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Reservoir engineeringFlow in porous media and transient inflow Advanced 16 min read

Line-source solution and the pressure function

The line-source solution is a formula for the pressure at any point of an unbounded, uniform reservoir (one that is the same everywhere and has no outer edge), at any moment after a well starts to produce at a constant rate. In this formula the well is replaced by a line of zero radius, and the pressure is written with the exponential integral (a special mathematical function). At the wall of the well, within seconds, the solution reduces to a logarithm of time. This is the pressure function of the well, pD(tD)p_D(t_D). The semilog methods of well testing (methods that plot pressure against the logarithm of time) are built on it.

Why it matters

This is the main solution of the diffusivity equation (the equation that describes how pressure spreads through a reservoir). We use it to calculate how the bottomhole pressure falls after a well is started, when and by how much the pressure will drop in a neighbouring well, and how far a test “sees”. If we add such solutions together, we can describe a well shut-in, a change of rate, several wells working together, and the effect of faults. Its limits show when we need other formulas: those for pseudo-steady-state or steady-state flow (the flow regimes that follow once the pressure disturbance has reached the edges of the reservoir).

Quick refresher

  • In an unbounded reservoir, the pressure depends not on distance and time separately but on one combination of the two, x=r2/(4ηt)x = r^2/(4\eta t). This is the square of the ratio of the distance to the radius of investigation (how far the pressure disturbance has travelled).
  • The solution is pi−p=qBμ4πkh E1(x)p_i - p = \frac{qB\mu}{4\pi kh}\,E_1(x), where E1(x)=−Ei(−x)E_1(x) = -\mathrm{Ei}(-x) is the exponential integral. It is large for small xx and practically zero for x>5x > 5.
  • When x<0.01x < 0.01, we can replace the function with a logarithm: E1(x)≈−ln⁡(1.781x)E_1(x) \approx -\ln(1.781x), with an error of less than 0.25%. At the wall of a well this condition holds within seconds after start-up. A hundred metres away it holds only after weeks or months.
  • At the well, pD=12(ln⁡tD+0.809)+Sp_D = \tfrac12(\ln t_D + 0.809) + S, where SS is the skin factor (a number that shows how much the zone right around the well helps or hinders flow). Every time the time grows tenfold, the pressure drop grows by the same amount.
  • The solution holds until the pressure disturbance reaches the boundaries. For a well at the centre of a circle, that is roughly until tD/reD2=0.25t_D/r_{eD}^2 = 0.25. After that, pseudo-steady-state or steady-state flow takes over.
  • If the bottomhole pressure is fixed at the well instead of the rate, the rate falls with time roughly as 1/pD(tD)1/p_D(t_D).
Key relationships
pi−p(r,t)=qBμ4πkh E1 ⁣(ϕμctr24kt)p_i - p(r,t) = \dfrac{qB\mu}{4\pi kh}\,E_1\!\left(\dfrac{\phi\mu c_t r^2}{4kt}\right)

line-source solution (SI)

E1(x)≈−ln⁡(1.781 x)for x<0.01E_1(x) \approx -\ln(1.781\,x)\quad \text{for}\ x < 0.01

logarithmic approximation

pD(tD)=12(ln⁡tD+0.809)+Sp_D(t_D) = \tfrac12\left(\ln t_D + 0.809\right) + S

pressure function of a well in an infinite reservoir, tD>25t_D > 25

pi−p=0.933 qBμkh E1 ⁣(ϕμctr20.01421 kt)p_i - p = 0.933\,\dfrac{qB\mu}{kh}\,E_1\!\left(\dfrac{\phi\mu c_t r^2}{0.01421\,kt}\right)

metric oilfield units: m³/d, mPa·s, mD, m, 1/MPa, h, MPa

qD(tD)≈2ln⁡tD+0.809q_D(t_D) \approx \dfrac{2}{\ln t_D + 0.809}

dimensionless rate at constant bottomhole pressure

Common pitfalls
  • Using the logarithmic formula far from the well. For x>0.56x > 0.56 it gives a negative drop, that is, a “rise” in pressure.
  • Confusing signs and notation. E1(x)E_1(x) and −Ei(−x)-\mathrm{Ei}(-x) are the same positive number. Euler's constant is 0.5772, but the flow formulas contain its exponential, 1.781.
  • Extending the logarithmic line back to the first moments after start-up. There the well can no longer be treated as a line.
  • Using the solution for an infinite reservoir after the disturbance has reached the boundaries.
  • Putting time in days or distance in feet into the argument with the constant 0.01421, which is made for hours and metres.

After this lesson you can

  • set up the problem of a well started at a constant rate in an unbounded reservoir, and explain why the well is replaced by a line source
  • use the exponential integral to calculate the pressure at a given point of the reservoir at a given moment, in metric and in oilfield units
  • use the logarithmic approximation, and check whether it is valid at the well and away from it
  • state the time limits of the solution, and choose the right formula for the pressure function pD(tD)p_D(t_D) for each period
  • explain how the solution at constant bottomhole pressure differs from the solution at constant rate, and where it is needed

The problem: a well in an unbounded reservoir

A well is started at a constant rate in a reservoir where the pressure is the same everywhere and equal to the initial pressure. What will the pressure be at any point of the reservoir at any moment, as long as the disturbance has not reached the boundaries? This is a problem for the diffusivity equation with three conditions (the initial and boundary conditions). First, the pressure is pip_i throughout the reservoir before start-up. Second, the rate at the well is constant. Third, the pressure is still pip_i at infinite distance.

Strictly, the condition at the well is set at its wall, at r=rwr = r_w. But a well has a radius of only about 0.1 m, while the pressure changes over distances of tens or hundreds of metres. So we replace the well by a line of zero radius, through which the same rate is withdrawn. This is the line source. For a producing well, “line sink” would be more accurate, but the term is used for both production and injection.

Constant-rate condition for the line source
lim⁡r→0(r ∂p∂r)=qBμ2πkh\lim_{r\to 0}\left(r\,\frac{\partial p}{\partial r}\right) = \frac{qB\mu}{2\pi kh}
where:
  • p(r,t)p(r, t)pressure at distance rr from the well axis at time tt, Pa
  • q, Bq,\ Brate at standard conditions and formation volume factor, m³/s, m³/m³
  • k, h, μk,\ h,\ \mupermeability, reservoir thickness, fluid viscosity, m², m, Pa·s

Units: SI

Holds when
  • The rate is constant from the moment of start-up.
  • The well penetrates the full thickness of the reservoir, and the inflow is uniform over the thickness.

