna-se muito grande e os parâmetros tornam-se ambíguos e instáveis. No caso do evento convertido e na combinação do evento refletido com o convertido, para os modelos de baixo e moderado contrastes, (δz) é muito bem resolvido, caso que não acontece para modelo de alto contraste. Diante desses resultados verifica-se que no procedimento de inversão quadrática de dados de AVO, fixado (δμ), a recuperação dos dois parâmetros variados é muito boa, no caso do evento refletido, e razoavelmente boa no caso do evento convertido, por esse motivo optou-se pela fixação do módulo de cisalhamento.

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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

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This text reflects on the techniques and the process of image production and its artistic composition to digital television in high defini- tion, whereas the 4:3 and 16:9 formats will exist until shutdown of the analog signal. Within this period, consumers of television programming that have analog receivers will continue to see the images in 4:3 format. That fact determines that the productions in high definition, while capturing images with larger viewing area and have high contrast ratio (>1000:1) must be main- tain the elements of visual storytelling within the smallest area and with the contrast ratio of the analog tv (30:1), at the risk of distorting visually the messages produced by the directors.

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Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

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Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

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We have completed a high-contrast direct imaging survey for giant planets around 57 debris disk stars as part of the Gemini NICI Planet-Finding Campaign. We achieved median H-band contrasts of 12.4 mag at 0.''5 and 14.1 mag at 1'' separation. Follow-up observations of the 66 candidates with projected separation <500 AU show that all of them are background objects. To establish statistical constraints on the underlying giant planet population based on our imaging data, we have developed a new Bayesian formalism that incorporates (1) non-detections, (2) single-epoch candidates, (3) astrometric and (4) photometric information, and (5) the possibility of multiple planets per star to constrain the planet population. Our formalism allows us to include in our analysis the previously known β Pictoris and the HR 8799 planets. Our results show at 95% confidence that <13% of debris disk stars have a ≥5 M Jup planet beyond 80 AU, and <21% of debris disk stars have a ≥3 M Jup planet outside of 40 AU, based on hot-start evolutionary models. We model the population of directly imaged planets as d 2 N/dMdavpropm α a β, where m is planet mass and a is orbital semi-major axis (with a maximum value of a max). We find that β < –0.8 and/or α > 1.7. Likewise, we find that β < –0.8 and/or a max < 200 AU. For the case where the planet frequency rises sharply with mass (α > 1.7), this occurs because all the planets detected to date have masses above 5 M Jup, but planets of lower mass could easily have been detected by our search. If we ignore the β Pic and HR 8799 planets (should they belong to a rare and distinct group), we find that <20% of debris disk stars have a ≥3 M Jup planet beyond 10 AU, and β < –0.8 and/or α < –1.5. Likewise, β < –0.8 and/or a max < 125 AU. Our Bayesian constraints are not strong enough to reveal any dependence of the planet frequency on stellar host mass. Studies of transition disks have suggested that about 20% of stars are undergoing planet formation; our non-detections at large separations show that planets with orbital separation >40 AU and planet masses >3 M Jup do not carve the central holes in these disks.

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We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey represents the largest, deepest survey for planets around high-mass stars (≈1.5-2.5 M ☉) conducted to date and includes the planet hosts β Pic and Fomalhaut. We obtained follow-up astrometry of all candidate companions within 400 AU projected separation for stars in uncrowded fields and identified new low-mass companions to HD 1160 and HIP 79797. We have found that the previously known young brown dwarf companion to HIP 79797 is itself a tight (3 AU) binary, composed of brown dwarfs with masses 58$^{+21}_{-20}$ M Jup and 55$^{+20}_{-19}$ M Jup, making this system one of the rare substellar binaries in orbit around a star. Considering the contrast limits of our NICI data and the fact that we did not detect any planets, we use high-fidelity Monte Carlo simulations to show that fewer than 20% of 2 M ☉ stars can have giant planets greater than 4 M Jup between 59 and 460 AU at 95% confidence, and fewer than 10% of these stars can have a planet more massive than 10 M Jup between 38 and 650 AU. Overall, we find that large-separation giant planets are not common around B and A stars: fewer than 10% of B and A stars can have an analog to the HR 8799 b (7 M Jup, 68 AU) planet at 95% confidence. We also describe a new Bayesian technique for determining the ages of field B and A stars from photometry and theoretical isochrones. Our method produces more plausible ages for high-mass stars than previous age-dating techniques, which tend to underestimate stellar ages and their uncertainties.

