Modelação do comportamento dinâmico de sistemas barragem-fundação-albufeira: análise sísmica de uma barragem de abóbadas múltiplas

Trabalho Final de Mestrado elaborado no Laboratório Nacional de Engenharia Civil (LNEC) para a obtenção do grau de Mestre em Engenharia Civil pelo Instituto Superior de Engenharia de Lisboa no âmbito do protocolo de cooperação entre o ISEL e o LNEC

Projeto de fundações e estrutura de ampliação de escola utilizando os eurocódigos estruturais

Trabalho Final de Mestrado para obtenção do grau de Mestre em Engenharia Civil na Área de Especialização estruturas

Projeto de estruturas de um edifício em betão armado com recurso ao programa de cálculo automático ETABS

Trabalho de Projeto para obtenção do grau de mestre em Engenharia Civil

Projeto de fundações e estrutura de um edifício em Lisboa

Trabalho de Projeto para obtenção do grau de Mestre em Engenharia Civil na Área de Especialização em Estruturas

Modèles d'atmosphères hors-ETL avec métaux : applications aux étoiles sous-naines chaudes

Avec la mise en place dans les dernières années d'une grappe d'ordinateurs (CALYS) dédiés aux calculs de modèles stellaires pour notre groupe de recherche, il nous est désormais possible d'exploiter à leur plein potentiel les modèles d'atmosphères hors équilibre thermodynamique local (HETL) en y incluant des éléments métalliques. Ce type de modèles, plutôt exigeant en temps de calcul, est toutefois essentiel pour analyser correctement les spectres d'étoiles chaudes comme les sous-naines de type O (sdO). Les travaux effectués dans le cadre de cette thèse ont comme point commun l'utilisation de tels modèles d'atmosphères pour faire l'analyse spectroscopique d'étoiles sous-naines chaudes dans des contextes variés. Le coeur de cette thèse porte sur Bd+28 4211, une étoile standard de type sdO très chaude, dans laquelle le problème des raies de Balmer, qui empêche de reproduire ces dernières avec une unique, et réaliste, combinaison de paramètres atmosphériques, est bien présent. Dans un premier temps nous présentons une analyse approfondie de son spectre ultraviolet (UV). Cela nous permet de déterminer les abondances de métaux dans l'atmosphère de l'étoile et de contraindre sa température effective et sa gravité de surface. Par la suite, ces résultats servent de point de départ à l'analyse du spectre optique de l'étoile, dans lequel le problème des raies de Balmer se fait sentir. Cette analyse nous permet de conclure que l'inclusion des abondances métalliques propres à l'étoile dans les modèles d'atmosphères HETL n'est pas suffisant pour surmonter le problème des raies de Balmer. Toutefois, en y incluant des abondances dix fois solaires, nous arrivons à reproduire correctement les raies de Balmer et d'hélium présentes dans les spectres visibles lors d'un ajustement de paramètres. De plus, les paramètres résultants concordent avec ceux indiqués par le spectre UV. Nous concluons que des sources d'opacité encore inconnues ou mal modélisées sont à la source de ce problème endémique aux étoiles chaudes. Par la suite nous faisons une étude spectroscopique de Feige 48, une étoile de type sdB pulsante particulièrement importante. Nous arrivons à reproduire très bien le spectre visible de cette étoile, incluant les nombreuses raies métalliques qui s'y trouvent. Les paramètres fondamentaux obtenus pour Feige 48 corroborent ceux déjà présents dans la littérature, qui ont été obtenus avec des types de modèles d'atmosphères moins sophistiqués, ce qui implique que les effets HETL couplés à la présence de métaux ne sont pas importants dans l'atmosphère de cette étoile particulière. Nous pouvons donc affirmer que les paramètres de cette étoile sont fiables et peuvent servir de base à une future étude astérosismologique quantitative. Finalement, 38 étoiles sous-naines chaudes appartenant à l'amas globulaire omega Centauri ont été analysées afin de déterminer, outre leur température et gravité de surface, leurs abondances d'hélium et de carbone. Nous montrons qu'il existe une corrélation entre les abondances photosphériques de ces deux éléments. Nous trouvons aussi des différences entre les étoiles riches en hélium de l'amas du celles du champ. Dans leur ensemble, nos résultats remettent en question notre compréhension du mécanisme de formation des sous-naines riches en hélium.

