This dissertation presents a study on velocity modeling using ocean-bottom seismometer data (OBS) collected in 2004 and 2006 on the western Scotian slope. Gas hydrate and free gas concentrations and their distribution along the Scotian margin were derived based on the velocity results modeled with two different OBS data sets. A strong velocity increase (140-300 m/s) associated with gas hydrate was modeled for a depth of 220 m below seafloor (bsf). At the base of that high velocity zone (330 mbsf) the velocity decreases with 50-130 m/s. This depth is associated with the depth of the bottom-simulating reflector (BSR) observed in previous 2-D seismic reflection data. The gas hydrate concentrations (2-18 %) based on these velocities were calculated with an effective medium model. The velocity modeling shows that a sparser OBS spacing (~ 1 km) reveals more velocity uncertainties and smaller velocity contrasts than a denser (100 m) spaced OBS array. The results of the travel-time inverse modeling are applied in a waveform inverse modeling with OBS data in the second part of the thesis. The modeling tests were performed to obtain information on OBS instrument spacings necessary to detect low-concentration gas hydrate occurrences. The model runs show that an increase in instrument spacing leads to an increasing loss of model smoothness. However, large instrument spacings (>500 m) are beneficial for covering a wide target region with only using a few instruments, but decreasing the lateral resolution limits of the subsurface targets. In general half of the instrument spacing defines the lower boundary for the lateral width of the target structure. Waveform modeling with the 2006 OBS data has shown that low frequencies (<8 Hz) in the source spectrum are necessary to recover the background velocity of the model. The starting model derived from travel-time inversion of the 2006 data is not close enough to the true model. Thus the first-arrival waveforms do not match within half a cycle. Modeling with a starting frequency of 8 Hz and and applying data with a low signal-to-noise ratio (1.25) introduces artifacts into the final model result without updating the velocity. / Graduate

The Gulf of Mexico Basin Opening project (GUMBO) is a study of the lithological composition and structural evolution of the Gulf of Mexico (GoM) that uses Ocean Bottom Seismometer (OBS) data from four transects in the Northern GoM. I examine 39 OBS shot records in the easternmost transect for shear wave arrivals and pick shear wave travel times from the 11 usable records. I then carry out a tomographic inversion of seismic refraction travel times. I use the resulting shear-wave velocity model in conjunction with a previously constructed P-wave model to examine the relationship between Vp and Vs. I compare velocities in the sediment and basement with empirical velocities from previous studies for the purpose of constraining lithological composition below the transect and make an interpretation of the structural evolution of the eastern GoM. The seismic velocities for crust landward of the Florida Escarpment are consistent with normal continental crust. Seaward of the Escarpment, velocities in the upper oceanic crust are anomalously high (Vp = 6.5 – 7 km/sec; Vs = 4.0 – 4.6 km/sec). A possible explanation for this observation is that GoM basalt formation consisted of basaltic sheet flows, forming oceanic crust that does not contain the vesicularity and lower seismic velocities found in typical pillow basalts. Increased magnesium and iron content could also account for these high velocities. Seismic refraction and reflection data provide a means of investigating the nature of the Moho in the northeastern GoM. I use a finite difference method to generate synthetic record sections for data from eight instruments that are part of the two easternmost GUMBO seismic lines (lines 3 & 4). I then vary the thickness of the Moho in these synthetic models and compare the results with the original receiver gather to examine the effects this variability has on amplitudes. The data from the instruments chosen for these two lines are representative of continental and transitional crust. The finite difference models indicate that the Moho beneath GUMBO 3 is ~1500 m thick based on the onset and amplitudes of PmP arrivals. All five instruments display consistent results. The instruments along GUMBO 4 suggest a Moho almost twice as thick as GUMBO 3 on the landward end of the transect that grades into a Moho of similar thickness (1750 m) in the deep water GoM. The three instruments used to model the Moho in this area show that the Moho ranges from ~1750 to 3500 m in thickness. The sharper boundary beneath continental crust in GUMBO Line 3 supports other evidence that suggests magmatic underplating and volcanism in the northern GoM during the mid-Jurassic. The thicker Moho seen on the landward end of GUMBO Line 4 that is overlain by continental crust was likely unaffected by GoM rifting. Therefore, the Moho beneath the Florida Platform might be as old as the Suwannee Terrane, and complex Moho structure is not uncommon for ancient continental crust. / text

