Commit Graph

9 Commits

Author SHA1 Message Date
Atgeirr Flø Rasmussen
dc6bcead91 Add test case for capillary inversion. 2014-02-21 08:32:15 +01:00
Atgeirr Flø Rasmussen
ebb6eaf742 Complete pressure test for dead-oil deck. 2014-02-19 13:41:20 +01:00
Atgeirr Flø Rasmussen
b134fe048a Still working on test_equil.cpp. 2014-02-05 11:26:29 +01:00
Atgeirr Flø Rasmussen
85be4b1263 Add (unfinished) test case. 2014-02-03 15:36:20 +01:00
Bård Skaflestad
76844c9c59 Include <numeric> for std::iota()
Header was missing in earlier revision.
2014-01-21 17:54:47 +01:00
Bård Skaflestad
6814b97698 Add reverse look-up mapping for region vectors
Class RegionMapping<> provides an easy way of extracting the cells
that belong to any identified region (e.g., as defined by EQLNUM) of
the deck.
2014-01-21 17:54:47 +01:00
Bård Skaflestad
4114da26bd Test cell subset phase pressure assignment. 2014-01-21 17:54:46 +01:00
Bård Skaflestad
c582d00fb6 Compute phase pressures in subset of cells
This commit adds support for assigning the initial phase pressure
distribution to a subset of the total grid cells.  This is needed in
order to fully support equilibration regions.  The existing region
support (template parameter 'Region' in function 'phasePressures()')
was only used/needed to define PVT property (specifically, the fluid
phase density) calculator pertaining to a particular equilibration
region.
2014-01-21 17:54:46 +01:00
Bård Skaflestad
4c39a8a595 Add basic equilibration facility
This commit adds a simple facility for calculating initial phase
pressures assuming stationary conditions, a known reference pressure
in the oil zone as well as the depth and capillary pressures at the
water-oil and gas-oil contacts.

Function 'Opm::equil::phasePressures()' uses a simple ODE/IVP-based
approach, solved using the traditional RK4 method with constant step
sizes, to derive the required pressure values.  Specifically, we
solve the ODE

      dp/dz = rho(z,p) * g

with 'z' represening depth, 'p' being a phase pressure and 'rho' the
associate phase density.  Finally, 'g' is the acceleration of
gravity.  We assume that we can calculate phase densities, e.g.,
from table look-up.  This assumption holds in the case of an ECLIPSE
input deck.

Using RK4 with constant step sizes is a limitation of this
implementation.  This, basically, assumes that the phase densities
varies only smoothly with depth and pressure (at reservoir
conditions).
2014-01-21 17:54:46 +01:00