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How to evaluate source potential and reservoir characterization with software? name them.

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Question added by Fazal Aleem , TRAINEE GEOLOGIST, EXPLORATION DEPARTMENT , OGDCL,PAKISTAN
Date Posted: 2014/01/25
Yousif  Hassan  Mohamed  salh
by Yousif Hassan Mohamed salh , hydrogeologist , Water and Environmental Sanitation Project, Blue Nile State, Sudan) (WES)

United States Department of the Interior

 

U.S. GEOLOGICAL SURVEY DIGITAL DATA SERIES DDS-33 3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00

 

Debra K. Higley 1., Michael P. Pantea 1., and Roger M. Slatt 2.

 

  1997

 

    • Below is Sussex Sandstone20x vertical exaggeration

U.S. DEPARTMENT OF THE INTERIOR, U.S. GEOLOGICAL SURVEY

 

Bruce Babbitt, Secretary Gordon Eaton, Director

  • For sale by: Book and Open-File Report Sales, U.S. Geological Survey
  • Denver Federal Center,
  • P.O. Box25425, Denver, CO80225

1.U.S. Geological Survey

2. Colorado School of Mines

 

 

U.S. GEOLOGICAL SURVEY DIGITAL DATA SERIES DDS-33 3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00 Table of Contents

 

  • To Display Information Click on the Following (Commonly Underlined) Highlighted Categories:

     

     

      United States Department of the Interior

     

    U.S. GEOLOGICAL SURVEY DIGITAL DATA SERIES DDS-33 3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00   READ ME FIRST

     

    Click on highlighted (generally underlined) text and images to open large-scale views, access other graphics or HTML-format text files, or jump to the labeled section of the document.

     

    This readme file contains the following information:

     

    1. QUICK INSTRUCTIONS - A) Software needed to open, link, run, and view the text and images on this CD-ROM, B) Software needed to run the movies located in the movies subdirectory, and C) How to open this CD-ROM.

       

    2. BACKGROUND INFORMATION ON THIS PUBLICATION

       

    3. REQUIREMENTS FOR PC/DOS AND WINDOWS SYSTEMS

       

    4. REQUIREMENTS FOR MACINTOSH SYSTEMS

       

    5. INSTALLING MOSAIC FOR PC/WINDOWS

       

    6. INSTALLING MOSAIC FOR MACINTOSH

       

    7. INSTALLING MOSAIC FOR UNIX

       

    8. COMPUTER PROGRAMS LOCATED IN THE "MAC," "PCWINDOW," AND "UNIX" SUBDIRECTORIES OF THE "SOFTWARE" FOLDER(Software functions are explained in readme files associated with software programs and summarized at the end of this readme file). The text and HTML files containing the detailed list and subdirectory location of software are named software (software.txt, software.htm).
    • mac directory for Macintosh computers
      • 1) NCSA Mosaic1.0.3, and2) Mosaic2.0.1 for A) Power Macintosh computers and B) Macintosh computers with68K series processors.
      • GIFConverter2.3.7
      • GraphicConverter2.2 (US)
      • JPEGView3.3.1
      • StuffIt Expander3.5.2
    • pcwindow directory for PC computers
      • NCSA Mosaic for Microsoft Windows v3.1, for Windows95 and Windows3.1 and3.2
      • LView Pro1.B and LView Pro1.C
      • StuffIt Expander for Windows
    • unix directory for UNIX computers
      • NCSA Mosaic2.6 - for11 different computer platforms

    QUICK INSTRUCTIONS

    A) Mosaic, Netscape, or other World Wide Web (WWW) network browser software is necessary to view and link the HTML (Hypertext Markup Language) text and GIF (Graphic Interchange Format) images located on this CD-ROM. All computer software on this CD-ROM are present in the "software" directory. Mosaic software are located in the "Mosaic" folder in each of the "mac" (Macintosh), "pcwindows" (PC Windows systems), and "unix" (UNIX) folders. Please refer to the readme files in these folders for information on how to load the software onto your system. Image viewer (such as Lview and JPEGView) software can be used to display the large-scale images. These software programs are commonly accessed by the network browsing software using text and image hooks, an invisible process to users.

    B) Movie player software (MoviePlayer, SimplePlayer, Fast Player, Sparkle, and others) is required to open and animate the single-fork stand-alone movies located in the movies directory. Our efforts to get license releases for Apple Computer, Inc. freeware came to naught. Apple QuickTime software for Macintosh and PC/Windows computers is necessary to animate movies. The QuickTime package, which includes MoviePlayer software, is located at the following Web site: http://quicktime.apple.com . An ftp.support.apple.com location is for those of you using File Transfer Protocol. Should these sites change, try searching the WWW using "quicktime software," or similar phrase. Instructions for copying the software from this and other sites are also explained. We recommend copying the packages during evenings or the weekend because of a very limited number of seats. Other movie player software are also available on the WWW. Try searching the web using "movie software" , movieplayer, or other text strings.

     

  • Software present on this CD ROM needs to be decompressed, generally by double clicking on the .HQX or .zip file.

    C) The home page (homepage.htm) for this document is located in both the root ("USGS_3D") directory and text ("ssx_txt") subdirectory. All HTML text files have ".htm" endings. Non-HTML text files display ".txt" endings.

    1. Some WWW-software is opened simply by double-clicking with the mouse on the homepage or other HTML file located on this CD-ROM. If your software does not have this capability then,
    2. Open Mosaic or other WWW browsing software,
    3. Select "open local" or "open file" under the "file" heading (generally a menu bar along the top of the open window); access the "USGS_3D" folder located on the CD-ROM; select and open homepage.htm.
    4. The home page banner includes the following "To Start Click Here..." highlighted phrase. Clicking on this will access the tour by opening the Table of Contents (3dstart.htm), which displays chapter names, HTML file names, and descriptions of the contents of this CD-ROM. This is a point-and-click type of publication; text and graphics hooks are highlighted.

     

     

    BACKGROUND INFORMATION ON THIS PUBLICATION

     

    This CD-ROM publication contains raw and interpreted data, maps, and other graphic displays linked to the geological history and characteristics of the Upper Cretaceous-age Sussex Sandstone of the House Creek oil field, Powder River Basin, Wyoming. Data were statistically analyzed and mapped in2-D and3-D, and included as ASCII-formatted, space-delimited data files. Files included on this CD-ROM can be retrieved for use in other applications, including graphics editing and display, mapping, and statistical programs. Graphics are stored as Graphics Interchange Format (GIF) and TARGA (TGA) images (see glossary for explanations of acronyms and words).

    World Wide Web (WWW) network browsing software is required to integrate the graphics images and text located on this CD-ROM. While included HTML (Hypertext Markup Language) documents (in the "ssx_txt" directory) can be viewed with standard word-processing software, the interactive capabilities of Web browsing software link text, images, movies, and data. Numerous graphics software programs can view and edit individual GIF and TARGA files which are located in the "ssx_gif," "ssx_tga," and several other directories.

    This CD-ROM was produced in accordance with both the ISO9660 and Macintosh HFS standards. Contained data and text files can be read by platforms supporting either of those standards. Also required is a CD-ROM drive and associated software. Provided graphics and movies are designed for use under DOS/Windows on IBM or100 percent compatible personal computers (PC's) and the Apple Macintosh family. The stand-alone EarthVision faces file is a3-D model intended for use on Silicon Graphics Corporation IRIS workstations. This ssxporos.faces file displays porosity distribution and sand-ridge boundaries for the House Creek field. The ssxporos.demo.Z and evview.Z compressed files are located in the "IRIS" subdirectory; these files are intended primarily for archive, but they can be loaded onto an IRIS workstation to create a stand-alone EarthVision3-D model.

    All brand and product names are trademarks or registered trademarks of their respective companies. The tm notation is not appended to these product names, largely because the HTML superscript notation did not work with all World Wide Web (WWW) browsers. The authors primarily use Mosaic as the reference for accessing the information on this CD-ROM. The Mosaic programs located on this CD-ROM are software that are written and upgraded at the National Center for Supercomputer Applications (NCSA) at the University of Illinois in Urbana-Champaign. Included with computer programs located in the "software" directory are general directions to copy Mosaic and other applications for your platform. Other network browsing programs are available and have been used to view this publication.

    Mosaic and associated software are available through anonymous FTP (file-transfer protocol) from NCSA. The ftp location is ftp.ncsa.uiuc.edu. Due to the number of people that use, and overload, the network, you may need to make several attempts to access and copy the files from NCSA. We recommend linking with the NCSA network early or late in the day. You are utilizing FTP on UNIX computers; remember that UNIX is case sensitive.

    The file-naming convention on this publication is primarily eight dot three. This indicates the file has a maximum of eight characters to the left of and three to the right of the ".". An asterisk (*) is used in this publication as a symbol to match all characters. It commonly indicates a longer file name, for example Mosa*.hqx would access all .hqx files that start with Mosa and end with .hqx, such as Mosaic.hqx.

    While this is dependent upon your system and software, stand-alone movies located in the "movie" directory can be opened by1) starting your movie viewer and opening the movie file,2) double-clicking on individual movie names or icons, or3) accessing the movies with imbedded links in the HTML documents, which is the slowest option of the three. The *.MOV movies are designed to run on Macintosh and PC/Windows computers. The movies were created using the QuickTime and GraphicConverter software programs on a Macintosh IIsi. Our experiments with MPEG formatted movies produced lower quality images and are not included with this publication. File names displayed on each movie image are saved as separate GIF and (or) TARGA files; single3-D images can also be displayed from the "3-D images and movies" subsections of the table of contents.

     

    • Note: The price of this CD-ROM does not include costs of the software located on the disc. Please consider the usage requests of the software authors and companies. Instructions for how to use programs and where to contact the companies are in text files, generally associated with the software programs.

     

    REQUIREMENTS FOR PC/DOS AND WINDOWS SYSTEMS

     

     

    1. IBM or100-percent compatible personal computer, with a minimum of an80386 microprocessor. A math co-processor or80486 or better microprocessor is recommended

       

    2. Microsoft or PC-DOS version3.1 or later

       

    3. Microsoft Windows version3.1 or later

       

    4. Microsoft compatible mouse

       

    5. Although4 megabytes (MB) of RAM work, we recommend8 MB or greater

       

    6. An extended-VGA video board with a minimum screen resolution of640 by480 pixels and256 colors.

       

    7. A hard disk drive with a minimum of10 MB free disk space

       

    8. CD-ROM drive and software supporting ISO9660 standards

       

    9. WWW browser, image viewer, and QuickTime viewer are required to link HTML text and graphics images.

     

    REQUIREMENTS FOR MACINTOSH SYSTEMS

     

     

    1. Operating System7.0 or greater

      Files located on this CD-ROM are accessed locally and linked by the WWW browsing software using the File command heading and Open File orOpen Local subheadings (generally). For that reason, MacTCP software is not required to view the files. MacTCP v.2.0.2 (or later) Apple software is needed to connect to a remote host (also known as cruising the Web). MacTCP now comes bundled with System7.5. Your software needs may be different, depending upon the network browser software utilized.

       

    2. Minimum of4 MB RAM;8 MB or greater is recommended

       

    3. Should you load Mosaic or other WWW software on your hard disk, suggested minimum disk space is3 MB.

       

    4. This program requires a Macintosh with a13" or larger color monitor and CD-ROM drive. The drive and software should support ISO9660 or HFS standards.

       

    5. QuickTime software was used to display the GIF movies and images located on this CD-ROM. QuickTime needs to be installed in the Extensions folder within your System folder. QuickTime will run on all Macs with68020,68030,68040, or PowerPC processors (essentially everything but Mac Pluses, SE s, and PowerBook100 s).

     

    INSTALLING MOSAIC FOR PC/WINDOWS

     

     

    1. Create a directory for NCSA Mosaic and copy into it the Microsoft Windows ZIP file that is specific for your Windows version.

       

    2. Follow the procedures that are specified in the readme.txt text file located in "../software/pcwindow/mosaic." Note that the executable version of Mosaic for Windows95 (Win95x20.exe) includes a32-bit driver. Installation of the executable for Windows3.1 and3.2 (Win31x20.exe) requires incorporating32-bit drivers; this software is available as Win32s with OLE v1.30a from NCSA. The NCSA program is also located in the "software" directory and is named w32sOLE.exe.

       

    3. A program element can be inserted for Mosaic by choosing New under the File menu. Refer to your computer system documentation for the iconcreation procedure. Mosaic.EXE is the executable file for Mosaic.

     

    INSTALLING MOSAIC FOR MACINTOSH

     

     

    1. Copy the compressed version of the NCSA Mosaic for Macintosh2.0.1 software to your hard drive. mosai68k.hqx is the compressed Mosaic file name for Macintoshes that have68020,68030, or68040 processors (this excludes Power Macintoshes, Mac Pluses, SE s, and PowerBook100 s).mosai68k.hqx is located in "software/mac/mosaic/mosai68k." Mosaic for Power Macintoshes is named mosaippc.hqx and is located in the "software/mac/mosaic/MosaiPPC" subdirectory. Decompressed versions of this software are also located in the subdirectories. Once you have copied the NCSA Mosaic .HQX file from this CD-ROM to your computer, open it using decompression software. One of these is StuffIt Expander software, which is located in the "/software/mac/stuffit" and "/software/pcwindow/stuffit" subdirectories on this CD-ROM.

       

    2. Decompressing the .HQX and resulting .sit file creates the Mosaic executable program. Following decompression, the .SIT and .HQX files can be deleted as they are of no further use. Double clicking on the resulting file (name or icon) will start Mosaic. This3-D tour is started by opening the homepage.htm file. This is accomplished by choosing "open file," "open local," or similar command under the "File" heading on the WWW browsing software.

     

    INSTALLING MOSAIC FOR UNIX

     

  • NCSA Mosaic for the X Window System version2.6 can be used on most UNIX-based workstations. External viewing programs, such as Ghostview and xv, are recommended for linking images and text.

     

    1. First copy the compressed Mosaic binary file that is specific for your computer platform to your hard drive. These are located in "/software/unixzip/mosaic." Uncompress the downloaded Mosaic binary (an example for a Silicon Graphics Corporation, Indigo computer is: "uncompress mosaic-indy.Z").

       

    2. Create the binary executable using the "chmod" command (for example, type "chmod755 mosaic-indy" ).

       

    3. Execute the resulting binary file, thereby opening Mosaic.

     

    COMPUTER PROGRAMS LOCATED IN THE "MAC," "PCWINDOW," AND "UNIX" SUBDIRECTORIES OF THE "SOFTWARE" FOLDER

    Each of the below software programs has its own folder(s) within the "mac," "pcwindow," and (or) "unix" subdirectories. Due to the eight-dot-three file-naming convention, most names were shortened. File and software names, and directory locations are listed below. Please refer to the readme files associated with most of the software for information on how to load the programs onto your computer. We recommend opening the readme files using word-processing programs, however, should you access readme files through the below links, return by using arrows, back, or other options on your network browsing software.

     

    mac directory

    GIFConverter2.3.7 (486 KB) (shareware) - GIFConverter is used to open and read numerous graphic file formats. Formats include GIF, TIFF, RIFF, PICT, JPEG (JFIF), MacPaint and Thunderscan. It can write these formats, as well as black-and-white EPS (encapsulated PostScript). GIFConverter is used to convert files for use in other programs, to view files, and to print them out. The readme.txt file is saved in the "GIFConv" subdirectory as readme.txt. The compressed application program is named GIFConv.SEA .

     

  • GraphicConverter2.2 (US) - The compressed file is named GraphicC.HQX. This software imports, exports, and converts graphics stored in numerous file formats. Some graphics editing capabilities are included. This shareware program was created by Thorsten Lemke. The read_me.txt file is in the "USGS_3D/software/mac/GraphicC" subdirectory. Use StuffIt Expander to decompress the GraphicC.HQX file.

     

  • JPEGView3.3.1 is stored as the JPEGView.HQX package and as files that resulted from decompressing the .HQX using StuffIt Expander on a Macintosh IIsi. JPEGView is image viewing software for both6800-series and PowerPC Macintoshes. JPEGView can open and display graphics as both single images and slide shows in JPEG, PICT, GIF, TIFF, BMP, MacPaint, or Startup Screen formats. The readme3.txt and JPEGView3.3 Blurb readme files are in the "USGS_3D/software/mac/JPEGView" subdirectory.

     

  • Mosaic - World-Wide-Web browsing software programs. Three Macintosh programs are stored. Also saved are decompressed .HQX files. The readme files are Mosaicv1.txt for Mosaic1.0.3, and Mosaicv2.txt for Mosaic2.0.1.
    • NCSA Mosaic1.0.3 - Mosaic version1.0.3 for Macintosh computers is named MosaiMac.HQX and is located in "software/mac/mosaic/mosaicv1."
    • NCSA Mosaic2.0.1 (PPC) - version of Mosaic for Power Macintosh computers is named MosaiPPC.HQX and is located in "software/mac/mosaic/MosaiPPC".
    • NCSA Mosaic2.0.1 (68K) - version of Mosaic for Macintoshes with68 processors is named Mosaic68.HQX and is located in "software/mac/mosaic/Mosai68K".

     

  • StuffIt Expander3.5.2 is used to uncompress and unarchive downloaded information. The program is stored in the "USGS_3D/mac/stuffit" location. This software was created by Aladdin Systems, Inc. The "StuffIt Expander tm Read Me" readme file is created when StuffIt.HQX is decompressed. This text file was also saved in the "StuffIt" subdirectory as read_me.txt. The StuffIt Expandertm 3.5.2 Install application was renamed StuffIt.InsStuffIt Expandertm is the executable program.

     

    pcwindow directory

     

  • LView Pro Shareware - PC/Windows viewing software for graphic images. Programs are LView Pro1.B for Microsoft Windows3.1 (Win31, Win32s), and LView Pro1.C for Microsoft Windows95 (Win95). Compressed software programs are located in "/software/pcwindow/LView" subdirectory.

     

  • NCSA Mosaic for Microsoft Windows v3.1. Compressed binary executable software programs and readme text files are located in the "/software/pcwindow/mosaic" subdirectory. File names are Win95x20.exe (Mosaic binary executable for Microsoft Windows95), Win31x20.exe (Mosaic binary executable for Microsoft Windows3.1 and3.2), and w32sOLE.exe (the Object Linking and Embedding software that gives16-bit operating systems the ability to run32-bit applications). This is better explained in the NCSA readme files that are named read3132.txt and readme.txt.

    StuffIt Expanderھ for Windows expands files compressed in the following formats: StuffIt (.sit), ZIP (.zip), ARC (.arc), Arj (.arj), and gzip (.gz). StuffIt Expander will also decompress files in uuencoded (.uue), BinHex (.hqx) and MacBinary (.bin) formats. Self-extracting archives created by StuffIt, ZIP, and Arj can also be expanded using StuffIt Expander. StuffIt.EXE binary executable is located in the "/software/pcwindow/stuffit" subdirectory.

     

    unix directory

     

  • NCSA Mosaic for the X Window System v2.6 - World-Wide-Web browsing software programs. Compressed binary versions of Mosaic for eleven different UNIX platforms are located in the "../USGS_3D/software/unix/mosaic" subdirectory. Please refer to the readme.txt and readme.sol(aris) readme files for additional information.

     

     

      README FOR MOVIES

     

    Software needed to run the movies

    QuickTime software of Apple Corporation is required to view the movies. Also needed is movie player software, most of which is freeware or shareware. Try searching the WWW using "movie+software" . The current WWW site for information on Apple QuickTime freeware is http://quicktime.apple.com. QuickTime and MoviePlayer software for Macintosh computers and PC/Windows computers can be downloaded from links at http:/www.apple.com, or can be copied using File Transfer Protocol (ftp) with the following command: ftp ftp.support.apple.com . Unfortunately, this anonymous-user ftp site has a small quota, even with an additional ftptoo.support.apple.com site. Because of a limited number of seats, we don't recommend accessing the site during business hours.

    Movies can be called up from the text, but access is much quicker directly from the movies folder. Should you have trouble displaying images, try increasing available memory by closing all unnecessary windows and software programs. Shrinking the size of the movies may also aid in their display. We recommend playing with the menu bar located at the top of the movies and the bounding scroll bars; both to improve the image display and to familiarize yourself with program capabilities, including print and file export.

     

    Explanation of movie images

    The six movies located in the "movies" folder display3-D distribution and volumes of porosity and permeability for the Upper Cretaceous age Sussex "B" sandstone across the southern two-thirds of the House Creek oil field, Powder River Basin, eastern Wyoming. Information on data sources, and technical and research methodology are in the techinfo.htm file located in the "ssx_txt" directory. A glossary is included (glossary.htm) in the "ssx_txt" subdirectory for definitions of computer and geologic terms.

    Figure1. Structure contour map on the top of the Upper Cretaceous Sussex Sandstone Member of the Cody Shale, and approximate age equivalents, Powder River Basin, Wyoming and Montana. Location of the House Creek field is shown. Areal extent of the Sussex "B" sandstones is delineated by black-colored fields. Shaded fill outlining the basin are outcrops of Lance Formation and Fox Hills Sandstone. The rectangle located next to the30-miles scale bar defines the area of studied outcrops of the Sussex and Shannon Members, much of the Salt Creek anticline, and the towns of Midwest and Edgerton. Contour interval is500 ft. Datum is mean sea level. A detailed (176 KB) version is named indexfig.gif.

