Identification and Exploitation of a High-Producing Field Extension With Integrated Reservoir Analysis

2000 ◽  
Vol 3 (03) ◽  
pp. 272-279 ◽  
Author(s):  
M.W. Waite ◽  
J.R. Weston ◽  
D.W. Davis ◽  
C.J. Pearn

Summary The Wafra field is located in the partitioned neutral zone between Kuwait and Saudi Arabia. The field produces oil from the Ratawi oolite reservoir, which has been under production since 1956. Barriers to fluid movement have severely restricted aquifer support to the overlying carbonate grainstone reservoir, leading to production-induced pressure depletion and low recovery rates. Creative integration of three-dimensional seismic aspects, well log stratigraphy, and engineering analysis revealed an unexploited reservoir extension that is more open to aquifer pressure support. Wells drilled along this extension are expected to yield higher initial production rates and longer sustained production. The model was used to drill two successful step-out wells that have increased field production by over 12,000 BOPD. Eight of ten additional wells have now been drilled as a follow-up to this success. This paper reviews the case history with a focus on the multidisciplinary integration that led to opportunity identification and exploitation. Introduction The Wafra field, jointly operated by Saudi Arabian Texaco and the Kuwait Oil Company, is located in the partitioned neutral zone (PNZ) between Kuwait and Saudi Arabia (Fig. 1). The field has produced from the Lower Cretaceous Ratawi reservoir since 1956. Liquid withdrawal over the years has depleted reservoir pressures in some parts of the field, leading to a decline in production. Based on prior reservoir characterization and simulation studies in 1995,1 a peripheral water injection and an extension development program have been undertaken in order to arrest the decline and increase the production by over 40,000 BOPD.2 In 1996, a 104 sq mile three-dimensional (3D) seismic survey was acquired to help design and implement these programs. Structural and Stratigraphic Framework The Wafra field is a large anticline approximately 6 by 10 miles in dimension (Fig. 2). The field is composed of a main NW-SE trending structural feature called the Main area, and a lower amplitude extension area east of the Main area called East Wafra. The Ratawi oolite reservoir is found at a depth of 6,135 ft subsea at the structural crest and had an original oil-water contact at about 6,520 ft subsea. Most of the structuring occurred in Middle Cretaceous time as sediment draped over deep-seated horst blocks. Oil migration and accumulation are thought to have occurred primarily in Early Eocene time. The Ratawi formation consists of a marine transgressive sequence of carbonate rocks deposited during Early Cretaceous time. The formation is composed of three distinct intervals: the lower-most Ratawi oolite reservoir, and the overlying Ratawi Limestone and Ratawi Shale cap rocks (Fig. 3). The Ratawi oolite reservoir was formed by a prograding carbonate sand shoaling sequence deposited on a low-angle carbonate ramp or detached platform. The commercially productive reservoir interval is composed primarily of porous grainstones and packstones. Less porous packstone, mudstone, and wackestone facies resulted from a more-restricted lagoonal environment in the central part of the field, and deeper marine shelf facies on the platform boundaries. Stratigraphic analysis of well log data provides an understanding of the depositional framework and serves as a basis for modeling facies distribution within the reservoir. Fig. 4a is a well log cross section traversing the Main area and East Wafra along the path A-B in Fig. 2. The gamma ray (GR) log curves are flattened on the base of the Ratawi limestone (cap rock) and span the interval of the Ratawi oolite reservoir. The GR curves indicate a remarkable character similarity from well to well that is almost exclusively related to the presence of uranium minerals.1 This determination is supported by x-ray analysis of core data that found an absence of clay. Additional evidence is found in comparisons of the GR (uranium, potassium and thorium) with the computed GR (potassium and thorium) from spectrometry gamma ray logs. The computed GR data show a largely diminished log character, implying that the GR log character is largely a function of uranium content. Hence, the correlative nature of the GR curves indicates that the uranium was present at the time of deposition—probably due to regional-scale climatic or environmental influences such as atmospheric fall-out from volcanic activity. This explains the consistent levels of uranium, independent of lithology and porosity, and allows detailed chronostratigraphic correlations to be made. Fig. 4b is an east-west stratigraphic cross section through the reservoir along the same path as in Fig. 4a, showing porosity logs with GR depositional time lines superimposed. The thick solid lines mark lithostratigraphic boundaries between an interval consisting primarily of porous grainstone, which for purposes of this paper will be referred to as the "upper reservoir," a tight interval of predominantly mudstone and packstone, referred to as the "Basal barrier," and a porous grainstone interval called the "lower reservoir." Almost all of the Ratawi oil production is from the upper reservoir grainstones. The chronostratigraphic facies heterogeneity evident in Fig. 4b owes its origin to a transgressive sequence of prograding grain shoals deposited in relatively shallow water.3 During the early stages of transgression, as the shoals prograded over the Wafra paleo-high, muds and finer grain carbonates were deposited in intershoal lagoons. As the sea level rose, carbonate sediment productivity and accumulation surpassed the rise in sea level, resulting in an overall shallowing with time. Evidence of this can be seen in the general coarsening upward character of the porosity logs. With progressively shallower water depths and associated higher depositional energy, the grain shoals became spatially more extensive while the lagoonal areas retreated, ending in fairly expansive grain shoals in the later stages of reservoir development. At the end of Ratawi oolite time, a rapid increase in relative sea level drowned the shoaling sequence, and deposited the deeper marine Ratawi limestone and shale members.

