Numerical simulation of gas migration through...
Transcript of Numerical simulation of gas migration through...
Computing and Visualization in Science manuscript No.(will be inserted by the editor)
Numerical simulation of gas migration through engineered andgeological barriers for a deep repository for radioactive waste
Brahim Amaziane · Mustapha El Ossmani · Mladen Jurak
Received: March 28, 2012 / Accepted: date
Abstract In this paper a finite volume method ap-
proach is used to model the 2D compressible and im-
miscible two-phase flow of water and gas in heteroge-
neous porous media. We consider a model describing
water-gas flow through engineered and geological barri-
ers for a deep repository of radioactive waste. We con-
sider a domain made up of several zones with differ-
ent characteristics: porosity, absolute permeability, rel-
ative permeabilities and capillary pressure curves. This
process can be formulated as a coupled system of par-
tial differential equations (PDEs) which includes a non-
linear parabolic gas-pressure equation and a nonlinear
degenerated parabolic water-saturation equation. Both
equations are of diffusion-convection types. An implicit
vertex-centred finite volume method is adopted to dis-
cretize the coupled system. A Godunov-type method isused to treat the convection terms and a conforming
finite element method with piecewise linear elements
is used for the discretization of the diffusion terms.
An upscaling technique is developed to obtain an ef-
fective capillary pressure curve at the interface of two
media. Our numerical model is verified with 1D semi-
analytical solutions in heterogeneous media. We also
present 2D numerical results to demonstrate the signif-
B. AmazianeUNIV PAU & PAYS ADOUR, IPRA–LMA, CNRS-UMR5142, Av. de l’universite, 64000 Pau, France.E-mail: [email protected]
M. El OssmaniUniversite Moulay Ismaıl, LM2I-ENSAM, Marjane II, B.P.4024, Meknes, 50000, Maroc.E-mail: [email protected]
M. JurakUNIV PAU & PAYS ADOUR, IPRA–LMA, CNRS-UMR5142, Av. de l’universite, 64000 Pau, France.E-mail: [email protected]
icance of capillary heterogeneity in flow and to illus-
trate the performance of the method for the FORGE
cell scale benchmark.
Keywords Finite volume · Heterogeneous porous
media · Hydrogen migration · Immiscible compressible ·Nuclear waste · Two-phase flow · Vertex-centred
PACS 47.40.-x · 07.05.Tp · 02.30.Jr · 47.11.Df ·47.56.+r · 47.55.Ca · 28.41.Kw · 47.55.-t
Mathematics Subject Classification (2000) 74Q99 ·76E19 · 76T10 · 76M12 · 76S05
1 Introduction
The modeling of multiphase flow in porous formations isimportant for both the management of petroleum reser-
voirs and environmental remediation. More recently,
modeling multiphase flow received an increasing atten-
tion in connection with the disposal of radioactive waste
and sequestration of CO2.
The long-term safety of the disposal of nuclear waste
is an important issue in all countries with a significant
nuclear program. Repositories for the disposal of high-
level and long-lived radioactive waste generally rely on
a multi-barrier system to isolate the waste from the bio-
sphere. The multi-barrier system typically comprises
the natural geological barrier provided by the reposi-
tory host rock and its surroundings and an engineered
barrier system, i.e. engineered materials placed within
a repository, including the waste form, waste canisters,
buffer materials, backfill and seals.
In this paper, we focus our attention on the numeri-
cal modeling of immiscible compressible two-phase flow
in heterogeneous porous media, in the framework of the
geological disposal of radioactive waste. As a matter of
2 Brahim Amaziane et al.
fact, one of the solutions envisaged for managing waste
produced by nuclear industry is to dispose it in deep
geological formations chosen for their ability to prevent
and attenuate possible releases of radionuclides in the
geosphere. In the frame of designing nuclear waste ge-
ological repositories, a problem of possible two-phase
flow of water and gas appears, for more details see
for instance [22,23]. Multiple recent studies have estab-
lished that in such installations important amounts of
gases are expected to be produced in particular due
to the corrosion of metallic components used in the
repository design. The creation and transport of a gas
phase is an issue of concern with regard to capability
of the engineered and natural barriers to evacuate the
gas phase and avoid overpressure, thus preventing me-
chanical damages. It has become necessary to carefully
evaluate those issues while assessing the performance of
a geological repository. As mentioned above, the most
important source of gas is the corrosion phenomena of
metallic components (e.g. steel lines, waste containers).
The second source, generally less important depending
on the type of waste, is the water radiolysis by radi-
ation issued from nuclear waste. Both processes would
produce mainly hydrogen. Hydrogen is expected to rep-
resent more than 90 % of the total mass of produced
gases, see e.g. [10,25] and the references therein.
Significant effort has been and continues to be ex-
pended in numerous national and international pro-
grams in attempts to understands the potential im-
pact of gas migration, and of two-phase gas-water pro-
cesses, on the performance of underground radioactive
waste repositories, and to provide modeling tools or ap-
proaches that will allow these impacts to be assessed.
The French Agency for the Management of Radioactive
Waste (Andra) [1] is currently investigating the feasibil-
ity of a deep geological disposal of radioactive waste in
an argillaceous formation. Recently, the Couplex-Gaz
benchmark was proposed by ANDRA, and the French
research group MOMAS [20] to improve the simulation
of the migration of hydrogen produced by the corro-
sion of nuclear waste packages in an underground stor-
age. This is a system of two-phase (water-hydrogen)
flow in a porous medium. This benchmark generated
some interest and engineers encountered difficulties in
handling numerical simulations for this model. One of
the purposes of this test case is to model the resatura-
tion of a disposal cell for intermediate- level long- lived
waste (known as Type-B waste) as soon as the cell is
closed until the end of the gas-production period, for
more details, see for instance [26]. Another benchmark
is currently being studied in the framework of the Euro-
pean Project FORGE: Fate Of Repository Gases [15].
The aim of this test case is to better understand the
mechanisms of the gas migration at the cell scale and
in particular to analyze the effect of the presence of
different material and interfaces on such mechanisms.
Verification of numerical models for immiscible com-
pressible flow in porous media by the means of appro-
priate benchmark problems is a very important step in
developing and using these models.
The usual set of equations describing this type of
flow is given by the mass balance law and Darcy-Muskat’s
law for each phase, which leads to a system of strongly
coupled nonlinear PDEs. In the subsurface, these pro-
cesses are complicated by the effects of heterogeneity
on the flow and transport. Simulation models, if they
are intended to provide realistic predictions, must ac-
curately account on these effects. Here, we will assume
that the porous medium is composed of multiple rock
types, i.e. porosity, absolute permeability, relative per-
meabilities and capillary pressure curves being differ-
ent in each type of porous media. Contrast in capillary
pressure of heterogeneous permeable media can have
a significant effect on the flow path in two-phase im-
miscible flow, see for instance [17] and the references
therein. Such heterogeneous porous media lead to a
possibly discontinuous solution at medium interfaces,
which is a consequence of the transmission conditions
at the interfaces. This should be taken into account in
the discretization.
