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Motivation



Assume the well is producing  q_w of water,  q_o of oil and  q_g of gas as measured daily at separator with pressure  P_s and temperature T_s

While moving down to depth  l along the hole the wellbore pressure  P_{wf}(l) will be growing due to gravity of fluid column and friction losses emerging from fluid contact with inner pipe walls . 

Wellbore temperature  T(l) will be also varying due to heat exchange with surrounding rocks.

The volume shares \{ s_w(l), \, s_o(l), \, s_g(l) \}, occupied by different phases will be varying along hole due to along-hole pressure-temperature variation, phase segregation and phase slippage.



Definition



Mathematical model of Multiphase Wellbore Flow predicts the temperature, pressure and flow speed distribution along the wellbore trajectory with account for:

  • tubing head pressure which is controled by gathering system or injection pump

  • wellbore design (pipe diameters, pipe materials and inter-pipe annular fillings)

  • fluid friction with tubing /casing walls

  • interfacial phase slippage

  • heat exchange between wellbore fluid and surrounding rocks via complex well design


Consider a 3-phase water-oil-gas flow:  \alpha = \{ w, \, o, \, g \}.


The  \alpha-phase volumetric flow fraction ( also called phase cut or  input hold-up or no-slip hold-up ) is defined as:

(1) \gamma_\alpha = \frac{q_\alpha}{q_t}

where  q_\alpha – volumetric flow rate of  \alpha-phase and  q_t is the total volumetric fluid production rate:

(2) q_t = \sum_\alpha q_\alpha = q_w + q_o + g_g



In multiphase wellbore flow each phase occupies its own area  A_\alpha of the total cross-sectional area  A of the lifting pipe. 

This area can be connected into a single piece of cross-sectional area (like in case of slug or annular flow) or dispersed into a number of connected spots (like in case of bubbly flow).

A share of total pipe cross-section area occupied by moving  \alpha-phase is called an  \alpha-phase in-situ hold-up and defined as: 

(3) s_\alpha = \frac{A_\alpha}{A}

so that a sum of all in-situ hold-ups is subject to natural constraint:

(4) \sum_\alpha s_\alpha = s_w + s_o + s_g = 1


When word hold-up is used alone it usually means in-situ hold-up and should not be confused with input hold-up or no-slip hold-up  which should be better called volumetric flow fraction.


The actual average cross-sectional velocity of moving  \alpha-phase is called in-situ velocity and defined as:

(5) u_\alpha = \frac{q_\alpha}{A_\alpha}

where  q_\alpha is the volumetric  \alpha-phase flowrate through cross-sectional area  A_\alpha.


The superficial velocity of  \alpha-phase is defined as the 

(6) u_{s \alpha} = \frac{q_\alpha}{A}= s_\alpha \cdot u_\alpha

The multiphase mixture velocity  is defined as total flow volume normalized by the total cross-sectional area:

(7) u_m = \frac{1}{A} \sum_\alpha q_\alpha = \sum_\alpha u_{s \alpha} = \sum_\alpha s_\alpha \cdot u_\alpha

The difference between velocities of  \alpha_1-phase and  \alpha_2-phase is called interfacial phase phase slippage:

(8) u_{\alpha_1 \alpha_2} = u_{\alpha_1} - u_{\alpha_2}

The multiphase fluid density  \rho_m is defined by exact formula:

(9) \rho_m = \sum_\alpha s_\alpha \rho_\alpha

where  \rho_\alpha – density of  \alpha-phase.


The two-phase gas-liquid model is defined in the following terms:

(10) u_m = u_{s g} + u_{s l} = s_g u_g + (1-s_g) u_l

The two-phase oil-water model is defined in the following terms:

(11) u_m = u_{s o} + u_{s w} = s_o u_o + (1-s_o-s_g) u_w


The 3-phase water-oil-gas model is usually built as a superposition of gas-liquid model and then oil-water model:




Input & Output



InputOutput

Ps, \, T_s, \ \{ q_w, q_o, \, q_g \} as values at separator

P(l), \, T(l), \, \{ s_w(l), \, s_o(l), \, s_g(l) \}, \, \{ q_w(l), \, q_o(l), \, q_g(l) \} as logs along hole



