935 resultados para Eu2O3 insulator layer
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Theoretical models are developed for the continuous-wave and pulsed laser incision and cut of thin single and multi-layer films. A one-dimensional steady-state model establishes the theoretical foundations of the problem by combining a power-balance integral with heat flow in the direction of laser motion. In this approach, classical modelling methods for laser processing are extended by introducing multi-layer optical absorption and thermal properties. The calculation domain is consequently divided in correspondence with the progressive removal of individual layers. A second, time-domain numerical model for the short-pulse laser ablation of metals accounts for changes in optical and thermal properties during a single laser pulse. With sufficient fluence, the target surface is heated towards its critical temperature and homogeneous boiling or "phase explosion" takes place. Improvements are seen over previous works with the more accurate calculation of optical absorption and shielding of the incident beam by the ablation products. A third, general time-domain numerical laser processing model combines ablation depth and energy absorption data from the short-pulse model with two-dimensional heat flow in an arbitrary multi-layer structure. Layer removal is the result of both progressive short-pulse ablation and classical vaporisation due to long-term heating of the sample. At low velocity, pulsed laser exposure of multi-layer films comprising aluminium-plastic and aluminium-paper are found to be characterised by short-pulse ablation of the metallic layer and vaporisation or degradation of the others due to thermal conduction from the former. At high velocity, all layers of the two films are ultimately removed by vaporisation or degradation as the average beam power is increased to achieve a complete cut. The transition velocity between the two characteristic removal types is shown to be a function of the pulse repetition rate. An experimental investigation validates the simulation results and provides new laser processing data for some typical packaging materials.
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Die bedeutendste Folge der Luftverschmutzung ist eine erhöhte Konzentration an Ozon (O3) in der Troposphäre innerhalb der letzten 150 Jahre. Ozon ist ein photochemisches Oxidationsmittel und ein Treibhausgas, das als wichtigste Vorstufe des Hydroxyradikals OH die Oxidationskraft der Atmosphäre stark beeinflusst. Um die Oxidationskraft der Atmosphäre und ihren Einfluss auf das Klima verstehen zu können, ist es von großer Bedeutung ein detailliertes Wissen über die Photochemie des Ozons und seiner Vorläufer, den Stickoxiden (NOx), in der Troposphäre zu besitzen. Dies erfordert das Verstehen der Bildungs- und Abbaumechanismen von Ozon und seiner Vorläufer. Als eine für den chemischen Ozonabbau wichtige Region kann die vom Menschen weitgehend unberührte marine Grenzschicht (Marine boundary layer (MBL)) angesehen werden. Bisher wurden für diese Region jedoch kaum Spurengasmessungen durchgeführt, und so sind die dort ablaufenden photochemischen Prozesse wenig untersucht. Da etwa 70 % der Erdoberfläche mit Ozeanen bedeckt sind, können die in der marinen Granzschicht ablaufenden Prozesse als signifikant für die gesamte Atmosphäre angesehen werden. Dies macht eine genaue Untersuchung dieser Region interessant. Um die photochemische Produktion und den Abbau von Ozon abschätzen zu können und den Einfluss antrophogener Emissionen auf troposphärisches Ozon zu quantifizieren, sind aktuelle Messergebnisse von NOx im pptv-Bereich für diese Region erforderlich. Die notwendigen Messungen von NO, NO2, O3, JNO2, J(O1D), HO2, OH, ROx sowie einiger meteorologischer Parameter wurden während der Fahrt des französischen Forschungsschiffes Marion-Dufresne auf dem südlichen Atlantik (28°S-57°S, 46°W-34°E) im März 