A Distributive Comparison of Enterprise Size in Korea and Taiwan

Research to date on the economic development of the Republic of Korea and Taiwan has frequently contrasted the two economies by depicting the former as centered on large-scale enterprises and the latter on small and medium-size enterprises (SMEs). The purpose of this study is to see if the appropriateness of this perception will also be verified by the statistical data. In Section I the authors utilized census data on the Korean and Taiwanese manufacturing sectors to compare the distribution pattern of the sizes of enterprises in the two economies. However, on examining the available data for making this comparison, the authors discovered that for Korea the statistics provided are those at the level of the establishment (a physical unit engaging in industrial activities such as a factory, workshop, office, or mine) while the statistics for Taiwan are those at the enterprise level. Mindful of this difference, the authors looked at the portion of the economy accounted for by large-scale establishments in Korea that employed 500 workers or more and by enterprises in Taiwan employing the same number of workers, and they discovered that the portion that these large-scale businesses account for, especially in the area of output, has steadily declined since the 1980s. When comparing the share of total production that these large-scale establishments/enterprises account for in the two economies, the authors concluded that those in Korea accounted for a larger share of that economy's production than did their counterparts in Taiwan. The authors then compared the portion of the economy accounted for by establishments in Korea and enterprises in Taiwan that employed less than ten workers, and they found that the portion of the two economies that these very small-scale production units accounted for has also been on the decline. Section II compares the portions of the two economies accounted for by large business groups. After comparing the percentage of GDP accounted for by the total sales of these business groups, the authors found that large business groups in Korea have played a far more important role in Korean economy than has been the case for such groups in Taiwan. This difference in the importance of such business groups in the two economies has also played an significant part in fostering the perceived dichotomy of large-scale enterprises playing the important role in Korea versus SMEs being the important players in Taiwan. Section III compares the percentage of total exports accounted for by SMEs, and shows that SMEs in Taiwan account for a larger share of exports than do their counterparts in Korea. This section also shows that in Taiwan the share of export sales for SMEs has consistently exceeded that for non-SMEs, while in Korea the relationship between enterprise size and the rate of export sales has been directly proportional. This difference in the size of the major export players is another factor fostering the perception of the Korean economy being centered on big business while Taiwan's is on SMEs. Although there were difficulties and limitations when comparing the data of the two economies, the statistical comparison undertaken in this study shows that in general big business has played the major role in the development of the Korean economy while in Taiwan's economic development this role has been played by SMEs. Thus the statistical data also verifies the perceived dichotomy of these two economies.

The role of home and host country characteristics in FDI: firm-level evidence from Japan, Korea and Taiwan

There is a large and growing empirical literature that investigates the determinants of outward foreign direct investment (FDI). This literature examines primarily the effect of host country characteristics on FDI even though home country characteristics also influence the decision of firms to invest abroad. In this paper, we examine the role of both host and home country characteristics in FDI. To do so, we constructed a firm-level database of outward FDI from Japan, Korea, and Taiwan. Our empirical analysis yields two main findings. First, host countries with better environment for FDI, in terms of larger market size, smaller fixed entry costs, and lower wages, attract more foreign investors. Second, firms from home countries with higher wages are more likely to invest abroad. An interesting and significant policy implication of our empirical evidence is that policymakers seeking to promote FDI inflows should prioritize countries with higher wages.

Gender-preferential intergenerational patterns in primary education attainment : a quantitative analysis of a case of rural Mindanao, the Philippines

The Philippines has achieved a relatively high standard of education. Previous researches, most of which deal with Luzon Island, have indicated that rural poverty alleviation began partly due to the increased investment in education. However, the suburban areas beyond Luzon Island have rarely been studied. This study examines a case from rural Mindanao, and investigates the determinants and factors associated with children's education, with a special focus on delays in schooling, which may be a cause of dropout and holdover incidences, as well as exploring gender-specific differential patterns. The result shows that after controlling other socioeconomic attributes, (1) delays in schooling, as well as years completed, are more favorable for girls than boys; (2) the level of maternal education is equally associated with the child(ren)’s education level regardless of their gender; and (3) paternal education is preferentially and favorably influential to the same-gender child(ren), i.e., son(s). To reduce the boy-unfriendly gender bias in primary education, this study suggests two future tasks, i.e., providing boy-specific interventions to enhance the magnitude of the father-son educational virtuous circle, and comparing the magnitude of gender-equal maternal education influence and boy-preferential paternal education influence to specify which effect is larger.

Bio-inspired FPGA Architecture for Self-Calibration of an Image Compression Core based on Wavelet Transforms in Embedded Systems

A generic bio-inspired adaptive architecture for image compression suitable to be implemented in embedded systems is presented. The architecture allows the system to be tuned during its calibration phase. An evolutionary algorithm is responsible of making the system evolve towards the required performance. A prototype has been implemented in a Xilinx Virtex-5 FPGA featuring an adaptive wavelet transform core directed at improving image compression for specific types of images. An Evolution Strategy has been chosen as the search algorithm and its typical genetic operators adapted to allow for a hardware friendly implementation. HW/SW partitioning issues are also considered after a high level description of the algorithm is profiled which validates the proposed resource allocation in the device fabric. To check the robustness of the system and its adaptation capabilities, different types of images have been selected as validation patterns. A direct application of such a system is its deployment in an unknown environment during design time, letting the calibration phase adjust the system parameters so that it performs efcient image compression. Also, this prototype implementation may serve as an accelerator for the automatic design of evolved transform coefficients which are later on synthesized and implemented in a non-adaptive system in the final implementation device, whether it is a HW or SW based computing device. The architecture has been built in a modular way so that it can be easily extended to adapt other types of image processing cores. Details on this pluggable component point of view are also given in the paper.

Topological invariance and spatial scaling of surface roughness in two highly eroded zones of Mexico: a comparative study

The Fractal Image Informatics toolbox (Oleschko et al., 2008 a; Torres-Argüelles et al., 2010) was applied to extract, classify and model the topological structure and dynamics of surface roughness in two highly eroded catchments of Mexico. Both areas are affected by gully erosion (Sidorchuk, 2005) and characterized by avalanche-like matter transport. Five contrasting morphological patterns were distinguished across the slope of the bare eroded surface of Faeozem (Queretaro State) while only one (apparently independent on the slope) roughness pattern was documented for Andosol (Michoacan State). We called these patterns ?the roughness clusters? and compared them in terms of metrizability, continuity, compactness, topological connectedness (global and local) and invariance, separability, and degree of ramification (Weyl, 1937). All mentioned topological measurands were correlated with the variance, skewness and kurtosis of the gray-level distribution of digital images. The morphology0 spatial dynamics of roughness clusters was measured and mapped with high precision in terms of fractal descriptors. The Hurst exponent was especially suitable to distinguish between the structure of ?turtle shell? and ?ramification? patterns (sediment producing zone A of the slope); as well as ?honeycomb? (sediment transport zone B) and ?dinosaur steps? and ?corals? (sediment deposition zone C) roughness clusters. Some other structural attributes of studied patterns were also statistically different and correlated with the variance, skewness and kurtosis of gray distribution of multiscale digital images. The scale invariance of classified roughness patterns was documented inside the range of five image resolutions. We conjectured that the geometrization of erosion patterns in terms of roughness clustering might benefit the most semi-quantitative models developed for erosion and sediment yield assessments (de Vente and Poesen, 2005).

