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Well testingInflow to a well Advanced 24 min read

Inflow at high rates: non-Darcy flow

Non-Darcy (inertial) flow is flow in the reservoir at such high velocities that the pressure drop grows faster than the velocity. An inertial resistance adds to the viscous resistance of Darcy's law, because the fluid speeds up and slows down again in the twisting pore channels. Near a well these losses are concentrated right at the wall of the wellbore. They show up as an additional skin (a number that shows how much the zone right around the well hinders flow) that is proportional to the rate, DqDq.

Why it matters

Inertial losses are almost always noticeable in gas wells, and in high-rate oil wells that are open over a short interval. If we do not separate them out, we mistake the skin measured at a high rate for damage to the near-wellbore zone (the rock right around the well), and we order a treatment that does not help. The potential of the well (the most it could produce), estimated from a single rate, then comes out far too high. Tests at several rates separate the damage skin from the inertial skin. From these tests we draw the inflow performance line of a gas well (the line that shows the rate the well gives at each bottomhole pressure), and we choose the operating rate and the design of the well bottom.

Read first:Skin factor

Quick refresher

  • Darcy's law is the limit for slow flow. At high velocities an inertial term, βρv2\beta\rho v^2, adds to the viscous term. Their ratio is the Forchheimer number, Fo=kβρv/μ\text{Fo} = k\beta\rho v/\mu.
  • This is not turbulence. The flow in the pores stays laminar (smooth, with no chaotic swirling). The extra losses come from the fluid speeding up and slowing down in channels whose width keeps changing.
  • The viscous losses are spread evenly over the logarithm of the distance (each tenfold step in distance takes the same pressure drop). The inertial losses fall off as 1/r1/r: half of them occur in the ring out to 2rw2r_w, and 95% out to 20rw20r_w. So they behave like a skin, but a skin that is proportional to the rate.
  • The apparent skin (the skin that a test at rate qq shows) is S′=S+DqS' = S + Dq, where DqDq is the Forchheimer number at the wall of the well. For gas, DD includes the gas density at standard conditions and the viscosity at the bottom of the well.
  • We separate SS and DD with tests at several rates. A straight line of S′S' against qq has the intercept SS (where it meets the vertical axis) and the slope DD. A straight line of Δm/q\Delta m/q against qq gives the coefficients aa and bb of the two-term equation.
  • Damage to the near-wellbore zone and partial penetration make DD several times larger: β\beta grows as permeability falls, and the inertial losses grow as the square of the velocity at the wall.
Key relationships
− dp dx=μk v+βρ v2-\dfrac{\dd p}{\dd x} = \dfrac{\mu}{k}\,v + \beta\rho\,v^2

Forchheimer equation, consistent units

S′=S+Dq,D=βρsck2πhμwrwS' = S + Dq,\qquad D = \dfrac{\beta\rho_{sc}k}{2\pi h\mu_w r_w}

apparent skin of a gas well, qq at standard conditions

m(pˉ)−m(pwf)=a q+b q2m(\bar p) - m(p_{wf}) = a\,q + b\,q^2

two-term gas inflow equation in pseudo-pressures

a=U(ln⁡rerw−34+S),b=UD,U=1.290 Tkha = U\left(\ln\dfrac{r_e}{r_w} - \dfrac34 + S\right),\quad b = UD,\quad U = 1.290\,\dfrac{T}{kh}

metric units: qq in thousand m³/d, mm in MPa²/(mPa·s)

Common pitfalls
  • Treating the whole skin measured at a high rate in a gas well as damage, and planning an acid treatment (pumping acid in to clear the rock around the well) on that basis.
  • Estimating the absolute open flow from a single rate with Darcy's formula. The inertial losses grow as the square of the rate, so the potential comes out too high.
  • Using the gas density at reservoir conditions in DD together with a rate at standard conditions, or using the viscosity at reservoir pressure instead of bottomhole pressure.
  • Plotting Δm/q\Delta m/q against qq with transient flow periods (stretches of production at one rate, while the pressure is still changing) of different lengths. Each flow period has its own coefficient aa.
  • Taking β\beta from a correlation and applying it to a particular reservoir without a check. The scatter of the correlations is an order of magnitude (a factor of ten).

After this lesson you can

  • explain where the inertial losses in a porous medium come from and why they are not turbulence; write the Forchheimer equation, and use the Forchheimer number to judge when the losses cannot be ignored
  • describe how we measure the inertial resistance coefficient β\beta on core (rock samples taken from a well) and estimate it from correlations (formulas fitted to measured data), and what it depends on
  • derive the steady-state inflow (flow whose pressures no longer change with time) with an inertial term, show that these losses are concentrated at the wall of the well, and so arrive at a skin that grows with the rate: S′=S+DqS' = S + Dq
  • calculate the coefficient DD of a gas well in metric and in oilfield units, and write the two-term gas inflow equation using pseudo-pressure (a modified pressure that allows for the changing viscosity and compressibility of gas)
  • separate the skin from the inertial losses with a test at several rates, draw the stabilised inflow performance line, and find the absolute open flow (the rate the well would give at zero bottomhole pressure)
  • explain why damage to the near-wellbore zone, partial penetration (only part of the reservoir thickness is open) and perforation make the inertial losses many times larger

Why Darcy's law stops working

Darcy's law describes slow flow. All of the pressure drop goes into viscous friction (the fluid rubbing against itself and against the rock), so the drop is proportional to the Darcy velocity (the flow rate divided by the area it crosses; see Rock permeability). At high velocities the flow becomes non-Darcy. Pore channels are not straight tubes. The fluid squeezes through narrow throats, spreads out in the pores, goes round the grains and keeps changing direction. At every narrow point it has to speed up, and just after it has to slow down again. Part of the pressure drop is spent on this. That part is proportional not to the velocity but to its square, like the kinetic energy ρv2/2\rho v^2/2. At low velocities this part is negligible. At high velocities it is comparable with the viscous part, and it can even exceed it.

Forchheimer equation
− dp dx=μk v+βρ v2-\frac{\dd p}{\dd x} = \frac{\mu}{k}\,v + \beta\rho\,v^2
where:
  • vvDarcy velocity: the flow rate per unit cross-sectional area (not the velocity in the pores), m/s
  • μ\mudynamic viscosity of the fluid, Pa·s
  • kkpermeability, m²
  • β\betainertial resistance coefficient of the rock, m⁻¹
  • ρ\rhofluid density, kg/m³
  • xxcoordinate along the flow, m

Units: SI (any consistent system of units)

Holds when
  • The flow is single-phase (one fluid) and isothermal (constant temperature). At every point the velocity points along the pressure gradient (the direction in which pressure changes fastest).
  • β\beta is a property of the rock, like kk. We find it by experiment (see below).
  • As v→0v \to 0, the second term vanishes and the equation becomes Darcy's law.

The first term is the viscous resistance and the second is the inertial resistance. In Russian-language literature this equation is also called the two-term law of filtration. There the second term is sometimes written as ρv2/l\rho v^2/l, where l=1/βl = 1/\beta is called the macro-roughness coefficient.

The ratio of the second term to the first shows how large the inertial term is. This ratio is the Forchheimer number:

Forchheimer number
Fo=βρv2μv/k=kβρvμ\text{Fo} = \frac{\beta\rho v^2}{\mu v/k} = \frac{k\beta\rho v}{\mu}
where:
  • Fo\text{Fo}ratio of the inertial resistance to the viscous, —
  • k, β, ρ, v, μk,\ \beta,\ \rho,\ v,\ \muas in the Forchheimer equation, m², m⁻¹, kg/m³, m/s, Pa·s

Units: no units; the quantities are in consistent units

Holds when
  • This is an estimate at one point of the flow. Near a well, vv and Fo change with distance.

At Fo = 0.01 the pressure gradient is 1% larger than Darcy's law gives. At Fo = 0.1 it is 10% larger. At Fo > 1 the inertial resistance dominates. The same quantity is called the modified Reynolds number for a porous medium.

Why is it mainly gas that matters? While the correction is small, Darcy's law sets the velocity: v≈k∣ dp/ dx∣/μv \approx k|\dd p/\dd x|/\mu. We put this into the Forchheimer number. At a given pressure gradient, the number is then proportional to ρ/μ2\rho/\mu^2: the viscosity enters squared. Gas in the reservoir is tens of times less viscous than light oil, but only a few times less dense. So at the same pressure gradient, the Forchheimer number for gas is hundreds of times larger.