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High-frequency seismograms contain features that reflect the random inhomogeneities of the earth. In this work I use an imaging method to locate the high contrast small- scale heterogeneity respect to the background earth medium. This method was first introduced by Nishigami (1991) and than applied to different volcanic and tectonically active areas (Nishigami, 1997, Nishigami, 2000, Nishigami, 2006). The scattering imaging method is applied to two volcanic areas: Campi Flegrei and Mt. Vesuvius. Volcanic and seismological active areas are often characterized by complex velocity structures, due to the presence of rocks with different elastic properties. I introduce some modifications to the original method in order to make it suitable for small and highly complex media. In particular, for very complex media the single scattering approximation assumed by Nishigami (1991) is not applicable as the mean free path becomes short. The multiple scattering or diffusive approximation become closer to the reality. In this thesis, differently from the ordinary Nishigami’s method (Nishigami, 1991), I use the mean of the recorded coda envelope as reference curve and calculate the variations from this average envelope. In this way I implicitly do not assume any particular scattering regime for the "average" scattered radiation, whereas I consider the variations as due to waves that are singularly scattered from the strongest heterogeneities. The imaging method is applied to a relatively small area (20 x 20 km), this choice being justified by the small length of the analyzed codas of the low magnitude earthquakes. I apply the unmodified Nishigami’s method to the volcanic area of Campi Flegrei and compare the results with the other tomographies done in the same area. The scattering images, obtained with frequency waves around 18 Hz, show the presence of high scatterers in correspondence with the submerged caldera rim in the southern part of the Pozzuoli bay. Strong scattering is also found below the Solfatara crater, characterized by the presence of densely fractured, fluid-filled rocks and by a strong thermal anomaly. The modified Nishigami’s technique is applied to the Mt. Vesuvius area. Results show a low scattering area just below the central cone and a high scattering area around it. The high scattering zone seems to be due to the contrast between the high rigidity body located beneath the crater and the low rigidity materials located around it. The central low scattering area overlaps the hydrothermal reservoirs located below the central cone. An interpretation of the results in terms of geological properties of the medium is also supplied, aiming to find a correspondence of the scattering properties and the geological nature of the material. A complementary result reported in this thesis is that the strong heterogeneity of the volcanic medium create a phenomenon called "coda localization". It has been verified that the shape of the seismograms recorded from the stations located at the top of the volcanic edifice of Mt. Vesuvius is different from the shape of the seismograms recorded at the bottom. This behavior is justified by the consideration that the coda energy is not uniformly distributed within a region surrounding the source for great lapse time.