Heterologous Expression of a Plant Small Heat-Shock Protein Enhances Escherichia Coli Viability under Heat And Cold Stress Ref.: 1

A small heat-shock protein (sHSP) that shows molecular chaperone activity in vitro was recently purified from mature chestnut (Castanea sativa) cotyledons. This protein, renamed here as CsHSP17.5, belongs to cytosolic class I, as revealed by cDNA sequencing and immunoelectron microscopy. Recombinant CsHSP17.5 was overexpressed in Escherichia coli to study its possible function under stress conditions. Upon transfer from 37°C to 50°C, a temperature known to cause cell autolysis, those cells that accumulated CsHSP17.5 showed improved viability compared with control cultures. Sodium dodecyl sulfate-polyacrylamide gel electrophoresis analysis of cell lysates suggested that such a protective effect in vivo is due to the ability of recombinant sHSP to maintain soluble cytosolic proteins in their native conformation, with little substrate specificity. To test the recent hypothesis that sHSPs may be involved in protection against cold stress, we also studied the viability of recombinant cells at 4°C. Unlike the major heat-induced chaperone, GroEL/ES, the chestnut sHSP significantly enhanced cell survivability at this temperature. CsHSP17.5 thus represents an example of a HSP capable of protecting cells against both thermal extremes. Consistent with these findings, high-level induction of homologous transcripts was observed in vegetative tissues of chestnut plantlets exposed to either type of thermal stress but not salt stress

Estimating Adaptacion of Dialogue Partners with Different Verbal Intelligence

This work investigates to what degree speakers with different verbal intelligence may adapt to each other. The work is based on a corpus consisting of 100 descriptions of a short film (monologues), 56 discussions about the same topic (dialogues), and verbal intelligence scores of the test participants. Adaptation between two dialogue partners was measured using cross-referencing, proportion of "I", "You" and "We" words, between-subject correlation and similarity of texts. It was shown that lower verbal intelligence speakers repeated more nouns and adjectives from the other and used the same linguistic categories more often than higher verbal intelligence speakers. In dialogues between strangers, participants with higher verbal intelligence showed a greater level of adaptation.

Prediction of wake effects on wind farm power production using a RANS approach. Part II. Offshore: Case studies from the UPWIND project

The estimation of power losses due to wind turbine wakes is crucial to understanding overall wind farm economics. This is especially true for large offshore wind farms, as it represents the primary source of losses in available power, given the regular arrangement of rotors, their generally largerdiameter and the lower ambient turbulence level, all of which conspire to dramatically affect wake expansion and, consequently, the power deficit. Simulation of wake effects in offshore wind farms (in reasonable computational time) is currently feasible using CFD tools. An elliptic CFD model basedon the actuator disk method and various RANS turbulence closure schemes is tested and validated using power ratios extracted from Horns Rev and Nysted wind farms, collected as part of the EU-funded UPWIND project. The primary focus of the present work is on turbulence modeling, as turbulent mixing is the main mechanism for flow recovery inside wind farms. A higher-order approach, based on the anisotropic RSM model, is tested to better take into account the imbalance in the length scales inside and outside of the wake, not well reproduced by current two-equation closure schemes.

A model of amacrine and ganglion cells for optical information processing

Based on a previously reported logic cell structure (see SPIE, vol. 2038, p. 67-77, 1993), the two types of cells present at the inner and ganglion cell layers of the vertebrate retina and their intracellular response, as well as their connections with each other, have been simulated. These cells are amacrines and ganglion cells. The main scheme of the authors' configuration is shown in a figure. These two types of cells, as well as some of their possible interconnections, have been implemented with the authors' previously reported optical-processing element. As it has been shown, the authors' logic structure is able to process two optical input binary signals, being the output two logical functions. Moreover, if a delayed feedback from one of the two possible outputs to one or both of the inputs is introduced, a very different behaviour is obtained. Depending on the value of the time delay, an oscillatory output can be obtained from a constant optical input signal. Period and length pulses are dependent on delay values, both external and internal, as well as on other control signals. Moreover, a chaotic behaviour can be obtained too under certain conditions

