RESERVOIR SCALE CHEMOSTRATIGRAPHY AND FACIES MODELING USING HIGH SAMPLE RATE GEOPHYSICAL SCANS OF WHOLE CORE

2021 ◽  
Author(s):  
John J. Degenhardt ◽  
◽  
Safdar Ali ◽  
Mansoor Ali ◽  
Brian Chin ◽  
...  

Many unconventional reservoirs exhibit a high level of vertical heterogeneity in terms of petrophysical and geo-mechanical properties. These properties often change on the scale of centimeters across rock types or bedding, and thus cannot be accurately measured by low-resolution petrophysical logs. Nonetheless, the distribution of these properties within a flow unit can significantly impact targeting, stimulation and production. In unconventional resource plays such as the Austin Chalk and Eagle Ford shale in south Texas, ash layers are the primary source of vertical heterogeneity throughout the reservoir. The ash layers tend to vary considerably in distribution, thickness and composition, but generally have the potential to significantly impact the economic recovery of hydrocarbons by closure of hydraulic fracture conduits via viscous creep and pinch-off. The identification and characterization of ash layers can be a time-consuming process that leads to wide variations in the interpretations that are made with regard to their presence and potential impact. We seek to use machine learning (ML) techniques to facilitate rapid and more consistent identification of ash layers and other pertinent geologic lithofacies. This paper involves high-resolution laboratory measurements of geophysical properties over whole core and analysis of such data using machine-learning techniques to build novel high-resolution facies models that can be used to make statistically meaningful predictions of facies characteristics in proximally remote wells where core or other physical is not available. Multiple core wells in the Austin Chalk/Eagle Ford shale play in Dimmitt County, Texas, USA were evaluated. Drill core was scanned at high sample rates (1 mm to 1 inch) using specialized equipment to acquire continuous high resolution petrophysical logs and the general modeling workflow involved pre-processing of high frequency sample rate data and classification training using feature selection and hyperparameter estimation. Evaluation of the resulting training classifiers using Receiver Operating Characteristics (ROC) determined that the blind test ROC result for ash layers was lower than those of the better constrained carbonate and high organic mudstone/wackestone data sets. From this it can be concluded that additional consideration must be given to the set of variables that govern the petrophysical and mechanical properties of ash layers prior to developing it as a classifier. Variability among ash layers is controlled by geologic factors that essentially change their compositional makeup, and consequently, their fundamental rock properties. As such, some proportion of them are likely to be misidentified as high clay mudstone/wackestone classifiers. Further refinement of such ash layer compositional variables is expected to improve ROC results for ash layers significantly.

Geophysics ◽  
1954 ◽  
Vol 19 (3) ◽  
pp. 478-489 ◽  
Author(s):  
Albert Orsinger ◽  
Robert Van Nostrand

Previous publications have outlined the general theory of electromagnetic wave propagation along an interface such as the air‐earth boundary and described model experiments in which this theory was verified. Equipment similar to that described for the laboratory experiments has been adapted for field use. Two large loops, one for transmitting and the second for receiving, are laid on the surface of the ground and a current square wave is passed through the transmitting loop. A similar arrangement of loops is placed on the surface of a metallic model. The signals from the two receiving loops are mixed in opposition. The layering in the model is then manipulated until the difference signal is a minimum, which condition signifies that the actual earth has been approximated in the model, after account is taken of the appropriate scaling factors. At five stations in Dallas County, Texas, this technique was used to determine the depth of the Austin chalk‐Eagle Ford shale contact, which varies from 50 to 400 feet, within an average accuracy of about five per cent.


Geophysics ◽  
1953 ◽  
Vol 18 (1) ◽  
pp. 54-69 ◽  
Author(s):  
J. E. White ◽  
R. L. Sengbush

Procedures are described for measuring various seismic velocities at shallow depths in the earth, and examples of the resulting logs are presented. Velocities in Austin chalk and Eagle Ford shale show that these formations are not isotropic, and velocities in loose sand are seen to increase smoothly with depth except for an abrupt increase in compressional speed at the water table. Elastic constants for chalk and shale are computed. A discussion is given of the literature dealing with a packing of spheres as a model for loose sand, and an approximate theory is presented which includes tangential forces between spheres.