2007 durchgeführt. Dabei sind für NO und NO2 die bisher niedrigsten gemessenen Werte zu verzeichnen. Die während der Messcampagne gewonnen Daten wurden hinsichtlich Ihrer Übereinstimmung mit den Bedingungen des photochemischen stationären Gleichgewichts (photochemical steady state (PSS)) überprüft. Dabei konnte eine Abweichung vom PSS festgestellt werden, welche unter Bedingungen niedriger NOx-Konzentrationen (5 bis 25pptv) einen unerwarteten Trend im Leighton-Verhältnis bewirkt, der abhängig vom NOx Mischungsverhältnis und der JNO2 Intensität ist. Signifikante Abweichungen vom Verhältnis liegen bei einer Zunahme der JNO2 Intensität vor. Diese Ergebnisse zeigen, dass die Abweichung vom PSS nicht beim Minimum der NOx-Konzentrationen und der JNO2 Werte liegt, so wie es in bisherigen theoretischen Studien dargelegt wurde und können als Hinweis auf weitere photochemische Prozesse bei höheren JNO2-Werten in einem System mit niedrigem NOx verstanden werden. Das wichtigste Ergebnis dieser Untersuchung, ist die Verifizierung des Leighton-Verhältnisses, das zur Charakterisierung des PSS dient, bei sehr geringen NOx-Konzentrationen in der MBL. Die bei dieser Doktorarbeit gewonnenen Erkenntnisse beweisen, dass unter den Bedingungen der marinen Granzschicht rein photochemischer Abbau von Ozon stattfindet und als Hauptursache hierfür während des Tages die Photolyse gilt. Mit Hilfe der gemessenen Parameter wurde der kritische NO-Level auf Werte zwischen 5 und 9 pptv abgeschätzt, wobei diese Werte im Vergleich zu bisherigen Studien vergleichsweise niedrig sind. Möglicherweise bedeutet dies, dass das Ozon Produktion/ Abbau-Potential des südlichen Atlantiks deutlich stärker auf die Verfügbarkeit von NO reagiert, als es in anderen Regionen der Fall ist. Im Rahmen der Doktorarbeit wurde desweiteren ein direkter Vergleich der gemessenen Spezies mit dem Modelergebnis eines 3-dimensionalen Zirkulationsmodel zur Simulation atmosphären chemischer Prozesse (EMAC) entlang der exakten Schiffsstrecke durchgeführt. Um die Übereinstimmung der Messergebnisse mit dem bisherigen Verständnis der atmosphärischen Radikalchemie zu überprüfen, wurde ein Gleichgewichtspunktmodel entwickelt, das die während der Überfahrt erhaltenen Daten für Berechungen verwendet. Ein Vergleich zwischen der gemessenen und der modellierten ROx Konzentrationen in einer Umgebung mit niedrigem NOx zeigt, dass die herkömmliche Theorie zur Reproduktion der Beobachtungen unzureichend ist. Die möglichen Gründe hierfür und die Folgen werden in dieser Doktorarbeit diskutiert.
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Reactive halogen compounds are known to play an important role in a wide variety of atmospheric processes such as atmospheric oxidation capacity and coastal new particle formation. In this work, novel analytical approaches combining diffusion denuder/impinger sampling techniques with gas chromatographic–mass spectrometric (GC–MS) determination are developed to measure activated chlorine compounds (HOCl and Cl2), activated bromine compounds (HOBr, Br2, BrCl, and BrI), activated iodine compounds (HOI and ICl), and molecular iodine (I2). The denuder/GC–MS methods have been used to field measurements in the marine boundary layer (MBL). High mixing ratios (of the order of 100 ppt) of activated halogen compounds and I2 are observed in the coastal MBL in Ireland, which explains the ozone destruction observed. The emission of I2 is found to correlate inversely with tidal height and correlate positively with the levels of O3 in the surrounding air. In addition the release is found to be dominated by algae species compositions and biomass density, which proves the “hot-spot” hypothesis of atmospheric iodine chemistry. The observations of elevated I2 concentrations substantially support the existence of higher concentrations of littoral iodine oxides and thus the connection to the strong ultra-fine particle formation events in the coastal MBL.