Application




Activity
InputOutput
1WPA – Well Performance AnalysisOptimizing the lift performance based on the IPR vs VLP models

Ps, \, T_s, \ \{ q_w, q_o, \, q_g \} as values at separator

P_{wf}(l = l_{datum}) as value at formation datum

2DM – Dynamic ModellingRelating production rates at separator to bottom-hole pressure with VLP

Ps, \, T_s, \ \{ q_w, q_o, \, q_g \} as values at separator

P_{wf}(l = l_{datum}) as value at formation datum

3PRT – Pressure TestingAdjust gauge pressure to formation datum

P_{wf}(l = l_{gauge}) as value at downhole gauge

P_{wf}(l = l_{datum}) as value at formation datum

4PLT – Production LoggingInterpretation of production logs

\{ p(l), \, T(l), \, u_m(l), \, s_w(l), \, s_o(l), \, s_g(l) \} as logs along hole

\{ q_w(l), \, q_o(l), \, q_g(l) \} as logs along hole

5RFP – Reservoir Flow ProfilingInterpretation of reservoir flow logs

\{ p(l), \, T(l), \, u_m(l), \, s_w(l), \, s_o(l), \, s_g(l) \} as logs along hole

\{ q_w(l), \, q_o(l), \, q_g(l) \} as logs along hole



Mathematical Model



The multiphase wellbore flow in hydrodynamic and thermodynamic equilibrium is defined by the following set of 1D equations: 

(12) \frac{\partial (\rho_m A)}{\partial t} + \frac{\partial}{\partial l} \bigg( A \, \sum_\alpha \rho_\alpha \, u_\alpha \bigg) = 0
(13) \sum_\alpha \rho_\alpha \bigg[ \frac{\partial u_\alpha}{\partial t} + u_\alpha \frac{\partial u_\alpha}{\partial l} - \nu_\alpha \Delta u_\alpha\bigg] = - \frac{dp}{dl} + \rho_m \, g \, \sin \theta - \frac{ f_m \, \rho_m \, u_m^2 \, }{2 d}
(14) (\rho \,c_p)_m \frac{\partial T}{\partial t}   - \bigg( \sum_\alpha \rho_\alpha \ c_{p \alpha} \ \eta_{s \alpha}\bigg) \ \frac{\partial p}{\partial t}   + \bigg( \sum_\alpha \rho_\alpha \ c_{p \alpha} \ u_\alpha \bigg) \frac{\partial T}{\partial l}  \ =  \ \frac{1}{A} \ \sum_\alpha \rho_\alpha \ c_{p \alpha} T_\alpha \frac{\partial q_\alpha}{\partial l}

where

m

indicates a mixture of fluid phases

(t,x,y,z)

time and space corrdinates ,

z -axis is orientated towards the Earth centre,

(x,y) define transversal plane to the z -axis

\alpha = \{w,o,g \}

water, oil, gas phase indicator

\mathbf{r} = (x, \ y, \ z)

position vector at which the flow equations are set


l (x, \ y, \ z)

measured depth along wellbore trajectory dl^2 = dx^2 + dy^2 + dz^2 starting from tubing head l (x = x_0, \ y=y_0, \ z = z_{THP}) = 0


q_\alpha(t, l) = \frac{d V_\alpha}{dt}

volumetric flow rate \alpha-phase fluid at wellbore depth l

u_\alpha(l)

in-situ velocity of \alpha-phase fluid flow

g = 9.81 \ \rm m/s^2

gravitational acceleration constant

\rho_\alpha(p, T)

\alpha-phase fluid density at pressure p and temperature T



\rho_m(l)  

cross-sectional average fluid density



\theta(l)

wellbore trajectory inclination to horizon



d(l)

cross-sectional average pipe flow diameter



A(l)

in-situ cross-sectional area A(l) = 0.25 \, \pi \, d^2(l)




f_m(u_m)

Darci flow friction coefficient at fluid velocity u_m

\lambda_t(p,T,s_w, s_o, s_g)

effective thermal conductivity of the rocks with account for multiphase fluid saturation