This is the same condition as at the wall of a real well, only moved to its axis: the whole flow rate passes through a cylinder of any small radius around the axis. The well radius drops out of the problem.

One variable instead of two

The line-source problem has no length scale of its own: the well radius has dropped out, and the reservoir is infinite. From the distance rr, the time tt and the hydraulic diffusivity η\eta (how fast pressure spreads through the rock), we can make only one dimensionless combination (a number without units): r2/(ηt)r^2/(\eta t). So the pressure depends not on distance and time separately, but only on this combination. It is called the Boltzmann variable:

Similarity variable (Boltzmann variable)
x=r24ηt=ϕμct r24kt=(rri)2,ri=4ηtx = \frac{r^2}{4\eta t} = \frac{\phi\mu c_t\,r^2}{4kt} = \left(\frac{r}{r_i}\right)^{2},\qquad r_i = \sqrt{4\eta t}
where:
  • xxdimensionless variable on which the solution depends, —
  • r, tr,\ tdistance from the well axis and time since start-up, m, s
  • η\etahydraulic diffusivity k/(ϕμct)k/(\phi\mu c_t), m²/s
  • rir_iradius of investigation at time tt (how far the disturbance has spread), m

Units: SI

Holds when
  • An unbounded homogeneous reservoir, a line source and a constant rate from start-up.

The variable xx is the square of the ratio of the distance to the radius of investigation. When x≪1x \ll 1, the point lies deep inside the drawdown cone (the region where the pressure has dropped). When x≈1x \approx 1, it is at the edge of the cone. When x≫1x \gg 1, the disturbance has not reached it yet. The pressure profiles at different times are similar to one another: if we stretch the distances in proportion to t\sqrt t, we get one and the same curve.

In other unit systems (2)
Metric oilfield units
x=ϕμct r20.01421 k tx = \frac{\phi\mu c_t\,r^2}{0.01421\,k\,t}

rr in m, tt in h, kk in mD, μ\mu in mPa·s, ctc_t in 1/MPa.

0.01421=4⋅3.553⋅10−30.01421 = 4\cdot3.553\cdot10^{-3}, where 3.553⋅10−33.553\cdot10^{-3} is the diffusivity factor in these units (Diffusivity equation).

Oilfield units
x=948 ϕμct r2k tx = \frac{948\,\phi\mu c_t\,r^2}{k\,t}

rr in ft, tt in h, kk in mD, μ\mu in cP, ctc_t in 1/psi.

948=1/(4⋅2.637⋅10−4)948 = 1/(4\cdot2.637\cdot10^{-4}).

Using one variable instead of two turns the partial differential equation into an ordinary differential equation, which we can integrate (the derivation is in the advanced section). The result:

Line-source solution
pi−p(r,t)=qBμ4πkh E1 ⁣(ϕμct r24kt),E1(x)=−Ei(−x)=∫x∞e−uu  dup_i - p(r, t) = \frac{qB\mu}{4\pi kh}\,E_1\!\left(\frac{\phi\mu c_t\,r^2}{4kt}\right),\qquad E_1(x) = -\mathrm{Ei}(-x) = \int_x^{\infty}\frac{\e^{-u}}{u}\,\dd u
where:
  • p(r,t)p(r, t)pressure in the reservoir at distance rr from the well axis, a time tt after start-up, Pa
  • pip_iinitial reservoir pressure, Pa
  • q, Bq,\ Brate at standard conditions and formation volume factor, m³/s, m³/m³
  • μ, k, h\mu,\ k,\ hfluid viscosity, permeability and reservoir thickness, Pa·s, m², m
  • ϕ, ct\phi,\ c_tporosity and total compressibility, —, 1/Pa
  • E1(x)E_1(x)exponential integral, —

Units: SI

Holds when
  • An unbounded homogeneous isotropic (the same permeability in every direction) reservoir of constant thickness. Before start-up the pressure is pip_i everywhere.
  • A constant rate from start-up. The well is replaced by a line source and penetrates the full thickness.
  • One slightly compressible fluid (these are the conditions of the diffusivity equation: Diffusivity equation).
  • There is no skin and no wellbore storage (the effect of the volume of fluid in the well itself). The formula describes the pressure in the reservoir, not in the well itself.

The pressure drop at any point equals half of the “unit” radial pressure drop, qBμ/(2πkh)qB\mu/(2\pi kh), multiplied by a function of one argument. In dimensionless variables it is pD=12E1 ⁣(rD2/(4tD))p_D = \tfrac12E_1\!\big(r_D^2/(4t_D)\big). The farther the point and the less time has passed, the larger the argument and the smaller the pressure drop.

In other unit systems (2)
Metric oilfield units
pi−p=0.933 qBμkh E1 ⁣(ϕμct r20.01421 k t)p_i - p = 0.933\,\frac{qB\mu}{kh}\,E_1\!\left(\frac{\phi\mu c_t\,r^2}{0.01421\,k\,t}\right)

qq in m³/d at standard conditions, μ\mu in mPa·s, kk in mD, hh and rr in m, ctc_t in 1/MPa, tt in h, pressure in MPa.

0.933=1/(4π⋅0.0853)0.933 = 1/(4\pi\cdot0.0853), where 0.08530.0853 is the constant of Darcy's law in these units; 0.01421=4⋅3.553⋅10−30.01421 = 4\cdot3.553\cdot10^{-3}.

Oilfield units
pi−p=70.6 qBμkh E1 ⁣(948 ϕμct r2k t)p_i - p = 70.6\,\frac{qB\mu}{kh}\,E_1\!\left(\frac{948\,\phi\mu c_t\,r^2}{k\,t}\right)

qq in STB/d (barrels of oil at standard conditions per day), μ\mu in cP, kk in mD, hh and rr in ft, ctc_t in 1/psi, tt in h, pressure in psi.

70.6=1/(4π⋅1.127⋅10−3)70.6 = 1/(4\pi\cdot1.127\cdot10^{-3}); 948=1/(4⋅2.637⋅10−4)948 = 1/(4\cdot2.637\cdot10^{-4}).

The exponential integral

The function E1(x)E_1(x) is the area under the curve e−u/u\e^{-u}/u from xx to infinity. For small xx it is large and behaves like a logarithm. For large xx it quickly falls towards zero. We can calculate it from a series, read it from tables, or use the built-in functions of software.

