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Theory of Seismic Imaging

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Seismic imaging methods are currently used to produce images of the Earth's subsurface properties at diverse length scales, from high-resolution, near-surface environmental studies for oil and gas exploration to long-period images of the entire planet. This book presents the physical and mathematical basis of imaging algorithms in the context of controlled-source reflection seismology. The approach taken is motivated by physical optics and theoretical seismology. The theory is constantly put into practice via a graded sequence of computer exercises using the widely available SU (Seismic Unix) software package. The material covered in this book is more than enough for a one-semester graduate course in seismic imaging, by the end of which students will not only be writing their own migration codes, patterned on codes in the book, but will be well-prepared to read the current literature.
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... Amplitudes of reflected arrivals depend on the impedance contrast at the reflector, i.e. the product of seismic velocity and density (e.g. Tatham and McCormack, 1991;Sheriff and Geldart, 1995;Scales, 1997;Yilmaz, 2001). To answer the question why fault reflections are not recorded more often at the strong velocity and density contrast near the AF (sections 4.2.2, 4.2.3), ...
... only P wave propagation (e.g. Scales, 1997). Basically, all studied models consist of two quarterspaces in which velocities vary with depth only. ...
... Therefore, I derived a one-dimensional P velocity model and from that build a traveltime table for all possible offsets and depths in the target volume using a finite-difference (FD) scheme (van Trier and Symes, 1991). The FD scheme is based on the geometrical optics or WKBJ approximation 2 of wave propagation (Scales, 1997). The FD grid spacing is 10 m in horizontal and vertical direction, and traveltimes for distances between grid nodes are interpolated linearily. ...
Technical Report
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The Dead Sea Transform (DST) is a prominent shear zone in the Middle East. It separates the Arabian plate from the Sinai microplate and stretches from the Red Sea rift in the south via the Dead Sea to the Taurus-Zagros collision zone in the north. Formed in the Miocene »17 Ma ago and related to the breakup of the Afro-Arabian continent, the DST accommodates the left-lateral movement between the two plates. The study area is located in the Arava Valley between the Dead Sea and the Red Sea, centered across the Arava Fault (AF), which constitutes the major branch of the transform in this region. A set of seismic experiments comprising controlled sources, linear profiles across the fault, and specifically designed receiver arrays reveals the subsurface structure in the vicinity of the AF and of the fault zone itself down to about 3–4 km depth. A tomographically determined seismic P velocity model shows a pronounced velocity contrast near the fault with lower velocities on the western side than east of it. Additionally, S waves from local earthquakes provide an average P -to-S velocity ratio in the study area, and there are indications for a variations across the fault. High-resolution tomographic velocity sections and seismic reflection profiles confirm the surface trace of the AF, and observed features correlate well with fault-related geological observations. Coincident electrical resistivity sections from magnetotelluric measurements across the AF show a conductive layer west of the fault, resistive regions east of it, and a marked contrast near the trace of the AF, which seems to act as an impermeable barrier for fluid flow. The correlation of seismic velocities and electrical resistivities lead to a characterisation of subsurface lithologies from their physical properties. Whereas the western side of the fault is characterised by a layered structure, the eastern side is rather uniform. The vertical boundary between the western and the eastern units seems to be offset to the east of the AF surface trace. A modelling of fault-zone reflected waves indicates that the boundary between low and high velocities is possibly rather sharp but exhibits a rough surface on the length scale a few hundreds of metres. This gives rise to scattering of seismic waves at this boundary. The imaging (migration) method used is based on array beamforming and coherency analysis of P -to-P scattered seismic phases. Careful assessment of the resolution ensures reliable imaging results. The western low velocities correspond to the young sedimentary fill in the Arava Valley, and the high velocities in the east reflect mainly Precambrian igneous rocks. A 7 km long subvertical scattering zone (reflector) is offset about 1 km east of the AF surface trace and can be imaged from 1 km to about 4 km depth. The reflector marks the boundary between two lithological blocks juxtaposed most probably by displacement along the DST. This interpretation as a lithological boundary is supported by the combined seismic and magnetotelluric analysis. The boundary may be a strand of the AF, which is offset from the current, recently active surface trace. The total slip of the DST may be distributed spatially and in time over these two strands and possibly other faults in the area.