Run-Time Scalable Hardware for Reconfigurable Systems

La optimización de parámetros tales como el consumo de potencia, la cantidad de recursos lógicos empleados o la ocupación de memoria ha sido siempre una de las preocupaciones principales a la hora de diseñar sistemas embebidos. Esto es debido a que se trata de sistemas dotados de una cantidad de recursos limitados, y que han sido tradicionalmente empleados para un propósito específico, que permanece invariable a lo largo de toda la vida útil del sistema. Sin embargo, el uso de sistemas embebidos se ha extendido a áreas de aplicación fuera de su ámbito tradicional, caracterizadas por una mayor demanda computacional. Así, por ejemplo, algunos de estos sistemas deben llevar a cabo un intenso procesado de señales multimedia o la transmisión de datos mediante sistemas de comunicaciones de alta capacidad. Por otra parte, las condiciones de operación del sistema pueden variar en tiempo real. Esto sucede, por ejemplo, si su funcionamiento depende de datos medidos por el propio sistema o recibidos a través de la red, de las demandas del usuario en cada momento, o de condiciones internas del propio dispositivo, tales como la duración de la batería. Como consecuencia de la existencia de requisitos de operación dinámicos es necesario ir hacia una gestión dinámica de los recursos del sistema. Si bien el software es inherentemente flexible, no ofrece una potencia computacional tan alta como el hardware. Por lo tanto, el hardware reconfigurable aparece como una solución adecuada para tratar con mayor flexibilidad los requisitos variables dinámicamente en sistemas con alta demanda computacional. La flexibilidad y adaptabilidad del hardware requieren de dispositivos reconfigurables que permitan la modificación de su funcionalidad bajo demanda. En esta tesis se han seleccionado las FPGAs (Field Programmable Gate Arrays) como los dispositivos más apropiados, hoy en día, para implementar sistemas basados en hardware reconfigurable De entre todas las posibilidades existentes para explotar la capacidad de reconfiguración de las FPGAs comerciales, se ha seleccionado la reconfiguración dinámica y parcial. Esta técnica consiste en substituir una parte de la lógica del dispositivo, mientras el resto continúa en funcionamiento. La capacidad de reconfiguración dinámica y parcial de las FPGAs es empleada en esta tesis para tratar con los requisitos de flexibilidad y de capacidad computacional que demandan los dispositivos embebidos. La propuesta principal de esta tesis doctoral es el uso de arquitecturas de procesamiento escalables espacialmente, que son capaces de adaptar su funcionalidad y rendimiento en tiempo real, estableciendo un compromiso entre dichos parámetros y la cantidad de lógica que ocupan en el dispositivo. A esto nos referimos con arquitecturas con huellas escalables. En particular, se propone el uso de arquitecturas altamente paralelas, modulares, regulares y con una alta localidad en sus comunicaciones, para este propósito. El tamaño de dichas arquitecturas puede ser modificado mediante la adición o eliminación de algunos de los módulos que las componen, tanto en una dimensión como en dos. Esta estrategia permite implementar soluciones escalables, sin tener que contar con una versión de las mismas para cada uno de los tamaños posibles de la arquitectura. De esta manera se reduce significativamente el tiempo necesario para modificar su tamaño, así como la cantidad de memoria necesaria para almacenar todos los archivos de configuración. En lugar de proponer arquitecturas para aplicaciones específicas, se ha optado por patrones de procesamiento genéricos, que pueden ser ajustados para solucionar distintos problemas en el estado del arte. A este respecto, se proponen patrones basados en esquemas sistólicos, así como de tipo wavefront. Con el objeto de poder ofrecer una solución integral, se han tratado otros aspectos relacionados con el diseño y el funcionamiento de las arquitecturas, tales como el control del proceso de reconfiguración de la FPGA, la integración de las arquitecturas en el resto del sistema, así como las técnicas necesarias para su implementación. Por lo que respecta a la implementación, se han tratado distintos aspectos de bajo nivel dependientes del dispositivo. Algunas de las propuestas realizadas a este respecto en la presente tesis doctoral son un router que es capaz de garantizar el correcto rutado de los módulos reconfigurables dentro del área destinada para ellos, así como una estrategia para la comunicación entre módulos que no introduce ningún retardo ni necesita emplear recursos configurables del dispositivo. El flujo de diseño propuesto se ha automatizado mediante una herramienta denominada DREAMS. La herramienta se encarga de la modificación de las netlists correspondientes a cada uno de los módulos reconfigurables del sistema, y que han sido generadas previamente mediante herramientas comerciales. Por lo tanto, el flujo propuesto se entiende como una etapa de post-procesamiento, que adapta esas netlists a los requisitos de la reconfiguración dinámica y parcial. Dicha modificación la lleva a cabo la herramienta de una forma completamente automática, por lo que la productividad del proceso de diseño aumenta de forma evidente. Para facilitar dicho proceso, se ha dotado a la herramienta de una interfaz gráfica. El flujo de diseño propuesto, y la herramienta que lo soporta, tienen características específicas para abordar el diseño de las arquitecturas dinámicamente escalables propuestas en esta tesis. Entre ellas está el soporte para el realojamiento de módulos reconfigurables en posiciones del dispositivo distintas a donde el módulo es originalmente implementado, así como la generación de estructuras de comunicación compatibles con la simetría de la arquitectura. El router has sido empleado también en esta tesis para obtener un rutado simétrico entre nets equivalentes. Dicha posibilidad ha sido explotada para aumentar la protección de circuitos con altos requisitos de seguridad, frente a ataques de canal lateral, mediante la implantación de lógica complementaria con rutado idéntico. Para controlar el proceso de reconfiguración de la FPGA, se propone en esta tesis un motor de reconfiguración especialmente adaptado a los requisitos de las arquitecturas dinámicamente escalables. Además de controlar el puerto de reconfiguración, el motor de reconfiguración ha sido dotado de la capacidad de realojar módulos reconfigurables en posiciones arbitrarias del dispositivo, en tiempo real. De esta forma, basta con generar un único bitstream por cada módulo reconfigurable del sistema, independientemente de la posición donde va a ser finalmente reconfigurado. La estrategia seguida para implementar el proceso de realojamiento de módulos es diferente de las propuestas existentes en el estado del arte, pues consiste en la composición de los archivos de configuración en tiempo real. De esta forma se consigue aumentar la velocidad del proceso, mientras que se reduce la longitud de los archivos de configuración parciales a almacenar en el sistema. El motor de reconfiguración soporta módulos reconfigurables con una altura menor que la altura de una región de reloj del dispositivo. Internamente, el motor se encarga de la combinación de los frames que describen el nuevo módulo, con la configuración existente en el dispositivo previamente. El escalado de las arquitecturas de procesamiento propuestas en esta tesis también se puede beneficiar de este mecanismo. Se ha incorporado también un acceso directo a una memoria externa donde se pueden almacenar bitstreams parciales. Para acelerar el proceso de reconfiguración se ha hecho funcionar el ICAP por encima de la máxima frecuencia de reloj aconsejada por el fabricante. Así, en el caso de Virtex-5, aunque la máxima frecuencia del reloj deberían ser 100 MHz, se ha conseguido hacer funcionar el puerto de reconfiguración a frecuencias de operación de hasta 250 MHz, incluyendo el proceso de realojamiento en tiempo real. Se ha previsto la posibilidad de portar el motor de reconfiguración a futuras familias de FPGAs. Por otro lado, el motor de reconfiguración se puede emplear para inyectar fallos en el propio dispositivo hardware, y así ser capaces de evaluar la tolerancia ante los mismos que ofrecen las arquitecturas reconfigurables. Los fallos son emulados mediante la generación de archivos de configuración a los que intencionadamente se les ha introducido un error, de forma que se modifica su funcionalidad. Con el objetivo de comprobar la validez y los beneficios de las arquitecturas propuestas en esta tesis, se han seguido dos líneas principales de aplicación. En primer lugar, se propone su uso como parte de una plataforma adaptativa basada en hardware evolutivo, con capacidad de escalabilidad, adaptabilidad y recuperación ante fallos. En segundo lugar, se ha desarrollado un deblocking filter escalable, adaptado a la codificación de vídeo escalable, como ejemplo de aplicación de las arquitecturas de tipo wavefront propuestas. El hardware evolutivo consiste en el uso de algoritmos evolutivos para diseñar hardware de forma autónoma, explotando la flexibilidad que ofrecen los dispositivos reconfigurables. En este caso, los elementos de procesamiento que componen la arquitectura son seleccionados de una biblioteca de elementos presintetizados, de acuerdo con las decisiones tomadas por el algoritmo evolutivo, en lugar de definir la configuración de las mismas en tiempo de diseño. De esta manera, la configuración del core puede cambiar cuando lo hacen las condiciones del entorno, en tiempo real, por lo que se consigue un control autónomo del proceso de reconfiguración dinámico. Así, el sistema es capaz de optimizar, de forma autónoma, su propia configuración. El hardware evolutivo tiene una capacidad inherente de auto-reparación. Se ha probado que las arquitecturas evolutivas propuestas en esta tesis son tolerantes ante fallos, tanto transitorios, como