Series for the exponential integral
E1(x)=−ln⁡x−0.5772+x−x22⋅2!+x33⋅3!−…E_1(x) = -\ln x - 0.5772 + x - \frac{x^2}{2\cdot2!} + \frac{x^3}{3\cdot3!} - \dots
where:
  • xxargument, x>0x > 0, —
  • 0.57720.5772Euler's constant, —

Units: no units

Holds when
  • The series converges for any x>0x > 0, but it is convenient only for x≤1x \le 1. For larger xx, use tables or a continued fraction (advanced section).

The first two terms are the logarithmic part: −ln⁡x−0.5772=−ln⁡(γx)-\ln x - 0.5772 = -\ln(\gamma x), where γ=e0.5772=1.781\gamma = \e^{0.5772} = 1.781. The remaining terms get small quickly when xx is small. Do not confuse Euler's constant, 0.5772, with its exponential: in flow formulas the letter γ\gamma stands for 1.781.

The exponential integral and its logarithmic approximation
xx
0.001
E1(x)E_1(x)
6.332
−ln⁡(1.781x)-\ln(1.781x)
6.331
Error of the logarithm
0.016%
xx
0.01
E1(x)E_1(x)
4.038
−ln⁡(1.781x)-\ln(1.781x)
4.028
Error of the logarithm
0.25%
xx
0.05
E1(x)E_1(x)
2.468
−ln⁡(1.781x)-\ln(1.781x)
2.419
Error of the logarithm
2.0%
xx
0.1
E1(x)E_1(x)
1.823
−ln⁡(1.781x)-\ln(1.781x)
1.725
Error of the logarithm
5.4%
xx
0.5
E1(x)E_1(x)
0.5598
−ln⁡(1.781x)-\ln(1.781x)
0.1159
Error of the logarithm
79%
xx
1
E1(x)E_1(x)
0.2194
−ln⁡(1.781x)-\ln(1.781x)
below zero
Error of the logarithm
not applicable
xx
2
E1(x)E_1(x)
0.0489
−ln⁡(1.781x)-\ln(1.781x)
below zero
Error of the logarithm
not applicable
xx
5
E1(x)E_1(x)
0.001148
−ln⁡(1.781x)-\ln(1.781x)
below zero
Error of the logarithm
not applicable

The error is the percentage by which the logarithmic approximation falls short of the exact value. For x>0.56x > 0.56 the logarithm is negative and no longer makes sense.

Exponential integral and its logarithmic approximation0.0010.010.111001234567Argument xFunction valuex = 0.01: 0.25% discrepancyx = 1: 0.219E₁(x)−ln(1.781x)

Graph against the argument x from 0.001 to 10 on a logarithmic scale; the vertical axis shows values from 0 to 7. The solid curve E1 falls from 6.3 at x = 0.001 to 4.0 at 0.01, 1.8 at 0.1 and 0.22 at 1, then presses against zero. The dashed straight line of the logarithmic approximation coincides with it up to 0.01, after which it goes below the curve and crosses zero at x = 0.56. The points x = 0.01 and x = 1 are marked.

CalculatedCalculated values of the function E1(x)E_1(x) and of the logarithmic approximation −ln⁡(1.781x)-\ln(1.781x). The argument scale is logarithmic. To the left of x=0.01x = 0.01 the two curves cannot be told apart. At the edge of the drawdown cone, at x=1x = 1, the function equals 0.219, but the logarithm is already negative.

This gives three regions. For x<0.01x < 0.01 we replace the function with a logarithm. For xx from 0.01 to about 5 we need the function itself. For x>5x > 5 it is less than 0.0012: the pressure at such a point has practically not changed.

The logarithmic approximation

If we put E1(x)≈−ln⁡(γx)E_1(x) \approx -\ln(\gamma x) into the solution, we get a formula without special functions. This is the logarithmic approximation:

Logarithmic approximation of the line-source solution
pi−p(r,t)=qBμ4πkh[ln⁡ktϕμctr2+0.809]p_i - p(r, t) = \frac{qB\mu}{4\pi kh}\left[\ln\frac{kt}{\phi\mu c_t r^2} + 0.809\right]
where:
  • p(r,t)p(r, t)pressure in the reservoir at distance rr, a time tt after start-up, Pa
  • pip_iinitial reservoir pressure, Pa
  • q, B, μ, k, h, ϕ, ctq,\ B,\ \mu,\ k,\ h,\ \phi,\ c_tas in the line-source solution, m³/s, m³/m³, Pa·s, m², m, —, 1/Pa
  • 0.8090.809ln⁡(4/γ)\ln(4/\gamma), where γ=1.781\gamma = 1.781, —

Units: SI; natural logarithm

Holds when
  • The conditions of the line-source solution.
  • x<0.01x < 0.01, that is, kt/(ϕμctr2)>25kt/(\phi\mu c_tr^2) > 25: the error is then less than 0.25%. At kt/(ϕμctr2)=5kt/(\phi\mu c_tr^2) = 5 the error is about 2%.

Deep inside the drawdown cone, the pressure depends linearly on both the logarithm of time and the logarithm of distance. The profile there has the same shape as in steady-state flow, but its level sinks with time. In dimensionless form, pD=12[ln⁡(tD/rD2)+0.809]p_D = \tfrac12\left[\ln(t_D/r_D^2) + 0.809\right].

In other unit systems (2)
Metric oilfield units (base-10 logarithm)
pi−p=2.149 qBμkh[log⁡10k tϕμctr2−2.098]p_i - p = 2.149\,\frac{qB\mu}{kh}\left[\log_{10}\frac{k\,t}{\phi\mu c_t r^2} - 2.098\right]

qq in m³/d, μ\mu in mPa·s, kk in mD, hh and rr in m, ctc_t in 1/MPa, tt in h, pressure in MPa.

2.149=ln⁡10/(4π⋅0.0853)2.149 = \ln 10/(4\pi\cdot0.0853); 2.098=−log⁡10(3.553⋅10−3)−0.809/ln⁡102.098 = -\log_{10}(3.553\cdot10^{-3}) - 0.809/\ln 10.

Oilfield units (base-10 logarithm)
pi−p=162.6 qBμkh[log⁡10k tϕμctr2−3.23]p_i - p = 162.6\,\frac{qB\mu}{kh}\left[\log_{10}\frac{k\,t}{\phi\mu c_t r^2} - 3.23\right]

qq in STB/d, μ\mu in cP, kk in mD, hh and rr in ft, ctc_t in 1/psi, tt in h, pressure in psi.