Overpressure, or abnormally low effective pressures, is hazardous in drilling operations and construction of sea-bottom facilities in deepwater environments. Estimation of the locations of overpressure can improve safety in these operations and significantly reduce overall project costs. Propagation velocities of both seismic P and S wave are sensitive to bulk elastic parameters and density of the sediments, which can be related to porosity, pore fluid content, lithology, and effective pressures. Overpressured areas can be analyzed using 4C seismic reflection data, which includes P-P and P-SV reflections. In this thesis, the effects on compressional (P) and shear (S) wave velocities are investigated to estimate the magnitude and location of excess pore pressure utilizing Eaton’s approach for pressure prediction (Eaton, 1969). Eaton’s (1969) method relates changes in pore pressure to changes in seismic P-wave velocity. The underlying assumption of this method utilizes the ratio of observed P-wave velocity obtained from areas of both normal and abnormal pressure. This velocity ratio evaluated through an empirically determined exponent is then related to the ratio of effective stress under normal and abnormal pressure conditions. Effective stress in a normal pressured condition is greater than the effective stress value in abnormally overpressured conditions. Due to an increased sensitivity of variations in effective pressure to seismic interval velocity, Ebrom et al. (2003) employ a modified Eaton equation to incorporate the S-wave velocity in pore pressure prediction. The data preparation and subsequent observations of seismic P and S wave velocity estimates in this thesis represent a preliminary analysis for pore pressure prediction. Six 2D receiver gathers in the regional dip direction are extracted from six individual ocean-bottom 4C seismic recording nodes for P-P and P-SV velocity analysis. The receiver gathers employed have minimal pre-processing procedures applied. The main processing steps applied were: water bottom mute, 2D rotation of horizontal components to SV and SH orientation, deconvolution, and frequency filtering. Most the processing was performed in Matlab with a volume of scripts designed by research scientists from the University of Texas, Bureau of Economic Geology. In this thesis, fluid pressure prediction is estimated utilizing several 4C multicomponent ocean-bottom nodes in the Atlantis Field in deepwater Gulf of Mexico. Velocity analysis is performed through a ray tracing approach utilizing P-P and P-SV registration. A modified Eaton’s Algorithm is then used for pore pressure prediction using both P and S wave velocity values. I was able to successfully observe both compressional and shear wave velocities to sediment depths of approximately 800 m below the seafloor. Using Hamilton (1972, 1976) and Eberhart-Phillips et al. (1989) regressions as background depth dependent velocity values and well-log derived background effective pressure values from deepwater Gulf of Mexico, I am able to solve for predicted effective pressure for the study area. The results show that the Atlantis subsurface study area experiences a degree of overpressure. / text

L'estiu de 2005, es varen instal·lar un sismòmetre de fons marí (OBS, sigles en anglès d'Ocean Bottom Seimometer) permanent, de tres components i banda ampla, i un sensor diferencial de pressió, a les immediacions de la plataforma petrolífera Casablanca (Repsol Investigaciones Petrolíferas S.A.), a uns 150 m de fondària i 50 km de la costa de Tarragona. Aquesta iniciativa, pionera a l'Estat espanyol, es va portar a terme en el marc del projecte Casablanca (REN2003-06577), concedit pel Ministerio de Educación y Ciencia a l'Institut Geològic de Catalunya (IGC) i l'Observatori de l'Ebre, amb l'objectiu de caracteritzar la detectabilitat de l'OBS i millorar el coneixement de la sismicitat i el risc sísmic a la zona. L'any 2007, després d'una reinstal·lació dels sensors en què es varen introduir millores, la transmissió satèl·lit en temps real del senyal al centre de recepció de dades sísmiques a l'IGC de Barcelona va possibilitar la integració de l'OBS a la xarxa sísmica de Catalunya.L'anàlisi de soroll sísmic ambiental a l'emplaçament de l'OBS Casablanca mostra nivells alts als tres components, especialment a baixes freqüències i a la banda microsísmica. Així mateix, s'observen variacions estacionals i la influència de les condicions meteorològiques i oceanogràfiques. La comparació dels nivells de soroll a l'OBS Casablanca amb el d'un altre OBS situat a la mar de Ligúria, amb una instrumentació semblant, però instal·lat a una fondària de 2500 m, mostra un comportament més sorollós a Casablanca, probablement a causa de la menor profunditat a què està situat.Tot i el seu comportament sorollós, l'OBS Casablanca ha enregistrat diversos sismes locals, regionals i telesismes. Malgrat la petita magnitud i l'escassesa de terratrèmols locals succeïts durant el període de funcionament de l'OBS, l'estació ha mostrat la seva utilitat de cara a la millora de les localitzacions hipocentrals dels sismes propers amb epicentre a la mar. Noves dades permetran la validació d'aquest resultat.El senyal de l'OBS Casablanca, juntament amb el d'estacions situades a la Península Ibèrica, el nord d'Àfrica i les Illes Balears, s'ha pogut utilitzar amb èxit en un estudi de tomografia d'ones superficials amb soroll sísmic ambiental realitzat al NE de la Península. El procediment de l'estudi tomogràfic ha inclòs un tractament del senyal a fi de minimitzar l'energia aportada pels terratrèmols i normalitzar les amplituds a totes les freqüències. Mitjançant el càlcul de la correlació creuada per a tots els parells d'estacions disponibles durant un període de més d'un any, s'ha trobat un senyal equivalent a la funció de Green del medi, que ha possibilitat la mesura de la velocitat de grup i de fase. La representació dels resultats en forma de mapes de