Subsídios para o projeto de estruturas sismo resistentes

Through this research is detailed the Brazilian seismic code focused on concrete projects design related to seismic engineering. At the beginning of the research is debated the fundaments of the seismic effects, the influence factors to the development of seismic effects and also relates the main data registration happened in Brazil. The second step is study the Brazilian seismic code explaining all the concepts related to it and does a compilation to the most important international seismic code. At this research is developed the designing of a building submitted to horizontal equivalent seismic forces and the modal process based on the answer spectrum based on the brazilin seismic code. It was also developed the design of a commercial building submitted to seismic loads based on the Brazilian code answer spectrum and compared to the same building submitted to wind loads.The research also focus on projects conception and detailing of seismic engineering Project design. At the study of seismic engineering it was concluded that seismic effects require special focus on concrete structures design, proving that is the essential consider the seismic effects

O enigmático problema das gigantes ricas em Lítio e as perspectivas com o satélite Kepler

Lithium (Li) is a chemical element with atomic number 3 and it is among the lightest known elements in the universe. In general, the Lithium is found in the nature under the form of two stable isotopes, the 6Li and 7Li. This last one is the most dominant and responds for about 93% of the Li found in the Universe. Due to its fragileness this element is largely used in the astrophysics, especially in what refers to the understanding of the physical process that has occurred since the Big Bang going through the evolution of the galaxies and stars. In the primordial nucleosynthesis in the Big Bang moment (BBN), the theoretical calculation forecasts a Li production along with all the light elements such as Deuterium and Beryllium. To the Li the BNB theory reviews a primordial abundance of Log log ǫ(Li) =2.72 dex in a logarithmic scale related to the H. The abundance of Li found on the poor metal stars, or pop II stars type, is called as being the abundance of Li primordial and is the measure as being log ǫ(Li) =2.27 dex. In the ISM (Interstellar medium), that reflects the current value, the abundance of Lithium is log ǫ(Li) = 3.2 dex. This value has great importance for our comprehension on the chemical evolution of the galaxy. The process responsible for the increasing of the primordial value present in the Li is not clearly understood until nowadays. In fact there is a real contribution of Li from the giant stars of little mass and this contribution needs to be well streamed if we want to understand our galaxy. The main objection in this logical sequence is the appearing of some giant stars with little mass of G and K spectral types which atmosphere is highly enriched with Li. Such elevated values are exactly the opposite of what could happen with the typical abundance of giant low mass stars, where convective envelops pass through a mass deepening in which all the Li should be diluted and present abundances around log ǫ(Li) ∼1.4 dex following the model of stellar evolution. In the Literature three suggestions are found that try to reconcile the values of the abundance of Li theoretical and observed in these rich in Li giants, but any of them bring conclusive answers. In the present work, we propose a qualitative study of the evolutionary state of the rich in Li stars in the literature along with the recent discovery of the first star rich in Li observed by the Kepler Satellite. The main objective of this work is to promote a solid discussion about the evolutionary state based on the characteristic obtained from the seismic analysis of the object observed by Kepler. We used evolutionary traces and simulation done with the population synthesis code TRILEGAL intending to evaluate as precisely as possible the evolutionary state of the internal structure of these groups of stars. The results indicate a very short characteristic time when compared to the evolutionary scale related to the enrichment of these stars

On soil-structurae interaction in large non-slender partially buried structures.

[EN]This paper addresses the seismic analysis of a deeply embedded non-slender structure hosting the pumping unit of a reservoir. The dynamic response in this type of problems is usually studied under the assumption of a perfectly rigid structure using a sub-structuring procedure (three-step solution) proposed specifically for this hypothesis.

Application of crescent shaped braces for reinforced concrete structures

The work done is about the seismic analysis of an existing reinforced concrete structure that is equipped with a special bracing device. The main objective of the research is to provide a simple procedure that can be followed in order to design the lateral bracing system in such a way that the actual behavior of the structure matches the desired pre-defined objective curve. a great attention is devoted to the internal actions in the structural elements produced by the braces. The device used is called: Crescent shaped braces. This device is a special type of bracing because it has a banana-like geometry that allows the designer to have more control over the stiffness of the structure, especially under cyclic behavior, Unlike the conventional bracing that resists only through its axial stiffness. This device has been installed in a hospital in Italy. However, it has not been exposed to any ground motion so far. Different analysis methods, such as static pushover and dynamic time-history have been used in the analysis of the structure.