\nu_\alpha(p,T)

kinematic viscosity of \alpha-phase

\lambda_r(P,T)

rock matrix thermal conductivity

T_\alpha(l)

temperature of \alpha-phase fluid flowing from reservoir into a wellbore

\lambda_\alpha(P,T)

thermal conductivity of \alpha-phase fluid

\mu_\alpha(p,T)

dynamic viscosity of \alpha-phase fluid

\rho_r(P,T)

rock matrix mass density



\eta_{s \alpha}(P,T)

differential adiabatic coefficient of \alpha-phase fluid



c_{pr}(P,T)

specific isobaric heat capacity of the rock matrix



c_{p\alpha}(P,T)

specific isobaric heat capacity of \alpha-phase fluid



\epsilon_\alpha (P, T)

differential Joule–Thomson coefficient of \alpha-phase fluid


Fig. 1. Wellbore Flow Model geometry



Equations  (12) –  (14) define a closed set of 3 scalar equations on 3 unknowns: pressure  p(l), temperature  T(l) and mixture-average fluid velocity  u_m(l) .


The model is set in 1D-model with  l-axis aligned with well trajectory  l(x,y,z):


The disambiguation of the properties in the above equation is brought in The list of dynamic flow properties and model parameters.


Equation   (12) defines the continuity of the fluid components flow or equivalently represent the mass conservation of each mass component  \{ m_W, \ m_O, \ m_G \} during its transportation along wellbore. 

Equation  (13) defines the motion dynamics of each phase (called Navier–Stokes equation), represented as linear correlation between phase flow speed   u_\alpha and pressure profile of mutliphase fluid p.



The term  \sum_\alpha \rho_\alpha \ c_{p \alpha} \ u_\alpha \frac{\partial T}{\partial l} represents heat convection defined by the wellbore mass flow. 


The term  \sum_\alpha \rho_\alpha \ c_{p \alpha} \ \eta_{s \alpha} \ \frac{\partial P_\alpha}{\partial t} represents the heating/cooling effect of the fast adiabatic pressure change.

This usually takes effect in the wellbore during the first minutes or hours after changing the well flow regime (as a consequence of choke/pump operation). 


The term  (\rho \,c_p)_m defines mass-specific heat capacity of the multiphase mixture and defined by exact formula:

(15) (\rho \,c_p)_m = \sum_\alpha \rho_\alpha c_\alpha s_\alpha




(16) (\rho \,c_{pt})_p \frac{\partial T}{\partial t}   - \sum_{a = \{w,o,g \}} \rho_\alpha \ c_{p \alpha} \ \eta_{s \alpha} \ \frac{\partial P_\alpha}{\partial t}   + \sum_{a = \{w,o,g \}} \rho_\alpha \ c_{p \alpha} \ u_\alpha \frac{\partial T}{\partial l}  \ =  \ \frac{\delta E_H}{ \delta V \delta t}

Equation  (14)  defines the heat flow continuity or equivalently represents heat conservation due to heat conduction and convection with account for adiabatic and Joule–Thomson throttling effect.

The term  \frac{\delta E_H}{ \delta V \delta t}  defines the speed of change of  heat energy  E_H volumetric density due to the inflow from formation into the wellbore.





Stationary Flow Model


Stationary wellbore flow is defined as the flow with constant pressure and temperature:   \frac{\partial T}{\partial t} = 0 and  \frac{\partial P_\alpha}{\partial t} = 0 .

This happens during the long-term (usually hours & days & weeks) production/injection or long-term (usually hours & days & weeks)  shut-in.


The temperature dynamic equation  (14) is going to be:

(17) \sum_\alpha \rho_\alpha \ c_{p \alpha} \ u_\alpha \frac{\partial T}{\partial l} \ = \ \frac{1}{A} \ \sum_\alpha \rho_\alpha \ c_{p \alpha} T_\alpha \frac{\partial q_\alpha}{\partial l}

The phase temperature  T_\alpha is the temperature of the  \alpha-phase flowing from reservoir into wellbore.