162.6=70.6⋅ln⁡10162.6 = 70.6\cdot\ln 10; 3.23=−log⁡10(2.637⋅10−4)−0.809/ln⁡103.23 = -\log_{10}(2.637\cdot10^{-4}) - 0.809/\ln 10.

The condition x<0.01x < 0.01 means that more than 25 r2/η25\,r^2/\eta of time has passed. Take the well of the examples below (η\eta = 350 m²/h). At the well wall, rr = 0.1 m, this takes 2.6 seconds. At 10 m from the axis it takes 7 hours. At 100 m it takes about a month, and by then the disturbance has long since reached the boundaries. So at the well we use the logarithm, and for points in the reservoir we use the function E1E_1 itself.

Worked examplePressure in the reservoir 10 hours after start-up
Given (assumed data)
Well and reservoir (lesson Flow regimes)
qq = 100 m³/d; BB = 1.3; μ\mu = 1.2 mPa·s; kk = 50 mD; hh = 15 m
Hydraulic diffusivity η\eta
350.4 m²/h (ϕ\phi = 0.20; ct=2.1125⋅10−3c_t = 2.1125\cdot10^{-3} MPa⁻¹)
Time after start-up
10 h; the disturbance has not yet reached the boundaries
Points
the well wall (rwr_w = 0.1 m), 30 m and 100 m from the axis
Solution
  1. Factor in front of the function: 0.933 qBμkh=0.933⋅156750=0.1940.933\,\dfrac{qB\mu}{kh} = 0.933\cdot\dfrac{156}{750} = 0.194 MPa.
  2. Argument x=r2/(4ηt)x = r^2/(4\eta t) with 4ηt=14,0164\eta t = 14{,}016 m²: 7.135⋅10−77.135\cdot 10^{-7} at the well wall, 0.0642 at 30 m, 0.713 at 100 m.
  3. Well wall: x≪0.01x \ll 0.01, so the logarithm is valid: E1≈−ln⁡(1.781x)=13.58E_1 \approx -\ln(1.781x) = 13.58. Pressure drop: 0.194⋅13.58=2.630.194\cdot13.58 = 2.63 MPa.
  4. 30 m: E1(0.0642)=2.232E_1(0.0642) = 2.232, pressure drop 0.433 MPa. The logarithm would give 0.421 MPa, which is 2.8% less.
  5. 100 m: E1(0.713)=0.364E_1(0.713) = 0.364, pressure drop 0.071 MPa. Here the logarithm gives −0.047 MPa, a meaningless “rise” in pressure.
  6. The radius of investigation at this moment: ri=4ηt=118r_i = \sqrt{4\eta t} = 118 m. At this distance x=1x = 1, and the pressure has fallen by 0.194⋅0.219=0.0430.194\cdot0.219 = 0.043 MPa.
Answer: After 10 h the pressure has fallen by 2.63 MPa at the well wall, by 0.433 MPa at 30 m and by 0.071 MPa at 100 m from it.

What it means. The first 30 m account for more than 80% of the pressure drop: the drawdown cone is steep at the well and gentle at its edge. The numbers agree with the “10 h” profile on the graph of the lesson Flow regimes. That profile was calculated numerically for a bounded region. The disturbance has not yet reached the boundary, so the region behaves like an infinite reservoir. The logarithmic approximation is reliable only deep inside the cone. At 30 m it is off by a few per cent, and at 100 m it cannot be used. The data in this example are assumed for illustration.

Pressure at the well: the pressure function

In well testing, the pressure is measured in the well itself, that is, at r=rwr = r_w, or rD=1r_D = 1. There the argument x=1/(4tD)x = 1/(4t_D) falls below 0.01 within seconds after start-up, and the solution reduces to a logarithm of time. If we add the pressure drop across the skin (Skin factor), we get the relationship on which all semilog methods are built:

Pressure function of a well in an infinite reservoir
pD(tD)=2πkh (pi−pwf)qBμ=12(ln⁡tD+0.809)+S,tD=ktϕμctrw2p_D(t_D) = \frac{2\pi kh\,(p_i - p_{wf})}{qB\mu} = \frac12\left(\ln t_D + 0.809\right) + S,\qquad t_D = \frac{kt}{\phi\mu c_t r_w^2}
where:
  • pD(tD)p_D(t_D)dimensionless drop in bottomhole pressure, —
  • pwfp_{wf}bottomhole flowing pressure of the producing well a time tt after start-up, Pa
  • tDt_Ddimensionless time based on the wellbore radius, —
  • SSskin factor, —
  • rwr_wwellbore radius, m
  • pi, q, B, μp_i,\ q,\ B,\ \muinitial pressure, rate, formation volume factor, viscosity, Pa, m³/s, m³/m³, Pa·s
  • k, h, ϕ, ctk,\ h,\ \phi,\ c_tpermeability, thickness, porosity, total compressibility, m², m, —, 1/Pa

Units: SI; in metric oilfield units tD=3.553⋅10−3 kt/(ϕμctrw2)t_D = 3.553\cdot10^{-3}\,kt/(\phi\mu c_tr_w^2) with tt in hours

Holds when
  • An unbounded reservoir and a constant rate from start-up.
  • tD>25t_D > 25 (error about 2%) or tD>100t_D > 100 (about 0.5%): for an ordinary well that is only seconds.
  • The skin is an extra pressure drop in a thin zone near the wellbore. It appears together with the flow.
  • The effect of wellbore storage (the fluid volume in the well itself) has ended (Wellbore storage).

Each tenfold increase in time raises pDp_D by 12ln⁡10=1.151\tfrac12\ln 10 = 1.151, and the skin shifts the whole relationship by a constant amount. The same formula can be read as the Dupuit equation (the steady-state radial flow equation) with a growing radius: pD=ln⁡(rd/rw)+Sp_D = \ln(r_d/r_w) + S, where rd=4ηt/γ≈0.75 rir_d = \sqrt{4\eta t/\gamma} \approx 0.75\,r_i is the radius of drainage (quasi-steady-state profile). The form with units, and how to find permeability and skin from measurements, are in the lesson Pressure drawdown analysis.

