Wednesday B: Data assimilation in 4D¶
Note that the practical Data Assimilation Diagnostics is a prerequisite for this practical. In this practical we will learn about the ways to run four dimensional data assimilation variants. So far we have worked with 3DEnVar, which assumes that all the observations are valid at the center of the window and does not involve the forecast model. JEDI supports three kinds four dimensional cost functions, 4DEnVar, 4DVar and weak constraint 4DVar. Here we will explore the configuration for running 4DEnVar, 4DVar and the special case of the 4DVar cost function, often called 3DVar-FGAT.
For this tutorial the key thing to keep in mind is the position in the window for the background and ensemble. For 3DVar and its variants the background and ensemble are valid at the center of the window. For 4DEnVar the backgrounds and ensembles are valid for each sub-window of the assimilation. For 4DVar and FGAT the background and ensemble are valid at the beginning of the window. The configurations for these three types of cost function are outlined in the below figure, shown with a 6 hour window.
This practical is grouped into the following steps:
Modify the 3DEnVar configuration to run 4DEnVar.
Modify the 3DEnVar configuration to run 3DEnVar-FGAT.
Modify the 3DEnVar configuration to run 4DVar.
Assess the assimilation runs.
Step 1: Revive your environment¶
Before anything can be run we need to revive the parts of the environment that are not preserved when the instance is stopped and restarted.
Begin by entering the container again:
cd ~/
singularity shell -e jedi-gnu-openmpi-dev_latest.sif
Your prompt should now look something like:
Singularity>
Once in the container be sure also to remove limits the stack memory to prevent spurious failures:
ulimit -s unlimited
ulimit -v unlimited
You should have already installed the fv3-jedi-tools
python package in previous practicals. But, it doesn’t hurt to make sure that the executable is in your path:
export PATH=$HOME/.local/bin:$PATH
Set the path to the JEDI build directory
JEDIBUILD=~/jedi/build-release/
Step 2: Run a 4DEnVar¶
Warning
The following exercises will involve modifying Yaml files. It is important to keep in mind that Yaml files are sensitive to indentation and indentation is used to decide which parts to read. When copying chunks of code from here into the Yaml files make sure to preserve the existing indentation. Do not use tabs, all indentation must be spaces.
The first exercise is to convert the yaml to run a 4DEnVar instead of 3DEnVar. By looking in the
Data/bkg
directory you can see that backgrounds are available every hour throughout the
window. This would allow for hourly sub-windows of 4DEnVar. However, for 4DEnVar it is also necessary
to have the ensemble available for every sub-window. Looking in e.g. Data/ens/mem001/
you can
see that the ensemble is available only every three hours. So in this exercise we will create a
4DEnVar with three sub-windows.
Begin by creating a copy of the 3denvar.yaml configuration file, that will be where we start from:
cd ~/jedi/tutorials/20201001_0000z
cp Config/3denvar_backup.yaml Config/4denvar.yaml
Now we need to modify the cost function, background and ensemble parts of the configuration to
enable 4DEnVar. Start by opening Config/4denvar.yaml
ready to edit it.
The cost function type is selected by the line:
cost function:
# Cost function construction
# --------------------------
cost type: 3D-Var
[...]
This should be changed to the cost function needed for 4DEnVar and to describe the sub-windows that are needed:
cost function:
# Cost function construction
# --------------------------
cost type: 4D-Ens-Var
subwindow: PT3H
[...]
Leave the other parts of the configuration, such as the window information, as they are for 3DEnVar. Note that we are using sub-windows of three hours but we are using three sub-windows in a 6 hour assimilation window. Each background is centered on a sub-window so the first sub-window extends from 2020-09-30T21:00:00 to 2020-09-30T22:30:00, the middle sub-window from 2020-09-30T22:30:00 to 2020-10-01T01:30:00 and the final sub-window from 2020-10-01T01:30:00 to 2020-10-01T03:00:00. Only the central sub-window will include observations across a three hour range. The edge sub-windows are trimmed to one and a half hours by the length of the assimilation window.
The background part of the configuration lives within the cost function:
section and is
given by:
cost function:
[...]
# Background
background:
filetype: geos
datapath: Data/bkg
filename_bkgd: geos.bkg.20201001_000000z.nc4
filename_crtm: geos.crtmsrf.c25.nc4
psinfile: true
state variables: [ua,va,t,ps,q,qi,ql,o3ppmv,phis,frocean,frlake,
frseaice,vtype,stype,vfrac,sheleg,ts,soilt,soilm,u10m,v10m]
[...]
In Jedi configuration files when there needs to be multiple states we typically use the
states
keyword and then provide the list of states. In Yaml lists are provided using dashes.
For the 3-hourly backgrounds that we intend to use, the configuration needs to be changed to:
cost function:
[...]
