Initialized Prediction
Overview
Teaching: min
Exercises: minQuestions
What are Initialized Prediction Experiments?
Objectives
Types of Experiments
Simulation: what the model thinks the climate looks like under certain conditions
These are not necessarily real conditions, they are typically idealized and do not correspond to any specific day or time. That is why we evaluate them using statistics (e.g. mean or variability over the simulation) and often compare these statistics between two simulations (e.g. a control and an experiment) or with the observed statistics.
- You ran a B1850 case and looked at the seasonal means and equatorial precipitation (Assignment #3)
- You ran an sensitivity experiment with the DWG SSTs and looked at how the mean precip compared with a control simulation (Assignment #4)
- You ran a ocean model simulations where you changed different things and looked at how the mean changed under the different experiments
- You ran the added heating experiments and compared the mean with and without added heating (Assignment #5)
Projection: what the model thinks the climate will look like in the future under different scenarios
- projections are a special case of a simulation under different future scenarios
- because they are run and evaluated in much the same way as standard simulations, we have not done any specific projection experiments.
- Example projection compset: BSSP585 This is the SSP585 scenario for GHGs (similar to RCP8.5 used in CMIP5) or BSSP585cmip6 is the exact configuration used for CMIP6 projections.
- A common comparison is between the projection experiment and the historical or pre-industrial control experiment
Prediction: a forecast for a specific date given initial conditions for each component
These types of experiment correspond to the model attempting to predict actual conditions that occurred. We can compare directly between what the model predicted and what actually happened (observations).
- Today we will learn about how to setup the model with initial conditions for making a forecast
Key Points
Initializing the Model
Overview
Teaching: min
Exercises: minQuestions
How to setup model initial conditions?
Objectives
Setting up Experiments - Review
To setup experiments with CESM, we setup and configure the following things:
- Compset to define what components are active
- Resolution
- Configuration changes in the
env_run.xml
file: - where do initial conditions come from?
RUN_TYPE
,RUN_STARTDATE
,RUN_REFDATE
,RUN_REFCASE
,GET_REFCASE
- how long to run?
STOP_OPTION
,STOP_N
,RESTART_N
,CONTINUE_RUN
- Output and other component specific details in the namelist (
user_nl_xxx
) files - Stage the initial conditions in the run directory if
GET_REFCASE=FALSE
- SourceMods for any source code changes
Understanding Initial Conditions in CESM
Initial conditions tell the model what state to start from. The files that contain this information are called restart and intial condition files. They represent an instantanous state of each model component at a given time. There are multiple restarts for each componenet of the model.
Initial Conditions in our B1850 simulation (Assignment #3)
Let’s take a look at the initial conditions we used for some of our previous experiments:
$ cd /glade/u/home/cstan/cases/b.day1.0
$ ./xmlquery RUN_TYPE,RUN_STARTDATE,RUN_REFDATE,RUN_REFCASE,GET_REFCASE,RUN_REFDIR
Results in group run_begin_stop_restart
RUN_TYPE: hybrid
RUN_STARTDATE: 0001-01-01
RUN_REFDATE: 0301-01-01
RUN_REFCASE: b.e20.B1850.f19_g17.release_cesm2_1_0.020
GET_REFCASE: TRUE
RUN_REFDIR: cesm2_init
RUN_TYPE=hybrid
, so this indicates the information in the other variables need to be set and that this run uses initial conditions from another CESM run to start it.
GET_REFCASE=TRUE
means that the code will get the initial condition/restart files for you from the RUN_REFDIR
. If it is FASLE, we have to “stage” (meaning copy) the initial condition/restart files in the case run directory ourselves. As an example, we did this in Assignment #4.
RUN_REFDIR
is set to the default value of cesm2_init
. This is a preset directory of initial condition files for starting CESM2 simulations. The full path is:
/glade/p/cesmdata/cseg/inputdata/cesm2_init/
RUN_REFCASE
tells it which files in RUN_REFDIR
to use. Let’s take a look:
$ ls /glade/p/cesmdata/cseg/inputdata/cesm2_init/b.e20.B1850.f19_g17.release_cesm2_1_0.020*
0101-01-01 0161-01-01 0301-01-01
The RUN_REFDATE
tells us which of these we are using (0301-01-01
)
$ ls /glade/p/cesmdata/cseg/inputdata/cesm2_init/b.e20.B1850.f19_g17.release_cesm2_1_0.020/0301-01-01/
b.e20.B1850.f19_g17.release_cesm2_1_0.020.cam.i.0301-01-01-00000.nc b.e20.B1850.f19_g17.release_cesm2_1_0.020.ww3.r.0301-01-01-00000
b.e20.B1850.f19_g17.release_cesm2_1_0.020.cam.r.0301-01-01-00000.nc rpointer.atm
b.e20.B1850.f19_g17.release_cesm2_1_0.020.cam.rs.0301-01-01-00000.nc rpointer.drv
b.e20.B1850.f19_g17.release_cesm2_1_0.020.cice.r.0301-01-01-00000.nc rpointer.glc
b.e20.B1850.f19_g17.release_cesm2_1_0.020.cism.r.0301-01-01-00000.nc rpointer.ice
b.e20.B1850.f19_g17.release_cesm2_1_0.020.clm2.r.0301-01-01-00000.nc rpointer.lnd
b.e20.B1850.f19_g17.release_cesm2_1_0.020.cpl.r.0301-01-01-00000.nc rpointer.ocn.ovf
b.e20.B1850.f19_g17.release_cesm2_1_0.020.mosart.r.0301-01-01-00000.nc rpointer.ocn.restart
b.e20.B1850.f19_g17.release_cesm2_1_0.020.pop.r.0301-01-01-00000.nc rpointer.ocn.tavg.5
b.e20.B1850.f19_g17.release_cesm2_1_0.020.pop.ro.0301-01-01-00000 rpointer.rof
These are all the files that the model needs to start this run. Notice that they begin with RUN_REFCASE
So what does RUN_STARTDATE
do?