Dimensionless pressure at the well wall from three formulas
tDt_D
1
Finite wellbore radius
0.802
Line source
0.522
Logarithm
0.405
Error of the logarithm
−50%
tDt_D
5
Finite wellbore radius
1.362
Line source
1.234
Logarithm
1.209
Error of the logarithm
−11%
tDt_D
10
Finite wellbore radius
1.651
Line source
1.568
Logarithm
1.556
Error of the logarithm
−5.8%
tDt_D
25
Finite wellbore radius
2.062
Line source
2.019
Logarithm
2.014
Error of the logarithm
−2.3%
tDt_D
100
Finite wellbore radius
2.723
Line source
2.708
Logarithm
2.707
Error of the logarithm
−0.58%
tDt_D
1000
Finite wellbore radius
3.861
Line source
3.859
Logarithm
3.858
Error of the logarithm
−0.056%

The skin is zero. “Finite wellbore radius” is the solution with the constant-rate condition set at the wall, r=rwr = r_w. It was calculated by numerical inversion of the Laplace transform (a mathematical method; see the advanced section). For the well of the examples, tD=25t_D = 25 is reached 2.6 s after start-up and tD=100t_D = 100 after 10 s.

Dimensionless pressure at the well wall in the first moments after start-up, from three formulas0.1110100100001234Dimensionless time tDDimensionless pressure pD25solid — finite wellbore radiusorange dashes — line sourcegrey dashes — logarithm

Graph of dimensionless pressure from 0 to 4 against dimensionless time from 0.1 to 1000 on a logarithmic scale. The solid curve for a finite wellbore radius rises smoothly from 0.31 at 0.1 to 3.86 at 1000. The dashed line-source curve starts almost from zero and catches up with it at a time of about 25. The straight line of the logarithmic approximation starts from zero at 0.45 and merges with the others to the right of 25. The point 25 is marked.

CalculatedCalculated dimensionless pressure at the well wall in the first moments after start-up, from three formulas: the finite-wellbore-radius solution, the line-source solution and the logarithmic approximation. The time scale is logarithmic. By tD=25t_D = 25 the three curves come together. To the left of that, the logarithmic line gives too small a pressure drop, and for tD<0.45t_D < 0.45 it goes below zero.

The practical conclusion has two parts. First, at the well the logarithmic formula is accurate within seconds after start-up. This is long before the effect of wellbore storage ends, and that effect is what actually governs the first minutes and hours of a pressure record. Second, do not extend the logarithmic line back to the moment of start-up itself: at small tDt_D the true pressure drop is larger than this line gives.

Where the solution stops working: the reservoir boundaries

The solution for an infinite reservoir is valid until the disturbance reaches the boundaries. Take a well at the centre of a circular region of radius rer_e. Its bottomhole pressure departs from the infinite-reservoir solution when the radius of investigation becomes equal to the radius of the region, that is, at tD/reD2≈0.25t_D/r_{eD}^2 \approx 0.25 (time to the boundary). The exact solution for a closed circle (at re/rwr_e/r_w = 3000) differs from it by 0.2% at tD/reD2=0.25t_D/r_{eD}^2 = 0.25, by 0.5% at 0.3 and by more than 1% at 0.4. After that a different formula applies. Which one depends on the condition at the boundary.

The pressure function of a well in different periods
Period
The first moments
Condition
tD≪1t_D \ll 1
pDp_D at the well
2tD/π2\sqrt{t_D/\pi}
Period
Infinite reservoir
Condition
tD>25t_D > 25 and tD/reD2<0.25t_D/r_{eD}^2 < 0.25
pDp_D at the well
12(ln⁡tD+0.809)\tfrac12(\ln t_D + 0.809)
Period
Closed circle, pseudo-steady-state regime
Condition
tD/reD2>0.3t_D/r_{eD}^2 > 0.3
pDp_D at the well
2tD/reD2+ln⁡reD−342t_D/r_{eD}^2 + \ln r_{eD} - \tfrac34
Period
Circle with constant pressure at the boundary
Condition
tD/reD2>0.5t_D/r_{eD}^2 > 0.5
pDp_D at the well
ln⁡reD\ln r_{eD}

Here reD=re/rwr_{eD} = r_e/r_w. The skin is added to each formula. For a well at the centre of a circle, the transition from the second row to the third is short. For elongated regions and for wells close to one boundary it is stretched out (shape factor).

Pressure function of a well at the centre of a closed circle for different region sizes and in an infinite reservoir4567894681012Base-10 logarithm of dimensionless time, log tDDimensionless pressure pD1000300010,000infinite reservoirnumbers on curves — region radiusin well radii

Graph of dimensionless pressure from 4 to 12 against the base-10 logarithm of dimensionless time from 4 to 9. The dashed straight line of the infinite reservoir rises from 5.0 to 10.8. Three solid curves for radius ratios of 1000, 3000 and 10,000 follow this line and, one after another, turn sharply upward: the first at a time logarithm of about 5.5, the second at about 6.4, the third at about 7.4.

CalculatedCalculated pressure function of a well at the centre of a closed circle, for three values of reD=re/rwr_{eD} = r_e/r_w, and in an infinite reservoir (dashed straight line). The horizontal axis is the base-10 logarithm of dimensionless time: 6 means tD=106t_D = 10^6. Each curve follows the common straight line as long as tD/reD2t_D/r_{eD}^2 is less than 0.25–0.3, and then turns upward: pseudo-steady-state depletion begins. If the area of the region grows a hundredfold, the departure comes a hundred times later.

The line-source solution is useful even after the disturbance has reached the boundaries. The diffusivity equation is linear, so we can add solutions together. The pressure from several wells is the sum of their contributions. A change of rate is treated as starting one more well at the same point. A sealing fault is replaced by an imaginary image well on the other side of it (Superposition principle, Pressure build-up analysis, A sealing fault near the well: the method of images).

Pressure in a neighbouring well

We need the formula with the function E1E_1 above all where the distance is large. One case is an interference test: the rate is changed in one well and the pressure is recorded in another. Another is estimating how wells affect each other. The logarithmic approximation is not suitable for such distances (see the example above).

Pressure drop at different distances from a well after it is started at a constant rate1310301000.0010.010.11Time after start-up t, hPressure drop, MPa50 m150 m250 m0.005 MPa

Graph of pressure drop from 0.001 to 1 MPa against time from 1 to 100 hours, both scales logarithmic. Three curves rise steeply and then flatten out: the 50 m curve passes 0.1 MPa a little after three hours and reaches 0.67 MPa by 100 hours; the 150 m curve crosses the level of 0.005 MPa at about 6.5 hours and reaches 0.27 MPa; the 250 m curve crosses it at about 18 hours and reaches 0.12 MPa. On each curve a point is marked at the level of 0.043 MPa: at 1.8, 16 and 45 hours.