Monitor sísmico interactivo

Este trabajo tiene como objetivos la monitorización en tiempo real de la actividad sísmica, tanto próxima como lejana, a partir de los datos sísmicos registrados por una estación de banda ancha, y el desarrollo de un sistema de difusión interactiva de información actualizada de terremotos, destinado al público general. Ambas fuentes de información se mostrarán a través de una Unidad de Visualización denominada “Monitor Sísmico Interactivo”. El registro de los datos sísmicos se realiza utilizando el sensor de tres componentes de la estación sísmica GUD, perteneciente a la Red Digital de Banda Ancha y transmisión digital del Instituto Geográfico Nacional, instalada en la Basílica del Valle de los Caídos, en lalocalidad de Guadarrama (Madrid). En la E.T.S.I. Topografía, Geodesia y Cartografía se ha instalado un ordenador con conexión a Internet, para la recepción y almacenamiento de los datos, y los programas Scream y Drumplot desarrollados por Guralp, necesarios para la monitorización de la señal sísmica en tiempo real. A partir de estos datos, mediante aplicaciones desarrolladas bajo programación Linux y haciendo uso de las herramientas que ofrece el software SAC (Seismic Analysis Code), se genera además un registro gráfico y una película animada de dicha segmentación para cada evento. Se ha configurado un servidor de correo y una cuenta para la recepción de dos tipos de mensajes de correo, enviados desde la sede central del Instituto Geográfico Nacional, con la información de los eventos registrados por GUD una vez revisados: - Mensajes enviados diariamente, con un listado de eventos ocurridos en los 30 últimos días. - Mensajes con la información en cuasi tiempo real de la última alerta sísmica. Se ha desarrollado el programa “saco” para la gestión del correo recibido que analiza la información sísmica, la almacena en ficheros y ejecuta sobre ellos las aplicaciones de dibujo. Estas aplicaciones han sido previamente desarrolladas bajo programación Linux y software GMT (Generic Mapping Tools), y a partir de ellas se generan automáticamente las distintas imágenes que se visualizan en el Monitor Sísmico: un mapa de sismicidad próxima en la Península Ibérica, un mapa de sismicidad lejana en el mundo, un mapa de detalle para localizar y representar la última alerta generada, los listados con la información de los eventos representados en los mapas, los registros gráficos y las películas animadas de dichos sismogramas. Monitor Sísmico Interactivo ha sido desarrollado para ofrecer además la posibilidad de interactuar con la Unidad de Visualización: se ha creado una base de datos para uso científico donde se almacenan todos los eventos registrados por GUD. Así el usuario puede realizar una petición, a través del envío de un mensaje de correo, que le permite visualizar de forma instantánea las imágenes que muestran la información de cualquier terremoto de su interés. ABSTRACT This study is aimed at real-time monitoring of both near and distant seismic activityfrom the seismic data recorded by a broadband seismic station, and the development of an interactive broadcast system of updated information of earthquakes, for the general public. Bothsources of information are displayed through a display unit called "Interactive Seismic Monitor". The seismic data recording is carried out by using the three-component sensor of the GUD seismic station, which belongs to the Digital Network Broadband and digital broadcast of the National Geographic Institute, housed in the Basilica of The Valley of the Fallen, in the town of Guadarrama (Madrid). A computer with Internet connection has been installed in E.T.S.I. Surveying, Geodesy and Cartography for receiving and storing data, together with Scream and Drumplot programs, developed by Guralp, which are necessary for monitoring the real time seismic signal. Based on the data collected, through programming applications developed under Linux system and using the software tools provided by the SAC (Seismic Analysis Code), a chart recorder and an animated gif image of the segmentation for each event are also generated. A mail server and a mail account have been configured for the receipt of two types of email messages, sent from the National Geographic Institute head office, with the information of the events recorded by GUD after being reviewed: - Messages sent daily, providing a list of events in the past 30 days. - Messages containing information on near real-time seismic of the last seismic alert. A program called "saco" has also been developed for handling mail received that analyzes the seismic data, which stores it in files and runs drawing applications on them. These applications have been previously developed under Linux system and software programming GMT (Generic Mapping Tools), and from them different images that are displayed on the Seismic Monitor are automatically generated: a near seismicity Iberian peninsula map, a distant seismicity world map, a detailed map to locate and represent the last seismic alert generated, the lists with the information of the events depicted in the maps,together with the charts and the animated gif image of such seismograms. Interactive Seismic Monitor has been developed to offer any user the possibility of interacting with the display unit: a database has been created for scientific use which stores all the events recorded by GUD. Thus, any user could make a request, by sending an e-mail that allows them to view instantly all the images showing the information of any earthquake of interest on the display unit.