permanentes y acumulativos. La plataforma evolutiva se ha empleado para implementar filtros de eliminación de ruido. La escalabilidad también ha sido aprovechada en esta aplicación. Las arquitecturas evolutivas escalables permiten la adaptación autónoma de los cores de procesamiento ante fluctuaciones en la cantidad de recursos disponibles en el sistema. Por lo tanto, constituyen un ejemplo de escalabilidad dinámica para conseguir un determinado nivel de calidad, que puede variar en tiempo real. Se han propuesto dos variantes de sistemas escalables evolutivos. El primero consiste en un único core de procesamiento evolutivo, mientras que el segundo está formado por un número variable de arrays de procesamiento. La codificación de vídeo escalable, a diferencia de los codecs no escalables, permite la decodificación de secuencias de vídeo con diferentes niveles de calidad, de resolución temporal o de resolución espacial, descartando la información no deseada. Existen distintos algoritmos que soportan esta característica. En particular, se va a emplear el estándar Scalable Video Coding (SVC), que ha sido propuesto como una extensión de H.264/AVC, ya que este último es ampliamente utilizado tanto en la industria, como a nivel de investigación. Para poder explotar toda la flexibilidad que ofrece el estándar, hay que permitir la adaptación de las características del decodificador en tiempo real. El uso de las arquitecturas dinámicamente escalables es propuesto en esta tesis con este objetivo. El deblocking filter es un algoritmo que tiene como objetivo la mejora de la percepción visual de la imagen reconstruida, mediante el suavizado de los "artefactos" de bloque generados en el lazo del codificador. Se trata de una de las tareas más intensivas en procesamiento de datos de H.264/AVC y de SVC, y además, su carga computacional es altamente dependiente del nivel de escalabilidad seleccionado en el decodificador. Por lo tanto, el deblocking filter ha sido seleccionado como prueba de concepto de la aplicación de las arquitecturas dinámicamente escalables para la compresión de video. La arquitectura propuesta permite añadir o eliminar unidades de computación, siguiendo un esquema de tipo wavefront. La arquitectura ha sido propuesta conjuntamente con un esquema de procesamiento en paralelo del deblocking filter a nivel de macrobloque, de tal forma que cuando se varía del tamaño de la arquitectura, el orden de filtrado de los macrobloques varia de la misma manera. El patrón propuesto se basa en la división del procesamiento de cada macrobloque en dos etapas independientes, que se corresponden con el filtrado horizontal y vertical de los bloques dentro del macrobloque. Las principales contribuciones originales de esta tesis son las siguientes: - El uso de arquitecturas altamente regulares, modulares, paralelas y con una intensa localidad en sus comunicaciones, para implementar cores de procesamiento dinámicamente reconfigurables. - El uso de arquitecturas bidimensionales, en forma de malla, para construir arquitecturas dinámicamente escalables, con una huella escalable. De esta forma, las arquitecturas permiten establecer un compromiso entre el área que ocupan en el dispositivo, y las prestaciones que ofrecen en cada momento. Se proponen plantillas de procesamiento genéricas, de tipo sistólico o wavefront, que pueden ser adaptadas a distintos problemas de procesamiento. - Un flujo de diseño y una herramienta que lo soporta, para el diseño de sistemas reconfigurables dinámicamente, centradas en el diseño de las arquitecturas altamente paralelas, modulares y regulares propuestas en esta tesis. - Un esquema de comunicaciones entre módulos reconfigurables que no introduce ningún retardo ni requiere el uso de recursos lógicos propios. - Un router flexible, capaz de resolver los conflictos de rutado asociados con el diseño de sistemas reconfigurables dinámicamente. - Un algoritmo de optimización para sistemas formados por múltiples cores escalables que optimice, mediante un algoritmo genético, los parámetros de dicho sistema. Se basa en un modelo conocido como el problema de la mochila. - Un motor de reconfiguración adaptado a los requisitos de las arquitecturas altamente regulares y modulares. Combina una alta velocidad de reconfiguración, con la capacidad de realojar módulos en tiempo real, incluyendo el soporte para la reconfiguración de regiones que ocupan menos que una región de reloj, así como la réplica de un módulo reconfigurable en múltiples posiciones del dispositivo. - Un mecanismo de inyección de fallos que, empleando el motor de reconfiguración del sistema, permite evaluar los efectos de fallos permanentes y transitorios en arquitecturas reconfigurables. - La demostración de las posibilidades de las arquitecturas propuestas en esta tesis para la implementación de sistemas de hardware evolutivos, con una alta capacidad de procesamiento de datos. - La implementación de sistemas de hardware evolutivo escalables, que son capaces de tratar con la fluctuación de la cantidad de recursos disponibles en el sistema, de una forma autónoma. - Una estrategia de procesamiento en paralelo para el deblocking filter compatible con los estándares H.264/AVC y SVC que reduce el número de ciclos de macrobloque necesarios para procesar un frame de video. - Una arquitectura dinámicamente escalable que permite la implementación de un nuevo deblocking filter, totalmente compatible con los estándares H.264/AVC y SVC, que explota el paralelismo a nivel de macrobloque. El presente documento se organiza en siete capítulos. En el primero se ofrece una introducción al marco tecnológico de esta tesis, especialmente centrado en la reconfiguración dinámica y parcial de FPGAs. También se motiva la necesidad de las arquitecturas dinámicamente escalables propuestas en esta tesis. En el capítulo 2 se describen las arquitecturas dinámicamente escalables. Dicha descripción incluye la mayor parte de las aportaciones a nivel arquitectural realizadas en esta tesis. Por su parte, el flujo de diseño adaptado a dichas arquitecturas se propone en el capítulo 3. El motor de reconfiguración se propone en el 4, mientras que el uso de dichas arquitecturas para implementar sistemas de hardware evolutivo se aborda en el 5. El deblocking filter escalable se describe en el 6, mientras que las conclusiones finales de esta tesis, así como la descripción del trabajo futuro, son abordadas en el capítulo 7. ABSTRACT The optimization of system parameters, such as power dissipation, the amount of hardware resources and the memory footprint, has been always a main concern when dealing with the design of resource-constrained embedded systems. This situation is even more demanding nowadays. Embedded systems cannot anymore be considered only as specific-purpose computers, designed for a particular functionality that remains unchanged during their lifetime. Differently, embedded systems are now required to deal with more demanding and complex functions, such as multimedia data processing and high-throughput connectivity. In addition, system operation may depend on external data, the user requirements or internal variables of the system, such as the battery life-time. All these conditions may vary at run-time, leading to adaptive scenarios. As a consequence of both the growing computational complexity and the existence of dynamic requirements, dynamic resource management techniques for embedded systems are needed. Software is inherently flexible, but it cannot meet the computing power offered by hardware solutions. Therefore, reconfigurable hardware emerges as a suitable technology to deal with the run-time variable requirements of complex embedded systems. Adaptive hardware requires the use of reconfigurable devices, where its functionality can be modified on demand. In this thesis, Field Programmable Gate Arrays (FPGAs) have been selected as the most appropriate commercial technology existing nowadays to implement adaptive hardware systems. There are different ways of exploiting reconfigurability in reconfigurable devices. Among them is dynamic and partial reconfiguration. This is a technique which consists in substituting part of the FPGA logic on demand, while the rest of the device continues working. The strategy followed in this thesis is to exploit the dynamic and partial reconfiguration of commercial FPGAs to deal with the flexibility and complexity demands of state-of-the-art embedded systems. The proposal of this thesis to deal with run-time variable system conditions is the use of spatially scalable processing hardware IP cores, which are able to adapt their functionality or performance at run-time, trading them off with the amount of logic resources they occupy in the device. This is referred to as a scalable footprint in the context of this thesis. The distinguishing characteristic of the proposed cores is that they rely on highly parallel, modular and regular architectures, arranged in one or two dimensions. These architectures can be scaled by means of the addition or removal of the composing blocks. This strategy avoids implementing a full version of the core for each possible size, with the corresponding benefits in terms of scaling and adaptation time, as well as bitstream storage memory requirements. Instead of providing specific-purpose architectures, generic architectural templates, which can be tuned to solve different problems, are proposed in this thesis. Architectures following both systolic and wavefront templates have been selected. Together with the proposed scalable architectural templates, other issues needed to ensure the proper design and operation of the scalable cores, such as the device reconfiguration control, the run-time management of the architecture and the implementation techniques have been also addressed in this thesis. With regard to the implementation of dynamically reconfigurable architectures, device dependent low-level details are addressed. Some of the aspects covered in