CalculatedCalculated pressure drop at points 50, 150 and 250 m from the well of the examples, after it is started at a rate of 100 m³/d. The reservoir is taken to be unbounded. Both scales are logarithmic. The dots on the curves mark the moment when the radius of investigation reaches that distance: by then the pressure has already fallen by 0.043 MPa. The dashed line is a drop of 0.005 MPa, which an accurate gauge can clearly detect.
Worked exampleWhen the response reaches a neighbouring well
Given (assumed data)
Active well
the well of the previous example: the factor in front of the function is 0.194 MPa, η\eta = 350.4 m²/h
Observation well
shut in (not producing), 150 m from the active well
Clearly detectable pressure change
0.005 MPa (gauge resolution 0.0001 MPa)
Solution
  1. The required value of the function: E1(x)=0.005/0.194=0.0258E_1(x) = 0.005/0.194 = 0.0258.
  2. From a table, or by trial and error, x=2.47x = 2.47 (as a check, E1(2.5)=0.0249E_1(2.5) = 0.0249).
  3. Time: t=r24ηx=15024⋅350.4⋅2.47=6.5t = \dfrac{r^2}{4\eta x} = \dfrac{150^2}{4\cdot350.4\cdot2.47} = 6.5 h.
  4. The radius of investigation reaches 150 m later, after r2/(4η)=16r^2/(4\eta) = 16 h. By that moment the pressure in the observation well has already fallen by 0.043 MPa.
  5. A coarse gauge that can tell apart only 0.05 MPa would “see” the response only after 18 h (E1=0.258E_1 = 0.258, x=0.91x = 0.91).
Answer: A response of 0.005 MPa will arrive at the well 150 m away after about 6.5 h — 2.5 times sooner than the radius of investigation “reaches” it.

What it means. The disturbance has no sharp front: the pressure far away starts to change at once, only very weakly. When the response is noticed depends on how sensitive the gauge is. The radius of investigation is a conventional boundary, where the pressure drop equals 0.11 of a “unit” qBμ/(2πkh)qB\mu/(2\pi kh). In an interference test, the arrival time and the size of the response give the hydraulic diffusivity and the flow capacity (permeability times thickness) of the reservoir between the wells. The data in this example are assumed for illustration.

If the bottomhole pressure is fixed instead of the rate

So far we have fixed a constant rate at the well, and the pressure came out of the calculation. It can be the other way round: the well works at a constant bottomhole pressure. An example is a flowing well (one that flows on its own, with no pump) with a constant wellhead pressure. Another is a well with a pump that holds the fluid level. Then the pressure does not fall; the rate does. The drawdown cone widens, and the same pressure difference acts over a longer and longer distance. The solution of this problem is also known. The dimensionless rate qD(tD)q_D(t_D) has been tabulated, and for large tDt_D it is expressed approximately through the pressure function:

Rate at constant bottomhole pressure
q(t)=2πkh (pi−pwf)Bμ qD(tD),qD(tD)≈1pD(tD)=2ln⁡tD+0.809q(t) = \frac{2\pi kh\,(p_i - p_{wf})}{B\mu}\,q_D(t_D),\qquad q_D(t_D) \approx \frac{1}{p_D(t_D)} = \frac{2}{\ln t_D + 0.809}
where:
  • q(t)q(t)rate at standard conditions a time tt after start-up, m³/s
  • pi−pwfp_i - p_{wf}constant difference between the initial reservoir pressure and the bottomhole pressure, Pa
  • qD(tD)q_D(t_D)dimensionless rate, —
  • pD(tD)p_D(t_D)pressure function of the well at constant rate, —
  • k, h, B, μk,\ h,\ B,\ \mupermeability, thickness, formation volume factor, viscosity, m², m, m³/m³, Pa·s

Units: SI; in metric oilfield units the factor 2π2\pi is replaced by the constant 0.536

Holds when
  • An unbounded reservoir, a constant bottomhole pressure from start-up, and no skin. With skin, qD≈1/(pD+S)q_D \approx 1/(p_D + S).
  • The approximation qD≈1/pDq_D \approx 1/p_D overestimates the rate: by about 2% at tD=104t_D = 10^4 and by less than 1% at tD>106t_D > 10^6.

The rate decreases in inverse proportion to the logarithm of time: slowly, but without stopping. In transient flow the ratio of rate to drawdown is higher than after pseudo-steady-state flow is reached, and it keeps falling. The same set-up (constant pressure at the inner boundary) is used for water influx from an aquifer into an accumulation. There we calculate the cumulative influx, the total volume of water that has flowed in (Unsteady-state water influx: the van Everdingen–Hurst method).

Worked exampleHow the rate falls at constant drawdown
Given (assumed data)
Reservoir and well
the same: kk = 50 mD, hh = 15 m, μ\mu = 1.2 mPa·s, BB = 1.3; in 1 h tDt_D = 35,039
Difference between the initial and bottomhole pressures
3.0 MPa, constant from start-up
Solution
  1. Factor: 0.536 kh ΔpBμ=0.536⋅750⋅3.01.56=773\dfrac{0.536\,kh\,\Delta p}{B\mu} = \dfrac{0.536\cdot750\cdot3.0}{1.56} = 773 m³/d.
  2. After 1 h: pD=5.637p_D = 5.637, and q≈773/5.637=137q \approx 773/5.637 = 137 m³/d. Exact solution: qD=0.1749q_D = 0.1749, q=135q = 135 m³/d.
  3. After one day (tD=840,947t_D = 840{,}947): pD=7.226p_D = 7.226, approximately 107 m³/d, exactly 106 m³/d.
  4. After 64 h, when the disturbance reaches the boundary of a region of radius 300 m: approximately 100 m³/d, exactly 99 m³/d.
Answer: At a constant drawdown of 3 MPa the rate falls from 135 m³/d an hour after start-up to 99 m³/d after 64 h. The approximation 1/pD1/p_D overestimates it by 1.5%.

What it means. The rate fell by a quarter, but not because of depletion: a negligible fraction of the hydrocarbons in place has been produced in that time. It fell because the drawdown cone has widened. In a permeable reservoir such a decline lasts only a few days, until the boundaries make themselves felt. In a tight reservoir it is stretched over months and years, and we cannot forecast production from a single measurement of productivity (duration of the regimes). The data in this example are assumed for illustration.