The numerical modeling and analysis of two-phase
flow in porous media has been a problem of interest for
many years and many methods have been developed.
There is an extensive literature on this subject. We will
not attempt a literature review here, but merely men-
tion a few references. We refer to the books [8,9,16] and
the references therein. Closely related to our work, we
refer for instance to [3,7,13,18,21,24] and the references
therein, where finite volume methods which employ in-
terface conditions were studied in the incompressible
case. In the area of multicomponent models numerical
simulations were presented in [2,6].
The purposes of this paper are to derive a robust
and accurate scheme on unstructured grids by using
a vertex centered finite volume method for the coupled
system modeling immiscible compressible two-phase flow
in highly heterogeneous porous media with different
capillary pressures and present numerical simulations
for an academic test and a benchmark test in the con-
text of hydrogen migration in a nuclear waste reposi-
tory.
In this paper, the wetting and nonwetting phases are
treated to be incompressible and compressible, respec-
tively. This treatment is indeed necessary when a com-
pressible nonwetting phase, such as hydrogen, is sub-
jected to compression during confinement. The problem
Numerical simulation of gas migration for radioactive waste 3
is written in terms of the phase formulation, i.e. where
the phase pressures and the phase saturations are pri-
mary unknowns. We will consider a domain made up
of several zones with different characteristics: porosity,
absolute permeability, relative permeabilities and cap-
illary pressure curves. This process can be formulated
as a coupled system of partial differential equations
which includes a nonlinear parabolic pressure equation
and a nonlinear degenerate diffusion-convection satura-
tion equation. Moreover the transmission conditions are
nonlinear and the saturation is discontinuous at the in-
terfaces separating different media. There are two kinds
of degeneracy in the studied system: the first one is the
degeneracy of the capillary diffusion term in the satura-
tion equation, and the second one appears in the evolu-
tion term of the pressure equation. In this work, we ad-
vance the applicability of the vertex centred finite vol-
ume method in heterogeneous media on unstructured
grids, where we show how to account for the discon-
tinuity in saturation from different capillary pressure
functions. An upscaling technique is developed to ob-
tain an effective capillary pressure curve at the interface
of two media. Our aim is to study a fully implicit finite
volume scheme for the 2D problem where a special dis-
cretization at the interfaces is developed and present
numerical simulations.
The rest of the paper is organized as follows. In sec-
tion 2 we give a short description of the mathematical
and physical model used in this study. In section 3 we
describe a fully implicit finite volume scheme obtained
by combining a Godunov method for the convection
terms and a conforming finite element method with
piecewise linear elements for the diffusion terms. The
space discretization is performed using a vertex-centred
finite volume method and an implicit Euler approach
is used for time discretization, and the nonlinear sys-
tem is solved by Newton-Krylov’s method at each time
step. Furthermore, we formulate an upscaling method
used to treat the nonlinear interface conditions in het-
erogeneous porous media consisting of different rock
types. Namely, the continuity of the capillary pressure
at the interfaces separating different media. Our nu-
merical model is verified with 1D semi-analytical solu-
tions from [14] for incompressible immiscible two-phase
flow in heterogeneous media. Section 4 is devoted to
the presentation of the results of this test. Computa-
tional studies which illustrate the robustness of our fi-
nite volume approach are discussed for the FORGE cell
scale benchmark in section 5. Lastly, some concluding
remarks are forwarded.
2 Mathematical model
In this section we briefly recall the conservation equa-
tions and the constitutive laws for the two-phase (gas
and water) immiscible flow model and introduce the
fractional flow formulation.
Let Ω ⊂ R2 be a bounded domain representing the
porous medium and ]0, T [ the time interval of interest.
The porous medium is characterized by the porosity Φ
and the permeability tensor K, which are spatially vary-
ing and constant in time fields. Other porous medium
properties involve relative permeability and capillary
pressure relationships, which are given functions of sat-
urations and also of position in the case of different rock
types. Let the lower case subscripts w and g denote the
water and gas phases respectively. The mass conserva-
tion equations for each phase form a coupled system of
PDEs (see, e.g., [4,8,9,16]): for α ∈ w, g, we have
Φ(x)∂
∂t(ραSα) + div(ραqα) = Fα, (1)
where the phase velocity qα is defined by the Darcy-
Muskat law:
qα = −λα(Sα)K(x)(∇Pα − ραg
), (2)
where ρα, Sα, Pα and µα are, respectively, the α phase
density, saturation, pressure and viscosity; kr,α is the
relative permeability, and λα = kr,α/µα is the mobility
of the α-phase; Fα is the source/sink term and g is the
gravity vector.
Additionally, the system satisfies a volume constraint:
Sw + Sg = 1, (3)
and the capillary pressure law:
Pc(Sw) = Pg − Pw, (4)
where Pc is a given capillary pressure function.
In the sequel we will use a fractional flow formula-
tion with the total velocity, and the gas pressure and
the water saturation as primary unknowns. We assume
that the water is incompressible and the gas density is
given by the ideal gas law; the viscosities are supposed
to be constant. We set P = Pg, S = Sw, ρg(P ) = cgP
where the compressibility cg is a given positive con-
stant. Furthermore, for notational convenience, we will
neglect the gravity force in the model and set the source
terms to zero.
Using the total velocity q = qw + qg and the coef-
ficients λ(S) = λw(S) + λg(S), fw(S) = λw(S)/λ(S),
a(S) = −λw(S)λg(S)P ′c(S)/λ(S) and α(S) as the prim-
itive function of a(S), we have
qw = fw(S)q−K∇α(S),
4 Brahim Amaziane et al.
and the water phase equation takes the form
Φ∂S
∂t+ div(fw(S)q−K∇α(S)) = 0. (5)
We will refer to equation (5) as the saturation equa-
tion. It will be used in the finite volume discretization
together with the pressure equation (6) which is defined
as a sum of equations (1) with certain weighting factor
R that will be defined later on, leading to:
Φ∂
∂t(ρg(P )(1− S)) +RρwΦ
∂S
∂t
− div([ρg(P )λg(S) +Rρwλw(S)]K∇P ) (6)
+ div(Rρwλw(S)K∇Pc(S)) = 0.
We assume the boundary ∂Ω to be divided in the
Dirichlet and the Neumann parts: ∂Ω = ΓN ∪ ΓD,
where ΓN ∩ΓD = ∅. Then the following boundary con-
ditions are imposed
ραqα · n = Qα, for α= w,g on ΓN ; (7)
S = Sbdw , P = P bdg on ΓD, (8)
where Qα are phase mass fluxes and Sbdw , P bdg are im-
posed values of the water saturation and the gas pres-
sure. To complete the system (5)–(8), we need to add
initial conditions for S and P .