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The presented thesis describes the formation of functional neuronal networks on an underlying micropattern. Small circuits of interconnected neurons defined by the geometry of the patterned substrate could be observed and were utilised as a model system of reduced complexity for the behaviour of neuronal network formation and activity. The first set of experiments was conducted to investigate aspects of the substrate preparation. Micropatterned substrates were created by microcontact printing of physiological proteins onto polystyrene culture dishes. The substrates displayed a high contrast between the repellant background and the cell attracting pattern, such that neurons seeded onto these surfaces aligned with the stamped structure. Both the patterning process and the cell culture were optimised, yielding highly compliant low-density networks of living neuronal cells. In the second step, cellular physiology of the cells grown on these substrates was investigated by patch-clamp measurements and compared to cells cultivated under control conditions. It could be shown that the growth on a patterned substrate did not result in an impairment of cellular integrity nor that it had an impact on synapse formation or synaptic efficacy. Due to the extremely low-density cell culture that was applied, cellular connectivity through chemical synapses could be observed at the single cell level. Having established that single cells were not negatively affected by the growth on patterned substrates, aspects of network formation were investigated. The formation of physical contact between two cells was analysed through microinjection studies and related to the rate at which functional synaptic contacts formed between two neighbouring cells. Surprisingly, the rate of synapse formation between physically contacting cells was shown to be unaltered in spite of the drastic reduction of potential interaction partners on the micropattern. Additional features of network formation were investigated and found consistent with results reported by other groups: A different rate of synapse formation by excitatory and inhibitory neurons could be reproduced as well as a different rate of frequency-dependent depression at excitatory and inhibitory synapses. Furthermore, regarding simple feedback loops, a significant enrichment of reciprocal connectivity between mixed pairs of excitatory and inhibitory neurons relative to uniform pairs could be demonstrated. This phenomenon has also been described by others in unpatterned cultures [Muller, 1997] and may therefore be a feature underlying neuronal network formation in general. Based on these findings, it can be assumed that inherent features of neuronal behaviour and cellular recognition mechanisms were found in the cultured networks and appear to be undisturbed by patterned growth. At the same time, it was possible to reduce the complexity of the forming networks dramatically in a cell culture on a patterned surface. Thus, features of network architecture and synaptic connectivity could be investigated on the single cell level under highly defined conditions.

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Die Photoemissions-Elektronenmikroskopie ist eine hervorragend geeignete Methode zur Untersuchung dynamischer Vorgänge auf realen polykristallinen Oberflächen im sub-μm Bereich. Bei der Anwendung auf Adsorbatsysteme lassen sich geringe Bedeckungsunterschiede, sowie Adsorbatstrukturen und -phasen unterscheiden. Die Methode erlaubt dabei ein breites Anwendungsspektrum über weite Temperaturbereiche und Systeme unterschiedlichster Bindungsenergie. Bei der Chemisorption von Sauerstoff auf polykristallinen Metallen wird unterschiedliches Aufwachsverhalten in den Helligkeitswerten im Mikroskopbild widergespiegelt. Bei Kupferproben zeigen Oberflächen mit unterschiedlicher kristalliner Richtung aufgrund der Symmetrie des fcc-Gitters ein ähnliches Verhalten. Das hexagonale Gitter des Titans zeigt dagegen große Unterschiede im Adsorptionsverhalten in Abhängigkeit der kristallinen Richtung. Diese Unterschiede konnten auf verschiedene Haftkoeffizienten und Oxidationsstufen der Metalle zurückgeführt werden. In einem Modell zur Photostromanalyse konnte beim Kupfer der Übergang von verschiedenen Überstrukturen bei wachsender Bedeckung gezeigt und die Übergänge ermittelt werden.. Auf den Titanoberflächen wurde so das Wachstum der Oxide TiO, TiO2 und Ti2O3 unterschieden und die Übergänge des unterschiedlichen Wachstums ermittelt. Bei der thermischen Desorption der Schichten konnten unterschiedliche Haftkoeffizient auf einzelnen Kristalliten qualitativ gezeigt werden. Diese erstmalig eingesetzte Analysemethode weist Ähnlichkeiten zur Thermo-Desorptions-Spektroskopie (TDS) auf, zeigt jedoch ortsaufgelöst lokale Unterschiede auf polykristallinen Oberflächen. Bei thermisch gestützten Oberflächenreaktionen ließen sich die Reaktionskeime deutlich identifizieren und mit einer Grauwertanalyse konnte die Oxidation der karbidischen Lagen zu Kohlenmonoxid und die Metalloxidation unterschieden werden. Dabei konnte gezeigt werden, daß die Reaktionskeime nur an Plattengrenzen auftreten, nicht jedoch auf der Oberfläche. Durch die Aufrauhung der Plattengrenzen mit zunehmender Reaktionsdauer nimmt die Zahl der Reaktionskeime kontinuierlich zu, die laterale Ausdehnung der Einzelreaktionen bleibt aber konstant. Bei der Physisorption von Xenon auf Graphit wurde erstmals für die Photoemissionsmikroskopie die resonanten Anregung ausgenutzt. Die verschiedenen Phasen des Adsorbats können dabei deutlich unterschieden werden; bei niedrigen Temperaturen (40K) findet ein gleichmäßiges Wachstum auf der gesamten Oberfläche statt, bei höheren Temperaturen von 60-65K ist dagegen ein Inselwachstum in verschiedenen Phasen zu beobachten. Die zeitliche Entwicklung des Wachstums, die örtliche Lage der Phasen und die Phasenübergänge (gas, fest inkommensurabel, fest kommensurabel) konnten bestimmt werden. Bei der Desorption der Schichten konnten die einzelnen Phasen ebenfalls getrennt werden und das unterschiedliche Desorptionsverhalten sowie die Phasenübergänge selber verifiziert werden.