this thesis are the area constrained routing for reconfigurable modules, or an inter-module communication strategy which does not introduce either extra delay or logic overhead. The system implementation, from the hardware description to the device configuration bitstream, has been fully automated by modifying the netlists corresponding to each of the system modules, which are previously generated using the vendor tools. This modification is therefore envisaged as a post-processing step. Based on these implementation proposals, a design tool called DREAMS (Dynamically Reconfigurable Embedded and Modular Systems) has been created, including a graphic user interface. The tool has specific features to cope with modular and regular architectures, including the support for module relocation and the inter-module communications scheme based on the symmetry of the architecture. The core of the tool is a custom router, which has been also exploited in this thesis to obtain symmetric routed nets, with the aim of enhancing the protection of critical reconfigurable circuits against side channel attacks. This is achieved by duplicating the logic with an exactly equal routing. In order to control the reconfiguration process of the FPGA, a Reconfiguration Engine suited to the specific requirements set by the proposed architectures was also proposed. Therefore, in addition to controlling the reconfiguration port, the Reconfiguration Engine has been enhanced with the online relocation ability, which allows employing a unique configuration bitstream for all the positions where the module may be placed in the device. Differently to the existing relocating solutions, which are based on bitstream parsers, the proposed approach is based on the online composition of bitstreams. This strategy allows increasing the speed of the process, while the length of partial bitstreams is also reduced. The height of the reconfigurable modules can be lower than the height of a clock region. The Reconfiguration Engine manages the merging process of the new and the existing configuration frames within each clock region. The process of scaling up and down the hardware cores also benefits from this technique. A direct link to an external memory where partial bitstreams can be stored has been also implemented. In order to accelerate the reconfiguration process, the ICAP has been overclocked over the speed reported by the manufacturer. In the case of Virtex-5, even though the maximum frequency of the ICAP is reported to be 100 MHz, valid operations at 250 MHz have been achieved, including the online relocation process. Portability of the reconfiguration solution to today's and probably, future FPGAs, has been also considered. The reconfiguration engine can be also used to inject faults in real hardware devices, and this way being able to evaluate the fault tolerance offered by the reconfigurable architectures. Faults are emulated by introducing partial bitstreams intentionally modified to provide erroneous functionality. To prove the validity and the benefits offered by the proposed architectures, two demonstration application lines have been envisaged. First, scalable architectures have been employed to develop an evolvable hardware platform with adaptability, fault tolerance and scalability properties. Second, they have been used to implement a scalable deblocking filter suited to scalable video coding. Evolvable Hardware is the use of evolutionary algorithms to design hardware in an autonomous way, exploiting the flexibility offered by reconfigurable devices. In this case, processing elements composing the architecture are selected from a presynthesized library of processing elements, according to the decisions taken by the algorithm, instead of being decided at design time. This way, the configuration of the array may change as run-time environmental conditions do, achieving autonomous control of the dynamic reconfiguration process. Thus, the self-optimization property is added to the native self-configurability of the dynamically scalable architectures. In addition, evolvable hardware adaptability inherently offers self-healing features. The proposal has proved to be self-tolerant, since it is able to self-recover from both transient and cumulative permanent faults. The proposed evolvable architecture has been used to implement noise removal image filters. Scalability has been also exploited in this application. Scalable evolvable hardware architectures allow the autonomous adaptation of the processing cores to a fluctuating amount of resources available in the system. Thus, it constitutes an example of the dynamic quality scalability tackled in this thesis. Two variants have been proposed. The first one consists in a single dynamically scalable evolvable core, and the second one contains a variable number of processing cores. Scalable video is a flexible approach for video compression, which offers scalability at different levels. Differently to non-scalable codecs, a scalable video bitstream can be decoded with different levels of quality, spatial or temporal resolutions, by discarding the undesired information. The interest in this technology has been fostered by the development of the Scalable Video Coding (SVC) standard, as an extension of H.264/AVC. In order to exploit all the flexibility offered by the standard, it is necessary to adapt the characteristics of the decoder to the requirements of each client during run-time. The use of dynamically scalable architectures is proposed in this thesis with this aim. The deblocking filter algorithm is the responsible of improving the visual perception of a reconstructed image, by smoothing blocking artifacts generated in the encoding loop. This is one of the most computationally intensive tasks of the standard, and furthermore, it is highly dependent on the selected scalability level in the decoder. Therefore, the deblocking filter has been selected as a proof of concept of the implementation of dynamically scalable architectures for video compression. The proposed architecture allows the run-time addition or removal of computational units working in parallel to change its level of parallelism, following a wavefront computational pattern. Scalable architecture is offered together with a scalable parallelization strategy at the macroblock level, such that when the size of the architecture changes, the macroblock filtering order is modified accordingly. The proposed pattern is based on the division of the macroblock processing into two independent stages, corresponding to the horizontal and vertical filtering of the blocks within the macroblock. The main contributions of this thesis are: - The use of highly parallel, modular, regular and local architectures to implement dynamically reconfigurable processing IP cores, for data intensive applications with flexibility requirements. - The use of two-dimensional mesh-type arrays as architectural templates to build dynamically reconfigurable IP cores, with a scalable footprint. The proposal consists in generic architectural templates, which can be tuned to solve different computational problems. •A design flow and a tool targeting the design of DPR systems, focused on highly parallel, modular and local architectures. - An inter-module communication strategy, which does not introduce delay or area overhead, named Virtual Borders. - A custom and flexible router to solve the routing conflicts as well as the inter-module communication problems, appearing during the design of DPR systems. - An algorithm addressing the optimization of systems composed of multiple scalable cores, which size can be decided individually, to optimize the system parameters. It is based on a model known as the multi-dimensional multi-choice Knapsack problem. - A reconfiguration engine tailored to the requirements of highly regular and modular architectures. It combines a high reconfiguration throughput with run-time module relocation capabilities, including the support for sub-clock reconfigurable regions and the replication in multiple positions. - A fault injection mechanism which takes advantage of the system reconfiguration engine, as well as the modularity of the proposed reconfigurable architectures, to evaluate the effects of transient and permanent faults in these architectures. - The demonstration of the possibilities of the architectures proposed in this thesis to implement evolvable hardware systems, while keeping a high processing throughput. - The implementation of scalable evolvable hardware systems, which are able to adapt to the fluctuation of the amount of resources available in the system, in an autonomous way. - A parallelization strategy for the H.264/AVC and SVC deblocking filter, which reduces the number of macroblock cycles needed to process the whole frame. - A dynamically scalable architecture that permits the implementation of a novel deblocking filter module, fully compliant with the H.264/AVC and SVC standards, which exploits the macroblock level parallelism of the algorithm. This document is organized in seven chapters. In the first one, an introduction to the technology framework of this thesis, specially focused on dynamic and partial reconfiguration, is provided. The need for the dynamically scalable processing architectures proposed in this work is also motivated in this chapter. In chapter 2, dynamically scalable architectures are described. Description includes most of the architectural contributions of this work. The design flow tailored to the scalable architectures, together with the DREAMs tool provided to implement them, are described in chapter 3. The reconfiguration engine is described in chapter 4. The use of the proposed scalable archtieectures to implement evolvable hardware systems is described in chapter 5, while the scalable deblocking filter is described in chapter 6. Final conclusions of this thesis, and the description of future work, are addressed in chapter 7.