Even though the restarts we start from begin on 0003-01-01, we can tell the model to begin our experiment with whatever we want the startdate to be. This is because our simulation does not need to match any specific, real date. You can see in my experiment that the RUN_STARTDATE
is set to 0001-01-01
and the output begins at that date:
$ cd /glade/scratch/cstan/archive/b.day1.0/atm/hist
$ ls -lt
Important Note: You can specify a new startdate for your run if the RUN_TYPE=hybrid. You cannot do this if your RUN_TYPE=branch.
Initial Conditions in our Added Heating Experiments (Assignment #5)
In the previous example, all this initial condition information was set for us by default as part of the compset definition. We did not have to set any of this ourselves.
In our added heating experiments (Assignment #5), we set this up ourselves using Dr. Swenson’s scripts. Let’s take a look:
$ cd /glade/u/home/cstan/cases/addheat
$ ./xmlquery RUN_TYPE,RUN_STARTDATE,RUN_REFDATE,RUN_REFCASE,GET_REFCASE,RUN_REFDIR
Results in group run_begin_stop_restart
RUN_TYPE: branch
RUN_STARTDATE: 0005-01-01
RUN_REFDATE: 0005-01-01
RUN_REFCASE: test1
GET_REFCASE: FALSE
RUN_REFDIR: cesm2_init
RUN_TYPE
is branch
, meaning that the model components are initialized from restart files generated by a user specified CESM.
RUN_REFCASE
is set to test1
which is the name of my case for experiment we did for Assignment #2.
GET_REFCASE
is set to FALSE
, so we must stage the restart files in the run directory for this case.
RUN_REFDIR
is not used since GET_REFCASE
is set to FALSE
.
RUN_STARTDATE
must match RUN_REFDATE
since this is a branch run.
Staging the restart files
One of the lines in our script for setting up the added heating runs is:
# Initial conditions for Branch run
cp $refdir/* $ptmp/$expname/run/
This resolves to:
cp /glade/scratch/cstan/archive/b.day1.0/rest/0005-01-01-00000/* /glade/scratch/cstan/addheat/run/
We copied the restart files from the restart directory to the run directory for our new case.
ls /glade/scratch/cstan/addheat/run/
CASEROOT rpointer.rof b.day1.0.clm2.r.0005-01-01-00000.nc
rpointer.atm b.day1.0.cam.h0.0004-12.nc b.day1.0.clm2.rh0.0005-01-01-00000.nc
rpointer.drv b.day1.0.cam.h1.0005-01-01-00000.nc b.day1.0.cpl.r.0005-01-01-00000.nc
rpointer.glc b.day1.0.cam.i.0005-01-01-00000.nc b.day1.0.mosart.h0.0004-12.nc
rpointer.ice b.day1.0.cam.r.0005-01-01-00000.nc b.day1.0.mosart.r.0005-01-01-00000.nc
rpointer.lnd b.day1.0.cam.rs.0005-01-01-00000.nc b.day1.0.mosart.rh0.0005-01-01-00000.nc
rpointer.ocn.ovf b.day1.0.cice.r.0005-01-01-00000.nc b.day1.0.pop.r.0005-01-01-00000.nc
rpointer.ocn.restart b.day1.0.cism.r.0005-01-01-00000.nc b.day1.0.pop.ro.0005-01-01-00000
rpointer.ocn.tavg.5 b.day1.0.clm2.h0.0004-12.nc b.day1.0.ww3.r.0005-01-01-00000
Now that we know better how initializing the model works, we will learn about initialized prediction experiments.
Key Points
An Initialized Prediction Experiment
Overview
Teaching: min
Exercises: minQuestions
How to setup an Initialized Prediction Experiment
How to setup an experiment with your own script
Objectives
An Initialized Prediction Experiment
We will run a subseasonal initialized prediction experiment with CESM. A whole suite of these experiments have been run with CESM1 and CESM2 following a protocol set forth by SubX which is a multi-model subseasonal prediction experiment. Many modeling groups ran a suite of hindcasts for subseasonal prediction following this protocol so they could all be compared. A paper about it is here
The experiment will be initialized on Jan 7, 2019 and run for 45 days.
Which version of the model?
We will use CESM2.1. This is a little different than the one we have been using (CESM2.1.1). It is located in /glade/u/home/ssfcst/cesm2_1
Which Resolution?