On soil-structure interaction in large non-slender partially buried structures

This paper addresses the seismic analysis of a deeply embedded non-slender structure hosting the pumping unit of a reservoir. The dynamic response in this type of problems is usually studied under the assumption of a perfectly rigid structure using a sub-structuring procedure (three-step solution) proposed specifically for this hypothesis. Such an approach enables a relatively simple assessment of the importance of some key factors influencing the structural response. In this work, the problem is also solved in a single step using a direct approach in which the structure and surrounding soil are modelled as a coupled system with its actual geometry and flexibility. Results indicate that, quite surprisingly, there are significant differences among prediction using both methods. Furthermore, neglecting the flexibility of the structure leads to a significant underestimation of the spectral accelerations at certain points of the structure.

Estimación de la peligrosidad sísmica mediante protocolos de juicios de expertos

Este trabajo estudia la aportación que los métodos de agregación de juicios de expertos pueden realizar en el cálculo de la peligrosidad sísmica de emplazamientos. Se han realizado cálculos en dos emplazamientos de la Península Ibérica: Mugardos (La Coruña) y Cofrentes (Valencia) que están sometidos a regímenes tectónicos distintos y que, además, alojan instalaciones industriales de gran responsabilidad. Las zonas de estudio, de 320 Km de radio, son independientes. Se ha aplicado un planteamiento probabilista a la estimación de la tasa anual de superación de valores de la aceleración horizontal de pico y se ha utilizado el Método de Montecarlo para incorporar a los resultados la incertidumbre presente en los datos relativos a la definición de cada fuente sismogenética y de su sismicidad. Los cálculos se han operado mediante un programa de ordenador, desarrollado para este trabajo, que utiliza la metodología propuesta por el Senior Seismic Hazard Analysis Commitee (1997) para la NRC. La primera conclusión de los resultados ha sido que la Atenuación es la fuente principal de incertidumbre en las estimaciones de peligrosidad en ambos casos. Dada la dificultad de completar los datos históricos disponibles de esta variable se ha estudiado el comportamiento de cuatro métodos matemáticos de agregación de juicios de expertos a la hora de estimar una ley de atenuación en un emplazamiento. Los datos de partida se han obtenido del Catálogo de Isosistas del IGN. Los sismos utilizados como variables raíz se han elegido con el criterio de cubrir uniformemente la serie histórica disponible y los valores de magnitud observados. Se ha asignado un panel de expertos particular a cada uno de los dos emplazamientos y se han aplicado a sus juicios los métodos de Cooke, equipesos, Apostolakis_Mosleh y Morris. Sus propuestas se han comparado con los datos reales para juzgar su eficacia y su facilidad de operación. A partir de los resultados se ha concluido que el método de Cooke ha mostrado el comportamiento más eficiente y robusto para ambos emplazamientos. Este método, además, ha permitido identificar, razonadamente, a aquellos expertos que no deberían haberse introducido en un panel. The present work analyses the possible contribution of the mathematical methods of aggregation in the assessment of Seismic Hazzard. Two sites, in the Iberian Peninsula, have been considered: Mugardos ( La Coruña) and Cofrentes (Valencia).Both of them are subjected to different tectonic regimes an both accommodate high value industrial plants. Their areas of concern, with radius of 320 Km, are not overlapping. A probabilistic approach has been applied in the assessment the annual probability of exceedence of the horizontal peak acceleration. The Montecarlo Method has allowed to transfer the uncertainty in the models and parameters to the final results. A computer program has been developed for this purpose. The methodology proposed by the Senior Seismic Analysis Committee (1997) for the NRC has been considered. Attenuation in Ground motion has been proved to be the main source of uncertainty in seismic hazard for both sites. Taking into account the difficulties to complete existing historical data in this subject the performance of four mathematical methods of aggregation has been studied. Original data have been obtained from the catalogs of the Spanish National Institute of Geography. The seismic events considered were chosen to cover evenly the historical records and the observed values of magnitude. A panel of experts have been applied to each site and four aggregation methods have been developed : equal weights, Cooke, Apostolakis-Mosleh and Morris The four proposals have been compaired with the actual data to judge their performance and ease of application. The results have shown that the Method of Cooke have proved the most efficient and robust for both sites. This method, besides, allow the reasoned identification of those experts who should be rejected from the panel

