Question 4 of 7: Double-porosity buildup – storativity, fracture permeability, skin, average pressure
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
EGBC National Exam — Petroleum Engineering, 2014-Dec. 3 hours, closed book. This sitting's own cover page reads “98-Pet-B5, Well Testing,” not Reservoir Mechanics, and every question is pressure-transient/well-test analysis (radial diffusivity, drawdown/buildup, double-porosity, sealing-fault, interference). NOTES item 4/5 state that five (5) questions constitute a complete exam and only the first five as they appear are marked; all seven questions on the paper are solved in full below. Three of the seven questions (Q3, Q4, Q6) are chart-reading questions built around semilog/log-log plots with no printed data table — every plotted value used below was read from the printed figure and is flagged check where it feeds a boxed result.
Reference texts: Lee, J., Well Testing, SPE Textbook Series Vol. 1 (diffusivity equation, type curves, radius of investigation); Earlougher, R.C., Advances in Well Test Analysis, SPE Monograph Vol. 5 (Horner analysis, superposition in time, interference and reservoir-limit tests); Bourdet, D., Well Test Analysis: The Use of Advanced Interpretation Models, Elsevier (double-porosity/Warren–Root model, sealing faults); Warren, J.E. & Root, P.J., “The Behavior of Naturally Fractured Reservoirs,” SPE Journal, 1963.
Find. Storativity ratio $\omega$, average fracture permeability $\hat{k}_f$, skin factor $S$, and average reservoir pressure.
Approach. A double-porosity (Warren–Root) buildup traces an S-shaped Horner curve: an early straight line (fracture system alone), a transition dip (matrix starts feeding the fractures), and a late straight line (total system) of the same slope as the early line. Fit both lines (forcing a shared slope), then read $\hat{k}_fh$ from that slope, $\omega$ from the vertical separation between the two lines, $S$ from $p_{1hr}$ on the late line, and $p^*$ by extrapolating the late line to a Horner ratio of 1.
Fig. 3 – Horner plot of the double-porosity buildup (digitized markers, with the fitted early/fracture and late/total-system straight lines). The characteristic S-shape – two parallel-slope lines separated by a flatter transition – is the diagnostic signature of a naturally fractured reservoir.
Fit the two parallel semilog lines. A shared-slope least-squares fit through the digitized early-time points (fracture line) and late-time points (total-system line) gives
$$m\approx 493\ \text{psi/cycle}\quad(\text{check: digitized})$$
with early-line intercept $b_e\approx3322$ psia and late-line intercept $b_l\approx2761$ psia (both at Horner ratio $=1$ on their own respective straight-line trends).
Average fracture permeability. Both lines have the same slope in the ideal Warren–Root model, so either one gives the same $(kh)_f$ via the formula sheet's double-porosity slope relation:
$$(kh)_f=\frac{162.6\,q\mu B_o}{m}=\frac{162.6(500)(3)(1.2)}{493}\approx 594\ \text{mD-ft}$$
$$\boxed{\hat{k}_f=(kh)_f/h\approx 118.8\ \text{mD}}$$
Storativity ratio $\omega$. The vertical gap between the two parallel lines (at any common Horner ratio) is $\Delta p=b_l-b_e\approx2761-3322=-561$ psi (i.e. the fracture-only line sits above the eventual total-system line by 561 psi at the same Horner ratio, since the fracture-only system depletes faster before matrix support kicks in), which converts to the storativity ratio via
$$\omega=10^{-|\Delta p|/m}=10^{-561/493}$$
$$\boxed{\omega\approx 0.073}$$
– a physically reasonable value (real naturally fractured reservoirs typically show $\omega\sim0.001$–0.1).
Skin factor. Extrapolating the LATE (total-system) line back to $\Delta t=1$ hr, i.e. Horner ratio $(t_p+1)/1=10{,}001$, gives $p_{1hr}\approx790$ psia. With the given $p_{wf}(\Delta t=0)=700$ psia, the buildup-test skin formula from the formula sheet gives
$$S=1.151\left[\frac{p_{1hr}-p_{wf}(\Delta t=0)}{|m|}-\log\!\left(\frac{\hat{k}_f}{\phi\mu c_t r_w^2}\right)+3.23\right]$$
$$S=1.151\left[\frac{790-700}{493}-\log\!\left(\frac{118.8}{(0.1)(3)(5\times10^{-6})(0.3)^2}\right)+3.23\right]$$
$$\boxed{S\approx -6.4}$$
Average reservoir pressure. Extrapolating the late (total-system) line all the way to a Horner ratio of 1 ($\Delta t\to\infty$, i.e. an infinite shut-in) gives the classic $p^*$ extrapolated pressure, taken as the average reservoir pressure estimate (no Dietz shape-factor correction is available from the given data, so $p^*$ is used directly – check):
$$\boxed{p^*\approx 2761\ \text{psia}}$$