  • Gas and gas-condensate wells (gas-condensate is gas that drops out liquid as the pressure falls) — almost always. These are the wells where the inertial skin is measured in every test.
  • Oil and water wells — when permeability is high, viscosity is low and rates are high, especially if only part of the reservoir thickness is open.
  • Perforation tunnels (holes shot through the casing into the rock) and gravel packs (a ring of gravel that holds back sand) — the flow squeezes into a small area, so the velocities in them are much higher than in the reservoir (Effect of completion on inflow).
  • Hydraulic fractures with proppant (cracks made by pumping fluid at high pressure and held open by grains called proppant) — the inertial losses in the proppant pack reduce the effective conductivity of the fracture (Inflow to a hydraulically fractured well).
  • Gas injection wells and gas flow tests on core — the same physics with the flow in the opposite direction.

The inertial resistance coefficient

The inertial resistance coefficient β\beta (the beta factor) is a property of the rock, like permeability. It has units of one over length: m⁻¹ in SI and ft⁻¹ in oilfield units (1 ft⁻¹ = 3.281 m⁻¹). The more twisting, uneven and narrow the pore channels are, the larger β\beta is. So, on the whole, it grows as permeability falls.

We measure β\beta on core (rock samples taken from a well) by flowing gas through a sample at several rates. As the gas moves along the sample it expands, so the Darcy velocity changes. But the mass flux G=ρvG = \rho v — the mass of gas passing through a unit area per second — is the same in every cross-section. We write the Forchheimer equation using GG, multiply it by the gas density, ρ=pM/(ZRT)\rho = pM/(ZRT), and integrate over the length of the sample (add up the pressure changes along it). The result is a straight line:

Gas test on core: the linear form of the Forchheimer equation
M (p12−p22)2ZRT L μ G=1k+β Gμ\frac{M\,(p_1^2 - p_2^2)}{2ZRT\,L\,\mu\,G} = \frac{1}{k} + \beta\,\frac{G}{\mu}
where:
  • p1, p2p_1,\ p_2absolute pressures (measured from zero, not from atmospheric pressure) at the inlet and outlet of the sample, Pa
  • GGmass flux: the mass flow rate of gas divided by the cross-sectional area of the sample, kg/(m²·s)
  • MMmolar mass of the gas, kg/mol
  • RRuniversal gas constant, 8.314, J/(mol·K)
  • TTtemperature of the test, K
  • LLlength of the sample, m
  • μ, Z\mu,\ Zgas viscosity and gas deviation factor (the correction that makes the ideal gas law fit a real gas; at the pressures of the test Z≈1Z \approx 1), Pa·s, —

Units: SI; pressures absolute

Holds when
  • The flow is isothermal and single-phase. ZZ and μ\mu do not change over the range of pressures in the test.
  • Gas slippage (the Klinkenberg correction: gas molecules slip along the pore walls, so the rock looks more permeable than it is) is small. To make sure of this, the test is run with back pressure (pressure held at the outlet), so that the mean pressure in the sample is about a megapascal. Otherwise slippage is allowed for separately (Rock permeability).

Plot the left-hand side (vertical axis) against G/μG/\mu (horizontal axis). The test points fall on a straight line. It meets the vertical axis at 1/k1/k, and its slope is β\beta. We use the same device — plotting the pressure losses per unit of rate against the rate — in well tests too.

Worked examplePermeability and the coefficient β\beta from a core test
Given (assumed data)
Sample
length 4.0 cm, diameter 2.54 cm
Gas
nitrogen: MM = 0.02801 kg/mol, μ\mu = 0.0178 mPa·s at 25 °C (298.15 K), Z=1Z = 1
Outlet pressure p2p_2
0.6000 MPa (absolute; held by a back-pressure regulator so that gas slippage is small)
Mass flux GG in four tests
0.05; 0.15; 0.30; 0.45 kg/(m²·s)
Inlet pressure p1p_1
0.6464; 0.7490; 0.9192; 1.1007 MPa (absolute)
Solution
  1. For each test, calculate the horizontal value X=G/μX = G/\mu and the vertical value YY — the left-hand side of the formula (pressures in pascals, μ=1.78⋅10−5\mu = 1.78\cdot10^{-5} Pa·s). Test 1: X1=2809X_1 = 2809 m⁻¹, Y1=9.178⋅1012Y_1 = 9.178\cdot10^{12} m⁻². Test 4: X4=25,281X_4 = 25{,}281 m⁻¹, Y4=15.015⋅1012Y_4 = 15.015\cdot10^{12} m⁻².
  2. Tests 2 and 3 give Y=10.633⋅1012Y = 10.633\cdot10^{12} and 12.826⋅101212.826\cdot10^{12} m⁻². These points lie on the same straight line.
  3. Find the slope from the first and last tests: β=(Y4−Y1)/(X4−X1)\beta = (Y_4 - Y_1)/(X_4 - X_1) =2.60⋅108= 2.60\cdot10^{8} m⁻¹.
  4. Find the intercept on the vertical axis: 1/k=Y1−βX1=8.448⋅10121/k = Y_1 - \beta X_1 = 8.448\cdot10^{12} m⁻². So k=1.184⋅10−13k = 1.184\cdot10^{-13} m² =120= 120 mD.
  5. Now the Forchheimer number. In test 1, Fo=kβG/μ=0.086\text{Fo} = k\beta G/\mu = 0.086. In test 4 it is 0.78, so the inertial resistance is 78% of the viscous resistance.
Answer: The permeability of the sample is about 120 mD, the inertial resistance coefficient about 2.60·10⁸ m⁻¹.

What it means. If we calculated the permeability by Darcy's law from test 4 alone, we would get 1/Y41/Y_4, which is 44% lower. The inertial losses would be “hidden” in a permeability that is too low. That is why gas permeability is measured at low rates, and β\beta is found from the slope over several rates. The correlation given below gives 2.4·10⁸ m⁻¹ for 120 mD, which is the same order of magnitude (the same power of ten). The data in this example are assumed for illustration.

When there is no core, we estimate β\beta from correlations (formulas fitted to measurements on many samples) with permeability, and sometimes with porosity as well. A widely used one for consolidated rocks (rocks whose grains are cemented together) is:

Correlation of the inertial resistance coefficient with permeability
β=7.64⋅1010k1.201\beta = \frac{7.64\cdot10^{10}}{k^{1.201}}
where:
  • β\betainertial resistance coefficient, m⁻¹
  • kkpermeability of the rock, mD

Units: empirical: β\beta in m⁻¹, kk in mD

Holds when
  • The rocks are consolidated and the gas flow is single-phase. Measurements scatter around the correlation by up to an order of magnitude (a factor of ten).
  • Irreducible water (water held in the rock that cannot be produced) or condensate that has dropped out narrows the channels. Then β\beta for gas increases, sometimes several times over.

β\beta is roughly proportional to k−1.2k^{-1.2}: a rock ten times less permeable has a β\beta 16 times larger. The correlation is good for a first estimate. For a project, we find β\beta (or, better still, the coefficient DD of the well) from core and well tests.

In other unit systems (1)
Oilfield units
β [ft−1]=2.33⋅1010k [mD]1.201\beta\,[\text{ft}^{-1}] = \frac{2.33\cdot10^{10}}{k\,[\text{mD}]^{1.201}}

β\beta in ft⁻¹, kk in mD.

7.64⋅1010=3.281⋅2.33⋅10107.64\cdot10^{10} = 3.281\cdot2.33\cdot10^{10}, where 3.281 converts ft⁻¹ to m⁻¹.

The order of magnitude of β\beta from the correlation
kk, mD
1
β\beta, m⁻¹
7.6⋅10107.6\cdot10^{10}
β\beta, ft⁻¹
2.3⋅10102.3\cdot10^{10}
kk, mD
10
β\beta, m⁻¹
4.8⋅1094.8\cdot10^{9}
β\beta, ft⁻¹
1.5⋅1091.5\cdot10^{9}
kk, mD
100
β\beta, m⁻¹
3.0⋅1083.0\cdot10^{8}
β\beta, ft⁻¹
9.2⋅1079.2\cdot10^{7}
kk, mD
1000
β\beta, m⁻¹
1.9⋅1071.9\cdot10^{7}
β\beta, ft⁻¹
5.8⋅1065.8\cdot10^{6}

The values are only a guide. At the same permeability, different rocks differ by a factor of several.