# Background
background:
states:
- filetype: geos
datapath: Data/bkg
filename_bkgd: geos.bkg.20200930_210000z.nc4
filename_crtm: geos.crtmsrf.c25.nc4
psinfile: true
state variables: [ua,va,t,ps,q,qi,ql,o3ppmv,phis,frocean,frlake,
frseaice,vtype,stype,vfrac,sheleg,ts,soilt,soilm,u10m,v10m]
- filetype: geos
datapath: Data/bkg
filename_bkgd: geos.bkg.20201001_000000z.nc4
filename_crtm: geos.crtmsrf.c25.nc4
psinfile: true
state variables: [ua,va,t,ps,q,qi,ql,o3ppmv,phis,frocean,frlake,
frseaice,vtype,stype,vfrac,sheleg,ts,soilt,soilm,u10m,v10m]
- filetype: geos
datapath: Data/bkg
filename_bkgd: geos.bkg.20201001_030000z.nc4
filename_crtm: geos.crtmsrf.c25.nc4
psinfile: true
state variables: [ua,va,t,ps,q,qi,ql,o3ppmv,phis,frocean,frlake,
frseaice,vtype,stype,vfrac,sheleg,ts,soilt,soilm,u10m,v10m]
[...]
Now there is a list of states, one for the middle of each of the sub-windows.
Now we need to provide lists of states for the ensembles in the background error covariance part of the yaml file.. The ensemble part of the configuration (for the first two members) looks like
cost function:
[...]
# Background error covariance
background error:
[...]
# Ensemble members
members:
- filetype: geos
state variables: *anvars
datapath: Data/ens/mem001
filename_bkgd: geos.ens.20201001_000000z.nc4
psinfile: true
- filetype: geos
state variables: *anvars
datapath: Data/ens/mem002
filename_bkgd: geos.ens.20201001_000000z.nc4
psinfile: true
[...]
For 4DEnVar with the three sub-windows this would be:
cost function:
[...]
# Background error covariance
background error:
[...]
# Ensemble members (32 members, three time slots each)
members:
- states:
- filetype: geos
state variables: *anvars
datapath: Data/ens/mem001
filename_bkgd: geos.ens.20200930_210000z.nc4
psinfile: true
- filetype: geos
state variables: *anvars
datapath: Data/ens/mem001
filename_bkgd: geos.ens.20201001_000000z.nc4
psinfile: true
- filetype: geos
state variables: *anvars
datapath: Data/ens/mem001
filename_bkgd: geos.ens.20201001_030000z.nc4
psinfile: true
- states:
- filetype: geos
state variables: *anvars
datapath: Data/ens/mem002
filename_bkgd: geos.ens.20200930_210000z.nc4
psinfile: true
- filetype: geos
state variables: *anvars
datapath: Data/ens/mem002
filename_bkgd: geos.ens.20201001_000000z.nc4
psinfile: true
- filetype: geos
state variables: *anvars
datapath: Data/ens/mem002
filename_bkgd: geos.ens.20201001_030000z.nc4
psinfile: true
[...]
This needs to be done for all ensemble members. You may wish to use 10 members instead of 32 if you get bored making these changes!
If you search on ‘3denvar’ in the configuration you’ll see that it is used in naming the hofx and analysis output. You may want to change these instances to ‘4denvar’ to preserve previous output.
Now you are ready to run the 4DEnVar data assimilation but before doing that note that for 4DEnVar each sub-window runs in parallel and since there are three sub-windows we need three times as many processors as previously, in this case 18. So to run 4DEnVar issue:
mpirun -np 18 $JEDIBUILD/bin/fv3jedi_var.x Config/4denvar.yaml Logs/4denvar.log
Note that the 4DEnVar run can be a bit sluggish due to the MPI oversubscription (these AWS nodes only have 8 physical cores). You may want to start working on the next step while it runs.
Step 3: Run a 3DEnVar-FGAT¶
Now we will run a 3DEnVar-FGAT. FGAT stands for First Guess at Appropriate Time. Essentially this type of data assimilation is an amalgam of 3DVar and 4DVar. Like 4DVar it uses the model forecast to assess \(h(x)\) at the correct time and does not assume that observations all lie at the middle of the window. Like 3DVar it does not involve the forecast model adjoint in the minimization.
Again begin by creating a copy of the 3denvar.yaml configuration file:
cp Config/3denvar_backup.yaml Config/3denvar-fgat.yaml
Since FGAT is a simplification of 4DVar (the adjoint model is just replaced with the identity model) the cost function for FGAT is the same as for 4DVar:
cost function:
# Cost function construction
# --------------------------
cost type: 4D-Var
[...]
From the above figure you can see that the only information that needs to be read in is at the
beginning of the window. Anything needed throughout the window is handled internally by running a
forecast of the model through the window. In a few places the date needs to be updated compared to
the 3denvar.yaml
configuration.