    Vertical exaggeration of the3-D images ranges from20 to60 times. The Sussex "B" sandstone is less than60 ft (18 m) thick and would look like a razor's edge without the exaggeration. The House Creek oil field is about1 mi (1.6 km) wide and, combined with the small Porcupine field at the southern boundary, is about36 mi (58 km) long. Reservoir-grade intervals in images are shown on the porosity (left) color bar by green through red (8 to21 percent porosity); low-porosity non-reservoir intervals are purple and blue (1 to8 percent porosity). Movies show:

     

    1. The field boundary, thickness of "B" sandstone intervals, color codes for porosity, permeability, and oil production increments, and index contour maps with location of reservoir slices in the field,

       

    2. Upward and seaward (eastward) increase in depositional energy, porosity, permeability, and oil production for each of the four stacked sand ridges that comprise the field. Stacking of high porosity and permeability intervals is also controlled by where each sand body is located relative to bounding sandstones. Greatest reservoir properties are when highest-depositional-energy facies of both sand ridges are stacked, as opposed to landward backstepping of the overlying sand ridge. An example of this is the sand ridge located below the E in figure20. The overlying sand ridge was deposited to the west.

       

    3. Concentration parallel and proximal to field axes of the greatest oil production, and thickness and lateral continuity of reservoir-grade sandstones,

       

    4. Reservoir compartmentalization resulting from laterally continuous permeability barriers between sand ridges. Permeability barriers (blue and purple colors on the porosity models) are mainly the low-depositional-energy mudstone and calcite-cemented sandstone facies. These are located toward the base of sand ridges, except where removed by erosion prior to or during deposition of overlying sand ridges.

       

    5. Vertical and lateral change in porosity and permeability. Porosity values are gridded at approximately1 ft (0.3 m) vertical increments. Well locations of core porosity data commonly exhibit diamond shapes. The diamonds show reservoir heterogeneity through the great variation in values over short vertical and lateral distances. Porosity calculated from well logs does not display as much variation because the data are smoothed by the well-logging process over ranges of several feet. Permeability movies also show this change at the well-bore level; all permeability data are core values. These are illustrated on figure20.

     

    Figure20. East-west oriented vertical slices of porosity (left, percent) and permeability (right, mD). This image (porpermv.gif) shows the highly variable porosity (left) and permeability (right) using core data. Porosity values/colors are reservoir grade (green through red) of8 through21 percent, and below-reservoir-grade low-porosity (blue) of less than8 percent. Permeability ranges are: purple and blue, up to5 mD; green,5 to16 mD; and yellow through red are greater than16 mD. Average permeability of Sussex "B" reservoir sandstones is15 mD. The close-spaced3-D grid essentially treats each well as a separate set of points for the purpose of showing the variation in porosity and permeability. The various diamond shapes and streaks of low through high porosity and permeability illustrate the interbedding of thin beds of reservoir- and non-reservoir-grade sandstone and mudstone. These diagrams include the eastward and upward increases in porosity and permeability, and stacking of sand ridges shown in previous images. This slice is located in the northwestern half of the field. Yellow dots are (left) core and well-log and (right) core sample locations. Slices are1.8 mi (2.8 km) wide and50 ft (15 m) high. Vertical exaggeration is30x. Respective names of the east-west porosity and permeability slide-image files are 3dew_img.htm and 3dvk_img.htm .

    Individual GIF files used to generate the movies are stored in the below directories (bounded by parentheses); GIF files are displayed in the text portion of this publication as single images, and as slide shows using an external viewer, such as JPEGView and LView.

    All movies are stored in the movies directory;

     

    • ewpermvf.MOV : east-west vertical slices of permeability for the northern half of the field area.0.70 MB (3dvk directory)

       

    • ewporosv.MOV : east-west oriented vertical slices of porosity across the field.13.9 MB (ewporosv directory)

       

    • hporosf.MOV : plan view of the field. Shown are horizontal slices of porosity from the base of the "B" sandstone upward.2.3 MB (hslice directory)

       

    • hporperf.MOV : plan view of the northern half of the field area. Shown are horizontal slices of permeability and porosity from the base of the "B" sandstone upward.3.2 MB (hporper directory)

       

    • nsporvf.MOV : north-south oriented vertical slices of porosity across the field.1.5 MB (3dgifns directory)

       

    • volporf.MOV : onion view along the eastern (seaward) margin of the field. Layers of porosity are stripped off, primarily in1-percent increments. Cumulative volumes are displayed for each porosity increment of the Sussex "B" sandstone.0.74 MB (esid_gif directory)

     

     

     

      U.S. GEOLOGICAL SURVEY DIGITAL DATA SERIES DDS-33 3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00 DIRECTORY OF SOFTWARE

     

    COMPUTER PROGRAMS LOCATED IN THE "MAC," "PCWINDOW," AND "UNIX" SUBDIRECTORIES OF THE "SOFTWARE" DIRECTORY. Please refer to associated readme text files for information on software requirements and installation processes.
    • mac directory
      • GIFConv - subdirectory (GIFConverter2.3.7 (486KB))
        1. readme.txt (readme text file)
        2. GIFConv.SEA (compressed GIFConverter2.3.7 application program)
        3. GIFConv.QT ( GIFConverter Quickstart text)
        4. GIFConv.N (notes, text)
      • GraphicC - subdirectory (GraphicConverter2.2 (US) folder)
        1. read_me.txt (readme file)
        2. GraphicC.HQX (compressed GraphicConverter package)
      • JPEGView - subdirectory (JPEGView3.3.1 program)
        1. readme3.txt (readme3.3 text file)
        2. JPEGView3.3 Blurb (readme text file)
        3. JPEGView.HQX (compressed JPEGView3.3.1)
      • The following files will result from decompression of JPEGView.HQX
        1. JPEGView (decompressed JPEGView application program)
        2. JPEGView.Help (JPEGView document)
        3. ParrotsJ.PEG (JPEGView document)
        4. Possible Conflicts (text file)
        5. JPEGView JFIF Preview (system extension file)
        6. AppleScript samples - subdirectory
          • Four JPEGView application programs
        7. AutoTypers - subdirectory
          • Seven AutoTyper application programs
      • Mosaic subdirectory
        1. Mosaicv1.txt (readme text file for NCSA Mosaic version1.0.3)
        2. Mosaicv2.txt (readme text file for NCSA Mosaic version2.0.1)
        3. Mosaicv1- subdirectory (Mosaic version1.0.3 for Macintosh)
          • LocalHom.htm (HTML-format home page information)
          • MosaiMac.HQX (compressed program)
          • Mosaicv1 (decompressed program)
        4. Mosai68K - subdirectory (Mosaic version2.0.1, Macintosh computers with68K processors)
          • Mosaic68.HQX (compressed program)
          • Mosai68K (decompressed program)
        5. MosaiPPC -subdirectory (Mosaic version2.0.1, Power Macintosh computers)
          • MosaiPPC.HQX (compressed program)
          • MosaiPPC (decompressed program)
    • StuffIt - subdirectory (StuffIt Expander3.5.2 program used to decompress other software packages)
      1. read_me.txt (readme text file)
      2. Stuffit.HQX (compressed program)
      3. stuffit.Ins (install program)
      4. StuffitE - Stuffit Expander (trademark) (decompressed on a68K computer)

     

  • pcwindow directory
    • LView - subdirectory (viewing software)
      1. LViewp1b.zip (1.B, shareware for PC's with Windows3.1)
      2. LViewpro.zip (1.C, shareware for PC's with Windows95)
      3. iregistb.txt (readme text file and licensing information for LView Pro1.B)
      4. iregistr.txt (readme text file and licensing information for LView Pro1.C)
    • Mosaic - subdirectory
      1. readme.txt (readme text file with installation information)
      2. read3132.txt (readme text file)
      3. Win95x20.exe (binary executable for PC's with Windows95)
      4. Win31x20.exe (binary executable for PC's with Microsoft Windows3.1 and3.2)
      5. w32sOLE.exe (Object Linking and Embedding software for32-bit applications).
    • stuffit - subdirectory (stuffit Expander for Windows decompression software)
      • stuffit.EXE (binary executable software)

     

  • unix directory
    • Mosaic Compressed executable binary Mosaic files for UNIX platforms. Format of this list is:1) file name,2) original NCSA file name of the binary, and3) computer platform information. Please refer to the readme text files for information on how to load them onto your disk.
      1. readme.txt --- readme-2.6 - (readme text file)
      2. readme.sol --- readme.solaris - (readme text file)
      3. Moalpha.Z --- Mosaic-alpha30-2.6.Z --- DEC Alpha, OSF13.0 (NO DTM, HDF, JPEG ,NO WAIS)
      4. Mosaidec.Z --- Mosaic-dec-2.6.Z --- DEC3100, Ultrix4.0 (DTM, HDF, JPEG, NO WAIS)
      5. Mosaichp.Z --- Mosaic-hp-2.6.Z --- HP9000/735, HP-UX9.01 (NO DTM,HDF,JPEG,WAIS)
      6. Mosaiibm.Z --- Mosaic-ibm-2.6.Z --- IBM RS/6000, AIX3.2 (DTM,HDF, JPEG, WAIS)
      7. Mosaindy.Z --- Mosaic-indy-2.6.Z --- SGI Indy, IRIX5.2 (DTM, HDF, JPEG, WAIS)
      8. Mosaisgi.Z --- Mosaic-sgi-2.6.Z --- SGI Indigo, IRIX4.0.5 (DTM, NO HDF, JPEG, WAIS)
      9. Moslinux.Z --- Mosaic-linux-2.6.Z --- Pentium, Linux1.1.94 (NO DTM,NO HDF,JPEG,NO WAIS)
      10. Msolaris.23Z --- Mosaic-solaris23-2.6.Z --- Sun, Solaris2.3 (NO DTM, HDF, JPEG, NO WAIS)
      11. Msolaris.24Z --- Mosaic-solaris24-2.6.Z --- Sun, Solaris2.4 (NO DTM, HDF, JPEG, NO WAIS)
      12. Mosaisun.Z --- Mosaic-sun-2.6.Z --- Sun, SunOS4.1.3 (DTM, HDF, JPEG, WAIS)
      13. Msunlres.Z --- Mosaic-sun-lresolv-2.6.Z --- Sun, SunOS4.1.3 (linked to libresolv.a)

     

     

      3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00

     

      GETTING STARTED - A BRIEF TUTORIAL

    This document explains how to access, use, and copy the various software, image, and text files located on this CD-ROM. The following terms and abbreviations are explained in the glossary that is included on the CD-ROM. NCSA (National Center for Supercomputing Applications) Mosaic and other World Wide Web (WWW) software allow the viewer to read and display individual image and HTML text files. Included in the readme1.htm file are directions for copying Mosaic and other software to your PC/Windows, Macintosh, and (or) UNIX platforms. readme1.txt is the standard text version of readme1.htm. Stand-alone movies are linked graphic interchange format (GIF) images for viewing on Macintosh and PC Windows computers. Because the MPEG format movies we created had poor visual quality, we decided not to include them on the CD-ROM. The EarthVision stand-alone model showing3-D porosity for the Sussex "B" sandstone is designed to run on IRIS workstations. Your computer's ability to view the images may be limited by its random access memory (RAM); it may help to close any unnecessary programs and open windows.

     

    • Note: Menu items can be selected either by using a mouse to click on the desired title banner at the top of Mosaic (or other network browsing software) documents, or by clicking on highlighted text and (or) images that have been labeled for this purpose. Scroll bars located at the bottom and (or) sides of documents, images, and movies are used for incrementing or paging through the items.

    Insert the CD ROM in your CD-ROM reader. Text and images are viewed using network browsing software. Text files are stored in the "ssx_txt" directory; links among these HTML files are shown in the table of contents and included in most displays. While many are saved as text files that can be opened using most word processing software, the WWW browsing display abilities result in much cleaner viewing. The movies, located in the "movie" directory, display3-D porosity and permeability across the House Creek field. These are animated by clicking on the *.MOV icons or file names. Movies can also be accessed from text hooks in some of the HTML files. The stand-alone3-D porosity model will only run on IRIS workstations and on SUN workstations that possess a special graphics template. The (zipped) ssxporos.demo.Z3-D model is located in the "IRIS" directory and can be started by opening the evview.Z file (zipped EarthVison View program).

    The Home Page, or start of the Mosaic document (or other network browsing software) can generally be invoked by double-clicking the Mosaic name or icon. Once the browsing software is initiated, start this3-D CD-ROM publication by opening the homepage.htm file under the open local or other file access command. These are commonly located under the File banner located at the top of your computer screen. We recommend that you peruse these menu items so that you will know your viewing, printing (also under File), and file-saving options. Depending on your computer system, size of the open window can be adjusted using the arrow key.

     

     

     

      3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00

     

      OVERVIEW

    This CD-ROM contains geologic and geochemical data collected as part of the Reservoir Characterization and3-D Reservoir/Basin Characterization for CD-ROM Projects of the U.S. Geological Survey. Information presented here is intended to address the national plans of Energy Information Transfer and Energy Environmental Investigations and Assessments. This publication contains raw and interpreted data, maps, and other graphic displays for the Upper Cretaceous Sussex Sandstone in the House Creek oil field, Powder River Basin, Wyoming. Location and geologic explanations are included in the Geology of the Sussex Sandstone and other sections.

    Data sources include1) core data from Kerr-McGee, Meridian Oil, and Woods Petroleum Corporations,2) bore-hole history and lease and field production information from Petroleum Information Corporation, and3) geologic, geophysical, and geochemical data generated and interpreted by USGS scientists.

    This publication is intended to serve a broad audience. An important purpose is to explain geologic and geochemical factors that control petroleum production from the House Creek field. This information may serve as an analog for other marine-ridge sandstone reservoirs. The3-D slide and movie images are tied to explanations and2-D geologic and geochemical images to1) visualize geologic structures in three dimensions,2) explain the geologic significance of porosity/permeability distribution across the sandstone bodies, and3) tie this to petroleum-production characteristics in the oil field. Digital publications are an important medium to archive maps, figures, and large volumes of geologic and geochemical data that would otherwise be lost. Movies, text, images including scanning electron photomicrographs (SEM), thin-section photomicrographs, and data files can be copied from the CD-ROM for use in external mapping, statistical, and other applications.

    Data has been statistically analyzed and mapped in2-D and3-D and included in the "data_set" directory as ASCII-formatted, row- and column-delimited data files. Files located on this CD-ROM can be read on UNIX, Macintosh, and PC/Windows computers. Information on how to access and read the contents is located in the following files: readme1.htm and .txt (readme first), and techinfo.htm (technical information on data sources).

     

     

    U. S. GEOLOGICAL SURVEY DIGITAL DATA SERIES DDS-33   3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00

     

  • To Display Additional Information Click on Highlighted (Generally Underlined) Categories:

     

     

      GEOLOGY OF THE SUSSEX SANDSTONE

     

      ABSTRACT

     

    The Upper Cretaceous Sussex "B" sandstone was deposited as a probable transgressive-marine sand-ridge complex in a mid-shelf position. The "B" sandstone is bounded by upper and basal disconformities and encased in mudstones and low-porosity and low-permeability sandstones of the Cody Shale. Reservoir characteristics are controlled primarily by depositional and diagenetic heterogeneity at megascopic (field), macroscopic (well), and microscopic (rock sample) levels. To simplify, this means production of oil is controlled by stacking and interbedding of sandstone and mudstone beds and by geochemical changes through time that affect flow of fluids through the rock.

    More than24.8 million barrels of oil (MMBO) have been produced from the Sussex "B" sandstone in the House Creek field, Powder River Basin, Wyoming. Greatest oil production, porosity, and permeability, the thickest reservoir sandstone intervals, and best lateral continuity of the primary reservoir facies are all located parallel and proximal to field axes. Decrease in reservoir quality west of the axes is due to greater heterogeneity from interbedding of low- and moderate-depositional-energy facies, with associated drop in porosity and permeability. Decrease in production east of the axes results primarily from a combination of seaward thinning of the primary reservoir facies and non-deposition of sand ridges.

    The House Creek field has two axis orientations; these are related to depositional patterns of the four sand ridges. Deposition of the "B" sandstone began in the southeastern corner of the field with sand ridge1; axis orientation is about north20 degrees west. Later-deposited sand ridges2 through4 are located west and north of sand ridge1; their axis orientations are approximately north32 degrees west. Progressive northward deposition of later sand ridges is probably concurrent with uplift of the northeast-trending Belle Fourche arch. Movement along the arch and of lineaments may have caused topographic highs that localized Sussex and Shannon deposition proximal to the arch.

     

      INTRODUCTION

     

    Three-dimensional images and stand-alone movies reveal porosity and permeability distribution within, and stacking patterns of sand ridges. These models show:

    1. The field and sand-ridge outlines, thickness and interbedding of sandstone/mudstone intervals, color codes for porosity, permeability, and production intervals, and index maps with location in the field of reservoir slices,

       

    2. Upward and seaward increase in depositional energy, porosity, permeability, and production for each sand ridge,

       

    3. Concentration parallel and proximal to field axes of the greatest production, and thickness and lateral continuity of reservoir-grade sandstones, and

       

    4. Reservoir compartmentalization resulting from laterally continuous permeability barriers between sand ridges. Permeability barriers are mainly the low-depositional-energy mudstone and calcite-cemented sandstone facies that are concentrated toward the base of sand ridges.

    Images and movies displaying3-D slices of the porosity and permeability models of the Sussex "B" sandstone are tied to descriptions of Powder River Basin and Sussex "B" sandstone geology, statistics on porosity and permeability distribution across the field, and images of core, outcrops, and thin-section and SEM photomicrographs. The purposes are to characterize relative influence of depositional and diagenetic processes on distribution of hydrocarbons in the House Creek field and to visualize these processes. Technical information on geologic, geochemical, and computer geologic methods of analysis are detailed inTechnical information on data sources (techinfo.htm). Diagenetic and depositional environment research (Higley,1994) is based on petrographic analysis of about60 thin sections, carbon and oxygen isotopic analysis of about20 samples of carbonates, cathodoluminescence, SEM, and X-ray diffraction studies, and core, outcrop, and well-log studies. Well-logs for approximately500 boreholes in the field area and120 within the House Creek and Porcupine oil fields were used to map locations of the Ardmore bentonite, tops and bases of the Sussex "B" sandstone and included sand ridges, and well-history data. Sussex and Shannon Sandstones Members core porosity and permeability data was derived for37 wells; this information for13 Sussex "B" sandstone intervals augmented well-log porosity data for an additional about90 wells.

    As detailed in readme First (readme1.htm), links among text, images, and movies are accomplished with pointing and clicking with computer mouse buttons. An asterisk (*) indicates a longer or variable file name. Most image files are saved in separate directories in Targa (*.tga and *.TGA) and GIF (*.gif and *.GIF) graphic formats. Images within this Geology of the Sussex Sandstone section and subsections are located in the "ssx_gif" and "ssx_tga" directories and are generally saved as full-size and scaled-down images. The "scaled down" images are half or less the dimensions and file size of the full-scale ones; they are accessed more quickly on this CD-ROM then are the large images. File names and sizes accompany figures.

     

      BACKGROUND GEOLOGY

     

    The Powder River Basin of Wyoming and Montana is an asymmetric Laramide-age structural basin with a steeply dipping western flank and a gently dipping eastern flank. The Upper Cretaceous Cody Shale, including the Sussex Sandstone Member and its age equivalents, underlies most of the Powder River Basin and outcrops along the western flank, west of the outcrops of Lance Formation and Fox Hills Sandstone shown as shaded fill on figure1. The informally named Sussex "B" sandstone unit of the Sussex Sandstone Member has a limited areal extent that is approximated by the outlines of the House Creek and Porcupine oil fields shown on figure1.

    The House Creek field is located on the gently-dipping eastern flank of the Powder River Basin in Wyoming. The field trends about N.40 degrees W., approximately parallel to present-day basin structure contours. It is about1 mi (1.6 km) wide and, combined with the small Porcupine field at the southern boundary, is about36 mi (58 km) long. A narrow zone of non-oil-productive, low-permeability marine mudstone separates these two fields. Oil from both fields is produced from the Upper Cretaceous Sussex "B" sandstone. Depths of the Sussex "B" sandstone in the fields ranges from about7,000 to9,000 ft (2,100 to2,700 m), and in thickness up to52 ft (16 m); average thickness of the reservoir interval totals about20 ft (6 m).

    Figure1. Structure contour map on the top of the Upper Cretaceous Sussex Sandstone Member of the Cody Shale, and approximate age equivalents, Powder River Basin, Wyoming and Montana. Location of the House Creek field is shown. Areal extent of the Sussex "B" sandstones is delineated by black-colored fields. Shaded fill outlining the basin are outcrops of Lance Formation and Fox Hills Sandstone. The rectangle located next to the30-miles scale bar defines the area of studied outcrops of the Sussex and Shannon Members, much of the Salt Creek anticline, and the towns of Midwest and Edgerton. Contour interval is500 ft. Datum is mean sea level. A detailed (176 KB) version is named indexfig.gif.

    This reservoir characterization of the House Creek oil field integrates depositional energy and environments, facies distribution, and burial diagenesis. These factors influence petroleum production by controlling;

     

    1. Reservoir heterogeneity,

       

    2. Vertical and lateral continuity and compartmentalization of sandstones,

       

    3. Locations and types of permeability barriers,

       

    4. Directions of maximum fluid flow at field, sand ridge, and bedform scales,

       

    5. Porosity/permeability distributions, and

       

    6. Emplacement and trapping of oil across the field.

     

    Cretaceous History of the Powder River Basin

    The informally named Sussex "B" sandstone is one of as many as12 separate sandstone bodies that are located at different vertical and lateral positions within the Sussex Sandstone Member (Anderman,1976; Crews and others,1976). Figure2 is a generalized stratigraphic section for Cretaceous and Tertiary sediments in the basin, including major unconformities.

    Figure2. Stratigraphic nomenclature for Late Cretaceous and Tertiary rocks, Powder River Basin (stratprb.gif,32 KB).

    The Cretaceous epicontinental seaway connected the Gulf of Mexico with the Arctic Ocean during deposition of the Upper Cretaceous Cody Shale, as shown on figure3 (Brenner,1978, Gill and Cobban,1973). The western margin of the seaway was marked by a tectonically active thrust belt that extended from Alberta to southern Nevada and included the actively growing Rocky Mountains. The eastern margin of the region was a relatively stable cratonic hinge zone that extended from Minnesota to eastern Kansas (Witzke and others,1983).