Inertial losses at the well: a skin that grows with the rate

Near a well the Darcy velocity increases towards the wellbore. The whole flow passes through the side surface of a cylinder of radius rr, so v=q/(2πrh)v = q/(2\pi rh). The viscous term of the Forchheimer equation grows towards the well as 1/r1/r, and the inertial term grows as 1/r21/r^2. We put this velocity into the equation and integrate from the wall of the well to the outer boundary, as in the derivation of the Dupuit equation (Steady-state radial flow):

Steady-state radial flow with inertial losses
pe−pw=qμ2πkhln⁡rerw+βρq2(2πh)2(1rw−1re)p_e - p_w = \frac{q\mu}{2\pi kh}\ln\frac{r_e}{r_w} + \frac{\beta\rho q^2}{(2\pi h)^2}\left(\frac{1}{r_w} - \frac{1}{r_e}\right)
where:
  • qqflow rate at reservoir conditions; for a liquid q=qsBq = q_s B, m³/s
  • pe, pwp_e,\ p_wpressure at the outer boundary and at the wall of the well, Pa
  • re, rwr_e,\ r_wradius of the outer boundary and radius of the well, m
  • k, h, μk,\ h,\ \mupermeability, reservoir thickness, viscosity, m², m, Pa·s
  • β, ρ\beta,\ \rhoinertial resistance coefficient and fluid density, m⁻¹, kg/m³

Units: SI; ln⁡\ln is the natural logarithm

Holds when
  • The inflow is steady-state and single-phase, and the liquid is slightly compressible (we treat gas below, through the mass flow rate).
  • The reservoir is homogeneous (the same everywhere). The well is an open hole (not cased or perforated) over the whole thickness. β\beta and ρ\rho are constant.

The drawdown (the pressure difference that drives the flow) is no longer proportional to the rate. A term proportional to q2q^2 adds to the term proportional to qq (the Dupuit equation). If the rate doubles, the viscous losses double and the inertial losses grow fourfold.

What matters most is where the pressure is lost. Here are the shares of the viscous and the inertial losses that fall on the ring between the wall of the well and the radius rr:

Shares of viscous and inertial losses within radius rr
δvisc(r)=ln⁡(r/rw)ln⁡(re/rw),δinert(r)=1/rw−1/r1/rw−1/re≈1−rwr\delta_{\text{visc}}(r) = \frac{\ln(r/r_w)}{\ln(r_e/r_w)},\qquad \delta_{\text{inert}}(r) = \frac{1/r_w - 1/r}{1/r_w - 1/r_e} \approx 1 - \frac{r_w}{r}
where:
  • δvisc, δinert\delta_{\text{visc}},\ \delta_{\text{inert}}the viscous and inertial pressure losses between rwr_w and rr, each as a share of the corresponding losses between rwr_w and rer_e, —
  • rrdistance from the well axis, m

Units: no units; radii in the same units

Holds when
  • Steady-state radial flow, as in the previous formula. The approximate equality holds when re≫rwr_e \gg r_w.

Half of the inertial losses fall on the ring from rwr_w to 2rw2r_w, 90% within 10rw10r_w and 95% within 20rw20r_w. For a typical well, that is within two metres of the axis. The viscous losses are spread much more widely: only about a third of them fall on the same two metres.

Shares of viscous and inertial pressure losses within a distance from the axis of the gas well0.1110100020406080100Distance from the well axis r, mShare of losses within r, %r = 0.22 m: 50%inertialviscous

Graph. The horizontal axis shows the distance from the well axis, from 0.1 to 500 metres, on a logarithmic scale. The vertical axis shows the share of the losses, from 0 to 100 per cent. The curve of the inertial losses rises steeply near the well: 50 per cent at a distance of 0.22 metres and about 90 per cent by one metre. The curve of the viscous losses is almost a straight line against the logarithm of the distance. It reaches 50 per cent only at about 7 metres.

CalculatedCalculated shares of the viscous and the inertial pressure losses within the distance rr from the axis of the lesson's well (rwr_w = 0.108 m, rer_e = 500 m). Almost all the inertial losses occur in the first metre.

The inertial losses are concentrated in a thin ring at the wellbore. So it is convenient to count them as part of the skin (Skin factor) — a skin that grows with the rate (the non-Darcy coefficient). We divide the inertial term by the “unit” of radial pressure drop, qμ/(2πkh)q\mu/(2\pi kh):

Rate-dependent skin
pe−pwf=qμ2πkh(ln⁡rerw+S+Dq),D=βρk2πhμrwp_e - p_{wf} = \frac{q\mu}{2\pi kh}\left(\ln\frac{r_e}{r_w} + S + Dq\right),\qquad D = \frac{\beta\rho k}{2\pi h\mu r_w}
where:
  • SSskin that does not depend on the rate: damage to the near-wellbore zone, geometry of penetration, perforation, —
  • DDnon-Darcy coefficient: the coefficient of the inertial skin, s/m³
  • DqDqinertial skin at the rate qq, —
  • pwfp_{wf}bottomhole flowing pressure of the producing well, Pa
  • q, μ, k, h, β, ρ, re, rwq,\ \mu,\ k,\ h,\ \beta,\ \rho,\ r_e,\ r_was in the formula above; qq is at reservoir conditions, SI

Units: SI; ln⁡\ln is the natural logarithm

Holds when
  • re≫rwr_e \gg r_w, so the term 1/re1/r_e is dropped.
  • The well is an open hole over the whole thickness, and β\beta at the wellbore is the same as in the reservoir. With damage and with partial penetration, DD is larger (see the last section).

The skin S′=S+DqS' = S + Dq that a test measures is called the apparent skin. The product DqDq is the Forchheimer number at the wall of the well: Dq=kβρvw/μDq = k\beta\rho v_w/\mu, where vw=q/(2πrwh)v_w = q/(2\pi r_w h) is the velocity at the wall. The inertial skin is large when the flow right at the wall is already clearly non-linear.

In other unit systems (2)
Metric oilfield units (liquid)
D [1/(m3/d)]=1.818⋅10−18 β ρ B kh μ rwD\,[1/(\text{m}^3/\text{d})] = 1.818\cdot10^{-18}\,\frac{\beta\,\rho\,B\,k}{h\,\mu\,r_w}

β\beta in m⁻¹, ρ\rho in kg/m³, BB in m³/m³, kk in mD, hh and rwr_w in m, μ\mu in mPa·s; qq in m³/d at standard conditions.

1.818⋅10−181.818\cdot10^{-18} is 0.9869⋅10−150.9869\cdot10^{-15} divided by 86,400⋅2π⋅10−386{,}400\cdot2\pi\cdot10^{-3}. It converts mD to m², days to seconds and mPa·s to Pa·s.

Oilfield units (liquid)
D [1/(STB/d)]=1.021⋅10−14 β ρ B kh μ rwD\,[1/(\text{STB/d})] = 1.021\cdot10^{-14}\,\frac{\beta\,\rho\,B\,k}{h\,\mu\,r_w}

β\beta in ft⁻¹, ρ\rho in g/cm³, BB in rb/STB (reservoir barrels per stock-tank barrel), kk in mD, hh and rwr_w in ft, μ\mu in cP; qq in STB/d (stock-tank barrels per day).

The same unit conversion as in the SI formula.

For gas, the density and the volume flow rate both change along the flow path. But their product, the mass flow rate, is the same at all radii. So the formula for a gas well uses the rate at standard conditions and the gas density at the same conditions. The viscosity is taken at the bottom of the well, where the inertial losses are concentrated (the derivation is in the advanced section):

Non-Darcy coefficient of a gas well
D=β ρsc k2πh μw rwD = \frac{\beta\,\rho_{sc}\,k}{2\pi h\,\mu_w\,r_w}
where:
  • DDnon-Darcy coefficient per unit of gas rate at standard conditions, s/m³
  • ρsc\rho_{sc}gas density at standard conditions: 1.204 γg1.204\,\gamma_g at 20 °C (γg\gamma_g is the gas specific gravity relative to air, that is, the gas density divided by the air density), kg/m³
  • μw\mu_wgas viscosity at the bottomhole pressure and reservoir temperature, Pa·s
  • β, k, h, rw\beta,\ k,\ h,\ r_was above, m⁻¹, m², m, m

Units: SI

Holds when
  • The mass flow rate is the same at all radii, and the inflow is isothermal.
  • The inertial losses are concentrated at the wellbore, so the viscosity is taken at the bottomhole pressure.
  • The well is an open hole over the whole thickness, and the near-wellbore zone is undamaged.