2018 ◽  
Vol 14 (1) ◽  
pp. 1
Author(s):  
Prof. Dr. Jamal Aziz Mehdi

The biological objectives of root canal treatment have not changed over the recentdecades, but the methods to attain these goals have been greatly modified. Theintroduction of NiTi rotary files represents a major leap in the development ofendodontic instruments, with a wide variety of sophisticated instruments presentlyavailable (1, 2).Whatever their modification or improvement, all of these instruments have onething in common: they consist of a metal core with some type of rotating blade thatmachines the canal with a circular motion using flutes to carry the dentin chips anddebris coronally. Consequently, all rotary NiTi files will machine the root canal to acylindrical bore with a circular cross-section if the clinician applies them in a strictboring manner


2020 ◽  
Vol 7 (3) ◽  
pp. 52-56
Author(s):  
MMATMATISA JALILOV ◽  
◽  
RUSTAM RAKHIMOV ◽  

This article discusses the analysis of the general equations of the transverse vibration of a piecewise homogeneous viscoelastic plate obtained in the “Oscillation of inlayer plates of constant thickness” [1]. In the present work on the basis of a mathematical method, the approached theory of fluctuation of the two-layer plates, based on plate consideration as three dimensional body, on exact statement of a three dimensional mathematical regional problem of fluctuation is stood at the external efforts causing cross-section fluctuations. The general equations of fluctuations of piecewise homogeneous viscoelastic plates of the constant thickness, described in work [1], are difficult on structure and contain derivatives of any order on coordinates x, y and time t and consequently are not suitable for the decision of applied problems and carrying out of engineering calculations. For the decision of applied problems instead of the general equations it is expedient to use confidants who include this or that final order on derivatives. The classical equations of cross-section fluctuation of a plate contain derivatives not above 4th order, and for piecewise homogeneous or two-layer plates the elementary approached equation of fluctuation is the equation of the sixth order. On the basis of the analytical decision of a problem the general and approached decisions of a problem are under construction, are deduced the equation of fluctuation of piecewise homogeneous two-layer plates taking into account rigid contact on border between layers, and also taking into account mechanical and rheological properties of a material of a plate. The received theoretical results for the decision of dynamic problems of cross-section fluctuation of piecewise homogeneous two-layer plates of a constant thickness taking into account viscous properties of their material allow to count more precisely the is intense-deformed status of plates at non-stationary external loadings.