    Figure3. Map showing Cretaceous epicontinental seaway paleogeography during Campanian time (Late Cretaceous) (modified from Brenner,1978, reprinted by permission, Gill and Cobban,1973) (wseaways.gif). The large rectangle is Wyoming, the small one shows location of the Powder River Basin.

    Late Cretaceous time was marked by episodic transgression and regression of the Cretaceous epicontinental sea (Weimer,1984), which resulted in deposition of primarily marine sediments in the northern part of the seaway. Kauffman (1977) lists as many as10 transgressive-regressive cycles for the Western Interior during Cretaceous time. This list includes marine transgression during the time of deposition of the Sussex Sandstone Member, followed by regression of the sea. These cycles are correlative around the world and were based on biostratigraphy and radiometry (Vail and others,1977).

    Distinct eastward changes in shelf, slope, and basin morphology have been mapped in the Powder River Basin by Loutit and others (1988), who believe that a eustatic sea level rise in latest Maastrichtian time, about67 million years ago (Ma), significantly affected sedimentation patterns on continental margins; this event roughly correlates with the start of the Laramide orogeny (Tweto,1975,1980). Lillegraven and Ostresh (1990), however, postulate that Upper Cretaceous time in the seaway is marked by a very slow regional regression of the shoreline that is consistent with global lowering of sea level for this time period; their data are based largely on mapping and analysis of ammonite zones. Their evidence indicates that shoreline position during Late Cretaceous time was relatively static and considerably west of Sussex "B" sandstone deposition.

    During Campanian time (74-84 Ma) most of the Powder River Basin was part of a broad muddy shelf. Pierre and Cody Shales deposition is characterized by mainly marine muds punctuated with relatively thin sands (Brenner,1979). During deposition of the Cody Shale, regional morphology consisted of a distinct shelf, slope, and basin configuration; relief on the shelf may have been about1,000 ft (300 m) in the eastern part of the Powder River Basin (Asquith,1970). The abrupt eastern termination of the Sussex Sandstone corresponds with thinning and eventual pinchout of the Sussex interval (Brenner,1979).

    The Upper Cretaceous Sussex "B" sandstone was deposited in a probable mid-shelf position in the Cretaceous epicontinental seaway (Higley,1994). Basin morphology during deposition of Sussex and Shannon shelf sandstone beds in the Powder River Basin is illustrated on figure4 (shelfmod.gif) (Tillman and Martinsen,1984).

    Figure4. Basin morphology during deposition of shelf sandstone beds in the Powder River Basin (Tillman and Martinsen,1984 reprinted by permission). The House Creek field is located about10 miles (16 km) east of and approximately parallel to Hartzog Draw field. Oil in the Hartzog Draw and Heldt Draw fields is produced from the Upper Cretaceous Shannon Sandstone.

    Actual proximity of the Sussex "B" sandstone relative to shoreline is unknown. The difficulty with sand-ridge models lies with transporting and reworking sediments this far from shore. This Sussex "B" and other Sussex and Shannon Sandstone mid-shelf sand ridges had the following sources of sand and sediment transport:

     

    1. Transgressive erosion of sediments,

       

    2. linked with shelf transport and

       

    3. storm currents,

       

    4. probable existence of lobate deltas of the Upper Cretaceous Eagle Formation to the west (Hobson and others,1982, Higley,1994).

    One source of sand for the Sussex Member and underlying Shannon Member is erosion of precursor marine and possible nonmarine strata during transgression, with redeposition in shoreface to mid-shelf environments as marine-ridge sandstones.

     

    Possible Structural Controls on Deposition of Shelf Sands

    Deposition of shelf sands may also result from local and regional tectonic activity in the region. Kauffman (1977) believed the eastern platform of the Powder River Basin showed minimal localized tectonic activity, as reflected in a broad uniform pattern of marine sedimentation. Topographic highs on the Cretaceous shelf could have developed as a result of;

     

    1. Recurrent faulting or folding,

       

    2. Deposition of thick accumulations of sediment (e.g., deltas),

       

    3. Preservation by draping and (or) compaction of paleotopography from unconformities, and

       

    4. Erosion and sculpting of sediments during a lowered sea level (Slatt,1984).

    An ordered sand-ridge field, such as the Shannon Sandstone in the Hartzog Draw area (figure4), located about10 mi (16 km) west of the House Creek field, develops from an initial, low-relief, highly variable topography (Gaynor and Swift,1988). Tillman and Martinsen (1984), stated that "Detailed subsurface correlations of the Shannon sand ridges throughout the Powder River Basin, using well-developed bentonite markers, show the reservoir facies to "rise and fall" parallel to their elongation, indicating that the ridges were not deposited in layer-cake fashion." Sandstone ridges in the Sussex "B" sandstone rise to the north and to the west. These stratigraphic patterns of development of the higher energy shelf-ridge facies are interpreted to reflect sea-floor topography during their deposition. If basin structural features resulted in topographic highs during deposition of the Sussex "B" and other offshore sandstones, they could have resulted in concentration of sand and (or) sand ridges on the muddy shelf.

    Holocene shelf sand ridges on the Texas shelf and the Georges Bank - Nova Scotia - Newfoundland - Labrador shelf system (Slatt,1984) were examined and compared to sand-ridge deposits from the Cretaceous epicontinental seaway. Ridges in the transgressive Holocene sand sheets are associated with topographically high banks. Sediments here are derived from reworking of underlying substrates with contemporaneous deposition of mud in adjacent low areas. Oceanic currents play a strong role in localizing sand ridges, in grain sorting efficiency, and in areal distribution and stacking patterns of sands and muds.

    Lithostratigraphic and biostratigraphic data suggest Sussex Sandstone depositional intervals east of the House Creek field are compressed rather than missing (Gill and Cobban,1966; Asquith,1970; Brenner,1979). This indicates a reduced sediment accumulation rate east of the field and greater rates of compaction for mudstone than sandstone. This also indicates the area of the House Creek field was a paleo-topographic high. Thickness of the "B" sandstone ranges from several feet along and east of the seaward margins of the field to almost60 ft (18 m) along the western margin; this is a lateral distance of1 to1.5 miles. Sediments along the western field margin consist mainly of moderate- to low-depositional energy sandstone and mudstone. This wedge shape also indicates oceanic currents which sculpted the Sussex "B" sandstone were a fractionation mill. Sediments were eroded from the front of the marine ridges and re-deposited landward (westward). This is illustrated by figure5. This north-south-oriented vertical slice of the Sussex "B" sandstone is located near the northern boundary of the study area. It was mapped using the basal disconformity surface at the datum; the actual shape of the "B" sandstone is probably wedge-shaped with a lower surface that curves downward to the left (landward). This is an oblique slice across the field, the wedge shape is even more pronounced when cut perpendicular to the field axes.

    Figure5. This north-south-oriented vertical slice of the3-D porosity model (3dns_img.htm) shows upward and westward (landward) increase in sediment thickness, and progressive westward deposition of later sands in the Sussex "B" sandstone (wedgessx.gif). Blue on the3-D model is primarily mudstone and sandstones containing less than8 percent porosity, green is mainly fine- to medium-grained sandstones exhibiting8 to12 percent porosity, and yellow contours are mainly medium-grained trough-cross-bedded sandstones that contain greater than12 percent porosity. Respective average porosity of the "B" sandstone and of reservoir intervals are about8 percent and12 percent. Slice width and thickness are about2.5 mi (4 km) and50 ft (15 m). Vertical exaggeration is60x. Yellow dots are well sample locations. Index contour map shows cumulative oil production per well; contour interval is40,000 barrels.

    Tectonic influences may have altered sea floor relief and slope of the shelf during deposition of the Sussex "B" sandstone. This would provide sources of sediment through changes in relative sea level and oceanic currents, and influence areas of sediment deposition. Slack (1981) believes the Belle Fourche arch (fig.1), and other associated northeast-trending structural lineaments in the northern two-thirds of the Powder River Basin controlled localization of all significant Shannon and Sussex productive sandstones. Sussex and Shannon production is concentrated along the arch in this area of the basin. The axis of the arch crosses the northern quarter of the House Creek field. Location of the arch is based on gravity data; structures are difficult to identify from conventional subsurface structure maps. Uplift and erosion throughout Wyoming prior to deposition of the Teapot Sandstone Member of the Mesaverde Formation (72 Ma) (fig.2) probably obliterated evidence of additional transgressive and regressive phases of deposition during the latter part of the Late Cretaceous (Gill and Cobban,1966).

    The Belle Fourche arch probably formed from subtle variations in regional structural patterns which are precursors to the Laramide orogeny (Slack,1981). Subtle uplift along the arch occurred from Lower Cretaceous Muddy through Upper Cretaceous Sussex deposition, a period of about35 m.y. The Belle Fourche arch was slightly positive during deposition of the Sussex Sandstone (Slack,1981), and marine ridge deposition over structural highs may have generated topographic highs along the arch.

    Other suggestions of greater topographic relief and subtle uplift in the House Creek field area are1) deposition of the Sussex "B" sandstone began in the southeastern corner of the field and progressed to the north, toward the arch,2) the thickest section of the Sussex "B" sandstone, and many intervals of Shannon Sandstone, are located near the axis of the arch,3) in fact, most of the productive Sussex and Shannon intervals are along this trend, and4) the thin, areally discontinuous Sussex "A" sandstone overlies the "B" sandstone along the western field boundary. The "A" sandstone, located just below the Ardmore bentonite, produces oil from the Triangle U field. This field is located on the axis of the Belle Fourche arch in T.46 N., R.75 W.

     

     

     

      DEPOSITIONAL MODEL OF THE SUSSEX "B" SANDSTONE

    The House Creek and Porcupine oil fields are delineated by a major marine-ridge system that is composed of complexly interbedded thin-bedded mudstone and sandstone of the Sussex "B" sandstone. The informally named Sussex "B" sandstone is one of as many as12 separate sandstone bodies that are located at different vertical and lateral positions within the Sussex Sandstone Member (Anderman,1976; Crews and others,1976). Core and outcrop studies were combined with well log and analytical data, plus published research, to assign depositional environments for the Sussex "B" sandstone. Sandstones and mudstones were mapped across the study area to evaluate scales, types, and timing of reservoir heterogeneities, including lateral and vertical continuity and extent of bedforms, interbedding of reservoir and non-reservoir (seal) units, and depositional changes across the field related to variations in facies thickness, depth, and distribution of permeability boundaries.

    The "B" sandstone was deposited in a probable mid-shelf position in the Cretaceous Epicontinental seaway. Four separate sand ridges comprise the "B" sandstone in the field area. Transgression during deposition created westward (landward) backstepping of later deposited sand ridges. Sand-ridge development began in the southeastern corner of the field and progressed to the northwest, based on stacking patterns and correlation of sand-ridges and contained mudstone-sandstone beds, Sussex "B" upper and basal disconformities, and the overlying Ardmore bentonite.

    Figure6 shows thickness (in feet) of the Sussex "B" interval between the upper and basal disconformities. Landward stacking of sandstones is evident from the westward increase in sediment thickness. When mapped using either the overlying Ardmore bentonite or the bounding disconformities as datums, the Sussex "B" sandstone is wedge-shaped. The Cody Shale interval between the bentonite and "B" sandstone also is wedge-shaped; however, the open end is toward the ocean. The bentonite is a time-equivalent layer of volcanic ash that was chemically altered to clays during burial. While this trend is clear within the House Creek and Porcupine fields, each reservoir must be evaluated separately for stacking patterns. The top of the Sussex "B" reservoir sandstone in the study area is located approximately20 to60 ft (6 to18 m) below the Ardmore bentonite, based on correlation of well-logs and core studies (Higley,1994). Variation in thickness of the Ardmore-Sussex "B" interval results from1) influence of depositional environment, depositional energy, and sediment supply on localization of sediments,2) greater rates of compaction for shale-rich versus sandstone beds, and3) local or basinal structural movement and its association with rates of deposition.

    Figure6. Isopach map of the Sussex "B" sandstone showing thickness in feet of the interval between bounding disconformities; contour interval is4 ft (1.2 m). Map scales are meters. The small index contour map is cumulative oil production; contour interval is40,000 barrels. The thin red line outlines the boundary of the House Creek field. Thin white lines in the southern half of the field are limits of sand-ridge1 and overlying sand-ridge2. The large-scale64 KB image is named ssxiso.gif .

    Based on thin-section, core, outcrop, well-log, and production data, the highest quality Sussex "B" reservoir intervals are fine- to medium-grained, glauconitic, thinly bedded, trough- and planar cross-bedded sandstones. These facies contain greater reserves, porosity, and permeability and exhibit fewer laterally continuous permeability barriers and baffles than the fine-grained massive, ripple-laminated, and wavy-bedded sandstones that also produce oil.

     

    Sand-ridge models -- tied to core and outcrop photographs

    Transport of shoreface and shelf sediments across this seaway resulted from complex interaction of oscillatory and unidirectional currents, created primarily by intermittent along-shelf, southerly storm flows (Gaynor,1991). Sandstone ridges are aligned obliquely to the prevailing transport direction, as is shown on figure7. Figure8 is an idealized vertical slice across three stacked sand ridges. Due to the great spatial scales (width and length) of Shannon and Sussex sand ridges, the ridges must be obliquely oriented with respect to fluid flows (Gaynor and Swift,1988), as opposed to the flows being perpendicular to ridge boundaries. Cross-ridge flow accelerates on the up-current flank of the ridge; consequently, it is the up-current flank that undergoes erosion (Gaynor and Swift,1988). This cross-ridge acceleration and down-ridge frictional deceleration results in a rotation of flow over the ridge that causes erosion of the up-current flank, aggradation of the crest of the ridge, and growth of the sand ridge (Gaynor and Swift,1988).

    This model also explains thinning of the Sussex "B" sand ridges proximal to the open ocean, aggradation of the reservoir intervals along the crests of the sand ridges, and decrease in grain size, sorting efficiency, and associated porosity and permeability of sandstones west of axes of individual sand ridges and for the entire "B" sandstone. Directions of maximum fluid flow for this sand-ridge model are parallel to the axes of each trough-cross-bedded bedform and also parallel to field axes. These flow directions result from depositional patterns of the trough-cross-bedded sandstones, and concentration along field axes of the thickest and most porous and permeable units.

    Figure7. Plan view of lithofacies distribution on a sand ridge, and generalized flow streamlines (srplanvs.gif). Flow streamline arrows are the directions of currents over the sand ridge. Scale is approximate. Click sand Ridge - plan view (modified from Gaynor and Swift,1988, reprinted by permission) to see the detailed (srplanvw.gif) image (208 KB).

    Figure8. Idealized east-west-oriented vertical section across three stacked sand ridges (ssxflowu.gif). General facies types are listed. No vertical or horizontal scales.

    Figure8 shows upward and seaward increase in depositional energy (yellow dotted and green areas), which is tied to increases in porosity and permeability. The basal disconformity (wavy line) is the horizontal datum for the3-D porosity and permeability models. The wedge shape of the Sussex "B" interval results from reworking by currents of seaward margins of sand ridges, and landward redeposition of sediment. The blue-lined areas are basal and landward low-depositional-energy facies; these exhibit low porosity, permeability, and petroleum production.

    The disconformity at the top of the Sussex "B" sandstone is generally marked by a thin chert-pebble sandstone (figure9A). Shading variation of the quartz (figure9B) results from fracturing of the grain in this cross-nicols photomicrograph view (light is transmitted differently due to rotation of the crystal axes). Quartz grains that were incorporated from underlying sand-ridge sediments commonly exhibit early stages of diagenesis within marine environments, primarily chamosite overgrowths under the quartz overgrowths. Grain-to-grain contacts within this facies are mainly point with lesser long-straight contacts.

    Figure9. A. Chert-pebble-lag core photograph, and B. crossed-nicols photomicrograph of a chert-pebble lag, No.14-9 Federal well. Chert pebble lag corelinks the detailed (576 KB) ctlagc.gif core image. The bimodal grain distribution (mix of large and small grains) is visible on both images. Chert pebble thin section shows the large-scale (736 KB) ctlagts.gif photomicrograph image. Labels are Q quartz, CT chert, and C calcite. Quartz grains incorporated from underlying central-ridge facies sandstones commonly "float" in a matrix of (blue stained) ferroan carbonate cement.

    Figures10,11, and12 are thin-section, outcrop, and core photographs of trough-cross-bedded sandstones. These sandstones are the primary reservoir facies; facies are further divided based on relative decrease in depositional energy into central ridgehigh-energy ridge margin, and low-energy-ridge margin(Tillman and others,1985).

    Figure10. This transmitted-light thin-section image is from8,014 ft (2,443 m) depth in the Empire-Federal "C" oil well. Deformation of glauconite (G) pellets and other soft sediments in trough-cross-bedded sandstones form microscopic and macroscopic permeability baffles to fluid flow. Note also that quartz (Q) grains surrounded by glauconite do not exhibit the later diagenetic quartz cementation. Mudstone (brown) and glauconite (green) are concentrated along the lower depositional energy laminae of trough-cross-bedded sandstones. Late-diagenetic dolomite cement is stained dark blue (D). Medium-blue epoxy fills pore spaces (ellipse with a line through it). Glauconite is1.4 MB thin section (glauts.gif) image.

    Figure11. Photograph of an outcrop of Sussex Sandstone Member low-energy-ridge-margin (LRM) sandstone; outcrop is located in NW. corner of sec.7, T.40 N., R.78 W., Natrona Co., Wyoming. LRM thickness is about1 ft (0.5 m). Greater dispersal of glauconite, clays, and mud in lower depositional energy facies decreases porosity and permeability. This thin trough-cross-bedded sandstone, and the bounding burrowed and bioturbated sandstone/mudstone facies, contain mudstone and glauconite laminae and beds that are preferentially eroded, causing greater relief. Blue and purple lines in this small-scale image separate bedding planes. Trough-cross-bedded sandstone 1 MB (ssxcrp2.gif) outcrop image.

    Figure12. Core photograph of trough-cross-bedded medium-grained sandstone from8,169-ft depth in the No.1 Mandel-Federal well. Depths are in feet. Arrow points up. Siderite (S) clasts are concentrated on the bedding planes. Trough-cross-bedded sandstone 512 KB (trs8169.gif) core image.

    Figures13 and14 show inter-ridge depositional environments that consist mainly of burrowed and intact mudstone laminae, and interbedding of mudstone with fine-grained sandstone. Abundant permeability barriers result in low levels of petroleum production. These facies, concentrated toward the base of sand ridges, compartmentalize the reservoir intervals.

    Figure13. Core photograph of wavy-bedded fine-grained sandstone from8,194-ft depth in the No.1 Mandel-Federal well. Dark lines are mudstone laminae that segregate the thin, discontinuous sandstone beds. A siderite drape (arrow) is located on a ripple reactivation surface. Core width is3.5 inches (9 cm). Arrows within core point up-hole. Wavy-bedded sandstone -688 KB core (wss8194.gif) image.

    Figure14. Core photograph of a bioturbated very fine grained sandstone from8,038-ft depth in the No.1 Empire Federal well. This facies exhibits very low porosity and low permeability and is a reservoir seal. Black arrow points to a mudstone lamina. Gold arrow shows a burrow trace. Core width is2 inches.Bioturbated siltstone -800 KB core (bss8038.gif) image.

     

     

     

    SUSSEX "B" SANDSTONE HETEROGENEITY

     

    Heterogeneity (essentially nonuniformity) in sandstone reservoirs is controlled by the following factors; (modified from Weber,1986; Schenk,1988,1992):

     

    1. The geometry of sandstone bodies (lens-shaped, tabular, etc.),
    2. Faulting and fracturing of the reservoir intervals; this influences oil trapping and retention, as well as influencing fluid flow at field and well scales,
    3. Mudstone and other low-permeability baffles that direct flow of fluids through the rocks,
    4. Vertical and lateral distribution of facies, and interbedding characteristics of the sandstone, mudstone, and other rock types,
    5. Sedimentary structures (cross-bedding, burrowing...),
    6. Laminae, (such as thin mudstone layers and calcite-cemented intervals), and
    7. Influence of diagenetic history on porosity/permeability preservation, destruction, and enhancement.

    Reservoir quality in the Sussex "B" sandstone is a function of sedimentologic and petrologic heterogeneity. This and the following section discuss the relative influences of the above factors on porosity and permeability distribution and development. Faulting, aside from minor fracturing as viewed in core, is undocumented for the Sussex "B" sandstone.

     

    Porosity And Permeability Distribution

    Initial porosity in the Sussex "B" sandstone in the basin was probably35-40 percent by volume for trough- and planar-cross-bedded facies. Because of poor sorting (more clay and mud) finer grained sandstones exhibit lower initial porosity and permeability. The porosity range is based on examination of54 thin sections and is tied to analogs. Pryor (1973) analyzed distribution of porosity and permeability in unconsolidated beach sands in the Gulf Coast; he found that initial porosity of39 to56 percent decreased rapidly with burial. Wilson and Sibley (1978) determined that the Cambrian Galesville Sandstone, of Wisconsin, exhibited initial porosity of45 to50 percent; this decreased during burial to about33 percent. This decrease resulted mainly from rearrangement of grains during early burial. Further reduction to24 to33 percent was due to later quartz pressure solution (dissolution of quartz grains and associated closer packing of grains), and emplacement in pores of dissolved quartz, kaolinite (clay), iron hydroxide, and adularia (a feldspar mineral).

    Sussex "B" sandstone porosity and permeability range up to about21 volume percent and200 millidarcies (mD), respectively, for core tests from15 widely scattered boreholes. Geometric mean of permeability for this791 core-plug data set is0.62 mD.