Change to
filename_bkgd: geos.bkg.20200930_210000z.nc4
in thebackground
part of the configuration.Change to
filename_bkgd: geos.ens.20200930_210000z.nc4
for each ensemble member.Change date to
date: '2020-09-30T21:00:00Z'
in thebackground error
part of the configuration.
Since 3DEnVar-FGAT requires the forecast model, information about the model setup needs to be
provided. This is included in the configuration inside the cost function
part:
cost function:
[...]
# Forecast model
model:
name: FV3LM
nml_file: Data/fv3files/input_geos_c25.nml
trc_file: Data/fv3files/field_table
nml_file_pert: Data/fv3files/inputpert_4dvar.nml
lm_do_dyn: 1
lm_do_trb: 0
lm_do_mst: 0
tstep: PT1H
model variables: [u,v,ua,va,t,delp,q,qi,ql,o3ppmv,phis,frocean,frlake,
frseaice,vtype,stype,vfrac,sheleg,ts,soilt,soilm,u10m,v10m]
[...]
This model, which is called FV3LM
in the system, is the standalone dynamical core. There is
no physics being run in this case but this is OK for testing purposes at low resolution.
Note that the model requires some variables not previously in the background, namely the addition of
u
and v
and delp
instead of ps
. The background variables should be made to be the same as the model
variables so the configuration looks like:
cost function:
[...]
# Background
background:
filetype: geos
datapath: Data/bkg
filename_bkgd: geos.bkg.20200930_210000z.nc4
filename_crtm: geos.crtmsrf.c25.nc4
psinfile: true
state variables: [u,v,ua,va,t,delp,q,qi,ql,o3ppmv,phis,frocean,frlake,
frseaice,vtype,stype,vfrac,sheleg,ts,soilt,soilm,u10m,v10m]
[...]
The 4DVar cost function in JEDI requires a linear model. For FGAT this is simply the identity linear model but this still needs to be provided in the configuration. It should be added in the inner loop part of the configuration as follows:
# Inner loop(s) configuration
variational:
[...]
# First outer loop
iterations:
- ninner: 10
linear model:
variable change: Identity
name: FV3JEDIIdTLM
tstep: PT1H
tlm variables: *anvars
[...]
As with 4DEnVar, it’s worth changing instances of 3denvar
in the configuration to
e.g. 3denvar-fgat
so that output of \(h(x)\) and the analysis is not overwritten.
Now you should be ready to run the 3DEnVar-FGAT data assimilation:
mpirun -np 6 $JEDIBUILD/bin/fv3jedi_var.x Config/3denvar-fgat.yaml Logs/3denvar-fgat.log
Step 4: Run a 4DVar¶
Evolving from the 3DEnVar-FGAT to 4DVar is very simple since the cost function and arrangement of the backgrounds and ensemble is unchanged. The only difference compared to 3DEnVar-FGAT is the linear model, which should now be the actual model adjoint.
Instead of starting from the 3DEnVar configuration file just start from the 3DEnVar-FGAT configuration file:
cp Config/3denvar-fgat.yaml Config/4dvar.yaml
Now replace the identity linear model:
# Inner loop(s) configuration
variational:
[...]
# First outer loop
iterations:
[...]
linear model:
variable change: Identity
name: FV3JEDIIdTLM
tstep: PT1H
tlm variables: *anvars
[...]
with the actual FV3 linear model:
# Inner loop(s) configuration
variational:
[...]
# First outer loop
iterations:
[...]
linear model:
variable change: Analysis2Model
name: FV3JEDITLM
nml_file: Data/fv3files/input_geos_c25.nml
trc_file: Data/fv3files/field_table
nml_file_pert: Data/fv3files/inputpert_4dvar.nml
tstep: PT1H
tlm variables: [u,v,t,delp,q,qi,ql,o3ppmv]
lm_do_dyn: 1
lm_do_trb: 0
lm_do_mst: 0
[...]
Also use 4dvar
in the the output analysis and \(h(x)\) files so as not to overwrite
the previous output.
Now you are ready to run a 4DVar analysis:
mpirun -np 6 $JEDIBUILD/bin/fv3jedi_var.x Config/4dvar.yaml Logs/4dvar.log
Note that 4DVar can take some time to run so feel free to explore the next steps while it completes.
Step 5: Apply the diagnostic tools¶
Now that you have run these different kinds of assimilation you can apply all the tools to assess
the health of the assimilation runs learnt earlier in the week. Try looking at some the statistics
of the outputs and comparing the increments between assimilation runs. Can you try adding outer
loops to the various systems and adjusting the number of inner loops? Keep in mind that for 4DVar
and FGAT the analysis is valid at the beginning of the window rather than the middle. The diagnostic
configuration files need to be modified for this. You will also need to modify both the background
and analysis in Config/create_increment_3denvar.yaml
each time you want to create the
increment from the analysis.