We will consider heterogeneous porous domains com-
posed of several subdomains with different material prop-
erties, including relative permeability and capillary pres-
sure curves. Each subdomain, or a rock type, has a
unique set of relative permeability curves and capillary
pressure curve. In a such domain the PDEs (5), (6), are
valid only in each subdomain separately, while on the
boundary of different subdomains one has to impose the
interface conditions. These conditions are composed by
the continuity of phase fluxes and the continuity of the
phase pressures on the boundary of different materials.
The pressure continuity can be unfulfilled if the phase
is not present at the both sides of the interface and
positive entry pressure exists, leading to the extended
capillary pressure condition [11].
The main difficulties related to the approximation
of the solution of system (5), (6) is the coupling of the
equations, the degeneracy of the diffusion term in the
saturation equation, the degeneracy of the temporal
term in the pressure equation and the nonlinear in-
terface conditions appearing in heterogeneous porous
media containing different rock types.
3 Finite volume discretization
For the spatial discretization of the two-phase flow equa-
tions we use the vertex centered finite volume method.
The method is based on two spatial grids: a primary
grid, which is a conforming finite element grid, and a
secondary grid composed of control volumes centered in
the vertices of the primary grid. All model data, perme-
ability, porosity, sources, capillary pressures and rela-
tive permeabilities are constant element-wise on the pri-
mary grid. The material interfaces are therefore aligned
with the edges of the primary grid and that the satura-
tion functions are associated to elements of the primary
grid. The primary unknowns are represented as P1/Q1
finite element functions over the primary grid.
The control volume of the secondary grid, centered
at the vertex xi, is constructed by joining the centers
of all elements having vertex xi with the centers of cor-
responding edges emanating from xi (see Figure 1). El-
ements of the primary mesh will be denoted by symbol
E, while the volume of the secondary mesh, centered at
xi, will be denoted Vi.
xi
xj
xk
xi
xj
xk
γEi,j
E E
Vi
nEi,k
Fig. 1 The control volume Vi centered at the vertex xi ofthe primary grid composed of elements E.
Note also that the boundary ∂Vi of the control vol-
ume Vi is composed of the segments γEi,j ⊂ E which
connect the center of element E to the edge of E given
by the vertices xi and xj . A unit normal to γEi,j , directed
out of Vi, is denoted nEi,j .
At the interface of two materials, with different cap-
illary pressure curves, the phase pressure is continuous
if the phase is on the both side of the interface. If the
material capillary pressure curves end at zero at the
water saturation equal to one (entry pressure equal to
zero), and the convention that non existent of the non-
wetting phase has the “pressure” equal to the wetting
phase pressure is used, then the phase pressures are al-
ways continuous across the material interface, even in
the case where the non-wetting phase is not present on
the both sides of the interface. The capillary pressure
is then also continuous across the material interface.
In the case of materials with different entry pressures,
Numerical simulation of gas migration for radioactive waste 5
a discontinuity of the non-wetting phase pressure and
the capillary pressure is possible until the entry pres-
sure is not reached (for more details, see for instance
[11]). Since in our application we use the van Genuchten
capillary pressure curves, for simplicity of presentation
we will not consider the possibility of non continuous
non-wetting phase pressure. Our discretization adapts
naturally to this general situation.
Before presenting our numerical scheme, first we will
describe the treatment of the material interfaces in the
numerical method since this treatment influence our
choice of the primary variables in the discrete system.
The continuity of the capillary pressure implies the
discontinuity of the saturation across the material inter-
face (see Figure 3). The capillary pressure will be there-
fore represented on the primary mesh by its values in
the vertices and interpolated as linear or bilinear func-
tion in the elements (P1/Q1 finite elements). The satu-
ration, in the other hand, will be defined from the cap-
illary pressure on each element E as SE = (PEc )−1(Pc),
where Pc is the capillary pressure variable, and PEc is
the capillary pressure curve associated to the element
E. In the vertices that are on the material interface, as
xi and xj in Figure 2, we obtain different values of the
saturations SEi , SEj in different elements E.
mat. I mat. II
xi
xj
SE1i SE2
i
SE1j SE2
j
E1 E2
Fig. 2 An example of the primary grid in the case of two ma-terial subdomains showing the discontinuity of the saturationat the interface.
For example, the values SE1i and SE2
i in the vertex
xi are calculated from the capillary pressure value Pc,iin xi by inverting the corresponding capillary pressure
functions PE1c (S) and PE2
c (S) as shown in Figure 3.
Using the capillary pressure and one phase pressure
as primary variables in the discretized equations and
calculating the saturation, as described above, clearly
implies the continuity of both phase pressures over the
material interfaces. But, we can also replace the cap-
illary pressure by the saturation as a primary variable
and preserve the phase pressure continuity. It is suffi-
Sw
Pc
PE1c PE2
c
P ic
Pc,i
SE1i SE2
iSi 1
Fig. 3 Material capillary pressure curves (full lines) and theeffective capillary pressure curve (dotted line). Calculation of
the local saturations SE1
i , SE2
i and the effective saturationSi, for a given capillary pressure Pc,i.
cient to choose in each vertex xi one of the local satura-
tions SEi , for some neighboring element E, and use it as
a primary unknown in xi. If the vertex xi is not on the
material interface, then all surrounding elements have
the same capillary pressure curve and the saturations
SEi are equal for all elements E containing xi. If not,
we have to select one neighboring element E = Ei as
the one defining the global saturation unknown in the
vertex xi; from SEi,ii we can then calculate the capillary
pressure Pc,i = PEic (SEi,i
i ) in xi and then also all local
saturations in all neighboring elements E. Therefore,
by selecting one of the local saturation as the primary
unknown we can restore the capillary pressure and cal-
culate corresponding saturation everywhere, preserving
the continuity of the capillary pressure. There is only
one restriction to the choice of defining the element Ei:
in presence of the capillary pressure curves with posi-
tive entry pressures we have to choose the element cor-
responding to the curve with the smallest entry pres-
sure in order to satisfy the extended capillary pressure
condition [11]. This implementation of the continuity of
phase pressures is used in [21].
As described above, the treatment of the material
interface has a disadvantage of introducing the deriva-
tive of the function S 7→ (PEc )−1(PEic (S)) into the Ja-
cobian matrix. This derivative can be very large in the
case of heterogeneities with strong differences in the
capillary pressure curves. As this is the case in our ex-
ample (see Figure 7), we prefer to use as unknown the
effective saturation instead of the local saturation on
such interfaces. The effective saturation Si at the ver-
tex xi that corresponds to the capillary pressure Pc,i is
6 Brahim Amaziane et al.
given as a solution of the nonlinear system
(
∫Vi
Φdx)Si =∑E
(
∫Vi∩E
Φdx)SEi . (9)
Pc,i = PEc (SEi ), ∀E, E ∩ Vi 6= ∅. (10)
Note that for given Pc,i one can find local saturations
SEi from (10) by inverting the capillary pressure func-
tions, and then the effective saturation Si is given as
a mean value of the local saturations in (9). More pre-
cisely, the effective saturation gives the same quantity
of the water in the control volume as the local satu-
rations if the mass lumping is used in the calculation.