    Core plus well-log average porosity is8.8 percent for the entire interval of the Sussex "B" sandstone, and about13 percent for reservoir intervals. These2,600 core plus well-log points have median porosity of8.4 percent. Porosity values were calculated from bulk density well-log traces for approximately100 wells; values were recalibrated to a specific grain density of2.68 g/cm3 (Higley,1994). Sonic log traces were used for porosity calculations for several wells. These porosity/permeability data files are located in the data_set directory.

    Figure15. Graph of core and well-log porosity versus depth for2,600 Sussex Sandstone Member points. The average8.8 percent porosity of the Sussex "B" sandstone and of reservoir intervals (13 percent) is also plotted. Scatter in data is considerable.

    Published reports of reservoir permeability and porosity in the House Creek field vary; Bauder (1981) listed a geometric average permeability of6.9 mD for the Sussex "B" sandstone. Sabel (1985) reported mean porosity and permeability of13 percent and15 mD, respectively, for reservoir sandstones in the House Creek field.

    Figure16. Volume percent porosity and permeability for791 core plug samples for30 wells, Sussex Sandstone Member (Higley,1994). Greater porosity correlates with permeability increase. Scatter in data is considerable. Dotted green lines are geometric averages for this data of8.8 percent porosity and0.62 mD permeability. Dashed red lines represent average porosity and permeability of13 percent and15 mD for reservoir intervals of the "B" sandstone. Yellow circles surround average porosity and permeability values for sand-ridge facies determined from core examination of8 wells. Sandstone facies are: chert-pebble lag, C; central-ridge, R; high-energy ridge-margin, H; low-energy ridge-margin, L; wavy-bedded, W; inter-ridge sandstone, S; and burrowed inter-ridge sandstone and mudstone, b.

    Sussex "B" sandstone facies and mineralogy vary greatly at megascopic (field scale), and even more so at macroscopic (well and rock), and microscopic (thin-section) scales. The most porous, permeable strata are the moderate- to high-depositional energy trough-cross-bedded medium-grained sandstones; these are primarily concentrated towards the tops of sand ridges. Increase in porosity and permeability is tied to increase in depositional energy. This results from:

     

    1. Better grain sorting and associated decrease in amounts of fine-grained sediment within pore throats and spaces,
    2. Greater vertical and lateral communication between porous/permeable beds,
    3. Fewer and thinner mudstone layers and other permeability barriers, and
    4. Decrease in low-permeability calcite-cemented (mainly fine-grained) sandstone.

    Amounts of calcite cements in17 trough-cross-bedded (H, R, and L in the above porosity/permeability figure) sandstone samples range from2.3 to34 percent, and average8.8 percent. Conversely,7 samples of inter-ridge burrowed mudstone to fine-grained sandstone (b, S, W) only averaged4.2 percent calcite cement. Resulting average minus-cement porosity is calculated at only18 percent. Extensive loss of porosity and permeability due to compaction and prior to calcite cementation, is indicated by the low percentage of calcite cement and large volume of mudstone and other soft sediments (about27 percent).

    Percent volumes of calcite cement and intergranular porosity for54 thin sections are shown on figure17; microporosity within clays and grains is not recorded. Thirteen percent porosity is average for reservoir intervals;8.8 percent is average for the entire Sussex "B" sandstone, based on core porosity/permeability of791 points. Intervals of greatest porosity generally contain less than3 percent calcite cement; calcite cement in this mainly trough-cross-bedded-sandstone facies is commonly spotty in thin sections, with evidence of extensive dissolution of cements.

    Figure17. Plot showing volume percentages of core porosity and calcite cement for the Sussex "B" sandstone. Low-porosity sandstones associated with greater than10 percent calcite cement commonly contain no effective porosity. This occurs mainly during the earliest stage of calcite cementation. The region with low porosity and minimal calcite cementation results from early diagenetic compaction. These samples are primarily burrowed and bioturbated sandstone and mudstone.

    Flow units are reservoir zones that exhibit similar fluid flow, porosity/permeability, reservoir potential, and production characteristics. Ebanks (1987) defined flow units as "volume of rock subdivided according to geological and petrophysical properties that influence the flow of fluids through it." Flow unit characteristics of the various Sussex "B" sandstone facies are assigned and detailed in Higley (1994); they are included below to show porosity/permeability/facies types for each reservoir and non-reservoir group of rock types.

    Sussex "B" sandstone fluid flow potential is rated E(xcellent), G(ood), F(air), and P(oor). These categories are general indicators of the reservoir favorability. Divisions are based on porosity and permeability characteristics of central ridge and other facies, probable directions of maximum fluid flow in the field, vertical and lateral continuity of reservoir and non-reservoir flow units (based on core, outcrop, and geophysical well-log examination), presence and number of permeability barriers and baffles, and petroleum production characteristics of wells. Table3 lists six flow units; these consist of three reservoir (E, G, F) and three low-permeability, non-reservoir (P5, P6, P7) units. Flow unit E exhibits excellent reservoir and fluid flow properties; G contains good reservoir properties, F exhibits marginal to fair reservoir properties, and the non-reservoir P units (P5, P6, P7) are permeability baffles and barriers bounding and interbedded with E, G, and F flow units. Determination of thickness and distribution of flow units across the field was based on examination of core from20 wells, well-log data for more than120 bore holes, and on outcrop studies.

     

    Table3. Flow-unit characteristics tied to ranges of permeability and porosity, and petrologic (rock) descriptions for Sussex "B" sandstone facies. Flow-unit ratings are from Higley (1994). Lithologic descriptions are based on outcrop studies and examination of core for about20 wells in the field area, permeability data are based on core analyses of15 wells within the House Creek field; porosity values are from core and well-logs for about120 wells in the field area.

    FLOW-UNIT RATING, PERMEABILITY (mD), POROSITY (PERCENT), AND PETROLOGIC CHARACTERISTICS

     

     

    E, >15 mD,10 to22 percent,

    Trough- and planar cross-bedded fine- to medium-grained sandstone that represents the highest depositional energy and greatest reservoir potential. While tabular, wavy-bedded, and ripple-laminated sandstones (flow unit G) near the tops of reservoir sand ridges may exhibit similarly high porosity and permeability values, fluid flow and other factors are different. Thickness of individual E units is as much as8 ft (2.4 m) but generally less than2 ft (0.6 m). Sand-ridge intervals composed of mostly E units are up to25 ft (7.6 m) thick, with an average of about10 ft (3 m). E units are thickest along field and ridge axes.

     

     

    G,12 to40 mD,8 to18 percent,

    Ripple-laminated, tabular, and wavy-bedded fine-grained sandstones that are commonly interbedded with thin trough-cross-bedded fine- to medium-grained sandstones (these are also assigned here to G because they are thin and laterally discontinuous). Thickness of flow-unit G ranges up to about15 ft (4.5 m) but is generally less than2 ft (0.6 m). Interbedding of flow units E and G, and to a lesser extent F, results from highly variable depositional energy conditions across the field.

     

     

    F,5 to20 mD,8 to18 percent,

    Ripple-laminated, tabular, and wavy-bedded very-fine and fine-grained sandstones. Reservoir favorability is further decreased by the interbedded, thin, calcite-cemented sandstones, numerous mudstone drapes, and biologic reworking. Thickness of F intervals is highly variable, ranging from several feet along and east of field axes, to more than20 ft (6 m) along the northwestern margin of the field. F units are located mainly near bases of sand ridges and along the western margin of the field.

     

     

    P5, .01 to2 mD,1 to13 percent,

    Burrowed and bioturbated mudstone and very-fine-grained sandstones that bound reservoir sandstones. This flow unit contains very low porosity and permeability and forms updip and overlying reservoir seals.

     

     

    P6, .01 to15 mD,1 to16 percent,

    Thinly bedded mudstone and calcite-cemented, fine-grained sandstones comprise P6. These form permeability barriers that are laterally continuous and separate upper and lower sand ridges, primarily ridges1 and2. P6 thickness is as much as10 ft (3.5 m), but is generally less than5 ft (1.5 m).

     

     

    P7, .01 to19 mD,1 to16 percent,

    This low-porosity and low-permeability unit is composed of thin mudstones and calcite- and quartz-cemented sandstones. Thickness ranges from inches to less than5 ft (1.5 m). P7 forms numerous discontinuous permeability baffles.

    An example of a Good to Excellent flow unit is the trough-cross-bedded medium-grained sandstone shown in figure18 (bedding planes are outlined in blue and purple in this snncrp1s.gif image). This is a non-productive probable lower-shoreface (near the beach) sandstone of the Shannon Sandstone Member. Even though this is a very porous sandstone, porosity, permeability, and fluid flow are all decreased by the thin sandstone beds (bounded by purple) that are highly cemented by quartz. Flow is influenced by orientations of trough-cross-bedding planes. Primary direction of maximum fluid flow is perpendicular to this image, and along the bedding planes of the individual cross-bedding laminae. Note also (for future reference) that individual beds have general lensate and tabular forms. The thin, highly cemented, low-permeability sandstone layers are massive in appearance, compared to the porous cross-bedded intervals that erode more readily.

    Figure18. This outcrop of a Shannon Sandstone Member trough-cross-bedded sandstone is located at Shepperson Ranch, west of Midwest and Edgerton, Wyoming (figure1). The thin, low-porosity, quartz-cemented beds are outlined in purple in this small-scale view. Porous and permeable intervals are bounded by a blue line. The1.2 MB image is named snncrp1.gif .

     

    Megascopic and Macroscopic (Field and Well) Scales

    Sussex "B" sandstone heterogeneity in the House Creek field results mainly from the following factors. Many of these factors are discussed in other sections, for example, the interbedding characteristics at macroscopic scales are detailed in the Depositional Model section.

    1. The lens shape of the reservoir interval (figure19), which has different fluid flow and petroleum production characteristics than, for example, a tabular reservoir. Sussex "B" sandstone production is concentrated along the axes of the field, and from the thickest intervals of stacked reservoir sandstones.
    2. The lensate form of the reservoir is distinct from the lens and tabular forms of individual reservoir sandstones that comprise the reservoir intervals. Each of these has its porosity/permeability/fluid flow-characteristics.
    3. Geometry and interbedding behavior of reservoir and non-reservoir facies controls fluid flow at well and bedform scales. Permeability boundaries to fluid flow occur at microscopic through megascopic scales.
    4. Connectivity and vertical- and lateral-continuity of oil-productive facies influences how much petroleum can be produced both from individual wells and from the field. They also govern how effective will be techniques of water-flood and other methods of secondary and tertiary oil recovery.
    5. Diagenetic/petrologic/depositional processes strongly influence porosity and permeability destruction, preservation, and creation; these are of course critical to migration of oil into the field and its subsequent recovery.

    Figure19. Illustrated are the lensate form of the reservoir, and of individual reservoir sandstones, in this vertical east-west slice showing3-D distribution of porosity across sand ridge1 and overlying sand ridge2. Yellow dots are locations of well-log porosity measurements. Blue and purple areas are primarily non-reservoir intervals. These are basal and landward low-depositional-energy sandstones and mudstones of individual sand ridges (porosity ranges up to8 percent). Green areas are reservoir-grade porosity of8 to12 percent. The breakover point between green and yellow is12 percent; this approximates the13 percent average porosity of reservoir intervals; yellow through red (20 percent porosity) are the best quality reservoir intervals. These are largely the medium-grained trough-cross-bedded sandstones, although even here there is considerable interbedding of low- through high-depositional-energy facies. Width of the reservoir at this slice is about2 mi (4 km). Vertical exaggeration is60x. This is 3dewlens.gif, slice10 of the3-D distribution of porosity model, as shown in the ewporosv.MOV movie.

    The reservoir sandstone intervals (green, yellow, orange, and red) are essentially lens shaped. These are composed of many thin, laterally discontinuous, interbedded sandstone and mudstone beds. The sandstone intervals pinch out along the eastern (seaward) margin and grade into non-reservoir (blue) and lower quality reservoir facies along the western field boundary. Datum is the basal disconformity (erosional surface). Using the overlying Ardmore bentonite as the datum, the field actually has a wedge shaped base and top. The same bulge (lens) is visible along the field axis, and reservoir intervals pinch-out to the east. A thin interval of high porosity (red) capping the field in some images is a remnant of the gridding process; a thin, areally discontinuous porous zone is located in several geophysical well logs at the top of the "B" sandstone.

    This3-D distribution of porosity slice (figure19) reveals;

     

    1. The lower (1) sand ridge exhibits the greatest porosity close to the seaward (eastern) margin of the field with porosity decreasing westward,
    2. The upper (2) sand ridge is composed of two separate sandstone units, close to the eastern and the western field margins. These sandstone bodies separate further and pinch out entirely a few slices to the north, and
    3. Lowest porosity intervals are basal and landward (westward) facies of most sandstone bodies. These low-porosity intervals compartmentalize the reservoir in this view and across much of the field. What this means is, in order to produce oil from both sandstones, both intervals must be perforated.

    Core porosity represents point sources, whereas well-log porosity is commonly smoothed over intervals of a few feet. Illustrating the high variability in porosity and permeability over short horizontal and vertical distances requires3-D images of core data, rather than porosity and permeability calculated from geophysical well logs (data sources and analytical procedures are detailed in the Technical information on data sources section of the Table of Contents).

    Figure20. East-west oriented vertical slices of porosity (left, percent) and permeability (right, mD). This image (porpermv.gif) shows the highly variable porosity (left) and permeability (right) using core data. Porosity values/colors are reservoir grade (green through red) of8 through21 percent, and below-reservoir-grade low-porosity (blue) of less than8 percent. Permeability ranges are: purple and blue, up to5 mD; green,5 to16 mD; and yellow through red are greater than16 mD. Average permeability of Sussex "B" reservoir sandstones is15 mD. The close-spaced3-D grid essentially treats each well as a separate set of points for the purpose of showing the variation in porosity and permeability. The various diamond shapes and streaks of low through high porosity and permeability illustrate the interbedding of thin beds of reservoir- and non-reservoir-grade sandstone and mudstone. These diagrams include the eastward and upward increases in porosity and permeability, and stacking of sand ridges shown in previous images. This slice is located in the northwestern half of the field. Yellow dots are (left) core and well-log and (right) core sample locations. Slices are1.8 mi (2.8 km) wide and50 ft (15 m) high. Vertical exaggeration is30x. Respective names of the east-west porosity and permeability slide-image files are 3dew_img.htm and 3dvk_img.htm .

    Variable distribution of porous zones is illustrated in figure21 A. and B. Shown are the respective3-D distribution and volumes of porosity for8 to21 percent, and12 to21 percent porosity. These views were chosen along the eastern margin of the field because deposition of the Sussex "B" sandstone began here, and upward and landward (westward) backstepping of later-deposited sand ridges is better displayed with this view than for other orientations. Average porosity of the Sussex "B" sandstone is about8.8 percent; average porosity of reservoir intervals is about13 percent.3-D distribution of intervals of porosity are explained and illustrated in the text (volporf.mov) sections of the table of contents.

    A

    B

    Figure21. A. This (por8vol.gif)3-D view of8 to21 percent porosity exhibits a total volume of358.6 million cubic meters. This is about 70 percent of the total volume of525.5 million cubic meters of the Sussex "B" sandstone within the field boundaries. The64 KB full-size image is named eside10f.gif B. This (por12vol.gif)3-D image of12 to21 percent porosity has a total volume of115.9 million cubic meters, which comprises less than 25 percent of the total volume of the "B" sandstone in the field. In comparison, the13 to21 percent porosity range is about62.2 million cubic meters; this is about 12 percent of the field volume. The64 KB full-size image is named eside10j.gif Green on the figures is8 to12 percent porosity. Yellow through red are12 to21 percent porosity. Blue arrow marks the boundary between sand ridge1 and2. The thin white line marks the upper disconformity surface of the "B" sandstone, except for the seaward margin of the House Creek field, which is outlined in red. The white arrows and line separate the northwestern and southeastern ridge systems; the gap in reservoir-grade porosity units is apparent. X and Y scales are shown in meters around the base of the block. Maximum thickness of the "B" sandstone is about60 ft (18 m). North arrow is included. Vertical exaggeration is80x.

    Macroscopic and Microscopic (Well and Sample) Scales

    Processes of porosity and permeability destruction from pervasive early cementation by calcite and (or) quartz, precipitation of clays, or by compaction are shown in figure22 (cmts4sm.gif).

    Figure22. Thin-section photomicrographs of four samples of the Sussex "B" sandstone. Q is quartz, CT shows the chert grains, K is kaolinite, C is calcite, Fshows feldspar grain (gray in the crossed-nicols view), MS are mudstone pore-fill and clasts, Oil coats grains and fills pores. Blue epoxy fills pore spaces. cmts4.gif is the full large-scale 2.4 MB image. Clockwise from upper left, images show;

    1. Absence of porosity and permeability resulting from precipitation of ferroan calcite (C), linked with dissolution of a feldspar (F) grain and peripheral dissolution of quartz (Q) and chert (CT) grains (cross-nicols light).

       

    2. Microporosity in an oil-stained, medium-grained sandstone resulted from late-diagenetic precipitation of kaolinite (K) in pore spaces (transmitted light).

       

    3. Low-depositional-energy facies have high levels of initial compaction with associated low levels of minus-cement porosity, later-diagenetic cements, or primary or secondary porosity. Quartz grains frequently show peripheral dissolution and only minor overgrowths (crossed-nicols light).

       

    4. Pervasive cementation by quartz is most common in thin-bedded, "clean," well-sorted sands with minimal evidence of prior cementation by calcite. Chlorite (green) rims some quartz grains. Because of the early cementation by quartz, mudstone clasts frequently exhibit only minor compaction. Porosity (blue) is minor (transmitted light).

    The3-D computer model images, including figures21 and22, show reservoir heterogeneity at megascopic (field) and macroscopic (well and rock) scales. Macroscopic heterogeneity includes stacking of sand ridges, lateral and vertical variation in porosity and permeability, upward and seaward increase in these properties, the lensate and tabular shapes of sandstone beds, and interbedding of high- and low-depositional energy facies. Microscopic heterogeneity, as shown by thin-section and SEM photomicrographs, results mainly from highly variable amounts and distributions of cements and authigenic and detrital clays; this porosity and permeability signature is highly facies related.

    Porosity in the Sussex "B" sandstone is mainly primary intergranular (pore volumes remaining from the time of deposition; intergranular means located between the grains). Secondary porosity results from corroded and dissolved feldspar and other lithic grains, which enhances porosity and permeability. Microporosity is present within pore-filling clays, largely kaolinite, and within some corroded chert and other grains. Microporosity is not effective porosity because the small pores are poorly connected. Intergranular plus intragranular porosity in thin sections is as much as17.5 percent. Average porosity for all thin sections is5.2 percent;3.4 percent of this is primary intergranular and as much as1.9 percent is secondary and intragranular porosity. Average thin-section porosity values for Sussex "B" facies are listed in table2; this is also located in the ssx_txt directory as the Ssxtable2.txt file. Format is tab-delimited, file is saved as an Microsoft Word text document. Tables located within the HTML documents are ASCII file formats.

    Thin-section porosity values are lower than core and average reservoir porosity for two main reasons. First, microporosity is not included in thin-section estimates but is measured during core analysis. The amount of microporosity may be considerable since clays comprise an average12 percent by volume of the Sussex "B;" clays are the primary permeability barrier at a microscopic scale. The percentage of microporosity should decrease up-section because the amounts of suspended-load sediment and most authigenic and detrital clays decreases upward. Second, three-dimensional effects of thin sections influence point-count results. These3-D effects include Sussex "B" grain-size sorting and distribution (which are rarely homogenous in sandstones), presence of horizontal laminae and drapes of glauconite and mudstone, orientation of grains and clasts, and other factors that influence heterogeneity.

    Sussex "B" sandstone primary and secondary porosity, and microporosity are shown on the following thin-section photomicrograph and SEM images. Pore spaces in all photomicrographs are filled with blue epoxy. Ferroan carbonates are stained blue (ferroan dolomite has dark blue crystals). Unless otherwise indicated, photomicrographs are with transmitted light. Scale bars on most images are0.1 mm. Porosity in the thin section is partially decreased by early diagenetic cementation of quartz grains. The original rounded quartz grains are outlined by green-colored chlorite crystals. Early diagenetic cementation preserves porosity and permeability in the Sussex "B" sandstone by supporting the grain framework and decreasing porosity loss through compaction.

    Figure23. A. Thin-section photomicrograph from8,012 ft (2,442 m) depth, No.1 Empire Federal "C" well (fdissols.gif). Dissolution of the large feldspar (F) grain, located near the center of the image, results in secondary porosity. The crystal structure and outline of the feldspar grain is still apparent. Primary (depositional) porosity borders this and other grains. Quartz grains are labeled Q. Microporosity results primarily from breakdown of feldspar into kaolinite (K on large-scale view) and other clay minerals; this causes a mottled appearance of the blue epoxy that fills pore spaces. MS is a mudstone clast. Scale bar is0.1 mm. The full-scale1.5 MB thin-section photomicrograph of feldspar dissolution is fdissol.gifB. Scanning electron microscope (SEM) image of kaolinite shows partings between booklets and minor amounts of "wispy" illite-smectite clay from the No.1-23 House Creek Federal well (semkaosm.gif). Scale bar, below the illite-smectite label, is4 micrometers. The656 KB SEM full-scale image of kaolinite booklets is semkao.gif.

     

     

     

    Diagenetic History of the Sussex "B" Sandstone

    The Sussex "B" sandstone exhibits a complex diagenetic history that strongly influenced porosity and permeability preservation, loss, and enhancement. These factors in turn affect emplacement, trapping, and production of petroleum. The Sussex "B" sandstone is a litharenite to feldspathic litharenite, based on the classification of Folk (1970). The early, middle, and late diagenetic stages are shown in the following figure24. High initial rates of compaction occur mainly in muds, and in sands that were not lithified, or supported, by early quartz and (or) calcite cementation. Rates of compaction decrease with time. The dashed lines are time periods of dissolution of grains and cements, which develops secondary porosity and permeability. Diagenetic stages were derived from examining the following;1) cores of10 wells,2)54 thin sections (including cathodoluminescent thin sections),3) numerous SEM images, and4) X-ray fluorescence (XRF) and diffraction (XRD) charts.