The only quantity that depends on pressure is the viscosity at the bottom of the well. Over the range of rates in an ordinary test it changes by about 10%. So we take the DD of a gas well as constant, as long as the penetration and the condition of the near-wellbore zone do not change. Tests measure exactly this DD.

In other unit systems (2)
Metric oilfield units
D [1/(thousand m3/d)]=1.818⋅10−15 β ρsc kh μw rwD\,[1/(\text{thousand m}^3/\text{d})] = 1.818\cdot10^{-15}\,\frac{\beta\,\rho_{sc}\,k}{h\,\mu_w\,r_w}

β\beta in m⁻¹, ρsc\rho_{sc} in kg/m³ (20 °C, 0.101325 MPa), kk in mD, hh and rwr_w in m, μw\mu_w in mPa·s; the rate is in thousand m³/d.

This is a thousand times the constant for a liquid, because the rate is in thousands of cubic metres.

Oilfield units
D [1/(Mscf/d)]=2.71⋅10−15 β k M psch μw rw TscD\,[1/(\text{Mscf/d})] = 2.71\cdot10^{-15}\,\frac{\beta\,k\,M\,p_{sc}}{h\,\mu_w\,r_w\,T_{sc}}

β\beta in ft⁻¹, kk in mD, MM in g/mol, pscp_{sc} in psia (pounds per square inch, absolute), TscT_{sc} in °R (degrees Rankine, the absolute temperature scale that goes with °F), hh and rwr_w in ft, μw\mu_w in cP; the rate is in thousand standard cubic feet per day.

The density at standard conditions is written as pscM/(RTsc)p_{sc}M/(RT_{sc}). The constant comes from converting the units.

Worked exampleInertial skin of a gas well from rock properties
Given (assumed data)
Reservoir
kk = 30 mD, hh = 12 m, the wellbore is open over the whole thickness, no damage
Well
rwr_w = 0.108 m; radius of the drainage area 500 m
Gas
the gas from the lesson on gas properties: γg\gamma_g = 0.65, reservoir temperature 80 °C
Rate
600 thousand m³/d at a bottomhole pressure of about 17 MPa
β\beta
from the correlation with permeability
Solution
  1. β=7.64⋅1010/301.201\beta = 7.64\cdot10^{10}/30^{1.201} =1.286⋅109= 1.286\cdot10^{9} m⁻¹.
  2. The gas density at standard conditions is ρsc=1.204⋅0.65=0.7826\rho_{sc} = 1.204\cdot0.65 = 0.7826 kg/m³. The gas viscosity at 17 MPa and 80 °C is μw=0.01794\mu_w = 0.01794 mPa·s.
  3. The numerator is βρsck=1.286⋅109⋅0.7826⋅30\beta\rho_{sc}k = 1.286\cdot10^{9}\cdot0.7826\cdot30 =3.019⋅1010= 3.019\cdot10^{10}, and the denominator is hμwrw=12⋅0.01794⋅0.108=0.02325h\mu_w r_w = 12\cdot0.01794\cdot0.108 = 0.02325. So D=1.818⋅10−15⋅3.019⋅1010/0.02325D = 1.818\cdot10^{-15}\cdot3.019\cdot10^{10}/0.02325 =2.36⋅10−3= 2.36\cdot10^{-3} (thousand m³/d)⁻¹.
  4. The inertial skin is Dq=2.36⋅10−3⋅600=1.42Dq = 2.36\cdot10^{-3}\cdot600 = 1.42.
  5. Check through the velocity at the wall. The mass flow rate is 5.435.43 kg/s, so the mass flux is Gw=5.43/(2π⋅0.108⋅12)=0.667G_w = 5.43/(2\pi\cdot0.108\cdot12) = 0.667 kg/(m²·s), and Fow=kβGw/μw=1.42\text{Fo}_w = k\beta G_w/\mu_w = 1.42. This is the same number.
  6. For an undamaged well in pseudo-steady state (the flow regime after the pressure disturbance has reached the boundaries), the logarithmic term is ln⁡(500/0.108)−0.75=7.690\ln(500/0.108) - 0.75 = 7.690. The share of the inertial skin in the resistance is 1.42/(7.690+1.42)=161.42/(7.690 + 1.42) = 16%.
Answer: D≈2.36⋅10−3D \approx 2.36\cdot10^{-3} (thousand m³/d)⁻¹. At 600 thousand m³/d the inertial skin of 1.42 is about 16% of the resistance of an undamaged well.

What it means. At the wall itself, the inertial resistance is 1.42 times the viscous resistance. But the Forchheimer number falls as 1/r1/r: at one metre from the axis it is about 0.15, and at ten metres about 0.015. This is an estimate for an open hole, made with a correlation. In real wells DD is usually larger. The flow squeezes into the perforation tunnels, the near-wellbore zone is damaged, and not the whole thickness works (see the last section). That is why DD is measured. The data in this example are assumed for illustration.

Gas inflow: the two-term equation in pseudo-pressures

The viscosity and the gas deviation factor ZZ change with pressure. So, as with Darcy's law, we integrate the Forchheimer equation for gas in terms of the pseudo-pressure m(p)=2∫p  dp/(μZ)m(p) = 2\int p\,\dd p/(\mu Z) (real gas pseudo-pressure; for its properties see Gas formation volume factor, compressibility and viscosity). Pseudo-pressure is a modified pressure that allows for these changes. The derivation is in the advanced section. Once the pressure disturbance has reached the boundaries of the drainage area (the area from which the well takes its fluid) and the inflow has become pseudo-steady-state (Pseudo-steady-state flow and the shape factor), the result is the two-term inflow equation:

Two-term gas inflow equation in pseudo-pressures
m(pˉ)−m(pwf)=a q+b q2a=U(ln⁡rerw−34+S),b=UDU=psc Tπkh Tsc\begin{gathered} m(\bar p) - m(p_{wf}) = a\,q + b\,q^2\\ a = U\left(\ln\frac{r_e}{r_w} - \frac34 + S\right),\qquad b = U D\\ U = \frac{p_{sc}\,T}{\pi kh\,T_{sc}}\end{gathered}
where:
  • m(p)m(p)gas pseudo-pressure, Pa²/(Pa·s)
  • pˉ, pwf\bar p,\ p_{wf}average pressure in the drainage area and bottomhole flowing pressure, absolute, Pa
  • qqgas rate at standard conditions, m³/s
  • UUthe “unit” of pseudo-pressure drop in radial inflow, Pa²/(Pa·s)/(m³/s)
  • T, Tsc, pscT,\ T_{sc},\ p_{sc}reservoir temperature, and temperature and pressure at standard conditions, K, K, Pa
  • a, ba,\ bviscous and inertial flow resistance coefficients, by the formulas
  • S, DS,\ Dthe rate-independent skin and the non-Darcy coefficient, —, s/m³

Units: SI; pressures absolute; ln⁡\ln is the natural logarithm

Holds when
  • The inflow is pseudo-steady-state, in a circular area with the well at the centre. For another shape of area we change the logarithmic term, as in the lesson on pseudo-steady-state flow.
  • Using m(pˉ)m(\bar p) instead of the volume-averaged pseudo-pressure is the usual approximation.
  • DD is taken with the gas viscosity at the bottom of the well. The gas in the reservoir is single-phase.

The coefficient aa is the resistance of the reservoir and the near-wellbore zone according to Darcy's law, and bb is the inertial resistance. In Russian-language practice they are known as the flow resistance coefficients. As long as μZ\mu Z is almost constant (for the gas of the lesson, up to about 10 MPa), Δm≈Δ(p2)/(μZ)\Delta m \approx \Delta(p^2)/(\mu Z). Then the equation becomes the two-term equation with squared pressures from the lesson Inflow performance relationship (IPR). Its coefficients AA and BB are aa and bb multiplied by μZ\mu Z.