Procedure for verification of sound source coverage over façades according to the International Standard ISO 140-5

This paper presents a new verification procedure for sound source coverage according to ISO 140?5 requirements. The ISO 140?5 standard applies to the measurement of façade insulation and requires a sound source able to achieve a sufficiently uniform sound field in free field conditions on the façade under study. The proposed method involves the electroacoustic characterisation of the sound source in laboratory free field conditions (anechoic room) and the subsequent prediction by computer simulation of the sound free field radiated on a rectangular surface equal in size to the façade being measured. The loudspeaker is characterised in an anechoic room under laboratory controlled conditions, carefully measuring directivity, and then a computer model is designed to calculate the acoustic free field coverage for different loudspeaker positions and façade sizes. For each sound source position, the method provides the maximum direct acoustic level differences on a façade specimen and therefore determines whether the loudspeaker verifies the maximum allowed level difference of 5 dB (or 10 dB for façade dimensions greater than 5 m) required by the ISO standard. Additionally, the maximum horizontal dimension of the façade meeting the standard is calculated and provided for each sound source position, both with the 5 dB and 10 dB criteria. In the last section of the paper, the proposed procedure is compared with another method used by the authors in the past to achieve the same purpose: in situ outdoor measurements attempting to recreate free field conditions. From this comparison, it is concluded that the proposed method is able to reproduce the actual measurements with high accuracy, for example, the ground reflection effect, at least at low frequencies, which is difficult to avoid in the outdoor measurement method, and it is fully eliminated with the proposed method to achieve the free field requisite.

Impact of new technologies and social networks on a secondary education theatre project

This paper describes the potential impact of social media and new technologies in secondary education. The case of study has been designed for the drama and theatre subject. A wide set of tools like social networks, blogs, internet, multimedia content, local press and other promotional tools are promoted to increase students’ motivation. The experiment was developed at the highschool IES Al-Satt located in Algete in the Comunidad de Madrid. The students included in the theatre group present a low academic level, 80% of them had previously repeated at least one grade, half of them come from programs for students with learning difficulties and were at risk of social exclusion. This action is supported by higher and secondary education professors and teachers who look forward to implanting networked media technologies as new tools to improve the academic results and the degree of involvement of students. The results of the experiment have been excellent, based on satisfactory opinions obtained from a survey answered by students at the end of the course, and also revealed by the analytics taken from different social networks. This project is a pioneer in the introduction and usage of new technologies in secondary high-schools in Spain.

From arrays of THz antennas to large-area emitters

Arrays of coherently driven photomixers with antenna (antenna emitter arrays, AEAs) have been evaluated as a possibility to overcome the power limitations of individual conventional photomixers with antenna (?antenna emitters?, AEs) for the generation of continuous-wave (CW) THz radiation. In this paper, ?large area emitters? (LAEs) are proposed as an alternative approach, and compared with AEAs. In this antenna-free new scheme of photomixing, the THz radiation originates directly from the acceleration of photo-induced charge carriers generated within a large semiconductor area. The quasi-continuous distribution of emitting elements corresponds to a high-density array and results in favorable radiation profiles without side lobes. Moreover, the achievable THz power is expected to outnumber even large AEAs. Last not least, the technological challenge of fabricating LAEs appears to be significantly less demanding.

On the simulation of the UPMSAT-2 microsatellite power

Simulation of satellite subsystems behaviour is extramely important in the design at early stages. The subsystems are normally simulated in the both ways : isolated and as part of more complex simulation that takes into account imputs from other subsystems (concurrent design). In the present work, a simple concurrent simulation of the power subsystem of a microsatellite, UPMSat-2, is described. The aim of the work is to obtain the performance profile of the system (battery charging level, power consumption by the payloads, power supply from solar panels....). Different situations such as battery critical low or high level, effects of high current charging due to the low temperature of solar panels after eclipse,DoD margins..., were analysed, and different safety strategies studied using the developed tool (simulator) to fulfil the mission requirements. Also, failure cases were analysed in order to study the robustness of the system. The mentioned simulator has been programed taking into account the power consumption performances (average and maximum consumptions per orbit/day) of small part of the subsystem (SELEX GALILEO SPVS modular generators built with Azur Space solar cells, SAFT VES16 6P4S Li-ion battery, SSBV magnetometers, TECNOBIT and DATSI/UPM On Board Data Handling -OBDH-...). The developed tool is then intended to be a modular simulator, with the chance of use any other components implementing some standard data.