    Figure24. Generalized paragenetic sequence of the Sussex "B" sandstone (diagenes.gif). Dashed lines indicate times of dissolution of cements or grains. Yellow zone is period of sediment compaction. Medium blue zone is period of migration of hydrocarbons from shale source rocks. Dark blue zone is time of oil emplacement into the House Creek and Porcupine fields.

     

    Very Early Diagenetic Stages

    Precipitation of chlorite, pyrite, and alteration of fecal pellets to glauconite results from reducing conditions in marine pore fluids; this occurs soon after burial. Accumulation of bacterial end-products in pore fluids often results in precipitation of carbonate minerals and iron sulfides (Clayton,1992). These end products affect pore water pH, Eh, and ionic strength.

    The earliest diagenetic event is compaction. This is most significant for sediments with a high mud content; sand-sized grains floating in the mudstone matrix exhibit few and minor diagenetic changes. This results from isolation of these grains from pore fluids that affected cementation and dissolution. Rate of compaction of sediments decreases through time; later diagenetic cementation of sandstones by calcite and quartz stabilizes the grain framework; this decreases porosity and permeability loss through rearrangement of grains.

    Even though three periods of calcite cementation are shown on figure24, there is actually an additional stage of very early diagenetic calcite cementation. Because it is very limited in scope and distribution, it was not added to the figure. The following transmitted (rfca1sm.gif) and plane-polarized (rfcasm.gif) light images are radial-fibrous ferroan calcite. Radial-fibrous and planar-laminar calcite precipitates rapidly from pore fluids that are highly supersaturated in the carbonate ion. Bounding quartz grains exhibit peripheral dissolution but do not contain the later diagenetic chlorite rims or quartz overgrowths.

    Figure25. A. Transmitted-light view of very early diagenetic radial-fibrous calcite (C) that displaced quartz (Q) grains and glauconite. Calcite precipitated within the glauconite pellet and blasted it apart. Grains float in the matrix of calcite cement and mudstone (MS). Rfca1.gif is the full 752 KB transmitted-light imageB.The star-pattern of the calcite is apparent on this plane-polarized view. Rfca.gif is the full 736 KB plane-polarized image. Blue color results from staining the thin section for ferroan calcite.

    An early-diagenetic stage of grain dissolution and replacement by calcite cement (alteration of lithics on figure24) is indicated by standard and cathodoluminescent (CL) examination of several thin sections. The Figure26 (clumcmts.gif) photomicroscope image of a chert-pebble lag shows the following:1) Chert, quartz, and feldspar float in a matrix of ferroan calcite (orange) cement,2) the "bright" spots or ghosts on the sample are not grains; they are calcite cement that is optically continuous with surrounding calcite cement. These are called ghosts because they show locations of grains that were replaced by the calcite. Ghosts are invisible using standard petrographic methods, except when floating grains and fragments suggest their origin. Because they are invisible, calculated minus-cement porosity volumes would be too great for these samples (sediment porosity near the time of deposition). Visual estimation of volume of grains and fragments removed during this stage is1 to5 percent.

    Figure26. Cathodoluminescent photomicrograph of ferroan calcite cement (orange and bright orange) within a chert-pebble lag. Calcite is optically continuous across this view. Grains of chert (CT), quartz (Q), and feldspar (striped grain) float in a matrix of calcite cement. The feldspar grain is partially replaced by this very early diagenetic calcite. Bimodal grain distribution and point contacts between grains are also shown. clumcmt.gif is the full-scale 736 KB image. Quartz overgrowths are black (visible on the full-scale image). Scale bar is0.1 mm.

    Bimodal grain distribution results from erosion of underlying ridge sediments and incorporation of grains into the chert lag. Quartz grains exhibit very minor (meniscal in appearance) quartz cementation, that in turn has peripheral dissolution by the early diagenetic calcite cement. Quartz grains commonly have coatings of early-diagenetic chamosite. The style of early diagenesis represented in this lag and the underlying sandstone is characteristic for marine pore fluids; the sediments were probably not exposed to fluctuating ground water in a vadose zone. The meniscal (concavo-convex) occurrence of authigenic quartz results mainly from peripheral dissolution of the poorly developed overgrowths.

     

    Early to Middle Diagenetic Stages

    Rims of chlorite grow perpendicular to quartz grain surfaces and appear to be intergrown with the quartz cement, as shown on the figure27 SEM image (semchlsm.gif). Quartz displays well-developed overgrowths. X-ray diffraction analysis (Higley,1994) indicates that most of the Sussex "B" chlorite is ferroan chlorite, or chamosite. Fuchtbauer (1983) postulates that chlorite, chamosite, and glauconite are found almost exclusively in marine environments.

    Figure27. Scanning electron microscope (SEM) images of early-diagenetic chlorite rims (bladed crystals) that coat quartz grains and are intergrown with quartz overgrowths, No.14-9 Federal well. Brown box shows location of the zoomed-in image. A pore space is labeled (ellipse with a line through it). Semchl.gif is the full-scale 768 KB image.

    Precipitation of (middle diagenesis) calcite cement prior to cementation by quartz is illustrated by the figure28 cross-plot of depth in feet from surface versus volumes of a) calcite cement, b) quartz cement, and c) core porosity and d) permeability. Sussex "B" sandstone average porosity and permeablity of13 percent and15 mD are shown, as well as Sussex core and Shannon outcrop exposures that approximate core facies described in Higley (1988,1994). Porosity and permeability exhibit general upward increase, which correlates with increase in depositional energy (trough-cross-bedded sandstone), and decrease in amounts of calcite cements. Twin spikes of about13 percent quartz cement are mirrored by low percentage of calcite cement.

    Figure28. Shown are 1) 20 to0 percent calcite (CO3++) and14 to4 percent quartz (QTZ) cements, 2) 20 to0 percent core porosity (POR), 3) 100 to0.01 mD permeability (K), and 4) photographs showing facies for the Sussex "B" sandstone, Empire Federal "C" oil well. TRSS is trough-cross-bedded sandstone intervals; these are concentrated near the top of the "B" sandstone and are the primary reservoir facies. "THIN-BEDDED VF-F SS, MS LAMINAE" refers to the thin-bedded horizontally stratified fine-grained sandstone and interbedded mudstone. Bioturbated mudstone is the blue-gray-colored rock located mainly at the base and top of this section. Heavy vertical bar on the right side of the figure is the perforated zone. The full-scale 144 KB image is empfedsr.gif.

    Early diagenetic alteration of the hash is indicated by presence of the competent siderite clasts on Sussex "B" trough-cross-bedded sandstones (figure29). The initial stage of calcite cementation in the Sussex "B" sandstone is probably contemporaneous with alteration to siderite of foraminiferal tests and other depositional carbonate hash (figure30).

    Figure29. Core photograph (trs8167s.gif) from8,167-ft depth in the Mandel Federal "C" well shows siderite clasts that were ripped up by high-energy currents and redeposited on the trough-cross-bedded sands of submarine dunes. Original horizontal bedding is shown in clasts by the stringers of quartz grains. The full-scale trs8167.gif image is992 KB.

    Figure30. Thin-section photomicrograph of a siderite clast in a chert-pebble lag, No.14-1 Federal well, Porcupine field (foramsm.gif). Foraminifera tests in the clast have been partially replaced by siderite (brown). Evidence for the marine origin of the siderite clasts includes alteration to siderite of Haplophragmoides andReophax foraminiferal tests. The full-size foram.gif image is768 KB.

     

    Middle to Late Diagenetic Stages

    A number of diagenetic stages are shown on the figure31A, B transmitted-light and crossed-nicols photomicrographs (pyrca1sm.gif, pyrca2sm.gif). Pyrite (P) framboids (similar in appearance to raspberries) are black in transmitted-light and crossed-nicols views. These late-diagenetic pyrite crystals are commonly associated with the dolomite and may result from changes in chemical composition of pore fluids resulting from migration of hydrocarbons into the Sussex "B" sandstone.

    Figure31. A. Transmitted-light and B. crossed-nicols thin-section photomicrographs of pyrite framboids (P) within ferroan dolomite (D) from a trough-cross-bedded sandstone at8,014-ft (2,443 m) depth in the Empire Federal "C" oil well. Quartz (Q) and feldspar (F) grains bound optically-continuous calcite (C) cement. G is a glauconite pellet. Medium blue is epoxy and mottled blue results from kaolinite clay (transmitted light view), dark blue on both views is the late-diagenetic ferroan dolomite. Full-size transmitted-light image is 752 KB pyrca1.gif. Full-size crossed-nicols view is 784 KB pyrca2.gif.

    Quartz and feldspar grains in the figure31 thin section display well-developed overgrowths. Overgrowth formation was followed by precipitation of optically continuous, non-ferroan, poikilotopic, zoned calcite cement (C). Figure31B reveals subsequent spotty dissolution of the calcite cement by distribution of optically continuous fragments. This was followed by filling of the secondary pore by ferroan dolomite and pyrite. Also visible are a glauconite pellet (G) that has been slightly altered to illite (bright speckles under crossed nicols), and plagioclase feldspar (F, left border of images) that underwent extensive late-diagenetic dissolution and recrystallization. Original grain outline is indicated by brown dead oil (latest diagenetic emplacement).

    Dissolution of the ferroan calcite cements resulted mainly from changes in pore fluid chemistry, primarily organic and carbonic acids associated with hydrocarbon generation and migration into the reservoir. This created secondary porosity, and provided the primary source of chemically reduced iron for pyrite and ferroan dolomite. Migration also resulted in dissolution of feldspar and subsequent precipitation of kaolinite in pores.

    Late-stage influx of oil into the field area is indicated by both petrologic analysis of thin sections and burial history reconstructions. Thin sections that are oil saturated generally exhibit well-developed quartz overgrowths, dissolution of unstable lithics, and other stages characteristic of middle to late diagenesis. The time of oil generation for source rocks of the Sussex "B" sandstone is within the time range of40 Ma to possibly10 Ma (Higley,1994). Cody Shale samples from six wells in and near the House Creek field are marginally mature for oil generation and migration; mean random vitrinite reflectance (Rm) for nine samples ranges from0.51 to0.56 percent Rm at current depths of7,700 to9,800 ft (2,300 to3,000 m). This Rm range is lower than the0.6 percent to0.65 percent Rm onset of oil generation for types II and III kerogen (Waples,1985) that characterize these marine shales. Absence (currently) of faulting, and encasement of the reservoir in low-permeability shales of the Cody Shale suggest that the oil was generated in place, or at least did not experience long-distance migration. Suppression of vitrinite is also a possibility, with this scenario the Rm values would be slightly greater than recorded. A possible source of oil within the House Creek field is more thermally mature Cody Shale that is located deeper in the basin (Higley,1994)

     

     

     

      PETROLEUM GEOLOGY OF THE SUSSEX "B" SANDSTONE

     

    The Powder River Basin is an asymmetric Laramide-age structural basin with a steeply dipping western flank and a gently dipping eastern flank. The Upper Cretaceous Cody Shale, including the Sussex Sandstone Member and its equivalents, underlies most of the Powder River Basin and outcrops along the western flank, west of the Lance Formation and Fox Hills Sandstone outcrops shown as stippled patterns on figure1 (indexfsm.gif).

    The areal extent of the Sussex "B" sandstone is also indicated on figure1; the eastern boundaries of the House Creek and Porcupine fields approximate the eastern limit of the "B" sandstone. While the western margin of the fields does not define the western limit of the "B" sandstone, it does show the limit of reservoir-grade facies. There is a probable upper sandstone of the "B" located along the northwestern margin of the House Creek field, although well data is insufficient to determine whether reservoir-grade facies are present. Sussex "B" sandstone facies west of the field margins are mainly low-porosity and low-permeability mudstones and interbedded thin sandstones.

     

    Figure1. Structure contour map on the top of the Upper Cretaceous Sussex Sandstone Member of the Cody Shale and approximate age equivalents, Powder River Basin, Wyoming and Montana. Location of the House Creek field is shown. Areal extent of the Sussex "B" sandstones is delineated by black-colored fields. Shaded fill outlining the basin are outcrops of Lance Formation and Fox Hills Sandstone. The rectangle located to the right of30-miles scale bar defines the area of studied outcrops of the Sussex and Shannon Members, much of the Salt Creek anticline, and the towns of Midwest and Edgerton. Contour interval is500 ft. Datum is mean sea level. A detailed (176 KB) version is named indexfig.gif.

    Most oil production in the Sussex "B" sandstone is from the House Creek field with only minor production from the Porcupine field. More than24.8 million barrels of oil (MMBO),21.2 million cubic feet of gas (MMCFG) and1.6 MM barrels of water have been produced from the Sussex "B" sandstone in the House Creek field (PI Production data through December,1996). Concentrated along field axes are greatest oil production, and the most porous, permeable, laterally continuous, and thickest sandstone beds; combination of these factors indicates the Sussex "B" sandstone and similar reservoirs would be good candidates for horizontal drilling. The figure32 (oilprod.gif) contour map of cumulative oil production across the field area shows concentration of greatest production along the southeastern and northwestern ridge systems. Estimated original oil in place (OOIP) was159 million barrels (Sabel,1985). Ultimate recovery is estimated at about45 MMBO and40 MMCFG, less than30 percent of the OOIP. The Porcupine field is located at the southern margin of the House Creek field. More than3 MMBO and5 MMCFG have been produced from all reservoirs within the Porcupine field; production is commingled for the Sussex "B" sandstone, the Muddy Sandstone Member of the Early Cretaceous Thermopolis Shale, and the Turner Sandy Member of the Upper Cretaceous Carlile Shale (Lawyer and others,1981).

    Figure32. Contour map of cumulative oil production across the House Creek field area. Field is delineated by the red line. Contour interval is40,000 barrels of oil. Map scale, in meters, is shown around the margin. Township and range line intersections are also drawn. Greatest production is proximal to field axes; these are also areas of stacked sand ridges; oil is commonly produced from2 sandstone bodies separated by a permeability barrier. Porosity and permeability generally decrease west of the eastern margins of the field, so increase in production along the field axes is a function of thickest intervals of stacked sandstones with greatest porosity and permeability.

    The House Creek field has two axis orientations; these result from depositional patterns of the four sand ridges. Deposition of the "B" sandstone began in the southeastern corner of the field with sand ridge1; axis orientation of this sand ridge is about north20 degrees west. Overlying and later deposited sand ridges2 through4 are located west and north of sand ridge1; their axis orientations are approximately north32 degrees west. Progressive northward deposition of later sand ridges is probably associated with contemporaneous uplift of the northeast-trending Belle Fourche arch, which cuts across the northern boundary of the field in figure1. The arch orientation is perpendicular to the field. Movement along the arch and lineaments may have caused topographic highs that localized Sussex and Shannon deposition along the arch (Higley,1994).

    Reservoir intervals exhibit upward and seaward increases in grain size, porosity, and permeability, both across sand ridges1-4, and for the individual stacked thin-bedded reservoir sandstones that comprise the sand ridges. Individual thin trough-cross-bedded sandstones commonly coarsen downward. Greatest oil production, porosity, permeability, thickest reservoir sandstone intervals, and best lateral continuity of the primary reservoir facies are all located parallel and proximal to field axes.

    Oil is stratigraphically trapped in the Sussex "B" sandstone by an updip and overlying change from porous and permeable sandstone to relatively impermeable mudstone, and by an areally discontinuous capping chert-pebble sandstone; there is no oil-water contact in the field. Rapid decline in porosity and permeability at the upper contact of the Sussex "B" sandstone is visible on well log traces, core and core data, and vertical slices of3-D porosity and permeability. Sussex "B" facies west and east of the field boundaries are non-oil-productive, low porosity and permeability sandstones and bioturbated mudstones. These are the low-depositional-energy facies. "Correlation of electric logs across the fields (in the area) shows that a thick section of relatively low-permeability sandstone or siltstone is present in dry holes down dip from the (House Creek) field on the southwest" (Berg,1975).

    Primary, secondary, and tertiary recovery of oil is strongly affected by reservoir heterogeneities. House Creek field heterogeneity includes concentration parallel and proximal to field axes of greatest oil production, porosity, permeability, and greatest thickness and stacking of reservoir sandstones. Production is adversely affected by complex interbedding of thin-bedded reservoir sandstones with low-permeability sandstones and mudstones. These numerous permeability barriers and baffles cause field- and well-scale compartmentalization. Production is also decreased by pore-filling kaolinite and ferroan-calcite cements. Thickness of the permeability barriers that separate and compartmentalize upper from lower sand ridges is variable across the field. These low-energy facies were sometimes removed by erosion prior to or during deposition of overlying sandstones. This is particularly common in the northwestern half of the field area.

    The following two figures are plan-view contour maps of the entire thickness of Sussex "B" sandstone in the House Creek field (figure6, ssxisos.gif), and of the reservoir sandstone interval (figure33, resisos.gif).

    Figure6. Isopach map of the Sussex "B" sandstone showing thickness in feet of the interval between bounding disconformities; contour interval is4 ft (1.2 m). Map scales are meters. The small index contour map is cumulative oil production; contour interval is40,000 barrels. The thin red line outlines the boundary of the House Creek field. Thin white lines in the southern half of the field are limits of sand ridge1 and overlying sand ridge2. The large-scale64 KB image is named ssxiso.gif .

    Figure33. Sussex "B" sandstone isopach showing thickness in feet of the reservoir-grade sandstone interval. The House Creek field is delineated by red lines; the faint white lines outline sand ridge boundaries. Contour interval is4 ft (1.2 m). Map scales are meters. In some areas, contours are extrapolated outside of data control. Reservoir sandstone intervals were determined by examining well-log traces of about120 wells, as well as core and petroleum production data; boundaries correspond to a cut-off of about8.5 percent porosity. This interval includes lower porosity sandstone and mudstone located within and between sand ridges. Index map is cumulative oil production across the field; contour interval is40,000 barrels of oil (BO) for the range0 to400,000 BO. Resiso.gif is the large-scale64 KB contour map of reservoir intervals.

    Illustrated by the figures6 and33 contour maps are:

     

    1. Transgressive deposition of the Sussex "B" sandstone resulted in the greatest thickness of sediment along the northwestern and southwestern boundaries of the field. This is true for both the "B" sandstone and for reservoir-grade intervals within the "B" sandstone. The primary factor causing differences in thickness for the two maps is the bounding basal and upper non-oil-productive mudstone/sandstone intervals. These are excluded from the reservoir sandstone map. These low-depositional-energy facies also increase in thickness to the west. Effects of compaction through time were not included; muds generally compact much more than sands.

       

    2. Areas of the thickest "B" sandstone do not correspond to the greatest oil production. This results mainly from variations in stacking patterns of the sand ridges and from westward decrease in depositional energy. Also, west of the field axes reservoir-grade sandstone beds are thinner and exhibit greater interbedding of high- and low-porosity-and-permeability facies, based on core and well-log examination. Thinning along the eastern margins of the field is due primarily to erosional reworking and associated landward redeposition of sands. Also, upper sand ridges are generally absent here because westward transgression resulted in landward backstepping of later ridges.

       

    3. The isopach of reservoir-grade sandstone intervals includes low-permeability zones within and between sand ridges; these zones compartmentalize the reservoir. Greater thickness on this isopach correlates better to the areas of increased oil production, than does the isopach of the entire Sussex "B" sandstone.

       

    4. Examination of well logs across and outside the field area indicates the eastern boundary of an additional upper sand ridge may be present along the northwestern edge of the field. There is insufficient data to conclude whether this ridge developed into a reservoir for oil, or merely contains low- and moderate-depositional energy mudstone and fine-grained sandstones. Due to low porosity, this ridge is excluded from the isopach map of reservoir sandstone thickness.

     

    Production History

    The House Creek field was discovered by Woods Petroleum in1968 (Berg,1975; Sabel,1985). Low initial production of90 barrels of oil per day (BOPD) for the No.1 State1319 discovery well resulted in low rates of early drilling for the field. The well is located in sec.36, T.44 N., R.73 W. within the "shadow zone" of low-depositional-energy facies that lies between the northwestern and southeastern ridge systems. The well is situated between sand ridges2 and3 on the following plan-view image of the top of the Sussex "B" sandstone (figure34, ewhslics.gif).

    Figure34. Plan-view map on the upper disconformity surface of the Sussex "B" sandstone within the House Creek field. Reservoir-grade intervals are shown by green through red (8 to21 percent porosity); low-porosity non-reservoir intervals are purple through blue (1 to8 percent porosity). Sand ridges1 through4 and field boundaries are delineated by yellow and tan; dashed lines separate townships and ranges. Basal sand ridges are1 and3.

    The following House Creek field production decline curve (figure35, declines.gif), for the period from January1976 through August1992, shows gradual decrease in barrels of oil recovered, mirrored by increasing gas production and associated increase in gas-oil ratio (GOR). GOR on the chart is multiplied by100,000 to better show the curve. Increases in gas production are primarily due to decrease in reservoir pressure as oil is pumped out. Original GOR was341 and initial field pressure was3,220 psi (Bauder,1981). Pronounced dips in the curves result mainly from periods of non-production due to maintenance and (or) economics.

    Figure35. Production decline curve for monthly intervals from1976 through August1992 in the House Creek field. Oil (BBL), gas (CFG) and gas/oil ratio (GOR) curves are shown. GOR is multiplied by100,000 to better view increase in through time of gas production relative to oil. Water production is not shown due to small volumes. Cumulative production to January1976 was8.73 MMB of oil and4.06 MMCF of gas (Petroleum Information Corp. production data).