By representing the capillary pressure value Pc,i as a
function of the effective saturation value Si we obtain
the effective capillary pressure curve P ic , associ-
ated to the vertex xi: Pc,i = P ic(Si). From (9) it follows
that the effective capillary pressure curve depends on
the geometry of the primary grid. An example of the
effective capillary pressure curve is given in Figure 3
(see also Figures 15 and 16).
An advantage of the effective saturation/capillary
pressure is that the derivative of the function
S 7→ (PEc )−1(P ic(S)) can be much smaller than the
derivative of S 7→ (PEc )−1(PEic (S)) in presence of ex-
tremely different curves, as one in Figure 7. More im-
portant is that in combination with the mass lumping
this term completely disappear from the accumulations
terms of the residual since, due to (9), we can approxi-
mate: ∫Vi
ΦSE dx ≈∫Vi
ΦdxSi,∫Vi
Φρg(P )(1− SE) dx ≈∫Vi
Φdxρg(Pi)(1− Si),
where only the effective saturation is used.
In order to avoid solving the nonlinear system (9)–
(10), we can tabulate, before starting the simulation,
the effective capillary pressure curves in each vertex of
the material interface. Then, the capillary pressure and
the local saturations are easily computable from the
effective saturation.
Finally, we describe our finite volume discretization.
Since all functions of saturation variable entering into
differential equations are given by elements, we will gen-
erally use the notation f |E(S) = fE(S) for an element
E of the primary mesh. First, we integrate the equation
(5) over the control volume Vi, we apply the divergence
theorem, a fully implicit time derivative discretization,
the mass lumping in the accumulation term and a full
upwind stabilization in the convective term, resulting
in the discrete saturation equation:1
1
∆t
∫Vi
Φdx(Sn+1i − Sni )
−∑E
∫∂Vi∩E
K∇αE(SE,n+1) · ndσ
+∑E
∑j∈C(i)
∫γEi,j
[fEw (SE,n+1i )(qn+1 · n)+ (11)
+ fEw (SE,n+1j )(qn+1 · n)−]dσ
+∑E
∫∂Vi∩ΓN
w ∩EQn+1w /ρw dσ = 0.
Here C(i) is the set of all indices j 6= i such that xi and
xj are the vertices of the same element E. For j ∈ C(i),γEi,j is the straight part of ∂Vi ∩ E which lays between
xi and xj (see Figure 1). Note that in the accumulation
term we use the effective saturations Sn+1i , Sni , while
in all other integrals we use the local saturation SE,n+1
obtained by inverting locally the capillary pressure. The
diffusion term can be further written as (the time level
(n+ 1) is omitted)∑E
∫∂Vi∩E
K∇αE(SE) · ndσ
=∑E
∑xk∈Ek 6=i
(αE(SEk )− αE(SEi ))
∫∂Vi∩E
K∇ϕk · ndσ.
where ϕk is the P1 (or Q1) finite element base function
on the triangle (quadrilateral) associated to the vertex
xk. All integrals are calculated by the midpoint numer-
ical integration rule applied to each segment γEi,j ⊂ ∂Vi.The second equation is obtained by integrating equa-
tions (1) for α = w, g over the control volume Vi. Water
equation is multiplied by ρg(Pn+1i )/ρw and added to
the gas equation. After mass lumping and cancellation
in the accumulation terms we get the discrete pressure
equation:
1
∆t
∑E
∫Vi∩E
Φdx(ρg(Pn+1i )− ρg(Pni ))(1− Sni )
−∑E
∫∂Vi∩E
mE,n+1i K∇Pn+1 · ndσ (12)
+∑E
∫∂Vi∩E
ρg(Pn+1i )λEw(SE,n+1)K∇PEc (SE,n+1) · ndσ
+∑E
∫∂Vi∩ΓN∩E
(ρg(Pn+1i )Qn+1
w /ρw +Qn+1g ) dσ = 0,
where
mEi = ρg(Pi)λ
Ew(SE) + ρg(P )λEg (SE).
1 x+ = max(x, 0), x− = min(x, 0).
Numerical simulation of gas migration for radioactive waste 7
Note that the equation (12) can be interpreted as a
discretization of the pressure equation (6) in which the
factor R is chosen in i-th discrete equation as R =
ρg(Pn+1i )/ρw. This choice, together with the mass lump-
ing, leads to a cancellation in the accumulation terms
and stabilisation of the method. Again, we have ex-
pressed the accumulation terms by using the effective
saturation Sni , rather than the local saturations.
All integrals in discrete pressure equation are ap-
proximated in similar way as the diffusion term in the
saturation equation. For example,∑E
∫∂Vi∩E
λEw(SE)K∇PEc (SE) · ndσ ≈
∑k∈C(i)
(P kc (Sk)− P ic(Si))∫∂Vi
λEw(SE)K∇ϕk · ndσ,
where we have left out the time level index n + 1 to
shorten the notation. The integrals are calculated by
applying the midpoint numerical integration rule to
each segment γEi,j composing ∂Vi. Note that, due to
(10), we could use the effective saturations in the cal-
culation of the capillary pressure through the effective
capillary pressure curves P kc , P ic .
Finally, the total volumetric velocity is each element
E is given by:
q(SE , P ) =− λE(SE)K∇P + λEw(SE)K∇PEc (SE).
It is calculated always in the interior of an element and
therefore can be calculated simply using linear/bilinear
interpolation of P and PEc (SE) in the element E.
The control volumes Vi are possibly heterogeneous
since the material properties are associated to the el-
ements of the primary mesh, and the material inter-
faces pass through edges of the primary mesh elements.
When applying the divergence theorem in the control
volume Vi we have apparently neglected the heterogene-
ity of the domain Vi and obtained only integrals over
∂Vi. This calculation is correct if the phase fluxes over
the material interface are continuous, leading to cancel-
lation of the integrals over the material interface inside
Vi. This is precisely the way how the flux continuity
over the material interface is taken into account. While
the phase pressure continuity is satisfied explicitly, the
flux continuity is taken into account only implicitly.
4 Verification on semi-analytical solution
In order to verify our treatment of heterogeneities we
have tested the code on semi-analytical solutions exist-
ing in the case of incompressible fluids. A 1D semi-
analytical solution of incompressible immiscible two-
phase flow in homogeneous domain, with capillary ef-
fects included, is obtained in [19]. The extensions to
heterogeneous domains are given in [12], including only
diffusion, and in [14], including both convection and
diffusion terms. We will present here only one example
from [14] consisting of a simple heterogeneous medium
composed of two porous domains separated by a sharp
interface at x = 0. Extension of the porous domain is
from x = −0.1 m to x = 0.1 m. The Brooks and Corey
model for the relative permeability and capillary pres-
sure functions is considered with entry pressure Pd and
pore size distribution index λ. The properties of the left
and the right porous sub-domains are given in Table 1.