In other unit systems (2)
Metric oilfield units
U=1.290 TkhU = 1.290\,\frac{T}{kh}

mm in MPa²/(mPa·s), qq in thousand m³/d at 20 °C and 0.101325 MPa, TT in K, kk in mD, hh in m; aa in MPa²/(mPa·s) per thousand m³/d, bb per (thousand m³/d)².

1.2901.290 is 1000⋅0.1013251000\cdot0.101325 divided by π⋅0.0853⋅293.15\pi\cdot0.0853\cdot293.15. Here 0.0853 is the constant of Darcy's law in these units.

Oilfield units
U=1422 TkhU = 1422\,\frac{T}{kh}

mm in psi²/cP, qq in Mscf/d (thousand standard cubic feet per day; standard conditions are 14.7 psia and 60 °F), TT in °R, kk in mD, hh in ft.

The same constant 1422 as in the formula for steady-state gas inflow (Steady-state radial flow).

We solve the quadratic equation for the rate. The absolute open flow (AOF) is the conventional rate at a bottomhole pressure equal to atmospheric pressure. We find it from the same formula:

Rate of a gas well from the two-term equation
q=−a+a2+4b Δm2b,Δm=m(pˉ)−m(pwf)q = \frac{-a + \sqrt{a^2 + 4b\,\Delta m}}{2b},\qquad \Delta m = m(\bar p) - m(p_{wf})
where:
  • qqgas rate at standard conditions, thousand m³/d
  • Δm\Delta mpseudo-pressure drop between the drainage area and the bottom of the well, MPa²/(mPa·s)
  • a, ba,\ bcoefficients of the two-term equation, by the formula above
  • qmaxq_{max}absolute open flow: qq at Δmmax=m(pˉ)−m(patm)\Delta m_{max} = m(\bar p) - m(p_{\text{atm}}), thousand m³/d

Units: metric oilfield (or any units consistent with aa and bb)

Holds when
  • The inflow is stabilised (the pressures no longer change with time) and the coefficients aa and bb are known. For b=0b = 0 the formula becomes q=Δm/aq = \Delta m/a.

Without the inertial term, the inflow performance line (with qq along the horizontal axis and Δm\Delta m along the vertical axis) would be a straight line. With the inertial term the line bends, and each further step of the drawdown gives a smaller increase in rate.

Tests at several rates: how to separate SS and DD

A test at one rate gives one apparent skin, S′=S+DqS' = S + Dq, which is the sum of two unknowns. To separate them, we test the well at several rates that differ clearly, best of all by a factor of two or three. We process the results in one of two ways.

From the skins of the flow periods. We interpret the pressure record of each flow period in the usual way, but in pseudo-pressures (Pressure drawdown analysis, Pressure build-up analysis). The record is the drawdown while the well flows, or the build-up after shut-in. This gives the flow capacity khkh (permeability times thickness) and the apparent skin Sj′S'_j. The points fall on a straight line:

Apparent skin of the flow periods
Sj′=S+D qjS'_j = S + D\,q_j
where:
  • Sj′S'_japparent skin of the jj-th flow period, from interpreting its pressure record, —
  • qjq_jrate of the jj-th flow period (for a build-up, the rate before shut-in), thousand m³/d
  • S, DS,\ Dintercept on the vertical axis and slope of the line, —, (thousand m³/d)⁻¹

Units: any; DD is in units that are the inverse of the rate units

Holds when
  • All flow periods are interpreted with one reservoir model, and the flow capacity khkh is the same for all of them.
  • The skin and DD do not change during the test (the well has already been cleaned up after completion).

The inertial pressure drop vanishes at once when the well is shut in, like any pressure drop across a skin. So the skin from a build-up curve contains the DqDq of the rate at which the well was flowing before shut-in.

From the inflow performance line. We divide the two-term equation by the rate: Δm/q=a+bq\Delta m/q = a + bq. If we plot the points of the flow periods with qq on the horizontal axis and Δm/q\Delta m/q on the vertical axis, they fall on a straight line with slope bb and intercept aa. But this is true only if the coefficient aa is the same for all flow periods. While the inflow is transient (the pressure disturbance is still spreading), aa contains a logarithmic term that grows with time, instead of ln⁡(re/rw)−3/4\ln(r_e/r_w) - 3/4. So it is different for flow periods of different lengths. This gives three kinds of test:flow-after-flow, isochronal and modified isochronal.

Multi-rate tests of gas wells
Type of test
Flow-after-flow
How it is run
3–5 flow periods one after another, each until the pressure stabilises
What it gives
aa and bb; in a tight reservoir (one with very low permeability) it takes a very long time
Type of test
Isochronal
How it is run
flow periods of equal length, with the pressure building up fully between them, plus one long flow period
What it gives
bb from the short flow periods, aa from the long one
Type of test
Modified isochronal
How it is run
flow periods and shut-ins of equal length
What it gives
about the same; the pressure before the flow period is used instead of pˉ\bar p

In Russian-language practice the first kind is called the method of steady-state withdrawals. Stabilisation means that the flow has reached the pseudo-steady-state regime. For a well at the centre of a circular area this happens at kt/(ϕμctA)≈0.1kt/(\phi\mu c_tA) \approx 0.1. For the well of the lesson (30 mD, area radius 500 m) that is about three days. In a similar reservoir with a permeability of 3 mD it is about a month.

Isochronal test: ratio of pseudo-pressure drop to rate for 6-hour flow periods and the stabilised line01002003004005006007001011121314151617Gas rate q, thousand m³/dΔm/q, MPa²/(mPa·s) per 10³ m³/dstabilised flow6 h flow periodsa(6 h) = 10.9a = 11.8; b = 6.94·10⁻³

Graph. The horizontal axis is the gas rate, from 0 to 700 thousand cubic metres per day. The vertical axis is the pseudo-pressure drop divided by the rate, from 10 to 17. Four points for the 6-hour flow periods, at 200, 350, 500 and 650 thousand cubic metres, with values 12.4, 13.3, 14.3 and 15.5, lie on a dashed straight line. It rises from 10.9 at zero rate to 15.8 at 700. The solid stabilised line runs parallel to it and 0.9 higher, from 11.8 to 16.6.

CalculatedAn isochronal test of the lesson's well, plotted as Δm/q\Delta m/q against the rate (calculated with the lesson's model). The points of four 6-hour flow periods lie on a line with slope bb. The stabilised line is parallel to it and lies higher by the difference of the logarithmic terms.
Worked exampleDamage skin and the coefficient DD from an isochronal test
Given (assumed data)
Well
the lesson's well (see the example above): kk = 30 mD, hh = 12 m, rwr_w = 0.108 m, the lesson gas, 80 °C
Test
four flow periods of 6 h each; after each one the well is shut in until the pressure recovers to 20 MPa
Rates qjq_j
200; 350; 500; 650 thousand m³/d
Interpretation of the flow periods in pseudo-pressures
khkh = 360 mD·m for all flow periods; apparent skins 2.76; 3.48; 4.32; 5.22
Solution
  1. The averages are qˉ=425\bar q = 425 thousand m³/d and Sˉ′=3.945\bar S' = 3.945.
  2. The slope from the first and last flow periods is D≈(5.22−2.76)/(650−200)D \approx (5.22 - 2.76)/(650 - 200) =5.47⋅10−3= 5.47\cdot10^{-3}. From all four flow periods (by least squares, the best-fit straight line) D=5.48⋅10−3D = 5.48\cdot10^{-3} (thousand m³/d)⁻¹.
  3. The intercept is S=Sˉ′−DqˉS = \bar S' - D\bar q =3.945−5.48⋅10−3⋅425= 3.945 - 5.48\cdot10^{-3}\cdot425 =1.62= 1.62.
  4. The estimate of DD for an open, undamaged hole (the example above) is 2.36⋅10−32.36\cdot10^{-3}. The measured DD is 2.3 times larger.
  5. At a rate of 650 thousand m³/d the inertial skin Dq=3.56Dq = 3.56 is 68% of the apparent skin 5.22.
Answer: The rate-independent skin is about 1.62. The non-Darcy coefficient is D≈5.48⋅10−3D \approx 5.48\cdot10^{-3} (thousand m³/d)⁻¹.