    Average cumulative oil production per well for111 wells (through July1993) in the House Creek field is120,000 barrels; average cumulative gas production is110,000 cubic feet. Initial production averaged154 barrels of oil per day (BOPD) for108 wells within the field boundaries. Average perforated thickness is14 ft (4.3 m). Most wells perforate both upper and lower sand ridges, and production is commingled (not separated out by upper or lower sandstones). The thickest perforated intervals are located in wells near the southwestern tip of the field, and along and west of the field axis in the northwestern half of the field.

    A combination of liquid expansion and solution was the original drive mechanism of the House Creek reservoir; pump production was necessary from the1968 discovery date (Sabel,1985). Completion practices consist primarily of casing, perforating, hydraulic fracturing, and, in some instances, acid treatment to increase productivity. "A secondary recovery waterflood, scheduled to start in early1986, is expected to increase production from12.5 to21.5 percent of the original oil in place" (Sabel,1985). Production to1995 is14 percent of original oil in place (OOIP).

    Woods Petroleum operated a secondary recovery unit from section12 of T.45 N. to the southern boundary of the field, and Inexco Oil operated the recovery unit for the rest of the field. A3-to-1 line drive flood was originally planned in order to minimize additional drilling. Woods predicted secondary recovery of83 percent of primary recovery; testing of residual oil in core samples indicates residual oil content of40 percent in water-swept areas (Sabel,1985).

    The southern half of the House Creek field is owned and operated by Kerr-McGee Corp. of Oklahoma, which took over the property from Sonat Exploration Co. in1991 (Lyle,1992). Kerr-McGee adjusted Sonat's3-to-1 line drive water-flood program to a1-to-1 pattern to increase recovery of oil. The1-to-1 pattern has one row of producers for one row of injectors (Lyle,1992). Increase in production will result from minimizing bypass of oil that would have occurred using the3-to-1 pattern because of a more even sweep of injected fluids parallel to field axes. Primary flow unit orientation for the most porous and permeable sandstones is parallel to field axes (Higley,1994). Kerr-McGee will convert28 wells from producers to injectors (Lyle,1992). With the new pattern, Kerr-McGee is planning about15 new wells, including4 injector wells, for a total of130 (Lyle,1992).

    The project is currently a polymer flood and qualifies for tertiary recovery status. Potassium hydroxide (KOH) is added to injected water to decrease swelling of clays and resulting loss of injected water through high-permeability stringers. Clays are primarily kaolinite (0.8 percent based on thin-section analysis) with trace amounts of illite, illite-smectite, and ferroan chlorite (chamosite) minerals. Quartz overgrowths isolate most chlorite from injected fluids. KOH removes oil near well bores thereby increasing formation permeability to injected water (Lyle,1992).

    The following thin-section photomicrograph (figure36, oilstnsm.gif) is an oil-productive, medium-grained trough-cross-bedded sandstone. Oil (dark brown) coats grains and fills voids. The large pore in the upper left quarter of the image is mainly secondary, resulting from dissolution of a (now-absent) probable feldspar (F) grain. This late-stage dissolution resulted in precipitation of kaolinite (K); associated microporosity causes decrease in permeability. The feldspar grain located below the labeled kaolinite exhibits intragranular porosity resulting from grain erosion; this enhances oil emplacement by creating secondary pore spaces. Other grains exhibit peripheral dissolution; this primarily improves permeability by improving interconnections between pores. Kaolinite resulted mainly from late-diagenetic migration of organic acids into the Sussex "B" sandstone and other chemical changes associated with oil generation and migration (Higley,1994). The large pores are void of oil because it drained out during coring and thin-section preparation.

    Figure36. Transmitted-light thin-section photomicrograph of an oil-productive trough-cross-bedded, medium-grained sandstone from the House Creek field. Oil (brown) coats primary and secondary pore spaces. Spotty distribution of oil in the kaolinite (K) results from low permeability and microporosity. Feldspar (F) grain is partially dissolved. Quartz (Q) and chert (CT) grains are labeled. Blue epoxy fills pore spaces (ellipse with a line through it). The full-size photomicrograph is oilstn.gif,1.4 MB .

     

     

    1) East-West-Oriented Vertical Slices of3-D Porosity

    Display images of the field by clicking on highlighted (generally underlined) key words. Alternately, the GIF files (including numerous incremental images that are not listed below) are stored in the ewporosv directory and can be displayed as a slide show using an external viewer, such as JPEGView or LView. Theewporosv.MOV (east-west vertical slices of porosity, single fork) is a14 MB stand-alone movie file located in the movies folder. Movies are called up much quicker directly from the folder than from the below text hook, although the animation speed is similar. Should you have trouble accessing and displaying images, try increasing available memory by closing all unnecessary windows and software programs.

    Technical information on data sources and methodologies is stored in techinfo.htm. Start the movie display of east-west-oriented vertical porosity slices using E-W movie (ewporosv.MOV). Before the movie can be opened, you may need to copy to your hard drive movie-viewing program; information on how to acquire this freeware and software is listed in the readme for movies file.

    Plan view of field area (hslicsmf.gif); north is at the top of the map. Seaward boundaries of sand ridges mark the approximate eastern limits of sandstone bodies that comprise the House Creek field. These boundaries are not labeled on the slices; however, they were used in the3-D computer gridding procedure to confine porosity limits within sand ridges. The subsequent (ssxhome.gif) image is vertical slice12 of the field at the -32,000 m Y-axis location; vertical exaggeration is20 times. Reservoir-grade intervals are shown on the left color bar by green through red (8 to21 percent porosity); low-porosity non-reservoir intervals are purple and blue (1 to8 percent porosity).

     

    West-east- and north-south-oriented vertical slices are spaced at500 m (1,524 ft) intervals. Explanation and index map are included on images. The two color bars represent1) porosity in increments of1 percent and2) contours of40 MBO per well; a barrel of oil is equivalent to42 U.S. gallons (158.76 liters). Vertical exaggeration of the3-D porosity model is40 times.

     

    Top view of field showing location of first slice

    Top view - rotated70 degrees from horizontal

    Top view - rotated45 degrees from horizontal

    Top view - rotated20 degrees from horizontal

    Slice1 - South end of field - Y-Axis slice at -35,500 m

    Slice2 - Y-Axis slice at -34,500 m

    Slice3 - Y-Axis slice at -34,000 m

    Slice4 - Y-Axis slice at -33,500 m

    Slice5 - Y-Axis slice at -33,000 m

    Slice6 - Y-Axis slice at -32,500 m

    Slice7 - Y-Axis slice at -32,000 m

    Slice8 - Y-Axis slice at -31,500 m

    Slice9 - Y-Axis slice at -31,000 m

    Slice10 - Y-Axis slice at -30,500 m

    Slice11 - Y-Axis slice at -30,000 m

    Slice12 - Y-Axis slice at -29,500 m

    Slice13 - Y-Axis slice at -29,000 m

    Slice14 - Y-Axis slice at -28,500 m

    Slice15 - Y-Axis slice at -28,000 m

    Slice16 - Y-Axis slice at -27,500 m

    Slice17 - Y-Axis slice at -27,000 m

    Slice18 - Y-Axis slice at -26,500 m

    Slice19 - Y-Axis slice at -26,000 m

    Slice20 - Y-Axis slice at -25,500 m

    Slice21 - Y-Axis slice at -25,000 m

    Slice22 - Y-Axis slice at -29,000 m

    1. Slice22 starts at slice13 - on the western flank of the field

      Slice23 - Y-Axis slice at -28,500 m

      Slice24 - Y-Axis slice at -28,000 m

      Slice25 - Y-Axis slice at -27,500 m

      Slice26 - Y-Axis slice at -27,000 m

      Slice27 - Y-Axis slice at -26,500 m

      Slice28 - Y-Axis slice at -26,000 m

      Slice29 - Y-Axis slice at -25,500 m

      Slice30 - Y-Axis slice at -25,000 m

      Slice31 - Y-Axis slice at -24,500 m

      Slice32 - Y-Axis slice at -24,000 m

      Slice33 - Y-Axis slice at -23,500 m

      Slice34 - Y-Axis slice at -23,000 m

      Slice35 - Y-Axis slice at -22,500 m

      Slice36 - Y-Axis slice at -22,000 m

      Slice37 - Y-Axis slice at -21,500 m

      Slice38 - Y-Axis slice at -21,000 m

      Slice39 - Y-Axis slice at -20,500 m

      Slice40 - Y-Axis slice at -20,000 m

      Slice41 - Y-Axis slice at -19,500 m

      Slice42 - Y-Axis slice at -19,000 m

      Slice43 - Y-Axis slice at -18,500 m

      Slice44 - Y-Axis slice at -18,000 m

      Slice45 - Y-Axis slice at -17,500 m

      Slice46 - Y-Axis slice at -17,000 m

     

     

    2) North-South-Oriented Vertical Slices of3-D Porosity

    GIF graphic images are stored in the 3dgifns (3-D north-south-oriented GIF files) directory. GIF and TARGA files located in folders are named and numbered such that external viewers can correctly sequence files. Images can be displayed as slide shows using an external viewer, such as JPEGView or LView, or can be accessed as the nsporvf.MOV (north-south vertical porosity slices, single forked) stand-alone movie in the movies folder. Movies are called up much quicker directly from the folder than using the below text hook, although the animation speed is similar.

    Technical information on data sources and methodologies is stored in techinfo.htm. Access and start the movie with north-south movie (nsporvf.MOV). Before the movies can be opened, you may need to copy to your hard drive a movie-viewing program; information on how to acquire this freeware and software is listed in the readme for movies file.

    The above image is north-south-oriented vertical slice7 of the Sussex "B" sandstone (slice7 is located at X-axis location40,000 m on the following index map). The3-D model is rotated clockwise about30 degrees. Yellow dots are borehole and sample locations. The below index plan-view map shows cumulative oil production. Also shown are location and orientation of the slice; these index maps are included on each image. Illustrated on the above map are:

     

    1. Two separate sand ridges that are compartmentalized by low-porosity (blue) mudstone and sandstone, which are the basal low-depositional energy facies of sand ridges,

       

    2. Concentration along the field axis of greatest oil production and thickest intervals of reservoir-grade sandstones (green through red colors,8.5 to21 percent porosity). Greatest oil production is from intervals exhibiting greater than average porosity of reservoir sandstones (yellow through red,12 porosity to21 percent porosity).

       

    3. Landward (to the left) backstepping of the upper over the lower sand ridge, and

       

    4. General lens shape of reservoir-grade intervals and variable thickness of the Sussex "B" sandstone and its components across the field.

    Slide show images north-south-oriented vertical slices are spaced at500-m (1,524 ft) intervals; spacing is approximate on the above map. Explanation and index map are displayed on images. Color bars list porosity in increments of1 percent and contours of40 MBO per well; a barrel of oil is equivalent to42 U.S. gallons (158.76 liters). Vertical exaggeration of the3-D porosity model is60 times.

     

    Slice1) X Axis is43,000 m

    Slice2) X Axis is42,500 m

    Slice3) X Axis is42,000 m

    Slice4) X Axis is41,500 m

    Slice5) X Axis is41,000 m

    Slice6) X Axis is40,500 m

    Slice7) X Axis is40,000 m

    Slice8) X Axis is39,500 m

    Slice9) X Axis is39,000 m

    Slice10) X Axis is38,500 m

    Slice11) X Axis is38,000 m

    Slice12) X Axis is37,500 m

    Slice13) X Axis is37,000 m

    Slice14) X Axis is36,500 m

    Slice15) X Axis is36,000 m

    Slice16) X Axis is35,500 m

    Slice17) X Axis is35,000 m

    Slice18) X Axis is34,500 m

    Slice19) X Axis is34,000 m

    Slice20) X Axis is33,500 m

    Slice21) X Axis is33,000 m

    Slice22) X Axis is32,500 m

    Slice23) X Axis is32,000 m

    Slice24) X Axis is31,500 m

    Slice25) X Axis is31,000 m

    Slice26) X Axis is30,500 m

    Slice27) X Axis is30,000 m

    Slice28) X Axis is29,500 m

    Slice29) X Axis is29,000 m

    Slice30) X Axis is28,500 m

    Slice31) X Axis is28,000 m

    Slice32) X Axis is27,500 m

    Slice33) X Axis is27,000 m

    Slice34) X Axis is26,500 m

     

     

    3)3-D Onion Views - Volumes of Porosity Ranges Across the Field

    Image files are stored in the esid_gif (east side view of the field) directory. GIF images are named and numbered such that external viewers can correctly sequence files in the folders. Images can be displayed as slide shows using an external viewer, such as JPEGView or LView, or can be accessed as thevolporf.MOV (volumetrics of porosity, single fork file format) stand-alone movie in the movies folder.

    Before the movies can be opened, you may need to copy to your hard drive a movie-viewing program; information on how to acquire this freeware and software is listed in the readme for movies file. Due to differences in processing speeds we recommend accessing the standalone movie from the movies folder; however, it can generally be started by clicking 3-D distribution and volumes of porosity in1 to2 percent increments.

     

      • The above Sussex "B" figure is an idealized cross section that slices through three stacked sand ridges. The image shows upward and seaward increase in depositional energy (yellow dotted and green areas) and associated increase in porosity and permeability. The basal wavy line is the horizontal datum for the3-D porosity and permeability models. Wedge shape results from transgressive deposition of sandstone. The (blue) lines are basal and landward low-depositional-energy facies; these exhibit low porosity, permeability, and petroleum production. No vertical or horizontal scales.

    Stripping of layers of porosity in the below images reveals areal distribution, interbedding, and compartmentalization of individual sandstone beds within the Sussex "B" sandstone. Core and borehole porosity data are not smoothed by the gridding process; the wide-spaced X and Y grid spacing results in separate treatment of individual wells. The close-spaced Z grid of about1-ft intervals displays variation in porosity over short vertical distances; this is particularly apparent in the northern half of the field area. Core porosity values change rapidly over short XYZ intervals when compared to well-log porosity data. This results from interbedding of thin porous sandstones with mudstones and calcite-cemented sandstones, and from smoothing of well-log porosity data due to logging procedures and equipment.

    Explanations are included on images; color bars represent porosity distribution in increments of1 percent. Yellow dots are core and borehole sample location in3-D space. Vertical exaggeration of the3-D porosity model is80 times.

    Small-scale3-D view toward the eastern field boundary shows volume and layers of porosity . Minimum reservoir, and average Sussex "B" sandstone porosity is8.5 percent (green); average porosity of reservoir intervals is about13 percent (yellow).

     

    SLIDE SHOW SINGLE IMAGES

    1)1 to21 percent porosity -525.5 million cubic meters. This is the total volume of the reservoir area.

    2)3 to21 percent porosity -524.6 million cubic meters

    3)5 to21 percent porosity -502.5 million cubic meters

    4)6 to21 percent porosity -465.4 million cubic meters

    5)7 to21 percent porosity -415.6 million cubic meters

    6)8 to21 percent porosity -358.6 million cubic meters. Minimum reservoir porosity is about8.5 percent. Eight percent porosity and greater comprises approximately70 percent of the volume of the Sussex "B" sandstone.

    7)9 to21 percent porosity -303.9 million cubic meters

    8)10 to21 percent porosity -241.3 million cubic meters

    9)11 to21 percent porosity -180.5 million cubic meters; or about35 percent of the field area.

    10)12 to21 percent porosity -115.9 million cubic meters; reservoir average porosity is about12.5 percent. Less than25 percent of the field volume is12 percent porosity and greater.

    11)13 to21 percent porosity -62.2 million cubic meters;13 percent and greater is less than15 percent of the field volume.

    12)14 to21 percent porosity -25.9 million cubic meters

    13)15 to21 percent porosity -6.6 million cubic meters

     

     

    4) Horizontal Slices of3-D Porosity - Above the Basal Disconformity

    Table of contents | Glossary | Geology Depositional model | Heterogeneity Diagenetic history | Petroleum geology 1) East-West porosity slices | 2) North-South porosity slices | 3) Onion views of3-D images | Horizontal slices of porosity | 5) Horizontal and East-West permeability and porosity slices

    GIF files are stored in the hslice (horizontal slice) directory and can be displayed as slides using an external viewer, such as JPEGView or LView. GIF files are named and numbered such that external viewers can correctly sequence files in the folders.

    Images are animated by the hporosf.MOV stand-alone movie located in the movies folder. Movies are called up much quicker directly from the folder than from the following text hook, although the animation speed of1 frame/second is analogous. Technical information on the movies, data sources, and research methodology is located in techinfo.htm.

    Top view of field area; north is top of map. Access the movie by clicking Plan-view distribution of porosity (hporosf.MOV). Before the movies can be opened you may need to copy to your hard drive a movie-viewing program; information on how to acquire this freeware and software is listed in the readme for movies file. Due to differences in processing speeds we recommend accessing the stand-alone movie from the movies folder.

     

  • Slide show images - Hslic10a.gif is a top view of the field area showing porosity distribution across the upper disconformity of the Sussex "B" sandstone. Hslic10k through hslic37 are images of the field spaced at1.4-ft (0.43 m) increments above the basal disconformity. Explanation is shown on images; color bars represent porosity in increments of1 percent. Sussex "B" sandstone average porosity, and minimum reservoir porosity, is about8 percent (green). Average porosity of reservoir sandstones is about12 percent (yellow). Horizontal scale is not shown on images.

    1)60 ft - hslic10a.gif - The upper disconformity surface of the Sussex "B" sandstone

    2) Basal view of field - hslic10k.gif - Porosity distribution on the basal disconformity surface (basal sand ridges1 and3) of the Sussex "B" sandstone

    3)1.4 ft above disconformity - hslic10l.gif Patches of reservoir-grade (green through red) porosity are present, mainly along seaward (eastern and southeastern) margins of sand ridges

    4)2.9 ft - hslic10m.gif - Patches begin to coalesce

    5)4.3 ft - hslic10n.gif - Region of reservoir-grade porosity increases in area, although it is still concentrated along the seaward margin of the earliest-deposited sand ridge (number1), located in the southeastern half of the field.

    6)5.7 ft - hslic10o.gif - Areas of reservoir-grade porosity (8 percent and greater) transgress to the southwest, parallel to field and sand-ridge boundaries.

    7)7.1 ft - hslic10p.gif - This and the following images show areal distribution of porosity at each Z-axis increment. Included are1) the continued transgressive deposition of sand ridges, as shown by porosity distribution,2) limited distribution of high porosity intervals (12 percent and greater), and3) compartmentalization of sand ridges resulting from deposition of low-porosity intervals of overlying sand ridges.

    8)8.6 ft - hslic10q.gif

    9)10 ft - hslic10r.gif

    10)11.4 ft - hslic10s.gif

    11)12.9 ft - hslic10t.gif

    12)14.3 ft - hslic10u.gif

    13)15.7 ft - hslic10v.gif

    14)17.1 ft - hslic10w.gif

    15)18.6 ft - hslic10x.gif

    16)20 ft - hslic10y.gif

    17)21.4 ft - hslic10z.gif

    18)22.9 ft - hslic11.gif

    19)24.3 ft - hslic12.gif

    20)25.7 ft - hslic13.gif

    21)27.1 ft - hslic14.gif

    22)28.6 ft - hslic15.gif

    23)30.0 ft - hslic16.gif

    24)31.4 ft - hslic17.gif

    25)32.9 ft - hslic18.gif - This marks the upper surface of sand ridges1 and2, in the southeastern half of the field area.

    26)34.3 ft - hslic19.gif

    27)35.7 ft - hslic20.gif

    28)37.1 ft - hslic21.gif

    29)38.6 ft - hslic22.gif

    30)40.0 ft - hslic23.gif - This marks the approximate upper limit of reservoir-grade sandstones of the uppermost sand ridge.

    31)41.4 ft - hslic24.gif

    32)42.9 ft - hslic25.gif - The small area of reservoir-grade porosity in the northwestern tip of the field area may represent the eastern border of a new sand ridge, based also on examination and mapping of geophysical borehole logs. Thickness and areal distribution of this sandstone bed are not documented due to limited drilling west of the field.

    33)44.3 ft - hslic26.gif

    34)45.7 ft - hslic27.gif

    35)47.1 ft - hslic28.gif

    36)48.6 ft - hslic29.gif

    37)50.0 ft - hslic30.gif

    38)51.4 ft - hslic31.gif

    39)52.9 ft - hslic32.gif

    40)54.3 ft - hslic33.gif

    41)55.7 ft - hslic34.gif

    42)57.1 ft - hslic35.gif

    43)58.6 ft - hslic36.gif

     

     

    5) Vertical and Plan View3-D Permeability Slices

    The two sets of image files included in this section are named:

     

    1. VERTICAL SLICES OF3-D PERMEABILITY
    2. PLAN VIEW SLICES OF3-D PERMEABILITY AND POROSITY

    The following two sets of GIF file lists are stored in the 3dvk (3-D vertical slices of permeability) and hporper (horizontal slices of porosity and permeability) directories. GIF files are named and numbered such that external viewers can correctly sequence files in the folders. Images can be displayed as slide shows using an external viewer, such as JPEGView or LView, or can be accessed as movies; links follow the below figures.

    Before the movies can be opened, you may need to copy to your hard drive a movie-viewing program; information on how to acquire this freeware and software is listed in the readme for movies file. Due to differences in processing speeds we recommend accessing the stand-alone movie from the movies folder.

    3-D permeability images are "smoother" than the3-D porosity models due to fewer data points; core permeability and porosity data from10 boreholes are augmented by well-log porosity data from an additional110 boreholes.

    North-South-Oriented Vertical Slices are spaced at500-m (1,524 ft) intervals and numbered from south to north. Plan-view images are numbered in1-ft (0.3 m) increments from the basal disconformity datum. Explanation and index map are shown on most images. Each slice has two color bars. They are1) variation in permeability in millidarcies (mD), and2) porosity in1-percent increments. Vertical exaggeration of the3-D models is listed on images. Yellow dots are sample locations in boreholes.