It carries the original reservoir temperature with heating/cooling effect from reservoir-flow throttling and well-reservoir contact throttling:

(18) T_\alpha = T_r + \epsilon_\alpha \, \delta P = T_r + \epsilon_\alpha \, (P_e - P_{wf})

The discrete computational scheme for  (17) will be:

(19) \bigg( \sum_\alpha \rho_\alpha^{k-1} \ c_{p \alpha}^{k-1} \ q_\alpha^{k-1} \bigg) T^{k-1} - \bigg( \sum_\alpha \rho_\alpha^k \ c_{p \alpha}^k \ q_\alpha^k \bigg) T^k = \sum_\alpha \rho_\alpha^k \ c_{p \alpha}^k \ (q_\alpha^{k-1} - q_\alpha^k) \, (T_r^k + \epsilon_\alpha^k \delta p^k )

where  \delta p^k = p_e^k - p_{wf}^k is drawdown,  p_e^k – formation pressure in  k-th grid layer,  p_{wf}^k – bottom-hole pressure across  k-th grid layer, T_r^k – remote reservoir temperature of   k-th grid layer.

The l-axis is pointing downward along hole with  (k-1)-th grid layer sitting above the k-th grid layer.

If the flowrate is not vanishing during the stationary lift ( \sum_{a = \{w,o,g \}} |q_\alpha^{k-1}| > 0) then   T^{k-1} can be calculated iteratively from previous values of the wellbore temperature  T^k as:





(20) (\rho \,c_{pt})_p \frac{\partial T}{\partial t}   - \ \phi \sum_{a = \{w,o,g \}} \rho_\alpha \ c_{p \alpha} \ \eta_{s \alpha} \ \frac{\partial P_\alpha}{\partial t}   + \bigg( \sum_{a = \{w,o,g \}} \rho_\alpha \ c_{p \alpha} \ \epsilon_\alpha \ \mathbf{u}_\alpha \bigg) \nabla P   + \bigg( \sum_{a = \{w,o,g \}} \rho_\alpha \ c_{p \alpha} \ \mathbf{u}_\alpha \bigg) \ \nabla T   - \nabla (\lambda_t \nabla T) = \frac{\delta E_H}{ \delta V \delta t}

The wellbore fluid velocity  u_\alpha can be expressed thorugh the volumetric flow profile  q_\alpha and tubing/casing cross-section area  \pi r_f^2 as:

(21) u_\alpha = \frac{q_\alpha}{\pi r_f^2}

so that 

(22) \bigg( \sum_{a = \{w,o,g \}} \rho_\alpha \ c_{p \alpha} \ \mathbf{u}_\alpha \bigg) \ \nabla T = \frac{\delta E_H}{ \delta V \delta t}



References



Beggs, H. D. and Brill, J. P.: "A Study of Two-Phase Flow in Inclined Pipes," J. Pet. Tech., May (1973), 607-617



The list of dynamic flow properties and model parameters



(t,x,y,z)

time and space corrdinates ,

z -axis is orientated towards the Earth centre,

(x,y) define transversal plane to the z -axis

\mathbf{r} = (x, \ y, \ z)

position vector at which the flow equations are set

l (x, \ y, \ z)

measured depth along wellbore trajectory dl^2 = dx^2 + dy^2 + dz^2 starting from tubing head l (x = x_0, \ y=y_0, \ z = z_{THP}) = 0

q_\alpha(t, l) = \frac{d V_\alpha}{dt}

volumetric flow rate \alpha-phase fluid at wellbore depth l

u_\alpha (t, l)

\alpha-phase flow speed at wellbore depth l

\vec g = (0, \ 0, \ g)

gravitational acceleration vector

g = 9.81 \ \rm m/s^2

gravitational acceleration constant

\rho_\alpha(p,T)

mass density of \alpha-phase fluid

\mu_\alpha(p,T)

viscosity of \alpha-phase fluid

\lambda_t(p,T,s_w, s_o, s_g)

effective thermal conductivity of the rocks with account for multiphase fluid saturation

\lambda_r(P,T)

rock matrix thermal conductivity

\lambda_\alpha(P,T)

thermal conductivity of \alpha-phase fluid

\rho_r(P,T)

rock matrix mass density

\eta_{s \alpha}(P,T)

differential adiabatic coefficient of \alpha-phase fluid

c_{pr}(P,T)

specific isobaric heat capacity of the rock matrix

c_{p\alpha}(P,T)

specific isobaric heat capacity of \alpha-phase fluid

\epsilon_\alpha (P, T)

differential Joule–Thomson coefficient of \alpha-phase fluid

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