2. Modeling A#

2.1. Characteristics of modeling A#

The modeling studied is HHDen plane deformations. The mesh is composed of 80 Q8 elements.

2.2. Tested features#

This modeling makes it possible in particular to verify the use of the time function PESA_MULT introduced in the map THM_DIFFU. This function is added as a factor of the terms PESA_X, PESA_Y, and PESA_Z, and makes it possible to make gravity dependent on time.

2.3. Results#

The figures below show the profiles of capillary pressures, gas pressures and saturation along the bar for various times. We can clearly observe the rebalancing to reach a steady state (nothing moves after \(\mathrm{0,5}s\)).

In this stationary state and in \(\mathrm{Pa}\):

\(\mathrm{Pgz}(x=0)=\mathrm{0,991}\mathrm{Pa}\) and \(\mathrm{Pgz}(x=3)=\mathrm{1,014}\mathrm{Pa}\)

\(\mathrm{Pc}(x=0)=\mathrm{22,8}\mathrm{Pa}\) and \(\mathrm{Pc}(x=3)=-\mathrm{6,62}\mathrm{Pa}\)

This gives \({\mathrm{\Delta P}}_{\text{lq}}=\mathrm{29,44}\mathrm{Pa}\) which corresponds well to the hydrostatic balance.

_images/10000201000001EB000001132E91440218C6DF73.png

Figure 2.3-a : capillary pressure profiles

_images/10000201000001EB00000113D79BBEB50291E5F9.png

Figure 2.3-b : gas pressure profiles

_images/10000201000001F70000015703D40A4673833E1B.png

Figure 2.3-c : saturation profiles

2.4. Tested value#

\(X(m)\)

Time \((s)\)

PRE1Aster \((\mathrm{Pa})\)

Relative error allowed

0.02

13.94

0.1%

0.1

21.92

0.1%

1

22.79

0.1%