... The processing sequence performed in this study included four stages: 1) pre-stack time processing, 2) building an interval velocity model in depth, 3) pre-stack depth migration and 4) post-stack processing ( Fig. 2.3). Migration is a process that moves dipping events to their supposedly true subsurface location and collapses diffraction (Scales, 1995). It can be performed either on CMP gathers prior stacking (pre-stack time migration) or on stacked data (post-stack time migration). ...
... This occurs especially when there is a decrease in velocities with depth for example below a salt layer (such as the Messinian salt layer in the Mediterranean), as average velocities cannot account for such a velocity inversion, the use of interval velocities is essential in order to avoid inaccurate scaling of the time migrated section to depth. The depth migrated section can be considered as close representation of the structural cross-section of the subsurface only if the velocitydepth model is sufficiently accurate (Yilmaz, 2001;Scales, 1995). For example, part of the present research focuses on the Jonah high (Ch. ...
Thesis
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Recent giant gas discoveries within deeply buried structural highs in the middle of the Levant basin have attracted the attention of the industrial and academic communities striving to understand the origin of these structures, their relations with the tectonic history of the basin, and their evolution through time. The location of the Levant basin, at the conjunction of two plate boundaries separating the African Plate from Eurasia in the north and from Arabia in the east, further questions the relationship between the basin’s deformation and the regional plate tectonic processes. In particular, several fundamental questions are addressed here: what is the origin of the deeply buried structures in the basin? Are they related to the Early Mesozoic rifting or to the Late Mesozoic – Early Tertiary Africa-Eurasia convergent phase? How are the structures in the basin related to the closure of the Tethys Ocean, to the onshore Syrian Arc fold belt (~1000 km – long fold belt extending from northern Egypt through Israel to Syria), and the Dead Sea transform? How far west did the Syrian Arc deformation extend, and how it varies in the deep basin? How many deformation episodes occurred, how long was each episode active and are they related to onshore activity? In order to answer these questions a basin-wide seismic analysis of ~500 2D time-migrated seismic reflection lines with accumulated length of ~27,000 km was carried out. In addition, five regional lines were selected and reprocessed using the Pre-Stack Depth Migration procedure (PSDM) that yields a depth section, correct for geometric distortions, and improves the imaging of the deep part of the sections. Based on this huge database, horsts were distinguished from folds; geometric relations such as onlap over preexisting structure were identified; thickness variations related to syn-tectonic deposition were examined; and distinct episodes of folding activity were identified. This analysis leads to several new understanding of the basins structure and development that were further tested by gravity and magnetic modeling. In what follows the main findings of this study are described. Seismic interpretation conducted in this study encompasses the sedimentary section deposited since ~160 Ma, which approximately coincides with the post-rift stage of the basin. Structural maps reveal three regional basement block separated by two structural steps. The continental block is vertically separated from the continental margin block by the 1-2 km high coastal plain step. Farther west (~60 km), the continental margin block is separated from the deep basin block by > 2km high and ~10 km wide Continental Margin Fault Zone (CMFZ). Superimposed on the regional 3-block structure, the basin hosts a variety of shorter wave structures which are the focus of this study. Interpretation and mapping of 72 folds throughout the basin demonstrated that most of them are asymmetric elongated structures, varying in length from less than 1 km to ~50 km and trending to the NNE with an average azimuth of 360. Few of them are associated with deep reverse faults. Timing of folding activity was identified by examining the geometry of the reflectors approaching each fold and by analyzing thickness variation along them. Combining this analysis with a set of nine isopach maps enabled to determine the temporal and spatial evolution of the folds in the entire Levant basin. Results show that the main folding activity started during the Santonian mostly along the continental margin block and the