Skip to content

Prepare initial conditions

Walter Kolczynski - NOAA edited this page Nov 17, 2021 · 36 revisions

Sections:


There are two types of initial conditions for the global-workflow:

  1. Warm start: these ICs are taken directly from either the GFS in production or an experiment "warmed" up (at least one cycle in).
  2. Cold start: any ICs converted to a new resolution or grid (e.g. GSM-GFS -> FV3GFS). These ICs are often prepared by chgres_cube (change resolution utility).

Most users will initiate their experiments with cold start ICs unless running high resolution (C768 deterministic with C384 EnKF) for a date with warm starts available. It is not recommended to run high resolution unless required or as part of final testing.

Resolutions:

  • C48 = 2­ degree ≈ 200km
  • C96 = 1­ degree ≈ 100km
  • C192 = 1/2­ degree ≈ 50km
  • C384 = 1/4 degree ≈ 25km
  • C768 = 1/8th degree ≈ 13km
  • C1152 ≈ 9km
  • C3072 ≈ 3km

Supported resolutions in global-workflow: C48, C96, C192, C384, C768

Automated Generation

Cycled mode

Not yet supported. See Manual Generation section below for how to create your ICs yourself (outside of workflow).

Free-forecast mode (atm-only)

Free-forecast mode in global-workflow includes getic and init jobs for the gfs suite. The getic job pulls inputs for chgres_cube (init job) or warm start ICs into your ROTDIR/COMROT. The init job then ingests those files to produce initial conditions for your experiment.

Users on machines without HPSS access (e.g. Orion) need to perform the getic step manually and stage inputs for the init job. The table below lists the needed files for init and where to place them in your ROTDIR.

Note for table: yyyy=year; mm=month; dd=day; hh=cycle

Operations/production output location on HPSS: /NCEPPROD/hpssprod/runhistory/rhyyyy/yyyymm/yyyymmdd/

Source Files Tarball name Where in ROTDIR
v12 ops gfs.thhz.sanl
gfs.thhz.sfcanl
com_gfs_prod_gfs.yyyymmddhh.anl.tar gfs.yyyymmdd/hh
v13 ops gfs.thhz.sanl
gfs.thhz.sfcanl
com2_gfs_prod_gfs.yyyymmddhh.anl.tar gfs.yyyymmdd/hh
v14 ops gfs.thhz.atmanl.nemsio
gfs.thhz.sfcanl.nemsio
gpfs_hps_nco_ops_com_gfs_prod_gfs.yyyymmddhh.anl.tar gfs.yyyymmdd/hh
v15 ops pre-2020022600 gfs.thhz.atmanl.nemsio
gfs.thhz.sfcanl.nemsio
gpfs_dell1_nco_ops_com_gfs_prod_gfs.yyyymmdd_hh.gfs_nemsioa.tar gfs.yyyymmdd/hh
v15 ops gfs.thhz.atmanl.nemsio
gfs.thhz.sfcanl.nemsio
com_gfs_prod_gfs.yyyymmdd_hh.gfs_nemsioa.tar gfs.yyyymmdd/hh
v16 ops gfs.thhz.atmanl.nc
gfs.thhz.sfcanl.nc
com_gfs_prod_gfs.yyyymmdd_hh.gfs_nca.tar gfs.yyyymmdd/hh/atmos
v16 retro gfs.thhz.atmanl.nc
gfs.thhz.sfcanl.nc
gfs_netcdfa.tar* gfs.yyyymmdd/hh/atmos

*For HPSS path, see retrospective table in pre-production parallel section below

Free-forecast coupled

Coupled initial conditions are currently only generated offline and copied prior to the forecast run. Copies of initial conditions from the prototype runs are currently maintained on Hera, Orion, and WCOSS-Dell and will automatically be used when setting up an experiment as an S2SW app. The locations used are determined by parm/config/config.coupled_ic. If you need prototype ICs on another machine, please contact Walter ([email protected]).

Manual Generation

Cold starts

The following information is for users needing to generate initial conditions for a cycled experiment that will run at a different resolution or layer amount than the operational GFS (C768C384L127).

The new chgres_cube code is available from the UFS_UTILS repository on GitHub (maintained by George Gayno) and can be used to convert GFS ICs to a different resolution or number of layers. Users may clone the develop/HEAD branch or the same version used by global-workflow develop (found in sorc/checkout.sh). The chgres_cube code/scripts currently support the following GFS inputs:

  • pre-GFSv14 (GFS-GSM)
  • GFSv14 (GFS-GSM)
  • GFSv15 (FV3GFS)
  • GFSv16 (FV3GFS)

Clone UFS_UTILS:

git clone --recursive https://github.com/NOAA-EMC/UFS_UTILS.git

Then switch to a different tag or use the default branch (develop).

Build UFS_UTILS:

sh build_all.sh
cd fix
sh link_fixdirs.sh emc $MACHINE

...where $MACHINE is "cray", "dell", "hera", "jet", or "orion".