Left domain Right domainPermeability 7 · 10−12 [m2] 5.3 · 10−12 [m2]Porosity 0.34 0.34Brooks-Corey λ 2.48 2.48
Brooks-Corey Pd 2218 [Pa] 2550 [Pa]
Table 1 Data used for comparison with semi-analytical so-lution.
The wetting and nonwetting phase viscosities are
respectively µw = 1 cP and µg = 0.9 cP.
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
-0.1 -0.05 0 0.05 0.1
x [m]
Wetting phase saturation at t=1000 s
exactnumerical
Fig. 4 Comparison with a semi-analytical solution.
The irreducible saturations in the both subdomains
are equal to zero and the initial conditions for the wetting-
phase saturation in the left and right subdomains are
taken as Sw = 1 and Sw = 0 respectively. To fix the
semi-analytical solution one has to fix also the ratio R
of the total and the non-wetting flux at the discontinu-
ity (see [14]) which is taken here to be R = 0.5. Com-
parison of the wetting-phase saturation given by the
semi-analytical and the numerical solution at t = 1000
sec is given in Figure 4. The numerical solution is cal-
culated with 200 points in x-direction and we observe
numerical convergence on refined meshes.
8 Brahim Amaziane et al.
5 FORGE cell scale benchmark
Long-term radioactive waste management usually con-
siders final disposal in a deep geological repository. This
includes a series of passive barriers, both engineered and
natural, in order to minimize the migration of radioac-
tivity and achieve the required level of safety for the
environment. As the repository system evolves, gases
that may be produced, such as hydrogen from the corro-
sion of metals and from the radiolysis of water, become
an important safety issue. Multi-disciplinary European
Commission project FORGE [15] is focused on gener-
ation and migration of waste-derived repository gases
and its influences on repository system performance.
For understanding the repository-scale gas migra-
tion and developing methodology for dealing with het-
erogeneities, the FORGE project Work Package 1 in-
cludes benchmark studies on numerical simulation of
gas migration through the underground nuclear waste
repository on different spatial scales. The smallest scale
considered contains only one canister and surrounding
materials, while larger scales include a module of hun-
dred canister and the whole repository. We will present
here only the cell scale benchmark.
5.1 Benchmark description
The domain of the FORGE cell scale benchmark is ax-
isymetric and composed of one waste canister, a ben-
tonite plug which isolates the canister from the access
drift, a zone damaged by excavation (EDZ) surrounding
the canister, the plug and the access drift. Finally, there
is the access drift with its backfill and the geological
medium (unperturbed rock). Axial cross-section of the
domain is presented in Figure 5. The axis of the domain
is horizontal, but the gravity force is neglected, and the
whole problem can be treated as two-dimensional by
means of axial symmetry.
Fig. 5 Axial cross-section of the computational domain.
The contact between the waste canister and the
EDZ, and equally the bentonite plug and the EDZ, is
not perfect. It is assumed that these materials are sep-
arated by a thin layer of a porous medium of very dif-
ferent characteristics, called interface (general retention
behaviour similar to a sand). The materials to be taken
into account include, therefore, the EDZ (of both the
cell and the access drift, which have the same charac-
teristics), the bentonite plug, the backfill of the access
drift, the geological medium and the interfaces (both
canister-EDZ and plug-EDZ interfaces). The waste can-
ister is constituted of a material impermeable to both
water and gas, and is not explicitly represented in the
model. It does not make part of the computational do-
main and it serves only as a source of the gas.
The gas-production term for the disposal cell is im-
posed on the external surface of the cylinder that rep-
resents the canisters.
Dimensions of the computational domain are given
on Figure 6 and in Table 2. Physical parameters of the
materials2 are given in Table 3.
Fig. 6 Dimensions in the computational domain. Values aregiven in Table 2.
Parameter Value Parameter Value
Lx 60 m Rx 20 mRd 3 m Ed 1 mLp 5 m Lc 40 mEc 0.5 m Rc 0.5 mEi 0.01 m Lr 11.5 m
Table 2 Dimensions in the Figure 6.
2 Originally, horizontal and vertical permeability Kh, Kv
were given, which is not consistent with supposed radial sym-metry of the problem. As a consequence we use an isotropicpermeability K, given by K = 3
√K2
hKv.
Numerical simulation of gas migration for radioactive waste 9
ParametersMaterials K[10−18m2] Φ n Pr [MPa]Access drift 50 0.4 1.5 2
Bentonite plug 10−2 0.35 1.6 16Geological mat. 7.9 10−3 0.15 1.5 15
EDZ 7.9 0.15 1.5 1.5Interface can. 1 1.0 4 10−2
Interface plug 7.9 0.3 4 10−2
Table 3 Material parameters: Permeability (K), porosity (Φ)and van Genuchten’s parameters, n and Pr.
The saturation functions are given by the van Ge-
nuchten law, where the irreducible saturations of the
gas and water are set to zero (S = Sw):
Pc(S) = Pr(S−1/m − 1)1/n, m = 1− 1/n,
kr,w(S) =√S[1−
(1− S1/m
)m]2,
kr,g(S) =√
1− S[1− S1/m
]2m.
The van Genuchten parameters for all materials are
given in Table 3, and in Figure 7 we show the capillary
pressure curves of all materials. The Interface curve is
so small compared to the other capillary pressure curves
that is practically invisible in Figure 7.
Figure 8 is an enlarged part of Figure 7, which shows
drastic difference between the curve in the interface and
the curves in other materials. This difference is a major
problem for numerical simulation.
0
5
10
15
20
25
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Pc [M
Pa]
Water saturation
Capillary pressure curves
Bentonite plugGeological medium
Access driftEDZ
Interface
Fig. 7 Capillary pressure curves for all materials.
Note that the benchmark deals with water-gas flow
in a porous medium under high capillary pressures which
leads to a degeneracy in the system.
The initial conditions. In the initial moment the Ge-
ological medium and the EDZ are saturated by water.
The Access drift and the Bentonite plug have water
0
0.5
1
1.5
2 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Pc
[MP
a]
Water saturation
Bentonite plugGeological medium
Access driftEDZ
Interface
Fig. 8 A zoom of the capillary pressure curves for all mate-rials.
saturation Sw = 0.7 and in the Interfaces we have
Sw = 0.05. Water saturated media (Geological medium
and EDZ) have the initial water pressure of 5 MPa. All
unsaturated media (Access drift, Bentonite plug, Inter-
faces) have the initial gas pressure of 0.1 MPa, and the
water pressure is deduced from the capillary pressure
law. Note that in the initial moment the phase pres-
sures are discontinuous.
The gas source term is active the first 10,000 years
and for one canister it produces a quantity of the gas
of 100 mol/year. After 10,000 years the gas production
stops. The gas source is implemented as the gas flux
boundary condition imposed on the boundary of the
waste canister.
The boundary conditions are the following: at the
outer radius of the calculation domain r = 20 m we have
Dirichlet’s boundary conditions Pw = 5 MPa, Sw = 1.