What it means. Damage and perforation give a small skin, about 1.62. But the apparent skin of 5.22 at the highest flow period is more than half inertial. An acid treatment would reduce only SS. The measured DD is 2.3 times larger than the estimate for an open hole. This may point to a constriction of the inflow near the well: the flow squeezes into the perforation tunnels, and part of the interval may not be working. But the correlation for β\beta scatters widely, so such a difference is not yet proof. The working interval is checked by production logging (a survey run in the producing well that shows where the fluid enters). The scatter of the points about the line is the usual error of interpretation, so we take at least three or four flow periods. The data in this example are assumed for illustration.

Apparent skin of the flow periods of an isochronal test against rate01002003004005006007000123456Gas rate q, thousand m³/dApparent skin S′S = 1.62slope D = 5.48·10⁻³open hole

Graph. The horizontal axis is the gas rate, from 0 to 700 thousand cubic metres per day. The vertical axis is the apparent skin, from 0 to 6. Four points at 200, 350, 500 and 650 thousand cubic metres, with skins 2.76, 3.48, 4.32 and 5.22, lie almost on a straight line that crosses the skin axis at about 1.6. A dashed straight line from the same point rises much more slowly, to about 3.3 at 700 thousand cubic metres.

CalculatedThe apparent skins of the four flow periods of the example, and the least-squares line (the best-fit straight line). The intercept on the vertical axis is the rate-independent skin SS, and the slope is DD. The dashed line shows the same skin with the DD of an open, undamaged hole.
How to plan a multi-rate test
  1. 1
    Clean up the well

    The skin must stay constant during the test. After completion, flow the well until all the mud filtrate (the liquid that leaked into the rock from the drilling fluid) has been produced and the rate is stable.

  2. 2
    Choose the rates

    Use 3–4 flow periods, usually with the rate increasing from one to the next. The largest rate is two to three times the smallest, but it must not cause sand production or destroy the near-wellbore zone.

  3. 3
    Choose the duration

    If there is enough time for each rate to stabilise, run the flow periods one after another. If not, use an isochronal scheme: flow periods of equal length and one long flow period.

  4. 4
    Record the pressure and the rate

    Use bottomhole gauges and measure the rate in every flow period. Record the pressure at the end of each flow period and during the shut-ins.

  5. 5
    Process in two ways

    Plot the skins of the flow periods against the rate, and plot Δm/q\Delta m/q against the rate. Agreement between the two estimates of DD is a quality check.

The inflow performance line of a gas well and the absolute open flow

Once SS and DD are known, and khkh has been found from the same pressure records, we can calculate the stabilised inflow performance line without waiting for the flow to stabilise. The formula with ln⁡(re/rw)−3/4\ln(r_e/r_w) - 3/4, for the drainage area of the well, gives the coefficient aa, and the product UDUD gives bb. We do the same in an isochronal test that has no long flow period.

Worked exampleStabilised inflow performance line of the lesson's well
Given (assumed data)
Test results (the example above)
SS = 1.616 (before rounding), DD = 5.48·10⁻³ (thousand m³/d)⁻¹, khkh = 360 mD·m
Drainage area
circular, rer_e = 500 m; rwr_w = 0.108 m; average pressure 20 MPa; 80 °C (353.15 K)
Pseudo-pressure of the lesson gas at 80 °C
mm(20 MPa) = 27,699; mm(15 MPa) = 16,573; mm(0.1013 MPa) = 0.8 MPa²/(mPa·s)
Solution
  1. U=1.2903⋅353.15/360=1.2657U = 1.2903\cdot353.15/360 = 1.2657 (the constant 1.290 with one more digit).
  2. Then ln⁡(500/0.108)=8.440\ln(500/0.108) = 8.440, a=1.2657⋅(8.440−0.75+1.616)a = 1.2657\cdot(8.440 - 0.75 + 1.616) =11.779= 11.779, and b=UD=6.936⋅10−3b = UD = 6.936\cdot10^{-3}.
  3. Take a bottomhole pressure of 15 MPa. Then Δm=27,699−16,573=11,126\Delta m = 27{,}699 - 16{,}573 = 11{,}126, and a2+4bΔm=447.4a^2 + 4b\Delta m = 447.4, whose square root is 21.152. So q=(21.152−11.779)/(2b)q = (21.152 - 11.779)/(2b) =676= 676 thousand m³/d. Without the inertial losses it would be Δm/a=945\Delta m/a = 945 thousand m³/d.
  4. For the absolute open flow, Δmmax=27,699−0.8=27,698\Delta m_{max} = 27{,}699 - 0.8 = 27{,}698. This gives qmax=1322q_{max} = 1322 thousand m³/d. Without the inertial losses it would be 23512351.
  5. At the 15 MPa flow period the inertial skin, Dq=3.70Dq = 3.70, is comparable with a/U=ln⁡(re/rw)−0.75+S=9.31a/U = \ln(r_e/r_w) - 0.75 + S = 9.31.
  6. If we draw a straight line through this single flow period, as for a liquid (qq proportional to Δm\Delta m), we get qmax=27,698⋅676/11,126q_{max} = 27{,}698\cdot676/11{,}126 =1683= 1683 thousand m³/d.
Answer: At a bottomhole pressure of 15 MPa the well will give about 676 thousand m³/d. The absolute open flow is about 1322 thousand m³/d.

What it means. The inertial losses reduce the rate at a drawdown of 5 MPa by 28%, and they reduce the absolute open flow by 44%. The larger the drawdown, the larger their effect. A straight line through a single flow period would overestimate the absolute open flow by 27%. A calculation without inertial losses would overestimate it by a factor of 1.8. The absolute open flow is only a conventional measure of potential. The real rate is limited by the tubing, by sand production and by water cones (water drawn up towards the well in the shape of a cone; Nodal analysis of the production system). The data in this example are assumed for illustration.

Stabilised inflow performance line of a gas well with and without inertial losses0500100015002000250005101520Gas rate q, thousand m³/dBottomhole pressure pwf, MPa676 at 15 MPawith inertial lossesAOF 1322by Darcy's lawAOF 2351

Graph. The horizontal axis is the gas rate, from 0 to 2500 thousand cubic metres per day. The vertical axis is the bottomhole pressure, from 0 to 20 megapascals. Both curves start at 20 megapascals and zero rate. The solid curve, with inertial losses, falls more steeply and reaches atmospheric pressure at 1322 thousand cubic metres. The dashed curve, by Darcy's law, reaches it at 2351. The point of 676 thousand cubic metres at 15 megapascals is marked.

CalculatedThe calculated stabilised inflow performance line of the lesson's well (average pressure 20 MPa), with inertial losses and without them (by Darcy's law). The points mark the rate at a bottomhole pressure of 15 MPa and the absolute open flows.

What increases the inertial losses at a well

The formulas for DD above apply to an open hole in an undamaged reservoir. Anything that raises the velocity at the wall, or raises β\beta where the velocity is highest, increases DD — usually several times over.

A damaged zone. The permeability in it is lower, so β\beta, which is roughly proportional to k−1.2k^{-1.2}, is higher. And the velocity is highest right at the wall. Suppose that in a ring of radius rsr_s the permeability is reduced to ksk_s and the inertial resistance coefficient has grown to βs\beta_s. If we repeat the integration over the two rings, we get:

Apparent skin with a damaged zone
S′=(kks−1)ln⁡rsrw+Dq,D=D0[βsβ(1−rwrs)+rwrs]S' = \left(\frac{k}{k_s} - 1\right)\ln\frac{r_s}{r_w} + Dq,\qquad D = D_0\left[\frac{\beta_s}{\beta}\left(1 - \frac{r_w}{r_s}\right) + \frac{r_w}{r_s}\right]
where:
  • ks, βsk_s,\ \beta_spermeability and inertial resistance coefficient of the damaged zone, mD, m⁻¹
  • rsr_sradius of the damaged zone, m
  • D0D_0non-Darcy coefficient of the same well without damage, (thousand m³/d)⁻¹

Units: any consistent units; DD and D0D_0 in the same units

Holds when
  • The damaged zone is a cylinder around the wellbore, and the flow in it is steady-state. The first term is the Hawkins formula (Skin factor).
  • re≫rsr_e \gg r_s, and the hole is open over the whole thickness.

Suppose the permeability in a zone of radius 0.5 m around a well of radius 0.108 m is reduced fivefold. By the correlation, β\beta grows by a factor of 51.2≈6.95^{1.2} \approx 6.9, and DD grows by a factor of about 5.6. The damage skin and the inertial skin grow together.