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The objective of this dissertation is to study the structure and behavior of the Atmospheric Boundary Layer (ABL) in stable conditions. This type of boundary layer is not completely well understood yet, although it is very important for many practical uses, from forecast modeling to atmospheric dispersion of pollutants. We analyzed data from the SABLES98 experiment (Stable Atmospheric Boundary Layer Experiment in Spain, 1998), and compared the behaviour of this data using Monin-Obukhov's similarity functions for wind speed and potential temperature. Analyzing the vertical profiles of various variables, in particular the thermal and momentum fluxes, we identified two main contrasting structures describing two different states of the SBL, a traditional and an upside-down boundary layer. We were able to determine the main features of these two states of the boundary layer in terms of vertical profiles of potential temperature and wind speed, turbulent kinetic energy and fluxes, studying the time series and vertical structure of the atmosphere for two separate nights in the dataset, taken as case studies. We also developed an original classification of the SBL, in order to separate the influence of mesoscale phenomena from turbulent behavior, using as parameters the wind speed and the gradient Richardson number. We then compared these two formulations, using the SABLES98 dataset, verifying their validity for different variables (wind speed and potential temperature, and their difference, at different heights) and with different stability parameters (zita or Rg). Despite these two classifications having completely different physical origins, we were able to find some common behavior, in particular under weak stability conditions.
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In this work a modelization of the turbulence in the atmospheric boundary layer, under convective condition, is made. For this aim, the equations that describe the atmospheric motion are expressed through Reynolds averages and, then, they need closures. This work consists in modifying the TKE-l closure used in the BOLAM (Bologna Limited Area Model) forecast model. In particular, the single column model extracted from BOLAM is used, which is modified to obtain other three different closure schemes: a non-local term is added to the flux- gradient relations used to close the second order moments present in the evolution equation of the turbulent kinetic energy, so that the flux-gradient relations become more suitable for simulating an unstable boundary layer. Furthermore, a comparison among the results obtained from the single column model, the ones obtained from the three new schemes and the observations provided by the known case in literature ”GABLS2” is made.
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This thesis presents a detailed and successful study of molecular self-assembly on the calcite CaCO3(10-14) surface. One reason for the superior applicability of this particular surface is given by reflecting the well-known growth modes. Layer-by-layer growth, which is a necessity for the formation of templated two-dimensional (2D) molecular structures, is particularly favoured on substrates with a high surface energy. The CaCO3(10-14) surface is among those substrates and, thus, most promising. rnrnAll experiments in this thesis were performed using the non-contact atomic force microscope (NC-AFM) under ultra-high vacuum conditions. The acquisition of drift-free data became in this thesis possible owing to the herein newly developed atom-tracking system. This system features a lateral tip-positioning precision of at least 50pm. Furthermore, a newly developed scan protocol was implemented in this system, which allows for the acquisition of dense three-dimensional (3D) data under room-temperature conditions. An entire 3D data set from a CaCO3(10-14) surface consisting of 85x85x500 pixel is discussed. rnrnThe row-pairing and (2x1) reconstructions of the CaCO3(10-14) surface constitute most interesting research subjects. For both reconstructions, the NC-AFM imaging was classified to a total of 12 contrast modes. Eight of these modes were observed within this thesis, some of them for the first time. Together with literature findings, a total of 10 modes has been observed experimentally to this day. Some contrast modes presented themselves as highly distance-dependent and at least for one contrast mode, a severe tip-termination influence was found. rnrnMost interestingly, the row-pairing reconstruction was found to break a symmetry element of the CaCO3(10-14) surface. With the presence of this reconstruction, the calcite (10-14) surface becomes chiral. From high-resolution NC-AFM data, the identification of the enantiomers is here possible and is presented for one enantiomer in this thesis. rnrnFive studies of self-assembled molecular structures on calcite (10-14) surfaces are presented. Only for one system, namely HBC/CaCO3(10-14), the formation of a molecular bulk structure was observed. This well-known occurence of weak molecule-insulator interaction hinders the investigation of two-dimensional molecular self-assembly. It was, however, possible to force the formation of an island phase for this system upon following a variable-temperature preparation. rnFor the C60/CaCO3(10-14) system it is most notably that no branched island morphologies were found. Instead, the first C60 layer appeared to wet the calcite surface. rnrnIn all studies, the molecules arranged themselves in ordered superstructures. A templating effect due to the underlying calcite substrate was evident for all systems. This templating strikingly led either to the formation of large commensurate superstructures, such as (2x15) with a 14 molecule basis for the C60/CaCO3(10-14) system, or prevented the vast growth of incommensurate molecular motifs, such as the chicken-wire structure in the trimesic acid (TMA)/CaCO3(10-14) system. rnrnThe molecule-molecule and the molecule-substrate interaction was increased upon choosing molecules with carboxylic acid moieties in the third, fourth and fifth study, using terephthalic acid, TMA and helicene molecules. In all these experiments, hydrogen-bonded assemblies were created. rnrnDirected hydrogen bond formation combined with intermolecular pi-pi interaction is employed in the fifth study, where the formation of uni-directional molecular "wires" from single helicene molecules succeeded. Each "wire" is composed of heterochiral helicene pairs, well-aligned along the [01-10] substrate direction and stabilised by pi-pi interaction.