A new analog trigger system for the Cherenkov Telescope array

La astronomía de rayos γ estudia las partículas más energéticas que llegan a la Tierra desde el espacio. Estos rayos γ no se generan mediante procesos térmicos en simples estrellas, sino mediante mecanismos de aceleración de partículas en objetos celestes como núcleos de galaxias activos, púlsares, supernovas, o posibles procesos de aniquilación de materia oscura. Los rayos γ procedentes de estos objetos y sus características proporcionan una valiosa información con la que los científicos tratan de comprender los procesos físicos que ocurren en ellos y desarrollar modelos teóricos que describan su funcionamiento con fidelidad. El problema de observar rayos γ es que son absorbidos por las capas altas de la atmósfera y no llegan a la superficie (de lo contrario, la Tierra será inhabitable). De este modo, sólo hay dos formas de observar rayos γ embarcar detectores en satélites, u observar los efectos secundarios que los rayos γ producen en la atmósfera. Cuando un rayo γ llega a la atmósfera, interacciona con las partículas del aire y genera un par electrón - positrón, con mucha energía. Estas partículas secundarias generan a su vez más partículas secundarias cada vez menos energéticas. Estas partículas, mientras aún tienen energía suficiente para viajar más rápido que la velocidad de la luz en el aire, producen una radiación luminosa azulada conocida como radiación Cherenkov durante unos pocos nanosegundos. Desde la superficie de la Tierra, algunos telescopios especiales, conocidos como telescopios Cherenkov o IACTs (Imaging Atmospheric Cherenkov Telescopes), son capaces de detectar la radiación Cherenkov e incluso de tomar imágenes de la forma de la cascada Cherenkov. A partir de estas imágenes es posible conocer las principales características del rayo γ original, y con suficientes rayos se pueden deducir características importantes del objeto que los emitió, a cientos de años luz de distancia. Sin embargo, detectar cascadas Cherenkov procedentes de rayos γ no es nada fácil. Las cascadas generadas por fotones γ de bajas energías emiten pocos fotones, y durante pocos nanosegundos, y las correspondientes a rayos γ de alta energía, si bien producen más electrones y duran más, son más improbables conforme mayor es su energía. Esto produce dos líneas de desarrollo de telescopios Cherenkov: Para observar cascadas de bajas energías son necesarios grandes reflectores que recuperen muchos fotones de los pocos que tienen estas cascadas. Por el contrario, las cascadas de altas energías se pueden detectar con telescopios pequeños, pero conviene cubrir con ellos una superficie grande en el suelo para aumentar el número de eventos detectados. Con el objetivo de mejorar la sensibilidad de los telescopios Cherenkov actuales, en el rango de energía alto (> 10 TeV), medio (100 GeV - 10 TeV) y bajo (10 GeV - 100 GeV), nació el proyecto CTA (Cherenkov Telescope Array). Este proyecto en el que participan más de 27 países, pretende construir un observatorio en cada hemisferio, cada uno de los cuales contará con 4 telescopios grandes (LSTs), unos 30 medianos (MSTs) y hasta 70 pequeños (SSTs). Con un array así, se conseguirán dos objetivos. En primer lugar, al aumentar drásticamente el área de colección respecto a los IACTs actuales, se detectarán más rayos γ en todos los rangos de energía. En segundo lugar, cuando una misma cascada Cherenkov es observada por varios telescopios a la vez, es posible analizarla con mucha más precisión gracias a las técnicas estereoscópicas. La presente tesis recoge varios desarrollos técnicos realizados como aportación a los telescopios medianos y grandes de CTA, concretamente al sistema de trigger. Al ser las cascadas Cherenkov tan breves, los sistemas que digitalizan y leen los datos de cada píxel tienen que funcionar a frecuencias muy altas (≈1 GHz), lo que hace inviable que funcionen de forma continua, ya que la cantidad de datos guardada será inmanejable. En su lugar, las señales analógicas se muestrean, guardando las muestras analógicas en un buffer circular de unos pocos µs. Mientras las señales se mantienen en el buffer, el sistema de trigger hace un análisis rápido de las señales recibidas, y decide si la imagen que hay en el buér corresponde a una cascada Cherenkov y merece ser guardada, o por el contrario puede ignorarse permitiendo que el buffer se sobreescriba. La decisión de si la imagen merece ser guardada o no, se basa en que las cascadas Cherenkov producen detecciones de fotones en píxeles cercanos y en tiempos muy próximos, a diferencia de los fotones de NSB (night sky background), que llegan aleatoriamente. Para detectar cascadas grandes es suficiente con comprobar que más de un cierto número de píxeles en una región hayan detectado más de un cierto número de fotones en una ventana de tiempo de algunos nanosegundos. Sin embargo, para detectar cascadas pequeñas es más conveniente tener en cuenta cuántos fotones han sido detectados en cada píxel (técnica conocida como sumtrigger). El sistema de trigger desarrollado en esta tesis pretende optimizar la sensibilidad a bajas energías, por lo que suma analógicamente las señales recibidas en cada píxel en una región de trigger y compara el resultado con un umbral directamente expresable en fotones detectados (fotoelectrones). El sistema diseñado permite utilizar regiones de trigger de tamaño seleccionable entre 14, 21 o 28 píxeles (2, 3, o 4 clusters de 7 píxeles cada uno), y con un alto grado de solapamiento entre ellas. De este modo, cualquier exceso de luz en una región compacta de 14, 21 o 28 píxeles es detectado y genera un pulso de trigger. En la versión más básica del sistema de trigger, este pulso se distribuye por toda la cámara de forma que todos los clusters sean leídos al mismo tiempo, independientemente de su posición en la cámara, a través de un delicado sistema de distribución. De este modo, el sistema de trigger guarda una imagen completa de la cámara cada vez que se supera el número de fotones establecido como umbral en una región de trigger. Sin embargo, esta forma de operar tiene dos inconvenientes principales. En primer lugar, la cascada casi siempre ocupa sólo una pequeña zona de la cámara, por lo que se guardan muchos píxeles sin información alguna. Cuando se tienen muchos telescopios como será el caso de CTA, la cantidad de información inútil almacenada por este motivo puede ser muy considerable. Por otro lado, cada trigger supone guardar unos pocos nanosegundos alrededor del instante de disparo. Sin embargo, en el caso de cascadas grandes la duración de las mismas puede ser bastante mayor, perdiéndose parte de la información debido al truncamiento temporal. Para resolver ambos problemas se ha propuesto un esquema de trigger y lectura basado en dos umbrales. El umbral alto decide si hay un evento en la cámara y, en caso positivo, sólo las regiones de trigger que superan el nivel bajo son leídas, durante un tiempo más largo. De este modo se evita guardar información de píxeles vacíos y las imágenes fijas de las cascadas se pueden convertir en pequeños \vídeos" que representen el desarrollo temporal de la cascada. Este nuevo esquema recibe el nombre de COLIBRI (Concept for an Optimized Local Image Building and Readout Infrastructure), y se ha descrito detalladamente en el capítulo 5. Un problema importante que afecta a los esquemas de sumtrigger como el que se presenta en esta tesis es que para sumar adecuadamente las señales provenientes de cada píxel, estas deben tardar lo mismo en llegar al sumador. Los fotomultiplicadores utilizados en cada píxel introducen diferentes retardos que deben compensarse para realizar las sumas adecuadamente. El efecto de estos retardos ha sido estudiado, y se ha desarrollado un sistema para compensarlos. Por último, el siguiente nivel de los sistemas de trigger para distinguir efectivamente las cascadas Cherenkov del NSB consiste en buscar triggers simultáneos (o en tiempos muy próximos) en telescopios vecinos. Con esta función, junto con otras de interfaz entre sistemas, se ha desarrollado un sistema denominado Trigger Interface Board (TIB). Este sistema consta de un módulo que irá montado en la cámara de cada LST o MST, y que estará conectado mediante fibras ópticas a los telescopios vecinos. Cuando un telescopio tiene un trigger local, este se envía a todos los vecinos conectados y viceversa, de modo que cada telescopio sabe si sus vecinos han dado trigger. Una vez compensadas las diferencias de retardo debidas a la propagación en las fibras ópticas y de los propios fotones Cherenkov en el aire dependiendo de la dirección de apuntamiento, se buscan coincidencias, y en el caso de que la condición de trigger se cumpla, se lee la cámara en cuestión, de forma sincronizada con el trigger local. Aunque todo el sistema de trigger es fruto de la colaboración entre varios grupos, fundamentalmente IFAE, CIEMAT, ICC-UB y UCM en España, con la ayuda de grupos franceses y japoneses, el núcleo de esta tesis son el Level 1 y la Trigger Interface Board, que son los dos sistemas en los que que el autor ha sido el ingeniero principal. Por este motivo, en la presente tesis se ha incluido abundante información