Texte remanié de: Diss.--Recht--München--Juristischen Fakultät der Universität München, 1969. / Bibliogr. p. 186-198. Notes bibliogr.

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In this thesis, a support vector machine (SVM) is used to develop a model to predict Arias Intensity. Arias Intensity is a measure of the strength of ground motions that considers both the amplitude and the duration of ground motions. In this research, a subset of the database from the “Next Generation and the duration of Ground-Motion Attenuation Models” project was used as the training data. The data includes 3525 ground motion records from 175 earthquakes. This research provides the assessment of historical earthquakes using arias intensity data. Support vector machine uses a Kernel function to transform the data into a high dimensional space where relationships between the variables can be efficiently described using simpler models. In this research, after testing several kernel functions, a Gaussian Kernel was selected for the predictive model. The resulting model uses magnitude, epicentral distance, and the shear wave velocity as the predictor of Arias Intensity.

In the last two decades, two major earthquakes have occurred in Japan: the 1995 Kobe earthquake and the 2011 Great East Japan earthquake. In the 2011 Great East Japan earthquake, many bridge structures were destroyed by the tsunamis, but it is interesting to study the ground motion induced damage and also how this earthquake differed from the one in 1995. In this thesis, the seismic response of a bridge designed according to the current Japanese Design Specifications was evaluated when it is subjected to near-field ground motions recorded during the 1995 Kobe earthquake and far-field ground motions recorded during the 2011 Great East Japan earthquake. For this purpose, a series of nonlinear dynamic response analysis was conducted and the seismic performance of the bridge was verified in terms of its displacement and ductility demand. It was found from the dynamic response analysis that the seismic response of the target bridge when subjected to the ground motions from the 2011 Great East Japan earthquake was smaller than during the 1995 Kobe earthquake. Although the ground motions from the 2011 Great East Japan earthquake were very strong, they were not as strong as the ground motions from the 1995 Kobe earthquake. The results obtained in this thesis clarify the validity of the Type I and Type II design ground motions. The target bridge used in this thesis was designed according to the post-1990 design specifications and showed limited nonlinear response when subjected to the different ground motions which shows how efficient the enhancement of the seismic performance of bridges has been since the 1990’s.

Joel Mondo Kisekini, for the Master of Science degree in Civil Engineering, presented on March 25, 2022, at Southern Illinois University Carbondale.TITLE: EFFECT OF SIMULTANEOUS APPLICATION OF THE TWO HORIZONTAL ORTHOGONAL GROUND MOTION COMPONENTS ON THE SEISMIC BEHAVIOR OF BUILDINGSMAJOR PROFESSOR: Dr. JALE TEZCAN During an earthquake, buildings are simultaneously excited by two horizontal and one vertical ground motion components. Modern seismic codes and guidelines such as ASCE/SEI 41-06 (Seismic rehabilitation of existing buildings, American Society of Civil Engineers), EUROCODE 8 (1998-1) (Design provisions for earthquake resistance of structures, European Committee for Standardization, 2003), FEMA 356 (Prestandard and Commentary for Seismic Rehabilitation of the Buildings) and FEMA P-2082 (NEHRP Recommended Seismic Provisions for new buildings and other structures) require the consideration of the effects of two horizontal orthogonal ground motions in seismic design of buildings. Therefore, the main objective of this study is to evaluate the simultaneous effect of two horizontal orthogonal ground motion components to seismic behavior of buildings. A four-story steel frame is modeled, and it is subjected to a set of twenty ground motion pairs recorded distances between x and y kilometer from epicenter. Three methods for combining peak response to individual component of ground motions is used to estimate the displacement responses. The combination rules used in this present study are 30%, SRSS, and 20%. The response of the four-story steel frame is investigated within the context of linear response history analysis and the results are compared to the peak responses obtained from time history analyses under bidirectional and unidirectional ground motion. The structural response includes the following parameters: nodal displacements and the critical angle of excitation. The output results showed that the maximum response under two components was, on average, 23 % more than the maximum response under a single component, and the two horizontal orthogonal seismic excitations increased the structure displacement response compared to unidirectional excitation.

We present a multi-epoch Hubble Space Telescope (HST) study of stellar proper motions (PMs) for four fields along the Orphan Stream. We determine absolute PMs of several individual stars per target field using established techniques that utilize distant background galaxies to define a stationary reference frame. Five Orphan Stream stars are identified in one of the four fields based on combined color-magnitude and PM information. The average PM is consistent with the existing model of the Orphan Stream by Newberg et al. In addition to the Orphan Stream stars, we detect stars that likely belong to other stellar streams. To identify which stellar streams these stars belong to, we examine the 2d bulk motion of each group of stars on the sky by subtracting the PM contribution of the solar motion (which is a function of position on the sky and distance) from the observed PMs, and comparing the vector of net motion with the spatial extent of known stellar streams. By doing this, we identify candidate stars in the Sagittarius and Lethe streams, and a newly found stellar stream at a distance of similar to 17 kpc, which we tentatively name the "Parallel Stream." Together with our Sagittarius stream study, this work demonstrates that even in the Gaia era, HST will continue to be advantageous in measuring PMs of old stellar populations on a star-by-star basis, especially for distances beyond similar to 10 kpc.