We will use f09_g17 (about 1x1deg).
Which compset?
We will run with all components active, so a B
compset.
The correct GHGs will need to be defined and this is also handled by the compset. For dates initialized before 2014, we use the BHIST
compset. For dates initialized in 2014 or later, we use the BSSP585
compset (this is nearly equivalent to RCP8.5 scenario). GHGs in 2014 are projected based on this scenario.
Since we will initialize on Jan 7, 2019, we will use the BSSP585
compset.
Namelist Configurations
To meet the output requirements of the SubX protocol, we will want to set the namelists to give us daily data for many variables and some additional variables that are not default in CESM. The namelist files can be copied from my experiment directory: ~cstan/cases/s2sfcst/user_nl_*
Initial Conditions
It is not easy or advisable to make your own initial conditions for each component of the model. If you want initial conditions, you need to get them from someone at NCAR. The Earth System Prediction Working Group is the best source.
The experiment will be a hybrid run (RUN_TYPE=hybrid
) in which the initial conditions are staged by the user (GET_REFCASE=FALSE
). They are located in:
/glade/scratch/cstan/fcst/rest/2019-01-07/
$ ls /glade/scratch/cstan/fcst/rest/2019-01-07/
b.e21.f09_g17.cam.i.2019-01-07-00000.nc
I2000Clm50BgcCrop.002runRealtime.cism.r.2019-01-07-00000.nc
I2000Clm50BgcCrop.002runRealtime.clm2.h0.2019-01-01-00000.nc
I2000Clm50BgcCrop.002runRealtime.clm2.h1.2019-01-01-00000.nc
I2000Clm50BgcCrop.002runRealtime.clm2.r.2019-01-07-00000.nc
I2000Clm50BgcCrop.002runRealtime.clm2.rh0.2019-01-07-00000.nc
I2000Clm50BgcCrop.002runRealtime.clm2.rh1.2019-01-07-00000.nc
I2000Clm50BgcCrop.002runRealtime.cpl.r.2019-01-07-00000.nc
I2000Clm50BgcCrop.002runRealtime.mosart.h0.2018-12.nc
I2000Clm50BgcCrop.002runRealtime.mosart.h1.2019-01-01-00000.nc
I2000Clm50BgcCrop.002runRealtime.mosart.r.2019-01-07-00000.nc
I2000Clm50BgcCrop.002runRealtime.mosart.rh0.2019-01-07-00000.nc
I2000Clm50BgcCrop.002runRealtime.mosart.rh1.2019-01-07-00000.nc
rpointer.atm
rpointer.drv
rpointer.glc
rpointer.ice
rpointer.lnd
rpointer.ocn.ovf
rpointer.ocn.restart
rpointer.ocn.tavg
rpointer.rof
The model will look for restart files that begin with the name RUN_REFCASE
, but our files don’t all begin with that name. We will need to copy them to our run directory and change their name so the model will find them. We will change most of them to b.e21.f09_g17
SourceMods
There are changes to source code in this run. We will need to copy the new SourceMods from my experiment directory ~cstan/cases/s2sfcst/SourceMods/
to the SourceMods in the experiment directory.
Configuration changes in env_run.xml
RUN_TYPE=hybrid
RUN_STARTDATE=2019-01-07
RUN_REFDATE=2019-01-07
RUN_REFCASE=b.e21.f09_g17
GET_REFCASE=FALSE
STOP_OPTION=ndays
STOP_N=45
Specific to this run configuration (these were obtained from NCAR and are not something you would know offhand):
./xmlchange –force CLM_NAMELIST_OPTS=use_init_interp=.true.
./xmlchange CCSM_BGC=CO2A
./xmlchange OCN_CHL_TYPE=diagnostic
./xmlchange OCN_TRACER_MODULES=iage
Since the run is short, we can reduce the wallclock times the run and archiving:
./xmlchange JOB_WALLCLOCK_TIME=01:00:00
./xmlchange –subgroup case.st_archive JOB_WALLCLOCK_TIME=01:00:00
Setup Experiment with a script
Go to your home directory and create a scripts directory.
Go to your scripts directory, create a file called s2sfcsts.sh
and open it in your preferred editor..
The .sh
indicates that we will write a bash
shell script. A bash shell script is a collection of Unix commands combined with a set of syntax rules for assigning variables and making loops and conditionals.
Note: The script we got from Dr. Swenson for the added heading experiments was a c-shell
script. It is also a collection of Unix commands, but it has a different set of syntax rules for assigning variables and making loops and conditionals.
Which to use is a matter of personal preference. You will likely see bash shell (.sh
) more often than c-shell (.csh
), so I will show you how to write a bash shell script.
We will write the script together. A copy is located here on Cheyenne for reference: ~cstan/scripts/s2sfcsts.sh
Once your script is ready, you can make is executable.
$ chmod +x s2sfcsts.sh
and run it
$ ./s2sfcsts.sh
It will take a few minutes to run since it has to do everything so setup and build the model. If it fails to build, you will get an error.
Want to learn more about unix commands and shell scripting? See the Software carpentry tutorial
Key Points