dispersió mostra zones d'altes i baixes velocitats, coherents amb les principals estructures geològiques de l'escorça i part del mantell superior. / Durante el verano de 2005, se instalaron un sismómetro de fondo marino (OBS, siglas en inglés de Ocean Bottom Seismometer) permanente, de tres componentes y banda ancha, y un sensor diferencial de presión, en las inmediaciones de la plataforma petrolífera Casablanca (Repsol Investigaciones Petrolíferas S.A.), a unos 150 m de profundidad y 50 km de la costa de Tarragona. Esta iniciativa, pionera en España, se llevó a cabo en el marco del proyecto Casablanca (REN2003-06577), concedido por el Ministerio de Educación y Ciencia al Institut Geològic de Catalunya (IGC) y al Observatori de l'Ebre, con el objetivo de caracterizar la detectabilidad del OBS y mejorar el conocimiento de la sismicidad y el riesgo sísmico en la zona. En el año 2007, después de una reinstalación en la que se introdujeron mejoras, la transmisión satélite en tiempo real de la señal al centro de recepción de datos sísmicos del IGC en Barcelona posibilitó la integración del OBS a la red sísmica de Cataluña.El análisis del ruido sísmico ambiental en el emplazamiento del OBS Casablanca muestra niveles altos en las tres componentes, especialmente a bajas frecuencias y en la banda microsísmica. También se observan variaciones estacionales y la influencia de las condiciones meteorológicas y oceanográficas. La comparación de los niveles de ruido en el OBS Casablanca con los de otro OBS situado en el mar de Liguria, de instrumentación similar, pero instalado a 2500 m de profundidad, muestra un comportamiento más ruidoso en Casablanca, probablemente a causa de la menor profundidad a la que está situado.Aunque de comportamiento ruidoso, el OBS Casablanca ha registrado numerosos seísmos locales, regionales y teleseísmos. A pesar de la pequeña magnitud y la escasez de terremotos locales durante el periodo de funcionamiento del OBS, la estación ha mostrado su utilidad de cara a la mejora de las localizaciones hipocentrales de los seísmos cercanos con epicentro en el mar. Nuevos datos permitirán la validación de este resultado.La señal del OBS Casablanca, junto con la de estaciones situadas en la Península Ibérica, el norte de África y las Islas Baleares, se ha podido utilizar con éxito en un estudio de tomografía de ondas superficiales con ruido sísmico ambiental realizado al NE de la Península. El procedimiento del estudio tomográfico ha incluido el tratamiento de la señal para minimizar la energía aportada por los terremotos y normalizar las amplitudes para todas las frecuencias. Mediante el cálculo de la correlación cruzada para todos los pares de estaciones disponibles durante un periodo de más de un año, se ha obtenido una señal equivalente a la función de Green del medio, que ha posibilitado la medida de la velocidad de grupo y de fase. La representación de los resultados en forma de mapas de dispersión muestra zonas de altas y bajas velocidades, coherentes con las principales estructuras geológicas de la corteza y parte del manto superior. / During the summer of 2005, a three-component broad-band permanent ocean bottom seismometer (OBS) and a differential pressure gauge were deployed near the Casablanca oil platform (Repsol Investigaciones Petrolíferas S.A.) at a depth of about 150 m and 50 km away from the Tarragona coast (NE Iberian Peninsula). This initiative, pioneer in Spain, was carried out within the framework of the Casablanca project (RES2003-06577), given by the Ministerio de Educación y Ciencia to the Institut Geològic de Catalunya (IGC) and to the Observatori de l'Ebre. The aim of this project was to characterize the OBS detection threshold and to improve the knowledge of the seismicity and seismic risk in the area around. In 2007 satellite transmission was implemented to have continuous and real time data, which allowed integrating the OBS into the Catalan Seismic Network.A seismic ambient noise analysis at the Casablanca OBS site shows high levels on the three components, especially at low frequencies and at the microseismic band. Seasonal variations and the meteorological and oceanographic conditions influence are also observed. The comparison between Casablanca OBS noise levels and those from another OBS placed at the Ligurian Sea, equipped with similar instrumentation but installed at a depth of 2500 m, shows that the Casablanca site is noisier, probably due to its shallower deployment.Despite its noisy behaviour, the Casablanca OBS has recorded a number of local and regional earthquakes and teleseisms. Only few close small events have occurred during the OBS running period. Nevertheless, the station has shown its utility to improve hipocentral locations of close earthquakes with the epicentre offshore.The Casablanca OBS signal, together with that from stations placed at the Iberian Peninsula, northern Africa and Balearic Islands, has been successfully used in a surface wave tomographic study from ambient noise in the NE Iberian Peninsula. The tomographic study includes a signal processing to minimize the energy from earthquakes and to normalize the amplitudes for all frequencies. A signal equivalent to the Green function has been obtained through the cross-correlation between all the possible station pairs during a period longer than one year, allowing the measurement of group and phase velocities. The results, which are presented as dispersion maps, show areas of high and low velocities that are coherent with the main crust and upper mantle geological structures.