Partial penetration. Suppose only an interval hwh_w out of the whole thickness hh is working. Then the velocity at the wall is h/hwh/h_w times higher. The damage skin, referred to the whole thickness, grows h/hwh/h_w times. The inertial losses grow as the square of the velocity, that is, (h/hw)2(h/h_w)^2 times. A pseudo-skin of flow convergence (an extra skin that comes from the flow bending towards the open interval), SppS_{pp}, adds to them (Partial penetration and well deviation):

Apparent skin with partial penetration
S′=Sd hhw+Spp+D0(hhw)2qS' = S_d\,\frac{h}{h_w} + S_{pp} + D_0\left(\frac{h}{h_w}\right)^{2} q
where:
  • SdS_ddamage skin of the penetrated interval (the part that is open), by the Hawkins formula, —
  • h, hwh,\ h_wreservoir thickness and the working (not merely perforated) interval, m
  • SppS_{pp}pseudo-skin of partial penetration, —
  • D0D_0non-Darcy coefficient of a well that penetrates the whole thickness, (thousand m³/d)⁻¹

Units: no units; D0qD_0 q in consistent units

Holds when
  • The damaged zone is thin compared with the interval, and the flow near the wellbore is radial towards the interval.
  • The inertial losses in the zone of flow convergence, farther from the wellbore, are small compared with the losses at the wall.

If a third of the thickness is open, the inertial skin is nine times larger. So a high DD together with a small SS often means that only part of the interval is working. Production logging in a producing well shows the working interval.

  • Perforation. The flow squeezes into individual tunnels, so the velocity in and around the tunnels is much higher than at an open hole. The inertial losses in the tunnels, especially those packed with gravel, are a noticeable part of DD in cased wells (wells lined with steel casing; see Effect of completion on inflow).
  • A hydraulic fracture increases the inflow area and makes the DD of the well several times smaller. But the inertial losses in the proppant pack reduce the effective conductivity of the fracture itself (Hydraulic fracturing: purpose and well selection).
  • Two-phase flow. Condensate that drops out of the gas, or water near the wellbore, narrows the channels for gas and increases both SS and DD.

Terms and symbols

Non-Darcy (inertial) flow
Flow in which an inertial resistance, proportional to the square of the velocity, adds to the viscous resistance of Darcy's law. It is noticeable in gas wells and high-rate wells.
Forchheimer equation
The two-term law of filtration, − dp/ dx=μv/k+βρv2-\dd p/\dd x = \mu v/k + \beta\rho v^2.
Inertial resistance coefficient β\beta
A property of the rock, with units of one over length. It increases as permeability decreases, and we measure it on core at several flow rates.
Forchheimer number Fo
The ratio of the inertial resistance to the viscous resistance, kβρv/μk\beta\rho v/\mu. At the wall of the well it equals the inertial skin DqDq.
Non-Darcy coefficient DD
The inertial skin per unit of rate. For a gas well with an open, undamaged hole it is βρsck/(2πhμwrw)\beta\rho_{sc}k/(2\pi h\mu_w r_w).
Apparent skin S′S'
The skin measured in a test at a single rate: S′=S+DqS' = S + Dq.
Flow resistance coefficients aa and bb
The coefficients of the two-term gas inflow equation Δm=aq+bq2\Delta m = aq + bq^2: the viscous and the inertial resistance.
Isochronal test
A test with flow periods of equal length, with shut-ins between them and one long flow period. It is used when stabilisation takes too long.

Common mistakes and misconceptions

Wrong

“Non-Darcy skin is turbulence in the reservoir.”

In fact

The flow in the pores stays laminar. The losses come from the fluid speeding up and slowing down in channels whose width keeps changing. The word “turbulent” in the names is historical.

Wrong

“From the build-up curve after flow at a high rate, the skin of the gas well is +5 — the near-wellbore zone is badly damaged.”

In fact

This is the apparent skin S+DqS + Dq. First we separate it by testing at several rates. In the lesson's example, the skin at the highest flow period is +5.2, but the rate-independent skin is about 1.6.

Wrong

“The absolute open flow can be estimated from a single rate by extending the inflow line according to Darcy's law.”

In fact

The inertial losses grow as the square of the rate, so such an estimate is too high. For the lesson's well, a straight line through the flow period at 15 MPa gives a quarter more, and a calculation with no inertial losses at all gives 1.8 times more. We need several flow periods and the two-term equation.

Wrong

“DD is a constant of the reservoir: calculate it from the correlation and do not test.”

In fact

DD is a characteristic of the well. It depends on the perforation, the working interval and damage, and it changes with time. An estimate from the correlation for an open, undamaged hole usually comes out lower than the DD of a real well.

Wrong

“The reservoir density of the gas and the viscosity at reservoir pressure are put into the formula for DD of a gas well.”

In fact

The mass flow rate is constant. So we take the density at standard conditions together with the rate at standard conditions. We take the viscosity at the bottomhole pressure, where the inertial losses are concentrated.

In depth: advanced detail

Derivation of the two-term equation for gas

We write the Forchheimer equation for radial gas inflow using the mass flow rate m˙=ρscq\dot m = \rho_{sc}q, which is the same at all radii. The Darcy velocity is v=m˙/(2πrhρ)v = \dot m/(2\pi rh\rho). We substitute it and multiply both sides by ρ/μ\rho/\mu:

Forchheimer equation for gas in terms of the mass flow rate
ρμ  dp dr=m˙2πkh⋅1r+β m˙2(2πh)2μ⋅1r2\frac{\rho}{\mu}\,\frac{\dd p}{\dd r} = \frac{\dot m}{2\pi kh}\cdot\frac{1}{r} + \frac{\beta\,\dot m^2}{(2\pi h)^2\mu}\cdot\frac{1}{r^2}
where:
  • m˙\dot mmass flow rate of the gas, kg/s
  • ρ=pM/(ZRT)\rho = pM/(ZRT)gas density at pressure pp, kg/m³
  • μ\mugas viscosity at pressure pp, Pa·s

Units: SI

Holds when
  • The inflow is isothermal and steady-state, to a well that is an open hole over the whole thickness.

The left-hand side equals MRT⋅pμZ  dp dr\dfrac{M}{RT}\cdot\dfrac{p}{\mu Z}\,\dfrac{\dd p}{\dd r}, that is, M2RT  dm dr\dfrac{M}{2RT}\,\dfrac{\dd m}{\dd r}. This is where the pseudo-pressure comes from. In the second term on the right, the viscosity changes with pressure. But this term is concentrated at the wall, so we can take the viscosity in it at the bottomhole pressure. We integrate from rwr_w to rer_e and use m˙=ρscq\dot m = \rho_{sc}q and ρsc=pscM/(RTsc)\rho_{sc} = p_{sc}M/(RT_{sc}). This gives:

Steady-state gas inflow with inertial losses
m(pe)−m(pw)=pscT qπkh Tsc(ln⁡rerw+βρsck2πhμwrw q)m(p_e) - m(p_w) = \frac{p_{sc}T\,q}{\pi kh\,T_{sc}}\left(\ln\frac{r_e}{r_w} + \frac{\beta\rho_{sc}k}{2\pi h\mu_w r_w}\,q\right)
where:
  • m(pe), m(pw)m(p_e),\ m(p_w)pseudo-pressure at the outer boundary and at the wall of the well, Pa²/(Pa·s)
  • μw\mu_wgas viscosity at the bottomhole pressure, Pa·s

Units: SI; pressures absolute

Holds when
  • The term 1/re1/r_e in the inertial part is dropped (re≫rwr_e \gg r_w).

The expression in brackets is the logarithmic term plus DqDq, with the coefficient DD of a gas well. For pseudo-steady-state inflow, we replace ln⁡(re/rw)\ln(r_e/r_w) by ln⁡(re/rw)−3/4\ln(r_e/r_w) - 3/4 and add the skin SS. This gives the two-term equation of the main section.