2017 ◽  
Vol 47 (2) ◽  
pp. 105-128 ◽  
Author(s):  
Christopher M. Lowery ◽  
R. Mark Leckie

Abstract The Cenomanian–Turonian Eagle Ford Shale of south Texas occupies an important gateway between the Western Interior Seaway (WIS) of North America and the Gulf of Mexico. While the Eagle Ford north of the San Marcos Arch and its stratigraphic equivalents to the east of the Sabine Arch are shallow-water sediments dominated by terrigenous clastics, the more distal localities in south Texas are dominated by hemi-pelagic carbonates draped over an Early Cretaceous carbonate platform, called the Comanche Platform, and adjacent submarine plateaus and basins. This region was strongly affected by major oceanographic changes during the Cenomanian-Turonian, particularly a significant transgression that drove localized upwelling and organic matter burial in the Lower Eagle Ford prior to the global Oceanic Anoxic Event 2 (OAE2). These pre-OAE2 organic-rich shales are the basis of Eagle Ford shale gas play, which has spurred commercial and academic research into many aspects of the geology of the Eagle Ford Group. Much of this research has been fairly locally focused, and little effort has been made to understand the timing of events across the platform. We compared new data from three study sites across south Texas—Lozier Canyon in Terrell Co.; Bouldin Creek in Travis Co., near the San Marcos Arch in the center of the Comanche Platform; and Swift Energy's Fasken Core in Webb Co., off the platform on the Rio Grande Submarine Plateau—as well as published data from near Big Bend National Park on the western margin, and from Atacosta and Karnes counties on the eastern margin. Using these data we document the occurrence of key foraminiferal species across the platform and present a regional biostratigraphic scheme incorporating five global planktic foraminiferal zones (and contemporaneous occurrences that may serve as proxies for the zonal markers, which tend to be rare in Texas) and four local origination or acme events that serve as useful secondary markers. The succession of events is: 1) highest occurrence (HO) Favusella washitensis, 2) lowest occurrence (LO) Rotalipora cushmani, 3) “Benthonic Zone”, 4) HO R. cushmani and/or Thalmaninella greenhornensis, 5) “Heterohelix shift”, 6) LO “Anomalina W”, 7) LO Helvetoglobotruncana helvetica, 8) HO H. sp., and 9) LO Dicarinella concavata. Overall, we show that lithologic and geochemical trends through most of the Eagle Ford, particularly the oxygenation at the onset of OAE2 and the concurrent shift to more carbonate-rich lithologies, are synchronous across the Comanche Platform. However, the transition from the Eagle Ford Group to the Austin Chalk varies in age. While Austin Chalk deposition began in the middle Turonian Marginotruncana schneegansi Zone on the Rio Grande Submarine Plateau, a transgressive surface on the Comanche Platform (known as the “Rubble Zone” in central Texas) represents a condensed interval at the top of the Eagle Ford that ends in the upper Turonian D. concavata Zone. This is part of a transgressive disconformity that extends north through the WIS, where it is associated with the Juana Lopez Calcarenite.


2013 ◽  
Vol 1 (2) ◽  
pp. SB61-SB83 ◽  
Author(s):  
Osareni C. Ogiesoba ◽  
Ray Eastwood

We conducted seismic multiattribute analysis by combining seismic data with wireline logs to determine hydrocarbon sweet spots and predict resistivity distribution (using the deep induction log) within the Austin Chalk and Eagle Ford Shale in South Texas. Our investigations found that hydrocarbon sweet spots are characterized by high resistivity, high total organic carbon (TOC), high acoustic impedance (i.e., high brittleness), and low bulk volume water (BVW), suggesting that a combination of these log properties is required to identify sweet spots. Although the lower Austin Chalk and upper and lower Eagle Ford Shale intervals constitute hydrocarbon-sweet-spot zones, resistivity values and TOC concentrations are not evenly distributed; thus, the rock intervals are not productive everywhere. Most productive zones within the lower Austin Chalk are associated with Eagle Ford Shale vertical-subvertical en echelon faults, suggesting hydrocarbon migration from the Eagle Ford Shale. Although the quality factor (Q) was not one of the primary attributes for predicting resistivity, it nevertheless can serve as a good reconnaissance tool for predicting resistivity, brittleness, and BVW-saturated zones. In addition, local hydrocarbon accumulations within the Austin Chalk may be related to Austin TOC-rich zones or to migration from the Eagle Ford Shale through fractures. Some wells have high water production because the water-bearing middle Austin Chalk on the downthrown side of Eagle Ford Shale regional faults constitutes a large section of the horizontal well, as evidenced by the Q attribute. Furthermore, the lower Austin Chalk and upper Eagle Ford Shale together appear to constitute a continuous (unconventional) hydrocarbon play.


2017 ◽  
Author(s):  
Peng Cheng ◽  
Michael Perz ◽  
Oluwafemi Ogunsuyi ◽  
Frank Meng ◽  
Xinxiang Li ◽  
...  

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