Seafloor compliance is a non-intrusive geophysical method sensitive to the shear modulus of the sediments below the seafloor. A compliance analysis requires the computation of the frequency dependent transfer function between the vertical stress, produced at the seafloor by the ultra low frequency passive source-infra-gravity waves, and the resulting displacement, related to velocity through the frequency. The displacement of the ocean floor is dependent on the elastic structure of the sediments and the compliance function is tuned to different depths, i.e., a change in the elastic parameters at a given depth is sensed by the compliance function at a particular frequency. In a gas hydrate system, the magnitude of the stiffness is a measure of the quantity of gas hydrates present. Gas hydrates contain immense stores of greenhouse gases making them relevant to climate change science, and represent an important potential alternative source of energy. Bullseye Vent is a gas hydrate system located in an area that has been intensively studied for over 2 decades and research results suggest that this system is evolving over time. A partnership with NEPTUNE Canada allowed for the investigation of this possible evolution. This thesis describes a compliance experiment configured for NEPTUNE Canada’s seafloor observatory and its failure. It also describes the use of 203 days of simultaneously logged pressure and velocity time-series data, measured by a Scripps differential pressure gauge, and a Güralp CMG-1T broadband seismometer on NEPTUNE Canada’s seismic station, respectively, to evaluate variations in sediment stiffness near Bullseye. The evaluation resulted in a (- 4.49 x10-3± 3.52 x 10-3) % change of the transfer function of 3rd October, 2010 and represents a 2.88% decrease in the stiffness of the sediments over the period. This thesis also outlines a new algorithm for calculating the static compliance of isotropic layered sediments.

Seafloor compliance is a non-intrusive geophysical method sensitive to the shear modulus of the sediments below the seafloor. A compliance analysis requires the computation of the frequency dependent transfer function between the vertical stress, produced at the seafloor by the ultra low frequency passive source-infra-gravity waves, and the resulting displacement, related to velocity through the frequency. The displacement of the ocean floor is dependent on the elastic structure of the sediments and the compliance function is tuned to different depths, i.e., a change in the elastic parameters at a given depth is sensed by the compliance function at a particular frequency. In a gas hydrate system, the magnitude of the stiffness is a measure of the quantity of gas hydrates present. Gas hydrates contain immense stores of greenhouse gases making them relevant to climate change science, and represent an important potential alternative source of energy. Bullseye Vent is a gas hydrate system located in an area that has been intensively studied for over 2 decades and research results suggest that this system is evolving over time. A partnership with NEPTUNE Canada allowed for the investigation of this possible evolution. This thesis describes a compliance experiment configured for NEPTUNE Canada’s seafloor observatory and its failure. It also describes the use of 203 days of simultaneously logged pressure and velocity time-series data, measured by a Scripps differential pressure gauge, and a Güralp CMG-1T broadband seismometer on NEPTUNE Canada’s seismic station, respectively, to evaluate variations in sediment stiffness near Bullseye. The evaluation resulted in a (- 4.49 x10-3± 3.52 x 10-3) % change of the transfer function of 3rd October, 2010 and represents a 2.88% decrease in the stiffness of the sediments over the period. This thesis also outlines a new algorithm for calculating the static compliance of isotropic layered sediments.