At the boundary of the canister the water flux is
zero and the gas flux is given by the gas source term.
At x = 0 m, for r ≤ 3 m, the boundary conditions
are of the Dirichlet’s type variable in time for water and
gas. The representation of these variations are given in
Figure 10. The gas pressure is deduced from the capil-
lary pressure law.
At all other parts of the boundary no flow boundary
condition is applied.
5.2 Output results
The benchmark requests different outputs from the sim-
ulation.
5.2.1 Evolution with time of fluxes through surfaces
Central concern of this benchmark is migration of the
gas produced by the canister corrosion. A good measure
of that migration is given by evolution in time of the
10 Brahim Amaziane et al.
Fig. 9 Boundary conditions in 2D computational domain.The waste canister is not a part of the computational domain.On its boundary the gas flux corresponding to the gas sourceterm is imposed.
phase fluxes through certain characteristic surfaces in
the model, which are given below.
Outer boundary of the model at r = 20 m (Sout in
Figure 11), fluxes counted positively out of the model.
Drift wall (Sdrift in Figure 11), fluxes counted pos-
itively toward the drift. Outside surface of the EDZ,
separated in 3 sections (see Figure 11): SEDZ1 (around
canister), SEDZ2 (around plug) and SEDZ3 (drift EDZ).
Fluxes counted positively out of the EDZ toward the
undisturbed rock. Inner cell surfaces (see Figure 11) :
Scell (section including interface and EDZ at canister-
plug junction), Sint1 (interface at canister-plug junc-
tion), Sint2 (interface at the drift wall). Fluxes counted
positively toward the drift.
5.2.2 Evolution with time along lines
Time evolution of all model variables are requested over
several lines. Lines at constant radius (see Figure 12):
Lint (passes through the interface), LEDZ (just outside
the cell EDZ), Lrock (inside the rock at a 5 m radius)
Lines at constant x (see Figure 12): Lx=0 m and
Lx=60 m (boundaries of the model), Lplug (in the mid-
dle of the plug), Lcell (in the middle of the canister).
5.2.3 Evolution with time at given points
Time evolution of all model variables are requested in
12 points (see Figure 13). Points 1 to 4, are at the same
radius as the centre of the interface: P1 and P4 (at the
boundaries), P2 (in the middle of the canister), P3 (at
canister-plug junction). Points 5 and 6 are at the same
radius as the centre of the cell EDZ: P5 (in the mid-
dle of the canister), P6 (at the canister-plug junction).
Point 7 is in the middle of the drift EDZ on x = 0
-4
-2
0
2
4
0.1 1 10 100 1000 10000 100000
Wate
r pre
ssure
[M
Pa]
Time [years]
Outer radius constant pressure
0.6
0.65
0.7
0.75
0.8
0.85
0.9
0.95
1
0.1 1 10 100 1000 10000 100000
Wate
r satu
ration
Time [years]
Outer radius constant saturation
Fig. 10 The Dirichlet boundary conditions on the Accessdrift boundary, for x = 0 and 0 ≤ r ≤ 3 m.
boundary. Points 8 to 12 are at 5 m radius: P8 and P12
(at the boundaries), P9 (at the same x as the middle ofthe canister), P10 (at the same x as the canister-plug
junction), P11 (at the same x as the intersection of the
drift and the interface).
5.3 Main difficulties
The geometry of the domain present the first difficulty
because of small diameter of the Interface (1 cm), com-
pared to other dimensions of the computational do-
main. Large computational time (100,000 years) force
us to use relatively coarse grid which then leads to a
grid with large difference in the elements size.
Second difficulty is the large difference in the capil-
lary pressure curves in the Interfaces and the curves in
the EDZ and the Bentonite plug. The continuity of the
capillary pressure through the material interface makes
the saturation in the Interface very sensible to varia-
tions of the saturations in surrounding materials, the
EDZ and the Bentonite plug. This instability is very
Numerical simulation of gas migration for radioactive waste 11
Fig. 11 Schematic representation of the surfaces troughwhich fluxes will be calculated.
Fig. 12 Schematic representation of the lines along whichresults should be calculated.
Fig. 13 Schematic representation of the points where resultsshould be calculated.
strong in the Interface near the plug and to avoid nu-
merical oscillations in the Interface, which can prevent
the Newton solver from converging, the time step must
often be reduced. This is serious difficulty because of
large final time of simulation.
Remark. Benchmark test case presented here is sim-
plified with respect to the original benchmark in two
aspects. First, we did not model gas dissolution in wa-
ter and dissolved gas transport by the convection and
the diffusion. We assume that all generated gas will be
present in the gas phase and we study its migration.
Second, we have changed the permeability of the In-
terface near the Canister, from originally 10−12 m2 to
10−18 m2. Original, very large permeability in the In-
terface near the Canister prevented the Newton solver
from converging, except for small time steps. No other
changes to the original data were done (see also foot-
note on page 8).
6 Simulation results
6.1 Simulation code and the grid
We have used simulation code developed in house based
on the numerical scheme presented in Section 3. The
non linear system of discretized equations is solved by
the inexact Newton method, using ILU preconditioned
GMRES linear solver. For linear and non linear solvers
we have used PETSc package, [5]. Fully implicit time
stepping was controlled by the convergence of the New-
ton solver.
Fig. 14 Simulation grid.
The grid used in the simulation, shown in Figure 14,
is composed of 1932 elements in the primary grid and it
is mostly uniform rectangular grid, except in the Access
drift and the EDZ, where general quadrilaterals and
triangles are used to fit the given geometry. In the EDZ
we have used five layers of elements, and four layers
in the Interfaces. Dimensions of the elements in radial
direction go from 25 mm in the Interface, to 1.6 m in
the Geological medium.
The effective capillary pressure curves were calcu-
lated as tables in all interface points before beginning
of the simulation; 9000 points are used in each table.
Since the effective capillary pressure curves depend on
local mesh geometry, we obtain one curve in each ver-
tex on the material interface. As an illustration, in Fig-
ure 15 we show one effective capillary pressure curve at
12 Brahim Amaziane et al.
the material interface between the EDZ and the Geo-
logical medium. Corresponding material curves are also
shown. From Figure 15 we see, as well as from the def-
inition (9), (10), that the effective capillary pressure
curves have the same monotonicity properties as the
material curves and represent a mesh dependent mean
value of the material capillary pressure curves. In Fig-
ure 16 we show one effective capillary pressure curve
on the boundary of the EDZ and the Interface near the
Canister. Since the geometry of the primary grid near
the Canister is very regular all effective curves are clus-
tered in a few groups of almost identical curves. We
can also note in Figure 16 that the material curve of
the Interface is too small to be represented at the scale
of the figure.
0
5
10
15
20
25
0 0.2 0.4 0.6 0.8 1
Capill
ary
pre
ssure
[M
Pa]
Water saturation
effectiveEDZ
Geol. med.
Fig. 15 The effective capillary pressure between the EDZand the Geological medium.