Inertial skin with changing rates and in transient flow

The inertial pressure drop, like the pressure drop across a skin, appears and disappears together with the rate, because the thin ring at the wellbore does not store fluid. So when we superpose the flow periods (Superposition principle; we add up the effects of each rate change), the transient part is the sum of the contributions of all the rate changes. The skin and the inertial term relate only to the current rate qnq_n:

Bottomhole pressure of a gas well after several rate changes
m(pi)−m(pwf)=U[∑j=1n(qj−qj−1) 12(ln⁡tD,j+0.809)+(S+Dqn) qn]m(p_i) - m(p_{wf}) = U\left[\sum_{j=1}^{n}(q_j - q_{j-1})\,\tfrac12\left(\ln t_{D,j} + 0.809\right) + (S + Dq_n)\,q_n\right]
where:
  • pip_iinitial reservoir pressure, MPa
  • qjq_jrate of the jj-th flow period, q0=0q_0 = 0, thousand m³/d
  • tD,jt_{D,j}dimensionless time from the start of the jj-th flow period: 3.553⋅10−3 k(t−tj−1)3.553\cdot10^{-3}\,k(t - t_{j-1}) divided by ϕμictirw2\phi\mu_i c_{ti}r_w^2, —
  • UU1.290 T/(kh)1.290\,T/(kh) in metric units, MPa²/(mPa·s) per thousand m³/d
  • μi, cti\mu_i,\ c_{ti}gas viscosity and total compressibility at the initial pressure, mPa·s, MPa⁻¹

Units: metric oilfield; tt in h, kk in mD, ϕ\phi as a fraction, rwr_w in m

Holds when
  • The reservoir is infinite, and the flow is radial (the logarithmic approximation).
  • The product μct\mu c_t is taken at the initial pressure. At large drawdowns, pseudo-time (a modified time that allows for the changing gas properties) is used instead of time.

The term (S+Dqn)qn(S + Dq_n)q_n is non-linear in the rate (the rate appears squared), so we cannot split it over the flow periods as we do the logarithmic terms. Two practical consequences follow. First, the skin from each pressure record is the S+DqS + Dq of the flow period in which it was recorded. Second, when the well is shut in, the bottomhole pseudo-pressure rises at once by U(S+Dqn)qnU(S + Dq_n)q_n.

The β coefficient of a packed bed of grains: gravel and proppant

The Ergun equation, known from chemical engineering, describes flow through a packed bed of grains — a gravel pack, proppant, loose sand — well. It has the form of the Forchheimer equation. If we compare the terms, we get the permeability and β\beta from the grain diameter dpd_p and the porosity (the share of the volume that is pore space):

Permeability and the β coefficient of a packed bed of grains
k=ϕ3dp2150 (1−ϕ)2,β=1.75 (1−ϕ)ϕ3dp=1.75 dp150 (1−ϕ) kk = \frac{\phi^3 d_p^2}{150\,(1 - \phi)^2},\qquad \beta = \frac{1.75\,(1 - \phi)}{\phi^3 d_p} = \frac{1.75\,d_p}{150\,(1 - \phi)\,k}
where:
  • dpd_pmean diameter of the grains (by the ratio of volume to surface), m
  • ϕ\phiporosity of the pack, fraction
  • k, βk,\ \betapermeability and inertial resistance coefficient, m², m⁻¹

Units: SI

Holds when
  • The pack is unconsolidated (loose), and the grains are of similar size. The constants 150 and 1.75 are empirical (found from experiments).

For a given pack, βk\beta k is proportional to the grain size. For example, for gravel with 1 mm grains and a porosity of 0.35, the permeability is about 700 D and β\beta is about 3⋅1043\cdot10^4 m⁻¹. The velocities in perforation tunnels packed with gravel are so high that, even with such a small β\beta, the inertial losses in them are significant.

Connections to other topics

Check yourself

  1. 1

    In a test of a gas well at two rates, the apparent skin is 3.1 at 300 thousand m³/d and 4.9 at 600 thousand m³/d. What are the rate-independent skin SS and the coefficient DD?

    1. A.SS = 1.3; DD = 0.006 (thousand m³/d)⁻¹
    2. B.SS = 3.1; DD = 0
    3. C.SS = 4.9; DD = 0.003 (thousand m³/d)⁻¹
    4. D.SS = 0; DD = 0.0082 (thousand m³/d)⁻¹
    Show the answer

    Correct answer: A. SS = 1.3; DD = 0.006 (thousand m³/d)⁻¹

    The slope is D=(4.9−3.1)/(600−300)=0.006D = (4.9 - 3.1)/(600 - 300) = 0.006 (thousand m³/d)⁻¹, and the intercept is S=3.1−0.006⋅300=1.3S = 3.1 - 0.006\cdot300 = 1.3. At 600 thousand m³/d the inertial skin is 3.6, which is more than the damage skin.

  2. 2

    What share of the inertial pressure losses falls on the ring between the wall of the well and a distance of five well radii (the drainage area is much larger)?

    1. A.about 95%
    2. B.about 80%
    3. C.about 50%
    4. D.about 20%
    Show the answer

    Correct answer: B. about 80%

    The share of the inertial losses within rr is about 1−rw/r=1−1/5=0.81 - r_w/r = 1 - 1/5 = 0.8. The viscous losses in the same ring are only ln⁡5/ln⁡(re/rw)\ln 5/\ln(r_e/r_w), which is about 20% when re/rwr_e/r_w is several thousand.

  3. 3

    How will the coefficient DD and the logarithmic term of the inflow equation change if the well is drilled with a bit (the cutting tool) of twice the diameter and everything else stays the same?

    1. A.DD will be halved, the logarithmic term will decrease by about 0.7
    2. B.both will be halved
    3. C.DD will not change, the logarithmic term will decrease by 0.7
    4. D.DD will decrease fourfold
    Show the answer

    Correct answer: A. DD will be halved, the logarithmic term will decrease by about 0.7

    DD is inversely proportional to rwr_w: the velocity at a wall of twice the area is half as high. The logarithmic term decreases by ln⁡2≈0.69\ln 2 \approx 0.69. At a value of about 8, that is less than 10%. So the radius of the wellbore matters much more for the inertial losses than for the viscous ones.

  4. 4

    Why do the gas density at standard conditions and the viscosity at the bottomhole pressure enter the formula for DD of a gas well?

    Show the answer

    The inertial term is proportional to ρv2\rho v^2. For gas, ρ\rho and vv both change with pressure. But their product, the mass flux, depends only on the area for a given mass flow rate. So ρv2=(ρv)2/ρ\rho v^2 = (\rho v)^2/\rho. When we integrate through the pseudo-pressure, what remains is the mass flow rate ρscq\rho_{sc}q, that is, the density at standard conditions together with the rate at standard conditions. The viscosity stays in the inertial term. That term is concentrated at the wall of the well, so we take the viscosity at the bottomhole pressure.

  5. 5

    An oil well has kk = 500 mD, all 10 m of the thickness open, μ\mu = 0.5 mPa·s, oil density in the reservoir 750 kg/m³, BB = 1.3, rwr_w = 0.108 m and a rate of 2000 m³/d. Do we need to take the inertial losses into account? And what if only a quarter of the thickness were working?

    Show the answer

    By the correlation, β=7.64⋅1010/5001.201\beta = 7.64\cdot10^{10}/500^{1.201} ≈4.4⋅107\approx 4.4\cdot10^7 m⁻¹. By the metric formula for a liquid, the numerator is 1.818⋅10−18 βρBk≈3.9⋅10−51.818\cdot10^{-18}\,\beta\rho Bk \approx 3.9\cdot10^{-5} and the denominator is hμrw=0.54h\mu r_w = 0.54. So D≈7.2⋅10−5D \approx 7.2\cdot10^{-5} (m³/d)⁻¹ and Dq≈0.14Dq \approx 0.14, which is about 2% of the logarithmic term. This is negligible. If a quarter of the thickness were working, DD would be 16 times larger and Dq≈2.3Dq \approx 2.3. The pseudo-skin of partial penetration would be added to it, and that is already a noticeable part of the resistance.

  6. 6

    Why are all the short flow periods of an isochronal test of equal length, and why do we need one long flow period?

    Show the answer

    While the inflow is transient, the coefficient aa contains a logarithmic term that grows with time. For flow periods of equal length that start from the same state (after the pressure has built up), this term is the same. So their points, plotted as Δm/q\Delta m/q against qq, lie on a straight line with the correct slope bb. The short flow periods do not give the stabilised coefficient aa. We find it from one long flow period that is carried to stabilisation: we draw a line through its point with the same slope. Or we calculate it from khkh and SS for the known drainage area.

Updated: 26 October 2026