The following analyses are available in the ``cooking'' part of OASIS3, controlled by cookart.f.
CONSERV (routine /prism/src/mod/oasis3/src/conserv.f) performs global flux conservation. The flux is integrated on both source and target grids, without considering values of masked points, and the residual (target - source) is calculated. Then all flux values on the target grid are uniformly modified, according to their corresponding surface. This analysis requires one input line with one argument:
# CONSERV operation
$CMETH
where $CMETH is the conservation method required. In this
version, only global flux conservation can be performed. Therefore
$CMETH must be GLOBAL.
SUBGRID can be used to interpolate a field from a coarse grid to a finer target grid (the target grid must be finer over the whole domain). Two types of subgrid interpolation can be performed, depending on the type of the field.
For solar type of flux field ($SUBTYPE = SOLAR), the operation
performed is:
(
) is
the flux on the fine (coarse) grid, 
(
) an auxiliary
field on the fine (coarse) grid (e.g. the albedo). The whole
operation is interpolated from the coarse grid with a grid-mapping type
of interpolation; the dataset of weights and addresses has to be given
by the user.
For non-solar type of field ($SUBTYPE = NONSOLAR), a
first-order Taylor expansion of the field on the fine grid relatively
to a state variable is performed (for instance, an expansion of the
total heat flux relatively to the SST):
() is the heat flux on the fine (coarse) grid, 
(
) an auxiliary field on the fine (coarse) grid (e.g. the SST) and
the derivative of the flux versus the
auxiliary field on the coarse grid. This operation is interpolated
from the coarse grid with a grid-mapping type of interpolation; the
dataset of weights and addresses has to be given by the user.
This analysis requires one input line with 7 or 8 arguments depending on the type of subgrid interpolation.
# SUBGRID operation with $SUBTYPE=SOLAR $CFILE $NUMLU $NID $NV $SUBTYPE $CCOARSE $CFINEwhere $CFILE and $NUMLU are the subgrid-mapping file name and associated logical unit (see section 7.5 for the structure of this file); $NID the identificator for this subgrid-mapping dataset within the file build by OASIS based on all the different SUBGRID analyses in the present coupling; $NV is the maximum number of target grid points use in the subgrid-mapping; $SUBTYPE = SOLAR is the type of subgrid interpolation; $CCOARSE is the auxiliary field name on the coarse grid (corresponding to
)
and $CFINE is the auxiliary field name on fine grid
(corresponding to ).
These two fields needs to be exchanged between their original model
and OASIS3 main process, at least as AUXILARY fields.
This analysis is performed from the coarse grid with a grid-mapping type
of interpolation based on the $CFILE file.
# SUBGRID operation with $SUBTYPE=NONSOLAR $CFILE $NUMLU $NID $NV $SUBTYPE $CCOARSE $CFINE $CDQDTwhere $CFILE, $NUMLU, $NID, $NV are as for a solar subgrid interpolation; $SUBTYPE = NONSOLAR; $CCOARSE is the auxiliary field name on the coarse grid (corresponding to
) and $CFINE
is the auxiliary field name on fine grid (corresponding to ); the
additional argument $CDQDT is the coupling ratio on the coarse
grid (corresponding to
) These three
fields need to be exchanged between their original model and OASIS3
main process as AUXILARY fields. This operation is performed from the
coarse grid with a grid-mapping type of interpolation based on the $CFILE file.
BLASNEW (routine /prism/src/mod/oasis3/src/blasnew.f) performs a linear combination of the current coupling field with any other fields after the interpolation. These can be other coupling fields or constant fields.
This analysis requires the same input line as BLASOLD.
A new analysis MASKP can be used to mask the fields after interpolation. MASKP has the same generic input line as MASK.