    Most vertical slices show two sand ridges separated by zones of lower porosity and permeability. Horizontal slices illustrate;

    1) the highly variable distribution of porosity and permeability in three dimensions,

    2) concentration of lowest porosity/permeability zones proximal to the basal disconformity and the western field margins,

    3) general upward and seaward increase in porosity and permeability within individual sand ridges, with

    4) stacking of greatest porosity/permeability along field axes that resulted from transgressive deposition (westward) of later sand ridges.

    Small-scale example of an east-west-oriented vertical slice of permeability across the field. The movie shows east-west vertical slices of permeability distribution.ewpermvf.MOV

    Small-scale plan-view images of permeability and porosity across the northwestern half of the field area. The movie shows plan-view distribution of permeability and porosity. hporperf.MOV .

     

     

    VERTICAL SLICES OF3-D PERMEABILITY

     

    Slice1) Y Axis at -26,500 m - permv11.gif 
      1. Southern extent of the3-D permeability model showing location of first slice

    Slice2) Y Axis at -26,000 m - permv12.gif

    Slice3) Y Axis at -25,500 m - permv13.gif

    Slice4) Y Axis at -25,000 m - permv14.gif

    Slice5) Y Axis at -24,500 m - permv15.gif

    Slice6) Y Axis at -24,000 m - permv16.gif

    Slice7) Y Axis at -23,500 m - permv17.gif

    Slice8) Y Axis at -23,000 m - permv18.gif

    Slice9) Y Axis at -22,500 m - permv19.gif

    Slice10) Y Axis at -22,000 m - permv20.gif

    Slice11) Y Axis at -21,500 m - permv21.gif

    Slice12) Y Axis at -21,000 m - permv22.gif

    Slice13) Y Axis at -20,500 m - permv23.gif

    Slice14) Y Axis at -20,000 m - permv24.gif

    Slice15) Y Axis at -19,500 m - permv25.gif

    Slice16) Y Axis at -19,000 m - permv26.gif

    Slice17) Y Axis at -18,500 m - permv27.gif

    Slice18) Y Axis at -18,000 m - permv28.gif

    Slice19) Y Axis at -17,500 m - permv29.gif

    Slice20) Y Axis at -17,000 m - permv30.gif

    Slice21) Y Axis at -16,500 m - permv31.gif

     

     

    PLAN VIEW SLICES OF3-D PERMEABILITY AND POROSITY

     

    .1)0 ft above basal disconformity - porper11.gif

    .2)1 ft above basal disconformity - porper12.gif

    .3)2 ft above basal disconformity - porper13.gif

    .4)3 ft above basal disconformity - porper14.gif

    .5)4 ft above basal disconformity - porper15.gif

    .6)5 ft above basal disconformity - porper16.gif

    .7)6 ft above basal disconformity - porper17.gif

    .8)7 ft above basal disconformity - porper18.gif

    .9)8 ft above basal disconformity - porper19.gif

    10)9 ft above basal disconformity - porper20.gif

    11)10 ft above basal disconformity - porper21.gif

    12)11 ft above basal disconformity - porper22.gif

    13)12 ft above basal disconformity - porper23.gif

    14)13 ft above basal disconformity - porper24.gif

    15)14 ft above basal disconformity - porper25.gif

    16)15 ft above basal disconformity - porper26.gif

    17)16 ft above basal disconformity - porper27.gif

    18)17 ft above basal disconformity - porper28.gif

    19)18 ft above basal disconformity - porper29.gif

    20)19 ft above basal disconformity - porper30.gif

    21)20 ft above basal disconformity - porper31.gif

    22)21 ft above basal disconformity - porper32.gif

    23)22 ft above basal disconformity - porper33.gif

    24)23 ft above basal disconformity - porper34.gif

    25)24 ft above basal disconformity - porper35.gif

    26)25 ft above basal disconformity - porper36.gif

    27)26 ft above basal disconformity - porper37.gif

    28)27 ft above basal disconformity - porper38.gif

    29)28 ft above basal disconformity - porper39.gif

    30)29 ft above basal disconformity - porper40.gif

    31)30 ft above basal disconformity - porper41.gif

    32)31 ft above basal disconformity - porper42.gif

    33)32 ft above basal disconformity - porper43.gif

    34)33 ft above basal disconformity - porper44.gif

    35)34 ft above basal disconformity - porper45.gif

    36)35 ft above basal disconformity - porper46.gif

    37)36 ft above basal disconformity - porper47.gif

    38)37 ft above basal disconformity - porper48.gif

    39)38 ft above basal disconformity - porper49.gif

    40)39 ft above basal disconformity - porper50.gif

    41)40 ft above basal disconformity - porper51.gif

    42)41 ft above basal disconformity - porper52.gif

    43)42 ft above basal disconformity - porper53.gif

    44)43 ft above basal disconformity - porper54.gif

    45)44 ft above basal disconformity - porper55.gif

    46)45 ft above basal disconformity - porper56.gif

    47)46 ft above basal disconformity - porper57.gif

    48)47 ft above basal disconformity - porper58.gif

    49)48 ft above basal disconformity - porper59.gif

    50)49 ft above basal disconformity - porper60.gif

    51)50 ft above basal disconformity - porper61.gif

    52)51 ft above basal disconformity - porper62.gif

    53)52 ft above basal disconformity - porper63.gif

    54)53 ft above basal disconformity - porper64.gif

    55)54 ft above basal disconformity - porper65.gif

    56)55 ft above basal disconformity - porper66.gif

     

     

    U.S. GEOLOGICAL SURVEY DIGITAL DATA SERIES DDS-33   3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00

     

     

    SELECTED REFERENCES

     

    Aigner, T., and Reineck, H.E.,1982, Proximity trends in modern storm sands from the Helgoland Bight (North Sea) and their implications for basin analysis: Senckenberg. Marit., v.14, p.183-215.

    Allen, P.A., and Homewood, P.,1984, Evolution and mechanics of a Miocene tidal sandwave: Sedimentology, v.31, p.63-81.

    Anderman, G.G.,1976, Sussex sandstone production, Triangle U field, Campbell County, Wyoming: Wyoming Geological Association,28th Annual Field Conference Guidebook, p.107-113.

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    Van Wagoner, J.C., Posamentier, H.W., Mitchum, R.M., Vail, P.R., Sarg, J.F., Loutit, T.S., and Hardenbol, J.,1988, An overview of the fundamentals of sequence stratigraphy and key definitions, in Wilgus, C.K., Hastines, B.S., Posamentier, H., and others, eds., Sea-Level Changes: An Integrated Approach: Society of Economic Paleontologists and Mineralogists Special Publication no.42, p.39-46.

    Walker, R.G.,1985, Comparison of shelf environments and deep-basin turbidite systems, in Tillman, R.W., Swift, D.J.P., and Walker, R.G., eds., Shelf Sands and Sandstone Reservoirs: Society of Economic Paleontologists and Mineralogists Short Course Notes no.13, p.465-502.

    Walker, R.G., and Bergman, K.M.,1993, Shannon Sandstone in Wyoming: a shelf-ridge complex reinterpreted as lowstand shoreface deposits: Journal of Sedimentary Petrology, v.63, p.839-851.

    Walker, T.R.,1984,1984 SEPM presidential address: diagenetic albitization of potassium feldspar in arkosic sandstones: Journal of Sedimentary Petrology, v.54, p.3-16.

    Waples, D.W.,1985, Geochemistry in petroleum exploration: Boston, International Human Resources Development Corporation,232 p.

    Weber, K.J.,1986, How heterogeneity affects oil recovery, in Lake, L.W., and Carroll, Jr., H.B., eds., Reservoir Characterization: New York, Academic Press, p.487-544.

    Weimer, R.J.,1983, Relation of unconformities, tectonics, and sea level changes, Cretaceous of the Denver Basin and adjacent areas, in Reynolds, M.W., and Dolly, E.D., eds., Mesozoic Paleogeography of the West-Central United States: Society of Economic Paleontologists and Mineralogists, Rocky Mountain Paleogeography Symposium2, p.359-376.

    _________1984, Relation of unconformities, tectonics, and sea-level changes, Cretaceous of Western Interior, USA, in Schlee, J. S., ed., Interregional Unconformities and Hydrocarbon Accumulations: American Association of Petroleum Geologists Memoir36, p.7-35.

    ________1992, Developments in sequence stratigraphy: foreland and cratonic basins: American Association of Petroleum Geologists Bulletin, v.76, no.5, p.965-982.

    Weimer, R. J., and Flexer, A.,1985, Depositional patterns and unconformities, Upper Cretaceous, eastern Powder River basin, Wyoming, in Nelson, G. E., ed., The Cretaceous Geology of Wyoming: Wyoming Geological Association36th Annual Field Conference Guidebook, p.131-147.

    Wilson, T.V., and Sibley, D.F.,1978, Pressure solution and porosity reduction in shallow buried quartz arenite: American Association of Petroleum Geologists Bulletin, v.62, no.11, p.2,329-2,334.

    Witzke, B.J., Ludvigson, G.A., Poppe, J.R., and Ravn, R.L.,1983, Cretaceous paleogeography along the eastern margin of the Western Interior seaway, Iowa, southern Minnesota, and eastern Nebraska and North Dakota, in Reynolds, M.W., and Dolly, E.D., eds., Mesozoic Paleogeography of the West-Central United States: Society of Economic Paleontologists and Mineralogists, Rocky Mountain Paleogeography Symposium2, p.225-252.

     

     

     

    Glossary -3-D Characterization of the House Creek Oil Field AuthigenicGenerated or formed in place. Specifically used with rock minerals and other constituents that were derived locally, and of minerals that precipitated at the same time, or subsequent, to the rock in which they are found.ASCII (American Standard Code for Information Interchange)A standard format for storing and transmitting data. American Standard Code for Information Interchange. A set of binary numbers that represent the alphabet, punctuation, numbers, and symbols that are used for text and communication protocols.BinaryA file format consisting of machine-readable executable code or binary data, as opposed to ASCII text files.BinHexA file conversion format that converts binary files to ASCII text files.BiostratigraphyAges, differentiation, and correlation of rock intervals based on the study of contained fossils.BioturbatedSediment that has been extensively reworked by worms, crustaceans, or other organisms. Burrows and other evidence of reworking are commonly minor due to the biologic activity.BugCommonly indicates a software or other computer-based error.Case sensitiveRefers to upper and lower case letters. UNIX is case sensitive, meaning that names of document links and file names must be identical. A program accessing "Cat.GIF" would not find the same file were it named "cat.GIF."ConcretionA hard round, oval, or other-shaped of mass of mineral or aggregate matter of varying sizes. Commonly forms by chemical precipitation around a nucleus or center, or replacement of precursor organic or inorganic material. An example is siderite (iron, calcium carbonate) concretions.DetritalFormed from detritus of preexisting rock. This is particularly for rocks, minerals, and sediments composed of precursor components.DiachronousA single rock unit that exhibits varying ages in different areas. A sedimentary formation, such as marine sands, that formed during transgression or regression of the shoreline, being progressively younger in the direction that the sea level is moving.DiagenesisChanges that influence sediments after deposition. These include compaction, cementation, and chemical alteration, dissolution, and precipitation of constituents. Excluded are surficial weathering, and metamorphism of preexisting sediments.DissolutionA void space or cavity in or between rocks that resulted from solution of part of the rock material.Document windowScrollable Mosaic or other WWW browser windows in which documents, slide shows, and movies are viewed.File Transfer Protocol (FTP)File Transfer Protocol is commonly used to transfer files from one computer platform to another.Flow unitIn petroleum geology, reservoir zones that exhibit similar fluid flow, porosity/permeability, reservoir potential, and production characteristics. The flow-unit definition includes a "volume of rock subdivided according to geological and petrophysical properties that influence the flow of fluids through it" (Ebanks,1987).FolderDirectory, sub-directory, and folder are used interchangeably to show addresses of files on this CD-ROM.FramboidA microscopic aggregate of pyrite crystals; these are often in spheroidal clusters, the form of which resembles raspberries.FTP (File Transfer Protocol)File Transfer Protocol is commonly used to transfer files from one computer platform to another.GIF (Graphics Interchange Format)GIF is a graphics file, commonly with the .gif or .GIF ending. The acronym refers to the Graphics Interchange format developed by CompuServe, Inc. This graphics format is used on numerous computer platforms and systems. GIF files can be for inline and movie images.HeterogeneityThe state or quality of being nonuniform, having dissimilar elements, not homogeneous. For example, a unit composed of interbedded thin- and thick-bedded sandstones and mudstones is heterogeneous.Home pageThe initial screen or graphic image in which links to related information are listed. A document that the user specifies for Mosaic or other network browsing software to display, commonly when the Mosaic program is started.HTML (Hypertext Markup Language)Acronym for Hypertext Markup Language. HTML files on this CD ROM follow the8.3 PC/DOS format. This file, for example, is named glossary.htm.ImageRefers to still image data. Subtypes recognized by graphics programs include JPEG, GIF, RGB, TAR, TIFF, X-PICT (PICT), X-XBM (X bitmap image), and other formats.JPEG (Joint Photographic Experts Group)Acronym for Joint Photographic Experts Group, an image-compression format used to transfer color images over computer networks.Laminar bedding1) Finest stratification of shale or fine-grained sandstone bedding,2) thin alternating layers of differing composition, and3) laminae, such as in shale, that can be split into thin layers.Laramide orogenyA time of regional deformation, commonly recorded across the eastern Rocky Mountains of the United States. Orogenic phases extended from Late Cretaceous until the end of Paleocene or Eocene time. To simplify, this was a period of mountain building and emplacement of igneous intrusives and mineral ore deposits.MeniscalThe curved upper surface of a nonturbulent liquid in a container. A crescent-shaped body. A concavo-convex lens.Minus-cement porosityThe percent volume of void space in a rock, added with volume of cements and other post-depositional pore-filling compounds. This is used as an estimate of porosity during the time of deposition of the rock.MosaicA World Wide Web (WWW) multimedia browser developed at the National Center for Supercomputing Applications at the University of Illinois, Urbana-Champaign. Versions are available for the Mac, PC, PC Windows, and X Windows.MOVFile type of a single-forked stand-alone QuickTime movie. The hporperf.MOV movie located in the movie directory of this CD ROM, for example, is designed to run on Macintosh and PC/Windows platforms.MPG, MPEG, CMPEGMoving Pictures Expert Group movie file type used primarily for PC/DOS and UNIX platforms. Special viewing applications are required to run MPG movies on your computer.NCSANational Center for Supercomputing Applications at the University of Illinois, Urbana-Champaign.OvergrowthSecondary material precipitated around a crystal grain of the same composition. Both grain and cement are in optical and crystallographic continuity.ParagenesisA sequential order of rock alteration, such as, compaction, precipitation of minerals, dissolution of grains and cements, and similar processes.PermeabilityThe capacity or ability of a porous medium, such as rock or soil, to transmit fluid; the rate of diffusion of a fluid under unequal pressure. The common unit of measure is the millidarcy (mD).Planar beddedLying or arranged in approximately parallel planes. Bedding in which the lower surface is a beveled erosional contact; cross bedding is characterized by planar foreset beds.PoikilotopicA fabric of recrystalized carbonate cements or rocks. Constituent crystals are varying sizes and commonly enclose smaller crystals of other minerals.PorosityThe percentage of bulk volume of a rock or other object that is occupied by void space, whether isolated or connected. Porosity is further subdivided into effective (or connected) pores, primary, secondary, and minus-cement categories. Primary porosity includes all depositional pore spaces; secondary porosity records the volume of void space resulting from dissolution and (or) fracturing of the rock or sediment. Minus-cement porosity category combines intergranular primary porosity and secondary porosity, in addition to authigenic cements and clays, as an estimate of the amount of porosity at the time of lithification; porosity resulting from intragranular dissolution is excludedQuickTimeA digital video standard developed by Apple Computer for PC/Windows and Apple computers. The QuickTime extension file is inserted into the Apple System Folder, and special viewing applications are required to view QuickTime "movies."Range1) Any series of contiguous townships of the U.S. Public Land Survey system. These are aligned parallel to a principal meridian and numbered consecutively in an east-west direction from the meridian.2) mountain range.3) The numerical difference between a series highest and lowest values.4) stratigraphic range.5) A geographic area over which an organism or group of organisms is located.RavinementA break in sedimentation resulting primarily from erosion. An example is a disconformity resulting from marine transgression and erosion of precursor sediments. Formation of a gully or ravine.RadiometryMethods of calculating an age for geologic materials by measuring the amounts of short-half-life radioactive elements, such as carbon-14, or of long-half-life radioactive elements plus their decay products, such as potassium-40/argon-40.Regression(Simply) The local or widespread retreat of seas from land surfaces and resulting changes in erosion and depositional patterns of strata.SEA (Self-Extracting Archive)Self-extracting archive (SEA). These compressed files contain one or more files and (or) programs. SEA s are generally decompressed by double-clicking on the name or icon. Further instructions are given during the decompression process.Secondary porosityPorosity developed in a rock subsequent to its emplacement or deposition. Processes are mostly dissolution of grains, cements, and other constituents due to changes in pressure and (or) pore-fluid composition.Section1) One of the36 units that subdivides a township. It is a piece of land that is generally one mile square.2) An exposed vertical or inclined surface, such as a cliff or quarry face.3) geologic term used for a columnar section, type section or thin section..sitThis ending on a file type indicates it has been compressed with Stuffit software. Stuffit Expander is used by Mosaic to decompress the file.TGA (TARGA)TARGA image file format; this commonly has a .tga or .TGA ending.TIFF (Tagged Image File Format)Acronym for Tagged Image File Format, a graphic file format developed by Aldus and Microsoft. TIFF is used as an image transfer format on computer networks.Transgression(Simply) The advance or spread of seas over land surfaces which cause changes in erosion and depositional patterns of marine and non-marine strata.Tabular cross beddingCross-bedded units that are bounded by planar, essentially parallel, surfaces to form tabular sandstone bodies.TownshipA unit of survey of the U.S. Public Land Survey. It is an area bounded on the east and west by meridians located about6 miles apart. A township is normally a square that is subdivided into36 sections, each of which are approximately1 mile square. Township, range, and section locations are shown on most topographic maps, for example.Trough cross beddingCross-bedding in which the lower surfaces are curved erosional contacts which result from scour and subsequent deposition.URL (Uniform Resource Locator)The acronym stands for Uniform Resource Locator, the addressing standard on the WWW. The URL contains information about the location, method of access, and path of files to be viewed.World Wide Web (WWW)The hypermedia document network system, abbreviated as WWW. WWW can be accessed over the Internet using Web browser software, such as Mosaic or Netscape.

     

     

    Table of contents | Glossary | Acknowledgments | Geology Depositional model | Heterogeneity Diagenetic history | Petroleum geology 1) East-West porosity slices | 2) North-South porosity slices | 3) Onion views of3-D images | 4) Horizontal slices of porosity | 5) Horizontal and East-West permeability and porosity slices | Technical information

     

      ACKNOWLEDGMENTS

    This research was supported by the following U.S. Geological Survey projects; Enhanced Oil Recovery, Reservoir Characterization, Graduate Intern, and3-D Reservoir/Basin Characterization for CD-ROM Publication. Many individuals and organizations contributed greatly to this publication. We wish to thank all of you for your technical advice, donation of time, data, and equipment, and for your assistance.

    Woods Petroleum and Meridian Oil Corporations donated reservoir and core analysis data. We would like to thank Steve Fillingham, Dick Morrow, and Bill Walford of Woods Petroleum Corp., and William Brown and Oscar Peters of Meridian Oil for their assistance. Kerr-McGee Corporation scientist John Roffers added information on secondary recovery operations. U.S. Geological Survey geologists Mark Pawlewicz and Thomas Finn provided vitrinite reflectance and X-ray diffraction analyses, respectively.

    We thank Ronald Charpentier, Ronald Johnson, Randy Schumann, Rick Scott, and Steve Sonnenberg for their reviews. Frederick (Nick) Zihlman and Randy Schumann, of the USGS, gave valuable advice on incorporation and use of WWW and other computer applications, and on producing CD ROMs. David K. Vaughan assisted in collecting porosity and permeability data and in constructing the2-D and3-D map models. Fran Gay did a superb job of scanning photographs and saving digital images.

    Numerous individuals, software companies, AAPG, SEPM, and NCSA have allowed us to install their shareware, freeware, and postcardware computer programs on this CD-ROM. We would like to thank all of you. Highlighted links are GIF-format-scanned copies of license agreements and copyright releases. A list, in no particular order, of contributors and their software programs follows:

     

    Thank you all for your contributions, /s/ Debra Higley <;

     

     

      3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00

     

      TECHNICAL INFORMATION

    INCLUDED IN THIS SECTION ARE THE FOLLOWING;

     

     

    SOURCES OF DATA

    Sources of information include published reports, core and outcrop studies, geochemical analyses of crude oil and core samples, core analyses, petroleum reserve and production data, and well data. The Sussex Sandstone core used in this study is located at the U.S. Geological Survey (USGS) core library in Denver (Higley,1988) and at the Colorado School of Mines in Golden, Colorado. Sources of field and well production data include Petroleum Information Corporation's (PI) production data on CD-ROM and Well History Control System databases; unless otherwise stated, data are current approximately through July1993. Meridian Oil Company and Woods Petroleum Corporation provided core analysis and reservoir production and statistical data. Our geologic and geochemical analyses was augmented by other sources of information; these include Kerr-McGee Corp., Woods Petroleum Corp., Meridian Oil, Petroleum Information Corp., and State of Wyoming Oil and Gas Conservation Commission.

     

    COMPUTER MAPPING AND STATISTICAL METHODOLOGY

    Microsoft Excel, DeltaGraph, and Canvas statistical and graphics programs on Macintosh computers were used to generate most of the charts and graphs used in figures. Statistical and graphical distributions of results from thin-section petrographic analyses and well-log and core-porosity and core-permeability data were calculated using Statistical Applications Software (SAS) on a VAX computer, and Microsoft Excel and DeltaGraph programs on Macintosh computers.