Performance of buildings with masonry infill walls during the 2011 Lorca earthquake

On Wednesday 11th May 2011 at 6:47 pm (local time) a magnitude 5.1 Mw earthquake occurred 6 km northeast of Lorca with a depth of around 5 km. As a consequence of the shallow depth and the small epicentral distance, important damage was produced in several masonry constructions and even led to the collapse of one of them. Pieces of the facades of several buildings fell down onto the sidewalk, being one of the reasons for the killing of a total of 9 people. The objective of this paper is to describe and analyze the failure patterns observed in reinforced concrete frame buildings with masonry infill walls ranging from 3 to 8 floors in height. Structural as well as non-structural masonry walls suffered important damage that led to redistributions of forces causing in some cases the failure of columns. The importance of the interaction between the structural frames and the infill panels is analyzed by means of non-linear Finite Element Models. The resulting load levels are compared with the member capacities and the changes of the mechanical properties during the seismic event are described and discussed. In the light of the results obtained the observed failure patterns are explained. Some comments are stated concerning the adequacy of the numerical models that are usually used during the design phase for the seismic analysis.

Comportamento sotto sisma di strutture rigide o deformabili: due casi di studio estremi

In Italia molti edifici sono stati costruiti senza tenere in considerazione l'azione sismica. La necessità di adeguare tali edifici in accordo con la normativa italiana vigente è stato il motivo scatenante di questa ricerca. Per l'adeguamento sismico, vengono qui proposti differenti approcci in base al tipo di struttura e, in particolare, in base alla loro deformabilità. Per le strutture flessibili come le scaffalature di acciaio adibite alla stagionatura del Parmigiano Reggiano, sono stati utilizzati dispositivi passivi di dissipazione energetica. Sono state condotte analisi di sensitività per determinare il coefficiente di smorzamento in grado di minimizzare lo stato tensionale nelle sezioni di interesse. I risultati delle analisi mostrano l'efficacia delle soluzioni proposte e potrebbero rappresentare un punto di partenza per la definizione di possibili contromisure standar per l'adeguamento sismico. Per le strutture rigide, come i ponti in muratura, sono stati definiti alcuni criteri per la modellazione e la verifica delle sezioni di interesse, utilizzando modelli semplificati ma dall'efficacia comprovata come termine di paragone.

Semi-engineered earthquake-resistant structures: one-storey buildings built up with gabion-box walls

This thesis studies the static and seismic behavior of simple structures made with gabion box walls. The analysis was performed considering a one-story building with standard dimensions in plan (6m x 5m) and a lightweight timber roof. The main focus of the present investigation is to find the principals aspects of the seismic behavior of a one story building made with gabion box walls, in order to prevent a failure due to seismic actions and in this way help to reduce the seismic risk of developing countries where this natural disaster have a significant intensity. Regarding the gabion box wall, it has been performed some calculations and analysis in order to understand the static and dynamic behavior. From the static point of view, it has been performed a verification of the normal stress computing the normal stress that arrives at the base of the gabion wall and the corresponding capacity of the ground. Moreover, regarding the seismic analysis, it has been studied the in-plane and out-of-plane behavior. The most critical aspect was discovered to be the out-of-plane behavior, for which have been developed models considering the “rigid- no tension model” for masonry, finding a kinematically admissible multiplier that will create a collapse mechanism for the structure. Furthermore, it has been performed a FEM and DEM models to find the maximum displacement at the center of the wall, maximum tension stresses needed for calculating the steel connectors for joining consecutive gabions and the dimensions (length of the wall and distance between orthogonal walls or buttresses) of a geometrical configuration for the standard modulus of the structure, in order to ensure an adequate safety margin for earthquakes with a PGA around 0.4-0.5g. Using the results obtained before, it has been created some rules of thumb, that have to be satisfy in order to ensure a good behavior of these structure.