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Agreement DE-FC26-02NT15342, Seismic Evaluation of ...

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the pressure trends were analyzed, as were rock and fluid properties for brine and<br />

hydrocarbon saturated cases. Finally the Ursa field depositional setting was compared to<br />

the Brushy Canyon depositional setting to establish the commonalities between the two<br />

deepwater settings. These observations and reservoir properties are essential in<br />

developing geologically realistic models that will be discussed in the next chapter for<br />

forward modeling.<br />

Forward modeling<br />

Forward modeling was performed on six geologic models built to represent three<br />

different reservoir intervals. The first reservoir interval is the Lower yellow reservoir<br />

interval, which will have two geologic models; an amalgamated sheet sand and a basin<br />

floor channel system. The second reservoir to be modeled is the Above Magenta<br />

reservoir, which will be modeled with an amalgamated and non-amalgamated channel<br />

complex. Finally, the Upper reservoir interval will be modeled with proximal and distal<br />

levee overbank facies. These reservoir intervals were chosen because they can be<br />

associated with high amplitude events on seismic data and each one represents one <strong>of</strong> the<br />

three common reservoir facies mentioned above (sheet sand, channel fill and<br />

levee/overbank). Each <strong>of</strong> these six geologic models were saturated with brine, oil, 10%<br />

and 50% gas respectively. The models were calibrated with the Ursa reservoir fluid and<br />

rock properties. Forward modeling was performed using a simple convolution between<br />

the impedance volume and extracted wavelet was preformed on each model. Also,<br />

Amplitude Versus Offset (AVO) modeling using the Zoeppritz equation was preformed<br />

on one pseudo well for each model. A total <strong>of</strong> 24 separate 2D synthetic models and 24<br />

AVO models were made, one for each reservoir facies and fluid case. For each reservoir<br />

interval that was modeled the two possible seismic facies interpretations were compared<br />

to determine if the lithology and fluids could be differentiated. This chapter will describe<br />

the method <strong>of</strong> developing the reservoir models and rock and fluid properties from the<br />

reservoir interval. This chapter will also give a general summary <strong>of</strong> the method used to<br />

develop each <strong>of</strong> the models and precedes the three chapters that will discuss each<br />

reservoir and its models and results in detail.<br />

Example <strong>of</strong> forward modeling method<br />

To generate the reservoir model, first the geologic model was created with an<br />

image file. This image was created as an 8-bit grayscale bitmap image which with a total<br />

<strong>of</strong> 256 possible colors associated with it where each color is represented by a number,<br />

black being 0 and white 255. The image is then scaled to the size <strong>of</strong> the reservoir by<br />

converting pixels to meters. This calibrated image is then output as a digital file using the<br />

United States National Institute <strong>of</strong> Health (NIH) imagej freeware<br />

(http://rsb.info.nih.gov/ij/). Each number/pixel represents a location in the reservoir<br />

model. Not every pixel was used to model the reservoir. Instead the model was sampled<br />

at 50 meter lateral spacing to match the Ursa seismic trace spacing. A matlab code<br />

(Appendix D) was written to sort the imajej output text file into columns that would<br />

eventually represent pseudo well logs spaced 50 m apart. Once these new 50-meter<br />

spaced bitmap pixel numbers were sorted, they were placed into an excel spreadsheet and<br />

converted to proper Vp, Vs, and density values associated with the reservoir interval<br />

being modeled. For all models, the horizontal scale was developed using the depositional<br />

history <strong>of</strong> the reservoir interval. The vertical scale was developed using the Ursa number<br />

<strong>Agreement</strong> <strong>DE</strong>-<strong>FC26</strong>-<strong>02NT15342</strong>, <strong>Seismic</strong> <strong>Evaluation</strong> <strong>of</strong> Hydrocarbon Saturation 83

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