This dissertation examines the pricing of the same credit risk in two currencies, and hence the valuation of credit-contingent foreign exchange products. Such pricing hinges upon the dependence of the credit risk and the foreign exchange rate. We recall the reduced-form model proposed by Ehlers (2007), which allows credit-currency dependence through correlation between the Brownian motions driving the default intensity and the exchange rate, and through a jump in the exchange rate at the default time. Four basic specifications of this model are considered. Two of these specifications have not previously appeared in the literature and one of these, based on a lognormal process for the default intensity, proves to be especially useful and tractable. The problem of hedging defaultable claims in one currency with similar claims in another is briefly considered, and it is shown that hedging against the default event and against credit spread movements are not in general equivalent.

Estudamos um caso especial do problema restrito dos três corpos, chamado problema circular de Sitnikov, quando dois corpos de massas iguais (chamadas de primárias) estão em uma órbita circular (configuração central de dois corpos), enquanto que um terceiro corpo de massa negligenciada (chamada infinitesimal) oscila sobre uma reta perpendicular ao plano das primárias (chamaremos esse movimento de vertical periódico). Aqui analisamos a estabilidade desse movimento periódico, com relação a pequenas perturbações nas direções ortogonais a reta onde ocorre o movimento. Chamaremos a atenção ao fenômeno de alternância entre estabilidade e instabilidade na família do movimento periódico vertical, conforme variamos a amplitude do movimento. / We studied a special case of the restricted three-body problem, named circular problem of Sitnikov, when two body of equal mass (called primaries) moving around each other on circular motion (central configuration of two body), while the third body of negligible mass (called infinitesimal) performs along a straight line orthogonal to the plane of the primaries (so called periodic vertical motions). We analyze the stability of the periodic vertical motions with respect to small perturbations orthogonal to the straight line where the motions occurs. We call attention to the phenomenom of alternation of stability and instability within the family of periodic vertical motions, whenever their amplitude is varied in a continuous manner.

Understand the behavior of queueing networks in heavy tra c is very important due to its importance in evaluating the network performance in related applications. However, in many cases, the stationary distributions of such networks are intractable. Based on di usion limits of queueing networks, we can use Re ected Brownian Motion (RBM) processes as reasonable approximations. As such, we are interested in obtaining the stationary distribution of RBM. Unfortunately, these distributions are also in most cases intractable. However, the tail behavior (large deviations) of RBM may give insight into the stationary distribution. Assuming that a large deviations principle holds, we need only solve the corresponding variational problem to obtain the rate function. Our research is mainly focused on how to solve variational problems in the case of rotationally symmetric (RS) data. The contribution of this dissertation primarily consists of three parts. In the rst part we give out the speci c stability condition for the RBM in the octant in the RS vi case. Although the general stability conditions for RBM in the octant has been derived previously, we simplify these conditions for the case we consider. In the second part we prove that there are only two types of possible solutions for the variational problem. In the last part, we provide a simple computational method. Also we give an example under which a spiral path is the optimal solution. / text

Estudamos um caso especial do problema restrito dos três corpos, chamado problema circular de Sitnikov, quando dois corpos de massas iguais (chamadas de primárias) estão em uma órbita circular (configuração central de dois corpos), enquanto que um terceiro corpo de massa negligenciada (chamada infinitesimal) oscila sobre uma reta perpendicular ao plano das primárias (chamaremos esse movimento de vertical periódico). Aqui analisamos a estabilidade desse movimento periódico, com relação a pequenas perturbações nas direções ortogonais a reta onde ocorre o movimento. Chamaremos a atenção ao fenômeno de alternância entre estabilidade e instabilidade na família do movimento periódico vertical, conforme variamos a amplitude do movimento. / We studied a special case of the restricted three-body problem, named circular problem of Sitnikov, when two body of equal mass (called primaries) moving around each other on circular motion (central configuration of two body), while the third body of negligible mass (called infinitesimal) performs along a straight line orthogonal to the plane of the primaries (so called periodic vertical motions). We analyze the stability of the periodic vertical motions with respect to small perturbations orthogonal to the straight line where the motions occurs. We call attention to the phenomenom of alternation of stability and instability within the family of periodic vertical motions, whenever their amplitude is varied in a continuous manner.