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Nanoscience aims at manipulating atoms, molecules and nano-size particles in a precise and controlled manner. Nano-scale control of the thin film structures of organic/polymeric materials is a prerequisite to the fabrication of sophisticated functional devices. The work presented in this thesis is a compilation of various polymer thin films with newly synthesized functional polymers. Cationic and anionic LC amphotropic polymers, p-type and n-type semiconducting polymers with triarylamine, oxadiazole, thiadiazole and triazine moieties are suitable materials to fabricate multilayers by layer-by-layer (LBL) self-assembly with a well defined internal structure. The LBL assembly is the ideal processing technique to prepare thin polymer film composites with fine control over morphology and composition at nano-scale thickness, which may have applications in photo-detectors, light-emitting diodes (LEDs), displays and sensors, as well as in solar cells. The multilayer build-up was investigated with amphotropic LC polymers individually by solution-dipping and spin-coating methods; they showed different internal orders with respect to layering and orientation of the mesogens, as a result of the liquid crystalline phase. The synthesized p-type and n-type semiconducting polymers were examined optically and electrochemically, suggesting that they are favorably promising as hole-(p-type) or electron-(n-type) transport materials in electronic and optoelectronic devices. In addition, we report a successful film deposition of polymers by the vacuum deposition method. The vapor deposition method provides a clean environment; it is solvent free and well suited to sequential depositions in hetero-structured multilayer system. As the potential applications, the fabricated polymer thin films were used as simple electrochromic films and also used as hole transporting layers in LEDs. Electrochemical and electrochromic characterizations of assembled films reveal that the newly synthesized polymers give rise to high contrast ratio and fast switching electrochromic films. The LEDs with vacuum deposited films show dramatic improvements in device characteristics, indicating that the films are promising as hole transporting layers. These are the result of not only the thin nano-scale film structures but also the combination with the high charge carrier mobility of synthesized semiconducting polymers.