Terms and symbols

Line source
An idealisation of a well: a line of zero radius through which a specified rate is withdrawn (or injected).
Exponential integral E1(x)E_1(x)
It equals ∫x∞e−u/u  du\int_x^\infty \e^{-u}/u\,\dd u, the same as −Ei(−x)-\mathrm{Ei}(-x). It sets the shape of the drawdown cone in an infinite reservoir.
Boltzmann variable xx
The quantity r2/(4ηt)r^2/(4\eta t), the square of the ratio of the distance to the radius of investigation. It is the only argument of the solution.
Logarithmic approximation
Replacing E1(x)E_1(x) by −ln⁡(1.781x)-\ln(1.781x) for x<0.01x < 0.01.
Constant γ\gamma
The number 1.781, the exponential of Euler's constant 0.5772. Here ln⁡(4/γ)=0.809\ln(4/\gamma) = 0.809.
Pressure function pD(tD)p_D(t_D)
The dimensionless drop in the bottomhole pressure of a well producing at a constant rate. In an infinite reservoir it is 12(ln⁡tD+0.809)+S\tfrac12(\ln t_D + 0.809) + S.
Dimensionless rate qD(tD)q_D(t_D)
The rate of a well at constant bottomhole pressure, in units of 2πkh Δp/(Bμ)2\pi kh\,\Delta p/(B\mu).

Common mistakes and misconceptions

Wrong

“The logarithmic formula is valid at any distance from the well.”

In fact

It holds only for x=r2/(4ηt)<0.01x = r^2/(4\eta t) < 0.01. In the lesson's example, after 10 h it is off by 3% at 30 m from the well, and at 100 m it gives a negative pressure drop.

Wrong

“The well radius enters the formula for the pressure in the reservoir.”

In fact

The line-source solution has no well radius in it: the pressure at distance rr depends on the rate, the reservoir properties and the time. The radius appears only when the solution is applied to the wall of the well itself.

Wrong

“Euler's constant is 1.781.”

In fact

Euler's constant is 0.5772. The flow formulas contain its exponential, γ=e0.5772=1.781\gamma = \e^{0.5772} = 1.781, and the constant 0.809 is ln⁡(4/γ)\ln(4/\gamma).

Wrong

“The solution for an infinite reservoir is suitable only for very large accumulations.”

In fact

It is suitable for any reservoir, as long as the disturbance has not reached the boundaries. In the region of radius 300 m used in the examples, that is the first 64 hours.

Wrong

“If the bottomhole pressure is held constant, the rate will also be constant.”

In fact

In transient flow the rate falls roughly as 1/(ln⁡tD+0.809)1/(\ln t_D + 0.809): the drawdown cone widens, and the same pressure difference acts over a greater distance.

In depth: advanced detail

Deriving the solution with the Boltzmann substitution

We look for the pressure as a function of one variable, x=r2/(4ηt)x = r^2/(4\eta t). The chain rule (the rule for differentiating a function of a function) gives r ∂p/∂r=2x  dp/ dxr\,\partial p/\partial r = 2x\,\dd p/\dd x and ∂p/∂t=−(x/t)  dp/ dx\partial p/\partial t = -(x/t)\,\dd p/\dd x. Putting these into the diffusivity equation gives an ordinary differential equation:

The diffusivity equation in the Boltzmann variable
x  d2p dx2+(1+x)  dp dx=0⇒ dp dx=C e−xxx\,\frac{\dd^2 p}{\dd x^2} + (1 + x)\,\frac{\dd p}{\dd x} = 0\quad\Rightarrow\quad \frac{\dd p}{\dd x} = C\,\frac{\e^{-x}}{x}
where:
  • p(x)p(x)pressure as a function of the Boltzmann variable, Pa
  • CCconstant of integration, Pa

Units: SI

Holds when
  • The conditions of the line-source solution: the initial condition and both boundary conditions can be written with the single variable xx.

This is a first-order equation for the derivative  dp/ dx\dd p/\dd x, and we can check its solution by putting it back into the equation. The condition on the well axis, 2x  dp/ dx→qBμ/(2πkh)2x\,\dd p/\dd x \to qB\mu/(2\pi kh) as x→0x \to 0, gives C=qBμ/(4πkh)C = qB\mu/(4\pi kh).

What remains is to integrate from xx to infinity, where the pressure equals the initial pressure: pi−p=C∫x∞e−u/u  du=C E1(x)p_i - p = C\int_x^\infty \e^{-u}/u\,\dd u = C\,E_1(x). The initial condition is satisfied automatically: as t→0t \to 0, the variable xx goes to infinity at every point with r>0r > 0. The substitution works because the problem has no well radius and no boundary radius, that is, no length that rr could be compared with.

How to calculate the exponential integral

For x≤1x \le 1 the series from the main section is enough. Its power terms alternate in sign and get smaller, so the error is no greater than the first term we leave out. At x=0.2x = 0.2, three power terms are enough. At x=1x = 1, you need six of them for four correct digits. For large xx the series converges slowly, so the function is calculated by a continued fraction (a fraction nested inside another fraction, again and again) or taken from tables. This is how the values in the tables and examples of this lesson were found. A two-sided bound (an upper and a lower limit) is useful for a quick check:

Two-sided bound for the exponential integral
12 e−xln⁡(1+2x)<E1(x)<e−xln⁡(1+1x)\frac12\,\e^{-x}\ln\left(1 + \frac{2}{x}\right) < E_1(x) < \e^{-x}\ln\left(1 + \frac{1}{x}\right)
where:
  • xxargument, x>0x > 0, —

Units: no units

Holds when
  • Valid for any x>0x > 0.

At x=1x = 1 the bounds are 0.202 and 0.255, and the exact value is 0.219. At x=5x = 5 they are 0.00113 and 0.00123, and the exact value is 0.00115. The bound helps you notice a gross error, such as a wrong sign of the argument or a base-10 logarithm used instead of a natural one.