    Generated maps primarily cover the southern two-thirds of the House Creek field, although geology, geochemistry, and petroleum potential of the entire field was researched. EarthVision (EV) version2.02 program on an IRIS workstation was used to generate contour maps and the3-D maps illustrating porosity and permeability distribution across the field. The mapping package is owned by Dynamic Graphics Corporation, Berkeley, Calif. The IRIS workstation had32 MB of memory and operating system5.3.

    The3-D maps of core and well-log porosity represent an area of105.28 to105.42 degrees longitude (X-axis grid dimensions of25,000 to43,000 m) and43.4 to43.5 degrees latitude (Y-axis grid dimensions of -16,000 to -35,000 m). Permeability data were derived from core analyses; data distribution are within about105.5 to105.6 degrees longitude (X-axis grid dimensions of26,500 to33,000 m) and43.7 to43.8 degrees latitude (Y-axis grid dimensions of -28,000 to -16,000 m). All data set references include only approximate X-Y coordinates; actual well locations are slightly different.

    The porosity/permeability and other geologic data sets created for this study were gridded by the EarthVision mapping programs using a biharmonic cubic spline algorithm that distributes tension among the grid nodes. Contour curvature is distributed rather than concentrated at nodes. Generated isopach, structure, and other contour maps display this curvature, as opposed to jagged contour lines. Most maps use a closely spaced grid with one to a maximum of eight data points (wells) evaluated from each grid node; these parameters display anomalies and wide variations on the maps, as opposed to smoothing data.3-D maps utilize single-data-point gridding to minimize extrapolation. Using these contour parameters, map features are sometimes exaggerated; this can result in mammiform (essentially bull's-eye) contours when adjacent or proximal wells have widely different data values.

    Vertical slices through the field show dispersal of permeability and porosity; slices were chosen based on3-D distribution of core data and well control. Most figures exhibit, and include, considerable Z-axis exaggeration; the purpose is to better show porosity and permeability distribution within the Sussex. Vertical exaggeration is listed on figures. The exaggeration results in a greatly increased upward and shoreward (westward) step in sand-ridge unit (sandstone bed) boundaries. Actual boundaries are at a much lower angle.

    3-D models of porosity respective grid spacings were100 by100 cells (200 by200 m), and250 by250 cells (85 by85 m) in the X-Y (east-west, and north-south) directions, and50 cells (1.5 ft) in the Z (depth) dimension; movie images were gridded using the closer (250 by250) cell spacing so animations would flow better. Permeability was gridded using a30 by30 grid cells in the X-Y direction and50 grid cells in the Z direction; the smaller X-Y grid spacing results from the smaller areal extent of this3-D data. The Z spacing grid nodes represent increments of about1.5 ft (0.5 m) for the interval from10 ft (3.5 m) below the Sussex "B" base to65 ft (20 m) above it. A closer grid was not practical because of the EV program parameters. The X-Y-Z grid parameters were chosen in order to treat porosity/depth values for each well separately. The purpose of this is to better see variation in porosity in3-D space, and to evaluate the effects of lateral permeability boundaries on the distribution of porosity. These permeability boundaries are located between individual reservoir sand ridges. They also bound the Sussex "B" sandstone interval.

    The *.RGB image files generated using EarthVision were converted on the IRIS workstation into *.GIF (Graphic Interchange Format) and *.TGA (TARGA) files. These graphics files were then downloaded onto Macintosh and PC computers. GraphicConverter version2.1.3 shareware on a Macintosh was used to generate the movies. Each GIF file folder was opened using the "convert all," command located under the file menu banner. Next, "select folder" and "convert" were selected. Movies were saved using640 X and430 Y pixels (movie width and height) and256 colors (8 bit). Selected compression settings were highest quality, and1 frame per second display time (for most of the movies). Movies were opened using Apple Computer, Inc., MoviePlayer version2.0b2 software and saved as single-forked stand-alones.

     

    GEOLOGIC METHODS OF ANALYSIS

    Outcrops of Sussex and Shannon Sandstones in the Salt Creek anticline area and Shannon Sandstone outcrops west of the anticline were examined and described. Due to the poor quality of Sussex outcrops, Shannon Sandstone outcrops were used as analogs to the Sussex and to depositional processes in the Cretaceous epicontinental seaway. Outcrops west of the Salt Creek anticline, just east of Shepperson Ranch, were also studied. The outcrops locations, shown with a blue rectangle on the following (indexfs3.gif) index map, are near Edgerton and Midwest, Wyoming, northeastern Natrona county in townships39 and40 north and ranges78 through80 west.

    Figure1. Structure contour map on the top of the Upper Cretaceous Sussex Sandstone Member of the Cody Shale, and approximate age equivalents, Powder River Basin, Wyoming and Montana. Location of the House Creek field is shown. Areal extent of the Sussex "B" sandstones is delineated by black-colored fields. Shaded fill outlining the basin are outcrops of Lance Formation and Fox Hills Sandstone. The rectangle located next to the30-mile scale bar defines the area of studied outcrops of the Sussex and Shannon Members, much of the Salt Creek anticline, Shepparson Ranch, and the towns of Midwest and Edgerton. Contour interval is500 ft. Datum is mean sea level.

     

    The Sussex Sandstone outcrops northwest of Edgerton, Wyoming, and along the northeastern flank of the Salt Creek anticline. Largely because of Pleistocene and present-day erosion, the uppermost sandstones of the Sussex are commonly missing (Brenner,1979). These missing intervals probably include the trough-cross-bedded sandstones that are the primary reservoir facies in the House Creek field. Exposed in outcrop are coarsening-upward sections of laminated mudstones to fine- to medium-grained sandstones. These thin-bedded sandstone facies have lower reservoir favorability.

    Facies assignments were determined from outcrop and core studies and by correlation of lithologic data to geophysical well logs. Sussex "B" core from20 wells were examined. Descriptions in Higley (1992,1994) include sedimentary structures, changes in depositional energy, grain-size distributions, degree and types of biologic activity, trace-fossil assemblages, generalized amounts of calcite and quartz cements, and presence of clasts of chert, glauconite, and siderite.

    Depths to the top and base of the Sussex "B" sandstone and of the sand ridges (sandstone bed) that comprise it were determined from outcrop, core, petrologic, geochemical, well-log, and published sources. Depths to the Ardmore bentonite, and to the top and base of the Sussex Sandstone Member and included Sussex "B" sandstone were picked from well-logs of more than620 wells within, west of, and slightly east of the House Creek field. These depths were added to a digital data file that also included American Petroleum Institute (API) number, well name, operator name, well location, and well symbol (oil producing, dry hole, etc.), total drill depth, producing formation, and completion year. Also added to the well file were depths to boundaries of major Sussex "B" sandstone flow units, as determined for about120 wells in the field (Higley,1994). Flow units are strata that exhibit similar fluid-flow characteristics. Examples are thick, trough-cross-bedded, medium-grained sandstones, and low-porosity, non-oil-productive shales. Porosity, permeability, formation and sand ridge tops, and other data are explained in the dreadme.htm file for the three data sets located in the data_set folder. Included files are named ssxporos.dat, corepor.dat, and ssxtops.dat.

     

    PETROLOGIC/GEOCHEMICAL METHODS OF ANALYSIS

    Cores from10 wells located in and near the House Creek and Porcupine oil fields were sampled for petrographic analysis. Thin sections of54 samples, X-ray diffraction (XRD) analyses, cathodoluminescence, and scanning electron microscope (SEM) studies were used to determine reservoir paragenesis, sandstone porosity, and mineralogical constituents of the Sussex "B" sandstone in the study area. Results of the petrographic analyses are presented in Higley (1992,1994) and listed in table2 (below).

    Cathodoluminesence analysis was used to evaluate early diagenetic events not visible with standard petrographic procedures. Calcite-cemented sandstones and chert-pebble sandstones were sampled. Locations of calcite-cemented facies were chosen based on core and thin-section examination. Specially prepared30-micrometer-thick thin sections for the cathodoluminesence studies were polished at low temperature and contain no epoxy or stains. We used a Technosyn Mark II cathodoluminescence stage with10-15 Kv beam potential and400-500 microampere beam current. The thin-section vacuum stage operated at range of50-100 millitorr. Samples were viewed through a Nikon Optiphot microscope fitted with8X oculars and a4X (0.12 numbered aperture) objective.

    Scanning electron microscope (SEM) examination of core samples determined mineralogical constituents, diagenetic history, shapes of pores, and petrologic characteristics of Sussex "B" sandstone, mudstone, and siderite core samples. SEM and other petrologic data are included in Higley (1992,1994).

     

    PETROPHYSICAL METHODS OF ANALYSIS

    The Ardmore bentonite through Sussex "B" sandstone interval was correlated by linking well log traces for120 wells. Traces include gamma, spontaneous potential (SP), resistivity, and bulk density. Steve Fillingham of Woods Petroleum Corp. (1985, personal communication), identified a10 MV SP deflection to define the gross sandstone interval; this was also noted in this study as a boundary between reservoir-grade sandstone beds, and non-reservoir mudstones and cemented sandstones. This boundary is also characterized by a rapid decrease in core and well-log porosity. The boundary occurs at approximately8.5 percent porosity, although this varies somewhat based on interbedding characteristics of mudstone/sandstone beds.

    Sussex Sandstone core porosity and permeability data for as many as30 wells in the area are included in the data_set porosity database and the2-D and3-D map images. Thirteen of these wells are within the field boundaries; well locations are shown below. Porosity values were calculated from bulk density well-log traces for approximately100 wells. Sonic log traces were used for porosity calculations for a few wells.

    Permeability baffles and barriers between stacked sandstones are characterized on well logs by sonic and bulk-density "spikes" of low porosity, variable gamma signatures that indicate shale breaks, and irregular spontaneous potential and resistivity traces that show stacked thin sandstones with intervening breaks. Limitations to the model include incomplete knowledge of reservoir heterogeneity, including information on fault and fracture systems, on continuity of small-scale permeability baffles such as shales and cemented sandstones, and permeability of porous facies and zones for which there are few core analogs.

    Porosity was calibrated to a specific grain density of2.68 g/cm3; this approximates average grain densities determined from the core analyses and estimated from thin-section examinations. Field outlines and sedimentologic boundaries were based on published information, well-log correlations, porosity and permeability profiles, oil-productive characteristics, location of sandstone and shale beds within the ridge system, and on core and outcrop studies.

     

    Thin-section petrographic data - Explanation of spreadsheet data

    Table1 shows names and locations of cored wells that were used in thin-section petrographic and other studies; depth to the top of the Sussex "B" sandstone is also listed. Table2 has volume percent of detrital grains, cements, and porosity for55 thin sections of Sussex "B" sandstone core samples from10 boreholes. Table2 is also saved as the tab-delimited ssxtabl2.txt file because each web-browsing program displays (or dissects) tables differently. Porosity and mineralogical determinations were derived using approximately300 point counts of each thin section. Thin sections were stained for calcite, potassium feldspar, plagioclase, and iron. Blue epoxy fills pore spaces. Minus-cement porosity (MCP) column includes volume percentages of chlorite, kaolinite, and pyrite, added to amounts of chert, quartz, calcite, dolomite, and feldspar cements. MCP is an estimate of porosity at the time of lithification. Photomicrographs for many thin sections are included in the geology text section of this publication.

     

     

    TABLE1

    Names and locations of wells in Campbell County, Wyoming, in which core was sampled for petrographic analysis of the Sussex "B" sandstone, Sussex Sandstone Member of the Upper Cretaceous Cody Shale. Locations are section, township, and range (glossary). An asterisk (*) marks the estimated core depth to the top of the Sussex "B" sandstone; other depths are actual core depths. 

      Well Name Location, Top Depth (ft.) 14-9 Federal 9, T.42 N., R.71 W. 7,781 1 Campbell 21, T.42 N., R.71 W. 7,700 1 Govt. Miles "A" 9, T.44 N., R.73 W. 8,189 1 Mandel Federal 22, T.44 N., R.73 W. 8,166 1-23 House Creek Fed. 23, T.44 N., R.73 W. 8,238 1 Empire-Federal "C" 29, T.45 N., R.73 W. 8,006 32-1 Marquiss "B" 32, T.45 N., R.73 W. 7,980 1 House Creek Fed. 13, T.45 N., R.74 W. 8,175 1-11 Red Unit 26, T.48 N., R.79 W. 9,028* Ucross State 11, T.52 N., R.81 W. 8,233*

     

     

    TABLE2

    Thin-section point-count data for Sussex "B" sandstone facies. Facies definitions use those of Tillman and Martinsen (1985). Data are average volume percentages for number (N) of thin-sections listed; Q, quartz grains; PQ, polycrystalline quartz; FSP, feldspar grains; RF, rock fragments; GL, glauconite; MM mudstone matrix; MC, clay matrix; MS, mudstone drapes; SID, siderite drapes; PY, pyrite; CHL, chlorite; QC, quartz cement; CT, chert cement; FSP, feldspar cement; CA, calcite cement; KA, kaolinite booklets; PO, porosity; MCP, minus-cement porosity. Sedimentary facies are listed under column nameFACIE for the entire data set (ALL), upper chert-pebble lag sandstone (CTSS), central ridge sandstone (CRSS), high- and low-energy ridge-margin sandstones (HRMS, LRMS), wavy-bedded sandstone (WBSS), and inter-ridge sandstone (IRSS) and siltstone (IRST) (Higley,1992,1994). 

    FACIE N Q PQ FSP RF GL MM MC MS SID PY CHL QC CT FSP CA KA PO MCP -------------------------------------------------------------------------------------------------------------------- ALL.54312.96.3135.13.05.91.80.90.60.97.72.11.511.0.85.430 -------------------------------------------------------------------------------------------------------------------- CTSS03270.83.5363.00.02.10.00.00.20.01.90.00.221.0.01.625

    CRSS17322.95.7144.70.73.92.12.90.30.88.52.11.39.50.47.731

    HRMS08302.77.1115.52.83.81.20.11.31.38.52.21.614.0.56.136

    LRMS03273.18.5126.71.47.61.20.81.01.111.1.93.89.70.92.432

    WBSS06322.16.9106.93.25.10.00.00.41.87.92.22.212.1.65.934

    IRSS10312.87.4115.53.37.23.20.20.70.78.32.21.58.51.35.429

    IRST07332.35.3103.410.13.3.30.20.60.64.52.60.76.80.62.119

     

     

    U.S. GEOLOGICAL SURVEY DIGITAL DATA SERIES DDS-33   3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00

     

    FORMATS AND EXPLANATIONS FOR SSXTOPS.DAT, SSXPOROS.DAT,COREPOR.DAT AND FLDOUTLN.PLY FILES

     

     

    The following data files were used to generate statistics and2-D and3-D images. Display quality of the below data file samples varies based on the Web browser and other factors. Files are located in the data_set folder. Sources of data are listed in the Technical information on data sources section (techinfo.htm):

     

      • Ssxtops.dat contains borehole location/elevation/well symbol/well name/depth to the Upper Cretaceous Ardmore bentonite, and depths to top and base of the underlying Sussex "B" sandstone and the separate sand ridges that comprise it

     

    • Ssxporos.dat contains borehole X-Y location, core and well-log porosity data, core permeability, and sample depths relative to the surface, the base of the Sussex "B" sandstone, and the base of the Ardmore bentonite.

     

    • Corepor.dat lists core porosity, permeability, water, and oil saturation data for Sussex and Shannon Member sandstones by borehole name and township-range-section location
    • fldoutln.ply (fields outline polygons) contains the x and y coordinates of the outlines of the House Creek and Porcupine oil fields. Coordinate system is the same as above data files. The two polygons used as clipping polygons for the3-D models and for display on the2-D maps. File format is space-delimited point data; X (1:8), Y(9:20)

    Ssxtops.dat has formation-tops data by borehole. Format is space-delimited ASCII. Headings are not present in files; heading descriptions and column locations follow the below well listings. Three or more spaces separate each data element. Blanks are marked with an * . Each of the525 boreholes has a listed township, range, and section (data is sorted relative to this location), and estimated distance in meters from the map origin; central meridian is106 degrees east and latitude is44 degrees north. All2-D and3-D map images are generated from this origin. Our well-log analysis was augmented by other sources of information; these include Kerr-McGee Corp., Woods Petroleum Corp., Meridian Oil, Petroleum Information Corp., and State of Wyoming Oil and Gas Conservation Commission.

    This file was used to delineate sand-ridge and reservoir-grade-sandstone boundaries for isopach maps and3-D images. Reservoir-grade sandstones are defined as greater than8.5 percent porosity, in combination with greater than8 millidarcies (mD) permeability, geophysical well-log signatures, core and thin-section data, and borehole production data. A10 MV spontaneous potential (SP) well-log deflection bounds gross sandstone intervals. This zone is characterized by a rapid decrease in core and well-log porosity. The boundary occurs at approximately8.5 percent porosity, although this varies.

     

     

    Listing of two wells from and format of the ssxtops.dat file

    API X Y TRS ELEV YR TD ARDEP SSXTP SSXBD SSXUT SSXUB SSXLT SSXLB SYMB NAME

    (1) -30380 N43W * * * *171-1 STUART-BRO (2) -30390 N43W- WATSON

     

     
    1. API (1:10 ) American Petroleum Institute well identification number
    2. X (15:19 ) Approximate distance in meters east of the map origin
    3. Y (23:28 ) Approximate distance in meters north or south of the map origin
    4. TRS (32:39 ) Township direction (north or south) and number, range direction (west or east) and number. Alpha format
    5. ELEV (43:46 ) Surface elevation of the borehole, in feet
    6. YR (50:51 ) Well completion year
    7. TD (55:59 ) Total drill depth from the surface, in feet
    8. ARDEP (63:66) Depth (in ft) from the surface to the Ardmore bentonite
    9. SSXTP (70:73) Depth (in ft) from the surface to the disconformity between the Sussex "B" sandstone and the overlying Cody Shale.
    10. SSXBD (77:80) Depth (in ft) from the surface to the basal disconformity between the Sussex "B" sandstone and the Cody Shale.
    11. SSXUT (84:87) Depth (in ft) from the surface to the top of the upper reservoir sandstones.
    12. SSXUB (91:94) Depth (in ft) from the surface to the base of the Sussex "B" upper reservoir sandstones.
    13. SSXLT (98:101) Depth (in ft) from the surface to the top of the Sussex "B" lower reservoir sandstones.
    14. SSXLB (105:108) Depth (in ft) from the surface to the base of the Sussex "B" lower reservoir sandstones.
    15. SYMB (112:113) Well symbols of dry and non-productive (17), injection (15), gas wells (20), oil (22), and oil and gas (29) wells
    16. NAME (113:132) Well name - in mixed alpha and numeric characters

    Ssxporos.dat contains core and well-log porosity, and core-permeability data by borehole for the Sussex "B" sandstone and bounding Cody Shale intervals. Format is space-delimited ASCII. Three or more spaces separate each data element. Heading descriptions and column locations follow the below data list. Blanks are marked with an *. Data are sorted relative to API number, which is also the primary link between data files. Within each borehole, data are sorted by sample depth.

    This file contains the raw data used to generate3-D porosity and permeability images. Core porosity and permeability values are listed for13 wells within and proximal to the House Creek field. Well-log porosity data are derived from bulk-density and sonic-log traces for about100 boreholes. Porosity was calibrated to a specific grain density of2.68 g/cm3; this approximates average grain densities determined from the core analyses and estimated from thin-section examinations.

     

    Listing of data for and format of the ssxporos.dat file

    API X Y SBASDP SARDEP SAMPDP POR PERM -24851 -1 -7082125.65 * -24851 -1 -7282145.71 * -2404413 -.71. -2404412 -5381657.80.5 -2404411 -5481668.922. -2404410 -5581679.90.5 -240449 -5681686.72. -240448 -5781697.10.5 -240447 -.93. -240446 -.248.2

     

     
    1. API (1:10) American Petroleum Institute well identification number
    2. X (14:18) Approximate distance in meters east of the map origin
    3. Y (22:27) Approximate distance in meters north or south of the map origin
    4. SBASDP (31:33) Distance (in ft) of sample above the basal disconformity of the Sussex "B" sandstone
    5. SARDEP (37:41) Distance (in ft) of sample below the base of the Ardmore bentonite
    6. SAMPDP (45:48) Depth (in ft) of the sample below ground surface
    7. POR (52:55) Core or well-log porosity (in percent)
    8. PERM (59:62) Core permeability (mD) for about13 wells. An * indicates no data

    The Corepor.dat file contains core porosity (volume %) and permeability (mD) measurement data (POR and PERM) of Sussex and Shannon Sandstone Members of the Cody Shale; data are listed by sample depth (DEPTH) in feet below ground surface, and borehole location. This file of data for37 boreholes is included for archival purposes. Format is tab-delimited ASCII. The below heading is present at the top of this list but not on the archived file. API number and X-Y location are not included, however this information is located in the ssxtops.dat file and can be accessed by linking the township-range-section (TRS) values for both files.

     

    WELL WELL_LOC DEPTH PERM POR OIL WATER WELL_NAME NUMBER TRS (FEET) (MD) (%) (%) (%) AND LOCATION

    12 N44W .095.40 * * NO.1-23 FEDERAL12 N44W.610.0 * * FED237312 N44W.216.0 * * SEC.23, T.44 N, R.73 W12 N44W.16.0 * *12 N44W.214.0 * *12 N44W.314.0 * *12 N44W.714.0 * *12 N44W.916.0 * *13 N44W .236.40.065.7 NO.1 GOVERNMENT MILES13 N44W .727.98.966.0 GOVT4413 N44W.715.017.826.8 SW NE SEC.9, T.44 N, R.73 W13 N44W.612.012.330.313 N44W.817.013.927.813 N44W.515.017.630.5 

     

     

      U.S. GEOLOGICAL SURVEY DIGITAL DATA SERIES DDS-33 3-D Reservoir Characterization of the House Creek Oil Field, Powder River Basin, Wyoming, V1.00

     

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