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Ice clouds have a strong effect on the Earth-atmosphere radiative energy balance, on the distribution of condensable gases in the atmosphere, as well as on the chemical composition of the air. The ice particles in these clouds can take on a variety of shapes which makes the description of the cloud microphysical properties more difficult. In the tropical upper troposphere/lower stratosphere (UTLS), a region where ice cloud abundance is relatively high, different types of ice clouds can be observed. However, in situ measurements are rare due to the high altitude of these clouds and the few available research aircraft, only three worldwide, that can fly at such altitudes.rnThis work focuses on in situ measurements of the tropical UTLS clouds performedrnwith a Cloud Imaging Probe (CIP) and a Forward Scattering Spectrometer Probern(FSSP-100), whereof the CIP is the key instrument of this thesis. The CIP is anrnairborne in situ instrument that obtains two-dimensional shadow images of cloud particles. Several cloud microphysical parameters can be derived from these measurements, e.g. number concentrations and size distributions. In order to obtain a high quality data set, a careful image analysis and several corrections need to be applied to the CIP observations. These methods are described in detail.rnMeasurements within the tropical UTLS have been performed during two campaigns:rnSCOUT-O3, 2005 in Northern Australia and SCOUT-AMMA, 2006 inWest Africa. Thernobtained data set includes first observations of subvisible cirrus clouds over a continental area and observations of the anvils of deep convective clouds. The latter can be further divided into clouds in mesoscale convective system outflows of different ages and clouds in overshooting cloud turrets that even penetrated the stratosphere. The microphysical properties of these three cloud types are discussed in detail. Furthermore, the vertical structure of the ice clouds in the UTLS is investigated. The values of the microphysical parameters were found to decrease with increasing altitude in the upper troposphere. Particle numbers and maximum sizes were also decreasing with increasing age of the outflow clouds. Further differences between the deep convective clouds and subvisible cirrus were found in the particle morphology as well as in the ratio of the observed aerosol particles to cloud particles which indicates that the different freezing processes (deposition, contact, immersion freezing) play different roles in the formation of the respective clouds. For the achievementrnof a better microphysical characterisation and description numerical fits have been adjusted onto the cloud particle size distributions of the subvisible cirrus as well as on the size distributions of the clouds at different altitudes in the UTLS.
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In dye-sensitized solar cells a blocking layer between the transparent electrode and the mesoporous titanium dioxide film is used to prevent short-circuits between the hole-conductor and the front electrode. The conventional approach is to use a compact layer of titanium dioxide prepared by spin coating or spray pyrolysis. The thickness of the blocking layer is critical. On one hand, the layer has to be thick enough to cover the rough substrate completely. On the other hand, the serial resistance increases with increasing film thickness, because the layer acts as an ohmic resistance itself. In this thesis an amphiphilic diblock copolymer is used as a functional template to produce an alternative, hybrid blocking layer. The hybrid blocking layer is thinner than the conventional, compact titanium dioxide film and thereby possesses a higher conductivity. Still, this type of blocking layer covers the rough electrode material completely and avoids current loss through charge recombination. The novel blocking layer is prepared using a tailored, amphiphilic block copolymer in combination with sol-gel chemistry. While the hydrophilic poly(ethylene oxide) part of the polymer coordinates a titanium dioxide precursor to form a percolating network of titania particles, the hydrophobic poly(dimethylsiloxane) part turns into an insulating ceramic layer. With this technique, crack-free films with a thickness down to 24 nm are obtained. The presence of a conductive titanium dioxide network for current flow, which is embedded in an insulating ceramic material, is validated by conductive scanning force microscopy. This is the first time that such a hybrid blocking layer is implemented in a solar cell. With this approach the efficiency could be increased up to 27 % compared to the conventional blocking layer. Thus, it is demonstrated that the hybrid blocking layer represents a competitive alternative to the classical approach.