CMFZ (more or less the nowadays continental shelf and slope), and also in the deep basin. Then, during the Late-Eocene and Oligocene, folding in the deep basin ceased, while intensive activity continued in the eastern part of the basin (continental margin block and CMFZ). Extensive folding in the deep basin renewed in the Early Miocene and continued during the Middle Miocene. Since the Late Miocene folding activity in the entire basin declined. In the Early Pliocene only few folds were active and only in the eastern part of the basin (the nowadays shelf area), and since the Late Pliocene no folding activity was detected anywhere in the basin Overall, the structural and the chronological similarity between offshore and onshore (Syrian Arc) folding reveals the existence of a wide deformation zone extending more than 100 km landwards of the present shoreline into Syria, Lebanon, Israel Sinai and western Egypt, and more than 200 km offshore towards the Eratosthenes seamount. This deformation zone started its activity in the Santonian (~85 Ma) and continued till the Early Pliocene (~4 Ma). In a larger scale deformation in the Levant area lines up with a series of compressional structures observed from Morocco to Syria along the northern margins of the African plate. Hence it is suggested here that the north-east African plate margin which shaped during Early Mesozoic rifting, played an essential boundary condition for the following tectonic evolution. The subsequent Late Mesozoic – Cenozoic compression zone therefore reflect the scissor like closure of the Tethys Ocean, when Africa-Arabia had experienced a counterclockwise rotational northward drift and the thin weak crust of the plate margins deformed accordingly. The interplay of plate kinematics and pre-existing continental weakness zones dictated the deformation orientation in the Levant basin for more than 80 m.y. Cessation of folding activity in the western part of the basin during Late Eocene – Oligocene is interpreted in this study as a result of the intensive shearing and folding along the CMFZ, which absorbed much of the deformation at that time and “protected” the NW part of the basin. Similarly, declining of folding in the entire basin since the Late Miocene and its final cessation in the Late Pliocene is interpreted as a result of the formation of new plate boundaries near Cyprus and along the Dead Sea Transform, which absorbed much of the deformation. In addition to the many folds described above, two major high structures were examined, Leviathan and Jonah. The Leviathan high, while seems to be at least partially congruent with the folding activity described above, differ in its dimensions and structure from the majority of the folds in the basin. It portrays a triangular wide shape in contrast to the elongated monocline or anticlines typical to Syrian Arc structures. The analysis presented here agrees with previous studies suggesting that it might be an early Mesozoic large horst, that was reactivated during the contractional phase of the basin and distinct monoclines were formed at its boundaries. However, unlike the Leviathan high, this study suggests that the Jonah high is an ancient horst that was not reactivated. The Jonah high is particularly enigmatic as it is associated with one of the largest magnetic anomalies in the basin, though no significant gravity anomaly is observed. Previous studies raised several possibilities explaining its origin: an ancient horst related to the early stage of basin formation (Late Paleozoic or early Mesozoic); a Syrian Arc fold (Late Cretaceous to Neogene); a giant volcanic seamount; and an intrusive magmatic body. This study suggests that the Jonah high is a horst bounded by grabens, most probably formed during continental breakup related to the Neo-Tethys formation. However, unlike other extensional structures that were reactivated and inverted during the Syrian Arc deformation, the Jonah high was never reactivated. Rather, it formed a prominent seamount that persisted for 120-140 million years until the Early Miocene, when it was finally buried. This conclusion was further examined by gravity and magnetic modeling showing that a basement high (horst) can explain the observations without the need to add magmatic intrusions or extrusions.
... Another principle goal of migration is to map the apparent dip that is seen on the zero-offset sections into true dip [2,26,31,33]. True dip angle is always greater than apparent dip angle. Consider a reflector dipping at an angle of θ in the true earth as in Figure 8.5. ...
... ) is known the wave emitted from each point of the source can be calculated, as follows [19]: ...
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