técnica relativa a estos sistemas. Existen actualmente importantes líneas de desarrollo futuras relativas tanto al trigger de la cámara (implementación en ASICs), como al trigger entre telescopios (trigger topológico), que darán lugar a interesantes mejoras sobre los diseños actuales durante los próximos años, y que con suerte serán de provecho para toda la comunidad científica participante en CTA. ABSTRACT -ray astronomy studies the most energetic particles arriving to the Earth from outer space. This -rays are not generated by thermal processes in mere stars, but by means of particle acceleration mechanisms in astronomical objects such as active galactic nuclei, pulsars, supernovas or as a result of dark matter annihilation processes. The γ rays coming from these objects and their characteristics provide with valuable information to the scientist which try to understand the underlying physical fundamentals of these objects, as well as to develop theoretical models able to describe them accurately. The problem when observing rays is that they are absorbed in the highest layers of the atmosphere, so they don't reach the Earth surface (otherwise the planet would be uninhabitable). Therefore, there are only two possible ways to observe γ rays: by using detectors on-board of satellites, or by observing their secondary effects in the atmosphere. When a γ ray reaches the atmosphere, it interacts with the particles in the air generating a highly energetic electron-positron pair. These secondary particles generate in turn more particles, with less energy each time. While these particles are still energetic enough to travel faster than the speed of light in the air, they produce a bluish radiation known as Cherenkov light during a few nanoseconds. From the Earth surface, some special telescopes known as Cherenkov telescopes or IACTs (Imaging Atmospheric Cherenkov Telescopes), are able to detect the Cherenkov light and even to take images of the Cherenkov showers. From these images it is possible to know the main parameters of the original -ray, and with some -rays it is possible to deduce important characteristics of the emitting object, hundreds of light-years away. However, detecting Cherenkov showers generated by γ rays is not a simple task. The showers generated by low energy -rays contain few photons and last few nanoseconds, while the ones corresponding to high energy -rays, having more photons and lasting more time, are much more unlikely. This results in two clearly differentiated development lines for IACTs: In order to detect low energy showers, big reflectors are required to collect as much photons as possible from the few ones that these showers have. On the contrary, small telescopes are able to detect high energy showers, but a large area in the ground should be covered to increase the number of detected events. With the aim to improve the sensitivity of current Cherenkov showers in the high (> 10 TeV), medium (100 GeV - 10 TeV) and low (10 GeV - 100 GeV) energy ranges, the CTA (Cherenkov Telescope Array) project was created. This project, with more than 27 participating countries, intends to build an observatory in each hemisphere, each one equipped with 4 large size telescopes (LSTs), around 30 middle size telescopes (MSTs) and up to 70 small size telescopes (SSTs). With such an array, two targets would be achieved. First, the drastic increment in the collection area with respect to current IACTs will lead to detect more -rays in all the energy ranges. Secondly, when a Cherenkov shower is observed by several telescopes at the same time, it is possible to analyze it much more accurately thanks to the stereoscopic techniques. The present thesis gathers several technical developments for the trigger system of the medium and large size telescopes of CTA. As the Cherenkov showers are so short, the digitization and readout systems corresponding to each pixel must work at very high frequencies (_ 1 GHz). This makes unfeasible to read data continuously, because the amount of data would be unmanageable. Instead, the analog signals are sampled, storing the analog samples in a temporal ring buffer able to store up to a few _s. While the signals remain in the buffer, the trigger system performs a fast analysis of the signals and decides if the image in the buffer corresponds to a Cherenkov shower and deserves to be stored, or on the contrary it can be ignored allowing the buffer to be overwritten. The decision of saving the image or not, is based on the fact that Cherenkov showers produce photon detections in close pixels during near times, in contrast to the random arrival of the NSB phtotons. Checking if more than a certain number of pixels in a trigger region have detected more than a certain number of photons during a certain time window is enough to detect large showers. However, taking also into account how many photons have been detected in each pixel (sumtrigger technique) is more convenient to optimize the sensitivity to low energy showers. The developed trigger system presented in this thesis intends to optimize the sensitivity to low energy showers, so it performs the analog addition of the signals received in each pixel in the trigger region and compares the sum with a threshold which can be directly expressed as a number of detected photons (photoelectrons). The trigger system allows to select trigger regions of 14, 21, or 28 pixels (2, 3 or 4 clusters with 7 pixels each), and with extensive overlapping. In this way, every light increment inside a compact region of 14, 21 or 28 pixels is detected, and a trigger pulse is generated. In the most basic version of the trigger system, this pulse is just distributed throughout the camera in such a way that all the clusters are read at the same time, independently from their position in the camera, by means of a complex distribution system. Thus, the readout saves a complete camera image whenever the number of photoelectrons set as threshold is exceeded in a trigger region. However, this way of operating has two important drawbacks. First, the shower usually covers only a little part of the camera, so many pixels without relevant information are stored. When there are many telescopes as will be the case of CTA, the amount of useless stored information can be very high. On the other hand, with every trigger only some nanoseconds of information around the trigger time are stored. In the case of large showers, the duration of the shower can be quite larger, loosing information due to the temporal cut. With the aim to solve both limitations, a trigger and readout scheme based on two thresholds has been proposed. The high threshold decides if there is a relevant event in the camera, and in the positive case, only the trigger regions exceeding the low threshold are read, during a longer time. In this way, the information from empty pixels is not stored and the fixed images of the showers become to little \`videos" containing the temporal development of the shower. This new scheme is named COLIBRI (Concept for an Optimized Local Image Building and Readout Infrastructure), and it has been described in depth in chapter 5. An important problem affecting sumtrigger schemes like the one presented in this thesis is that in order to add the signals from each pixel properly, they must arrive at the same time. The photomultipliers used in each pixel introduce different delays which must be compensated to perform the additions properly. The effect of these delays has been analyzed, and a delay compensation system has been developed. The next trigger level consists of looking for simultaneous (or very near in time) triggers in neighbour telescopes. These function, together with others relating to interfacing different systems, have been developed in a system named Trigger Interface Board (TIB). This system is comprised of one module which will be placed inside the LSTs and MSTs cameras, and which will be connected to the neighbour telescopes through optical fibers. When a telescope receives a local trigger, it is resent to all the connected neighbours and vice-versa, so every telescope knows if its neighbours have been triggered. Once compensated the delay differences due to propagation in the optical fibers and in the air depending on the pointing direction, the TIB looks for coincidences, and in the case that the trigger condition is accomplished, the camera is read a fixed time after the local trigger arrived. Despite all the trigger system is the result of the cooperation of several groups, specially IFAE, Ciemat, ICC-UB and UCM in Spain, with some help from french and japanese groups, the Level 1 and the Trigger Interface Board constitute the core of this thesis, as they have been the two systems designed by the author of the thesis. For this reason, a large amount of technical information about these systems has been included. There are important future development lines regarding both the camera trigger (implementation in ASICS) and the stereo trigger (topological trigger), which will produce interesting improvements for the current designs during the following years, being useful for all the scientific community participating in CTA.