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il profilo verticale del gas dipende sia dal potenziale galattico, e quindi dalla distribuzione di materia, sia dalla dispersione di velocit`a del gas La nostra analisi teorica ha mostrato che l’altezza scala dell’idrogeno gassoso ad un certo raggio `e fortemente legata alla componente di massa dominate: nelle parti centrali, dove domina la materia barionica, il disco gassoso incrementa il suo spessore esponenzialmente con una lunghezza scala pari al doppio di quella del disco stellare; dalle zone intermedie fino alla fine del disco, il profilo verticale del gas `e influenzato dalla distribuzione di DM. In queste zone lo spessore del disco gassoso cresce con il raggio in maniera circa lineare. Tale fenomeno viene definito gas flaring. Lo scopo principale di questa tesi `e la ricerca di una nuova tecnica per poter stimare il profilo vertical del gas in galassie con inclinazione intermedia.
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Silicon-on-insulator (SOI) is rapidly emerging as a very promising material platform for integrated photonics. As it combines the potential for optoelectronic integration with the low-cost and large volume manufacturing capabilities and they are already accumulate a huge amount of applications in areas like sensing, quantum optics, optical telecommunications and metrology. One of the main limitations of current technology is that waveguide propagation losses are still much higher than in standard glass-based platform because of many reasons such as bends, surface roughness and the very strong optical confinement provided by SOI. Such high loss prevents the fabrication of efficient optical resonators and complex devices severely limiting the current potential of the SOI platform. The project in the first part deals with the simple waveguides loss problem and trying to link that with the polarization problem and the loss based on Fabry-Perot Technique. The second part of the thesis deals with the Bragg Grating characterization from again the point of view of the polarization effect which leads to a better stop-band use filters. To a better comprehension a brief review on the basics of the SOI and the integrated Bragg grating ends up with the fabrication techniques and some of its applications will be presented in both parts, until the end of both the third and the fourth chapters to some results which hopefully make its precedent explanations easier to deal with.
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In questa tesi viene seguito il lavoro di test delle schede ROD del layer 2 del Pixel Detector dell’ esperimento ATLAS, che mira a verificare la loro corretta funzionalità, prima che vengano spedite nei laboratori del CERN. Queste nuove schede gestiscono i segnali in arrivo dal Pixel Detector di ATLAS, per poi inviarli ai computer per la successiva elaborazione. Le schede ROD andranno a sostituire le precedenti schede SiROD nella catena di acquisizione dati dell’esperimento, procedendo dal nuovo strato IBL, e proseguendo con i tre layer del Pixel Detector, corroborando l’aggiornamento tecnologico e prestazionale necessario in vista dell’incremento di luminosità dell’esperimento.
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Il lavoro descrive la progettazione, implementazione e test sperimentale di un meccanismo, integrato nel kernel linux 4.0, dedicato al riconoscimento delle perdite dei frame Wi-Fi.