0
10
20
30
40
50
60
70
80
90
100
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Capill
ary
pre
ssure
[M
Pa]
Water saturation
effectiveInterface
EDZ
Fig. 16 The effective capillary pressure between the EDZand the Interface.
6.2 Gas pressure evolution
The gas pressure is a primary variable in our model.
It is taken to be equal to the water pressure in wa-
ter saturated region. From imposed initial conditions
the gas pressure is initially discontinuous. It is assumed
that the fully saturated materials (EDZ and Geological
medium) are initially put into contact with unsaturated
materials (Interfaces and Access drift) which results in
discontinuity of water and gas pressures in the initial
moment. After the start of the simulation the gas pres-
sure becomes immediately continuous, as it can be seen
from Figure 17, for t = 1 day. Then, in the EDZ and the
Access drift, it stays relatively small and uniform until
sufficient quantity of gas is generated, when it starts to
grow (see Figure 17 for t = 2, 000 years). The maximum
gas pressure is attained at one corner of the Canister
at the end of the gas production interval (t = 10, 000
years).
6.3 Evolution with time of fluxes through surfaces
In the first year of the simulation the initial water pres-
sure discontinuity produce very strong flow of water
from the Geological medium to the EDZ. The water
flow through SEDZ1, after initial very strong flow into
EDZ, shortly changes direction and between 0.001 an
0.1 year flows to the Geological medium. After that
stays directed towards the EDZ (Figure 18). The water
flow through SEDZ3 (Figure 19) stays directed to the
EDZ until extinction of the gas source when its goes to
zero, but shows some small oscillations at later times,
obviously of numerical origin. The water flow through
SEDZ2 (Figure 18) is slightly positive (from the EDZ to
the Geological medium) which is a consequence of much
stronger water flow through the EDZ (surface Scell,
Figure 18) towards the Access drift. The flow of water
from the EDZ to the Access drift (surface Sdrift, Fig-
ure 19) stays very strong even after extinction of the gas
source. Water flow through the interfaces is negligible.
The EDZ is the main path for the water flow, which
goes from the Geological medium to the Access drift.
The Interfaces do not participate to the water flow since
they are mostly field with the gas (see Figure 26) keep-
ing water mobility very low. They prevent the flow of
water from the EDZ to the Bentonite plug, which resat-
urates primary from the Access drift. This slows down
the plug resaturations, which take approximately 2,000
years and explains small water flux from the EDZ to the
Geological medium through SEDZ2. Finally, the water
flux through the EDZ-Acess drift interface stops ap-
proximately at 23,000 years, when the hole domain, ex-
cept the Interfaces, is resaturated.
Numerical simulation of gas migration for radioactive waste 13
Fig. 17 Gas pressure (in MPa) in the domain at different times: 1 day, 1 year, 2,000 years and 100,000 years.
-150
-100
-50
0
50
100
0.1 1 10 100 1000 10000 100000
Wate
r flux [kg/y
ear
]
Time [years]
S_EDZ_2S_EDZ_1
S_cellS_int_1S_int_2
S_out
Fig. 18 Water fluxes through SEDZ1, SEDZ2, Scell, Sint1
and Sint2.
The gas flow in Figures 20 and 21 shows that the
gas is flowing through the EDZ in direction of the Ac-
cess drift (surface Scell, Figure 21) and and form the
EDZ to the Access drift, through Sdrift (Figure 21).
These two fluxes are the strongest ones. The flow of
the gas through the Interfaces (Sint1 and Sint2 in
Figure 20) is approximately 10-15 times smaller than
the flow through the EDZ in the direction of the Ac-
cess drift (Scell in Figure 21), and it is smaller than
the gas flow from EDZ into the undisturbed rock. We
may conclude, therefore, that importance of the inter-
-400
-200
0
200
400
0.1 1 10 100 1000 10000 100000
Wate
r flux [kg/y
ear]
Time [years]
S_driftS_EDZ_3
Fig. 19 Water fluxes through Sdrift and SEDZ3.
face for the gas migration is weak. The most of the
gas flows through the EDZ, whose properties has the
largest influence on behavior of the system. However,
the Interfaces keep their importance as a capillary bar-
rier that slows down the resaturation of the Canister
and the Bentonite plug.
Let us also note that in the first year of the simula-
tion the gas is flowing from the Access drift to the EDZ
(Sdrift in Figure 21) under the influence of the bound-
ary condition imposed on the boundary of the Access
drift and because the gas is replacing the water that is
entering into the Access drift.
14 Brahim Amaziane et al.
The flow of the gas from the EDZ to the Geologi-
cal medium (surfaces SEDZ1 and SEDZ2 in Figure 20) is
approximately 5-8 times smaller than the flow through
the EDZ and the Interface (surface Scell in Figure 21),
and is a consequence of the gas replacing the water that
is entering into the EDZ. Similarly, we have the flow of
the gas from the Access drift EDZ into undisturbed
rock (SEDZ3 in Figure 21) which is induced by a strong
flow of the water in the opposite direction. After ap-
proximately 23,000 years the gas is finally evacuated to
the Access drift and from there, through the boundary
with imposed pressure, out of the system.
6.4 Evolution with time at given points
In this subsection we show the water saturation and
the water and the gas pressures in some of prescribed
points.
In Figure 22 we show water saturation in all points
outside of the EDZ and the Interface, and in Figure 23
we show the points in the Interface and the EDZ. We
see from Figure 22 that desaturation of the Geologi-
cal medium is very weak and that it is stronger in the
points closer to the Access drift, due to strog water flow
into the Access drift and some counter flow of the gas.
This weak desaturation is to be expected due to weak
permeability and strong capillary pressure curve of the
undisturbed rock.
In the points P2, P3 and P4 (Figure 23) which lay
in the Interface we observe a low water saturation un-
til 27,000 years when the resaturation of the Interface
starts. This behaviour is a consequence of very low
capillary pressure curve in the Interface (see Figure 7)
which keeps the Canister and the Bentonite plug iso-
lated of the EDZ and the Geological medium and slows
-0.01
0
0.01
0.02
0.03
0.04
1 10 100 1000 10000 100000
Gas flu
x [kg/y
ear]
Time [years]
S_EDZ_2S_EDZ_1
S_int_1S_int_2
S_out
Fig. 20 Gas fluxes through SEDZ1, SEDZ2, Sint1, Sint2 andSout.
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0.25
0.1 1 10 100 1000 10000 100000
Gas flu
x [kg/y
ear]
Time [years]
S_driftS_cell
S_EDZ_3
Fig. 21 Gas fluxes through SEDZ3, Scell and Sdrift.
0.994
0.995
0.996
0.997
0.998
0.999
1
1.001
1.002
0.1 1 10 100 1000 10000 100000
Wate
r satu
ration
Time [years]
P1P8P9
P10P11P12
Fig. 22 Time evolution of the water saturation in points P1
and P8-P12.
down the resaturation of the Plug (and the Canister
in reality). Almost all gas must be evacuated from the
EDZ for resaturation of the Interface to start.