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Krebs ist eine der häufigsten Krankheiten und stellt eine der wichtigsten medizinischen Herausforderungen des 21. Jahrhunderts dar. Eine frühzeitige Diagnose ist dabei essentiell für eine individuell angepasste Therapie zur Verbesserung der Lebensqualität und -erwartung der Patienten. Hierbei kommen der 68Ge/68Ga-Generator und das daraus resultierende PET-Nuklid 68Ga immer stärker in den Fokus von Wissenschaft und Medizin. rnrnFür eine erfolgreiche Therapie stellt die Chemoresistenz (Multi-Drug-Resistance) zahlreicher Tumore eine schwerwiegende Komplikation dar. Für das Therapieversagen ist die Aktivierung des Transportproteins p-Glykoprotein (pGP) maßgeblich mit verantwortlich. Mit Hilfe der Schiff’schen Base [68Ga]MFL6.MZ konnte die Aktivitätsänderung von pGP unter verschiedener Beeinflussung erstmals in vivo beobachtet werden. So zeigte sich, dass sich unter azidotischen Bedingungen in Tumoren die Aktivität des pGP erhöht und somit vermehrt auch Zytostatika, die pGP-Substrate sind, aus den Tumoren transportiert werden. Durch Aufklärung der Abhängigkeit der pGP-Aktivität von dessen Signalkaskade konnte gezeigt werden, dass durch eine Blockade der MAP-Kinase p38 eine Erniedrigung der pGP-Aktivität zu verzeichnen ist. Die ebenfalls in der Signalkaskade eingebundene MAP-Kinase ERK1/2 hingegen spielt hier nur eine untergeordnete Rolle.rnrnNeben dem Versagen der Chemotherapie stellt auch die Metastasierung eines Malignoms massive Einschnitte in die Lebensqualität von Erkrankten dar. Befallen die Metastasen das Skelett eines Menschen, wird dies zumeist erst spät registriert. 68Ga-markierte Bisphosphonate bieten nun die Möglichkeit, Patienten quantitativ auf Knochenmetastasen hin untersuchen zu können. So konnten zu Beginn einfache Phosphonate wie EDTMP und DOTP nicht die nötige in vivo Stabilität bzw. hohe radiochemische Ausbeuten liefern und sind damit für die Anwendung am Menschen uninteressant. Jedoch die DOTA-basierten Bisphosphonate allen voran der Ligand BPAMD zeigen ein großes Potential. In vivo-Versuche an Ratten mit Knochenmetastasen zeigten, dass sich [68Ga]BPAMD an den Metastasen anreichert und einen sehr guten Kontrast zum gesunden Knochen darstellt. Der Tracer konnte erstmals am Menschen angewendet werden und zeigte in ausgewählten Regionen eine höhere Anreicherung als eine zuvor durchgeführte PET-Aufnahme mit [18F]Fluorid. Der Ligand BPAMD bietet außerdem den Vorteil, neben 68Ga auch andere dreiwertige Radionuklide wie das therapeutische 177Lu komplexieren zu können. Durch Studien zur Komplexbildung und Stabilität konnte auch [177Lu]BPAMD in der klinischen Anwendung erprobt werden und zeigte eine Anreicherung an den Knochenmetastasen. So ist es nun möglich, Knochenmetastasen mittels 68Ga-PET zu diagnostizieren, eine entsprechende Dosisberechnung anzustellen und anschließend mit dem gleichen Liganden eine Therapie mit [177Lu]BPAMD durchzuführen.

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The temporal bone is ideal for low-dose CT because of its intrinsic high contrast. The aim of this study was to retrospectively evaluate image quality and radiation doses of a new low-dose versus a standard high-dose pediatric temporal bone CT protocol and to review dosimetric data from the literature.

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With the increasing advances in hip joint preservation surgery, accurate diagnosis and assessment of femoral head and acetabular cartilage status is becoming increasingly important. Magnetic resonance imaging (MRI) of the hip does present technical difficulties. The fairly thin cartilage lining necessitates high image resolution and high contrast-to-noise ratio (CNR). With MR arthrography (MRA) using intraarticular injected gadolinium, labral tears and cartilage clefts may be better identified through the contrast medium filling into the clefts. However, the ability of MRA to detect varying grades of cartilage damage is fairly limited and early histological and biochemical changes in the beginning of osteoarthritis (OA) cannot be accurately delineated. Traditional MRI thus lacks the ability to analyze the biological status of cartilage degeneration. The technique of delayed gadolinium-enhanced MRI of cartilage (dGEMRIC) is sensitive to the charge density of cartilage contributed by glycosaminoglycans (GAGs), which are lost early in the process of OA. Therefore, the dGEMRIC technique has a potential to detect early cartilage damage that is obviously critical for decision-making regarding time and extent of intervention for joint-preservation. In the last decade, cartilage imaging with dGEMRIC has been established as an accurate and reliable tool for assessment of cartilage status in the knee and hip joint.This review outlines the current status of dGEMRIC for assessment of hip joint cartilage. Practical modifications of the standard technique including three-dimensional (3D) dGEMRIC and dGEMRIC after intra-articular gadolinium instead of iv-dGEMRIC will also be addressed.