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L'indagine ha riguardato il profilo del vento nei primi 30 metri dello strato limite atmosferico stabile nell'ambito della teoria di similarità locale. Ad oggi, diversi esperimenti hanno confermato la validità della teoria per strati-limite su terreni livellati e superfici omogenee. Tali condizioni ideali sono però infrequenti nella realtà ed è perciò importante capire quali siano i limiti della similarità locale per strati-limite su terreni complessi e superfici disomogenee. Entrambe le condizioni sono presenti a Ny-Alesund (Svalbard, Norvegia) dove il Consiglio Nazionale delle Ricerche (CNR), nel 2009, ha installato una torre di 30 m, la Amudsen-Nobile Climate Change Tower (CCT), per lo studio dello strato-limite artico. Il lavoro di tesi ha riguardato misure di vento e turbolenza acquisite sulla CCT da maggio 2012 a maggio 2014. Il confronto tra le velocità del vento misurate dagli anemometri installati sulla CCT, ha rivelato criticità nel dato sonico manifestatesi con sovrastime sistematiche e maggiore erraticità rispetto alle misure provenienti dagli anemometri a elica. Un test condotto fra diversi metodi per il calcolo dei gradienti verticali della velocità del vento ha rivelato scarsa sensibilità dei risultati ottenuti al particolare metodo utilizzato. Lo studio ha riguardato i gradienti verticali adimensionali della velocità del vento nei primi 30-m dello strato limite stabile. Deviazioni significative tra i tra le osservazioni e i valori predetti dalla similarità locale sono state osservate in particolare per i livelli più distanti dal suolo e per valori crescenti del parametro di stabilità z/L (L, lunghezza di Obukhov locale). In particolare, si sono osservati gradienti adimensionali inferiori a quelli predetti dalle più usate relazioni di flusso-gradiente. Tali deviazioni, presenti perlopiù per z/L>0.1, sono state associate ad un effetto di accentuazione della turbolenza da parte delle irregolarità del terreno. Per condizioni meno stabili, z/L<0.1, scarti positivi tra i gradienti osservati e quelli attesi sono stati attribuiti alla formazione di strati limite interni in condizioni di vento dal mare verso la costa. Sono stati proposti diversi metodi per la stima dell'effetto della self-correlazione nella derivazione delle relazioni di flusso-gradiente, dovuta alla condivisione della variabile u*. La formula per il coefficiente lineare di self correlazione e le sue distribuzioni di probabilità empiriche sono state derivate e hanno permesso di stimare il livello di self-correlazione presente nel dataset considerato.
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I Big Data hanno forgiato nuove tecnologie che migliorano la qualità della vita utilizzando la combinazione di rappresentazioni eterogenee di dati in varie discipline. Occorre, quindi, un sistema realtime in grado di computare i dati in tempo reale. Tale sistema viene denominato speed layer, come si evince dal nome si è pensato a garantire che i nuovi dati siano restituiti dalle query funcions con la rapidità in cui essi arrivano. Il lavoro di tesi verte sulla realizzazione di un’architettura che si rifaccia allo Speed Layer della Lambda Architecture e che sia in grado di ricevere dati metereologici pubblicati su una coda MQTT, elaborarli in tempo reale e memorizzarli in un database per renderli disponibili ai Data Scientist. L’ambiente di programmazione utilizzato è JAVA, il progetto è stato installato sulla piattaforma Hortonworks che si basa sul framework Hadoop e sul sistema di computazione Storm, che permette di lavorare con flussi di dati illimitati, effettuando l’elaborazione in tempo reale. A differenza dei tradizionali approcci di stream-processing con reti di code e workers, Storm è fault-tolerance e scalabile. Gli sforzi dedicati al suo sviluppo da parte della Apache Software Foundation, il crescente utilizzo in ambito di produzione di importanti aziende, il supporto da parte delle compagnie di cloud hosting sono segnali che questa tecnologia prenderà sempre più piede come soluzione per la gestione di computazioni distribuite orientate agli eventi. Per poter memorizzare e analizzare queste moli di dati, che da sempre hanno costituito una problematica non superabile con i database tradizionali, è stato utilizzato un database non relazionale: HBase.
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Polymers that are used in clinical practice as bone-defect-filling materials possess many essential qualities, such as moldability, mechanical strength and biodegradability, but they are neither osteoconductive nor osteoinductive. Osteoconductivity can be conferred by coating the material with a layer of calcium phosphate, which can be rendered osteoinductive by functionalizing it with an osteogenic agent. We wished to ascertain whether the morphological and physicochemical characteristics of unfunctionalized and bovine-serum-albumin (BSA)-functionalized calcium-phosphate coatings were influenced by the surface properties of polymeric carriers. The release kinetics of the protein were also investigated. Two sponge-like materials (Helistat® and Polyactive®) and two fibrous ones (Ethisorb and poly[lactic-co-glycolic acid]) were tested. The coating characteristics were evaluated using state-of-the-art methodologies. The release kinetics of BSA were monitored spectrophotometrically. The characteristics of the amorphous and the crystalline phases of the coatings were not influenced by either the surface chemistry or the surface geometry of the underlying polymer. The mechanism whereby BSA was incorporated into the crystalline layer and the rate of release of the truly incorporated depot were likewise unaffected by the nature of the polymeric carrier. Our biomimetic coating technique could be applied to either spongy or fibrous bone-defect-filling organic polymers, with a view to rendering them osteoconductive and osteoinductive.