In the points P5 and P6 that lay in the center of
the EDZ a desaturation is significant only after 2,000
years (see Figure 23). This means that the generated
gas is efficiently evacuated to the Access drift until ap-
proximately 2,000 years, when the gas starts to accu-
mulate in the EDZ. In the point P7 the desaturation is
more significant (Figure 23), but this is influenced by
the boundary condition imposed on boundary of the
Access drift (compare to imposed water saturation in
Figure 10).
The gas pressure is shown in Figure 24 for points
P2-P7 which lay in the EDZ and in the Interfaces. In
the remaining points, P1 and P8-P12, we present the
water pressure in Figure 25.
In Figure 24 we show also the boundary condition
on the gas pressure imposed on the boundary of the
Numerical simulation of gas migration for radioactive waste 15
0
0.2
0.4
0.6
0.8
1
0.1 1 10 100 1000 10000 100000
Wate
r satu
ration
Time [years]
P2P3P4P5P6P7
Fig. 23 Time evolution of the water saturation in pointsP2-P7.
Access drift. This pressure is supposed to model inter-
action of the computational domain with the rest of the
repository. In this figure the gas pressure in the points
P2 and P5 are almost the same; similarly, the pressure
in the points P3 and P6 are almost the same, and the
pressures in P4 and P7 are almost equal to the gas pres-
sure imposed on the Access drift boundary. Since the
points P2, P5 and P3, P6 are close, this is to be ex-
pected. In the other hand, in the points P4 and P7 we
see strong influence of the Dirichlet boundary condition
at the boundary of the Access drift. The maximum gas
pressure achieved in the simulation is 5.43 MPa. This
results show that the pressurisation at the cell scale, due
to the gas generation by the canister corrosion, strongly
depends on interaction of the Canister with the rest of
the repository, which is represented here by time vary-
ing boundary condition on the Access drift.
0
1
2
3
4
5
6
0.1 1 10 100 1000 10000 100000
Gas p
ressure
[M
Pa]
Time [years]
P2P3P4P5P6P7
Fig. 24 Time evolution of the gas pressure in points P2-P7
and the gas pressure imposed on the boundary of the Accessdrift.
Evolution in time of the water pressures in the points
P1 and P8-P12 are presented in Figure 25. The initial
discontinuity of the water pressure produce immediate
pressure drop in the Geological medium. This pressure
drop attains it minimum before 100 years due to strong
initial water flux into the EDZ and the Access drift.
When these fluxes stabilize (see Figures 18 and 19) the
water pressure starts to increase, until reaching its ini-
tial value of 5 MPa after 10,000 years.
0
1
2
3
4
5
0.1 1 10 100 1000 10000 100000
Wate
r pre
ssure
[M
Pa]
Time [years]
P1P8P9
P10P11P12
Fig. 25 Time evolution of the water pressure in points P1
and P8-P12.
One of the main concerns in the nuclear waste repos-
itory safety assessment is the raise of the pressure of the
gas produced by the canister. In our simulation we find
that the pressure raise is quite small (0.43 MPa) and
therefore it does not present a threat to the safety of therepository. However, we have seen that the gas pressure
is strongly influenced by the gas pressure imposed on
the boundary of the Access drift, which is by itself an
assumption on interaction between one repository cell
with the rest of the repository. The other parameters
that influence the gas pressure buildup are the proper-
ties of the EDZ which determine the ability of the EDZ
to conduct the gas into the Acces drift, and thus reduce
the pressure buildup.
6.5 Evolution with time along lines
From solution over different lines we present only the
water saturation over line Sint which goes through the
Interfaces (Figure 26) which is the most interesting one,
since the behavior of the solution is the most complex
in the Interfaces. The Interfaces have a very small cap-
illary pressure curve which keeps it desaturated if there
is some quantity of the gas in the EDZ. Therefore we
16 Brahim Amaziane et al.
see that after initial partial resaturation at 2,000 years,
water saturation diminish and stays approximately con-
stant up to 25,000 years. Around 27,000 years the water
saturation decrease to its minimum value (see also Fig-
ure 23) – probably due to local accumulation of the gas
that is evacuated from the Geological medium and the
EDZ to the area close to the Interfaces – and then starts
slowly to increase again. The resaturation starts from
the Access drift side.
0
0.2
0.4
0.6
0.8
1
0 10 20 30 40 50 60
t=0.0 yearst=2000 years
t=10000 yearst=27000 yearst=60000 years
t=100000 years
Fig. 26 Water saturation over the line Sint given at severaltime instances.
It is of great importance to evaluate the role of the
Interfaces in the gas migration in the repository since
the meshing of the Interfaces in 3D model, on the scale
of whole repository, produces prohibitively large grids.
From our simulations we can conclude that the role ofthe Interface in the gas migration in minor compared
to the role of the EDZ. The main impact of the Inter-
face on the gas migration is to slow down resaturation
of the Bentonite plug (and the Canister). In the other
hand, modeling of the Interfaces as a porous medium
with very low capillary pressure curve is not an accurate
description of physical reality. We conclude, therefore,
that an upscaling of the Interfaces with the EDZ, that
is forming a new EDZ with slightly different properties
and eliminating the Interfaces, could produce a simpler
model of the repository, without perturbing important
gas migration characteristics.
7 Conclusion
We have presented a vertex centered finite volume nu-
merical scheme for the water-gas flow through highly
heterogeneous porous media. The method is fully im-
plicit and it includes a treatment of heterogeneities by
using an upscaling technique and the concept of the ef-
fective saturation. Our numerical model is verified with
1D semi-analytical solutions in heterogeneous media.
We also apply the method to the FORGE cell scale
benchmark developed for the evaluation of the hydro-
gen migration in an underground nuclear waste repos-
itory. Note that the benchmark deals with water-gas
flow in a porous medium under high and discontinuous
capillary pressures which leads to a degeneracy in the
system. The benchmark is presented in all details fol-
lowed by the numerical results obtained by our C++
homemade code based on the numerical scheme pre-
sented in this paper. The simulator uses the open source
library PETSc for solving discrete nonlinear systems.
The simulation shows that the most of the gas is
evacuated through the EDZ towards the Access drift.
Only a small quantity of the gas enters into the Geo-
logical medium and then slowly returns into the EDZ
to be evacuated from the system. The Interfaces have
only a secondary role in the gas transport, but they
slow down the process of re-saturation of the Bentonite
plug by keeping it isolated from the EDZ. The whole
system is strongly influenced by the Dirichlet boundary
condition imposed on the Access drift boundary.
Acknowledgements The research leading to these resultshas received funding from the European Atomic Energy Com-munitys Seventh Framework Programme (FP7/2007-2011) un-der Grant Agreement no230357, the FORGE project. Thiswork was partially supported by the GnR MoMaS (PACEN/CNRS,ANDRA, BRGM,CEA, EDF, IRSN) France, their supportsare gratefully acknowledged.
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