2012 ◽  
Vol 9 (1) ◽  
pp. 94-97
Author(s):  
Yu.A. Itkulova

In the present work creeping three-dimensional flows of a viscous liquid in a cylindrical tube and a channel of variable cross-section are studied. A qualitative triangulation of the surface of a cylindrical tube, a smoothed and experimental channel of a variable cross section is constructed. The problem is solved numerically using boundary element method in several modifications for a periodic and non-periodic flows. The obtained numerical results are compared with the analytical solution for the Poiseuille flow.


2012 ◽  
Vol 16 (7) ◽  
pp. 1845-1862 ◽  
Author(s):  
F. Jørgensen ◽  
W. Scheer ◽  
S. Thomsen ◽  
T. O. Sonnenborg ◽  
K. Hinsby ◽  
...  

Abstract. Geophysical techniques are increasingly being used as tools for characterising the subsurface, and they are generally required to develop subsurface models that properly delineate the distribution of aquifers and aquitards, salt/freshwater interfaces, and geological structures that affect groundwater flow. In a study area covering 730 km2 across the border between Germany and Denmark, a combination of an airborne electromagnetic survey (performed with the SkyTEM system), a high-resolution seismic survey and borehole logging has been used in an integrated mapping of important geological, physical and chemical features of the subsurface. The spacing between flight lines is 200–250 m which gives a total of about 3200 line km. About 38 km of seismic lines have been collected. Faults bordering a graben structure, buried tunnel valleys, glaciotectonic thrust complexes, marine clay units, and sand aquifers are all examples of geological structures mapped by the geophysical data that control groundwater flow and to some extent hydrochemistry. Additionally, the data provide an excellent picture of the salinity distribution in the area and thus provide important information on the salt/freshwater boundary and the chemical status of groundwater. Although the westernmost part of the study area along the North Sea coast is saturated with saline water and the TEM data therefore are strongly influenced by the increased electrical conductivity there, buried valleys and other geological elements are still revealed. The mapped salinity distribution indicates preferential flow paths through and along specific geological structures within the area. The effects of a future sea level rise on the groundwater system and groundwater chemistry are discussed with special emphasis on the importance of knowing the existence, distribution and geometry of the mapped geological elements, and their control on the groundwater salinity distribution is assessed.


2020 ◽  
Vol 2020 (8) ◽  
Author(s):  
H. Hernández-Arellano ◽  
M. Napsuciale ◽  
S. Rodríguez

Abstract In this work we study the possibility that the gamma ray excess (GRE) at the Milky Way galactic center come from the annihilation of dark matter with a (1, 0) ⊕ (0, 1) space-time structure (spin-one dark matter, SODM). We calculate the production of prompt photons from initial state radiation, internal bremsstrahlung, final state radiation including the emission from the decay products of the μ, τ or hadronization of quarks. Next we study the delayed photon emission from the inverse Compton scattering (ICS) of electrons (produced directly or in the prompt decay of μ, τ leptons or in the hadronization of quarks produced in the annihilation of SODM) with the cosmic microwave background or starlight. All these mechanisms yield significant contributions only for Higgs resonant exchange, i.e. for M ≈ MH /2, and the results depend on the Higgs scalar coupling to SODM, gs. The dominant mechanism at the GRE bump is the prompt photon production in the hadronization of b quarks produced in $$ \overline{D}D\to \overline{b}b $$ D ¯ D → b ¯ b , whereas the delayed photon emission from the ICS of electrons coming from the hadronization of b quarks produced in the same reaction dominates at low energies (ω < 0.3 GeV ) and prompt photons from c and τ , as well as from internal bremsstrahlung, yield competitive contributions at the end point of the spectrum (ω ≥ 30 GeV ). Taking into account all these contributions, our results for photons produced in the annihilation of SODM are in good agreement with the GRE data for gs ∈ [0.98, 1.01] × 10−3 and M ∈ [62.470, 62.505] GeV . We study the consistency of the corresponding results for the dark matter relic density, the spin-independent dark matter-nucleon cross-section σp and the cross section for the annihilation of dark matter into $$ \overline{b}b $$ b ¯ b , τ+τ−, μ+μ− and γγ, taking into account the Higgs resonance effects, finding consistent results in all cases.


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