A well of finite radius and the first moments

If the constant-rate condition is set not on the axis but at the well wall, at rD=1r_D = 1, the solution is written with Bessel functions (special mathematical functions). It can be written compactly only in Laplace space (after a mathematical transformation of the time variable). For the dimensionless pressure at the wall:

Finite wellbore radius: the Laplace transform
pˉD(s)=K0(s)s3/2 K1(s)\bar p_D(s) = \frac{K_0(\sqrt{s})}{s^{3/2}\,K_1(\sqrt{s})}
where:
  • pˉD(s)\bar p_D(s)Laplace transform of the function pD(tD)p_D(t_D) at the well wall, —
  • ssvariable of the Laplace transform, —
  • K0, K1K_0,\ K_1modified Bessel functions of the second kind, —

Units: no units

Holds when
  • An unbounded reservoir, a constant rate at the well wall, no skin and no wellbore storage.

We go back to the function of time numerically, for example with the Stehfest algorithm. This is how the “finite wellbore radius” column in the table of the main section was found. When tD≪1t_D \ll 1, the solution behaves as 2tD/π2\sqrt{t_D/\pi}. As long as the disturbance has moved from the wall by no more than a fraction of the well radius, the curvature of the wall is not felt, and the flow to the wall is linear. When tD>100t_D > 100, the solution differs from the logarithmic formula by less than 0.6%.

In practice, the first moments of a pressure record are governed not by the well radius but by the volume of the wellbore. While the liquid or gas in the wellbore is expanding, the inflow from the reservoir lags behind the rate at the wellhead (Wellbore storage). The finite-wellbore-radius solution is really needed when the “well” is large. This is how water influx into an accumulation is calculated: the inner boundary is the contour of the accumulation itself (Unsteady-state water influx: the van Everdingen–Hurst method).

Connections to other topics

Check yourself

  1. 1

    A point in the reservoir is at a distance equal to the radius of investigation at a given moment. What are the argument xx and the dimensionless pressure drop pDp_D there?

    1. A.x=0.01x = 0.01, pD≈2p_D \approx 2
    2. B.x=1x = 1, pD≈0.11p_D \approx 0.11
    3. C.x=1x = 1, pD=0p_D = 0
    4. D.x=4x = 4, pD≈0.002p_D \approx 0.002
    Show the answer

    Correct answer: B. x=1x = 1, pD≈0.11p_D \approx 0.11

    By definition x=(r/ri)2x = (r/r_i)^2, so at r=rir = r_i the argument equals 1. Then pD=12E1(1)=12⋅0.219≈0.11p_D = \tfrac12E_1(1) = \tfrac12\cdot0.219 \approx 0.11: at the “edge” of the cone the pressure has already fallen, by about one ninth of a “unit” of radial pressure drop. It has not stayed at its initial value.

  2. 2

    A well produces at 80 m³/d (BB = 1.2; μ\mu = 1.0 mPa·s) in a reservoir with kk = 100 mD, hh = 10 m, ϕ\phi = 0.20, ct=1.5⋅10−3c_t = 1.5\cdot10^{-3} MPa⁻¹. By how much will the pressure fall at a point 100 m from it after 10 h?

    Show the answer

    Factor: 0.933⋅80⋅1.2⋅1.0/(100⋅10)=0.08960.933\cdot80\cdot1.2\cdot1.0/(100\cdot10) = 0.0896 MPa. Argument: numerator ϕμctr2=0.20⋅1.0⋅1.5⋅10−3⋅1002=3.0\phi\mu c_tr^2 = 0.20\cdot1.0\cdot1.5\cdot10^{-3}\cdot100^2 = 3.0, denominator 0.01421⋅100⋅10=14.210.01421\cdot100\cdot10 = 14.21, so x=0.211x = 0.211. This is greater than 0.01, so we need the function itself: E1(0.211)≈1.18E_1(0.211) \approx 1.18 (from the series: −ln⁡0.211−0.577+0.211−0.011=1.18-\ln 0.211 - 0.577 + 0.211 - 0.011 = 1.18). Pressure drop: 0.0896⋅1.18≈0.1060.0896\cdot1.18 \approx 0.106 MPa.

  3. 3

    How soon after start-up can we use the logarithmic formula instead of the function E1E_1 at the wall of an ordinary well?

    1. A.After a few days
    2. B.Within seconds
    3. C.After a few hours
    4. D.Only after pseudo-steady-state flow is reached
    Show the answer

    Correct answer: B. Within seconds

    We need tD>25t_D > 25. One “unit” of dimensionless time, rw2/ηr_w^2/\eta, is a fraction of a second: for the well of the examples, tD=25t_D = 25 is reached after 2.6 s. Hours and days are needed only for points tens or hundreds of metres from the well.

  4. 4

    A well produces at a constant rate in an infinite reservoir. By how much does the dimensionless drop in bottomhole pressure pDp_D increase between 10 and 100 h, and between 100 and 1000 h?

    1. A.By 1.151 and by 11.51
    2. B.It depends on the skin
    3. C.By 1.151 in both cases
    4. D.By 2.303 in both cases
    Show the answer

    Correct answer: C. By 1.151 in both cases

    pD=12(ln⁡tD+0.809)+Sp_D = \tfrac12(\ln t_D + 0.809) + S: every tenfold increase in time adds 12ln⁡10=1.151\tfrac12\ln 10 = 1.151, whatever time you start from and whatever the skin, because the skin enters as a constant term. That is why a plot of pressure against the logarithm of time is a straight line.

  5. 5

    Why does the well radius not enter the formula for the pressure in the reservoir at distance rr from the well, but does enter the formula for the bottomhole pressure?

    Show the answer

    In the line-source solution the well is a line. The pressure in the reservoir depends only on the rate, the reservoir properties, the distance and the time. The bottomhole pressure is the same solution at the point r=rwr = r_w: the well radius appears as the distance at which we calculate the pressure. The smaller the radius, the closer to the axis we take the point, and the greater the pressure drop.

  6. 6

    A well has been started and the bottomhole pressure is held constant. How does its rate change while the disturbance has not reached the boundaries?

    1. A.It falls in inverse proportion to time
    2. B.It rises: the drawdown cone covers an ever greater volume
    3. C.It stays constant
    4. D.It falls roughly in inverse proportion to the logarithm of time
    Show the answer

    Correct answer: D. It falls roughly in inverse proportion to the logarithm of time

    The dimensionless rate is qD≈2/(ln⁡tD+0.809)q_D \approx 2/(\ln t_D + 0.809): the cone widens, the pressure difference is spread over a longer distance, the pressure gradient at the wall gets smaller, and the rate falls slowly. A linear decline, or a decline in inverse proportion to time, is not typical of radial inflow in an infinite reservoir.

Updated: 2 October 2026