Configure your conversion:

cd util/gdas_init
vi config

Read the doc block at the top of the config and adjust the variables to meet you needs (e.g. yy, mm, dd, hh for SDATE).

Submit conversion script:

./driver.$MACHINE.sh

...where $MACHINE is currently "dell" or "cray" or "hera" or "jet" or "orion". Additional options will be available as support for other machines expands.

3 small jobs will be submitted:

  • 1 jobs to pull inputs off HPSS
  • 2 jobs to run chgres_cube (1 for deterministic/hires and 1 for each EnKF ensemble member)

The chgres jobs will have a dependency on the data-pull jobs and will wait to run until all data-pull jobs have completed.

Check output:

In the config you will have defined an output folder called $OUTDIR. The converted/chgres'd output will be found there, including the needed abias and radstat initial condition files. The files will be in the needed directory structure for the global-workflow system, therefore a user can move the contents of their $OUTDIR directly into their $ROTDIR/$COMROT.

Report bugs:

Please report bugs to George Gayno ([email protected]) and Kate Friedman ([email protected]).

Warm starts (from production)

The GFSv15 was implemented into production on June 12th, 2019 at 12z. The GFS was spun up ahead of that cycle and thus production output for the system is available from the 00z cycle (2019061200) and later. Production output tarballs from the prior GFSv14 system are located in the same location on HPSS but have "hps" in the name to represent that it was run on the Cray, where as the GFS now runs in production on the Dell and has "dell1" in the tarball name.

See production output in the following location on HPSS:

/NCEPPROD/hpssprod/runhistory/rhYYYY/YYYYMM/YYYYMMDD

Example location:

/NCEPPROD/hpssprod/runhistory/rh2021/202104/20210420

Example listing for 2021042000 production tarballs:

[Kate.Friedman@m72a2 ~]$ hpsstar dir /NCEPPROD/hpssprod/runhistory/rh2021/202104/20210420 | grep gfs | grep _00. | grep -v idx
[connecting to hpsscore1.fairmont.rdhpcs.noaa.gov/1217]
******************************************************************
*   Welcome to the NESCC High Performance Storage System         *
*                                                                *
*   Current HPSS version: 7.5.3                                  *
*                                                                *
*                                                                *
*       Please Submit Helpdesk Request to                        *
*        [email protected]                               *
*                                                                *
*  Announcements:                                                *
******************************************************************
Username: Kate.Friedman  UID: 2391  Acct: 2391(2391) Copies: 1 COS: 0 Firewall: off [hsi.6.3.0.p1-hgs Thu May 7 09:16:23 UTC 2020]
/NCEPPROD/hpssprod/runhistory/rh2021/202104:
drwxr-xr-x    2 nwprod    prod           11776 Apr 19 23:44 20210420
[connecting to hpsscore1.fairmont.rdhpcs.noaa.gov/1217]
-rw-r-----    1 nwprod    rstprod  51268255744 Apr 22 05:29 com_gfs_prod_enkfgdas.20210420_00.enkfgdas.tar
-rw-r--r--    1 nwprod    prod     220121310720 Apr 22 06:42 com_gfs_prod_enkfgdas.20210420_00.enkfgdas_restart_grp1.tar
-rw-r--r--    1 nwprod    prod     220124178944 Apr 22 07:04 com_gfs_prod_enkfgdas.20210420_00.enkfgdas_restart_grp2.tar
-rw-r--r--    1 nwprod    prod     220120305664 Apr 22 07:24 com_gfs_prod_enkfgdas.20210420_00.enkfgdas_restart_grp3.tar
-rw-r--r--    1 nwprod    prod     220116934656 Apr 22 07:38 com_gfs_prod_enkfgdas.20210420_00.enkfgdas_restart_grp4.tar
-rw-r--r--    1 nwprod    prod     220121547776 Apr 22 07:56 com_gfs_prod_enkfgdas.20210420_00.enkfgdas_restart_grp5.tar
-rw-r--r--    1 nwprod    prod     220125794816 Apr 22 08:09 com_gfs_prod_enkfgdas.20210420_00.enkfgdas_restart_grp6.tar
-rw-r--r--    1 nwprod    prod     220117037568 Apr 22 08:23 com_gfs_prod_enkfgdas.20210420_00.enkfgdas_restart_grp7.tar
-rw-r--r--    1 nwprod    prod     220117203968 Apr 22 08:33 com_gfs_prod_enkfgdas.20210420_00.enkfgdas_restart_grp8.tar
-rw-r-----    1 nwprod    rstprod   9573153280 Apr 22 02:49 com_gfs_prod_gdas.20210420_00.gdas.tar
-rw-r--r--    1 nwprod    prod      1020249088 Apr 22 02:49 com_gfs_prod_gdas.20210420_00.gdas_flux.tar
-rw-r--r--    1 nwprod    prod     92950728704 Apr 22 03:05 com_gfs_prod_gdas.20210420_00.gdas_nc.tar
-rw-r--r--    1 nwprod    prod     10647806464 Apr 22 02:50 com_gfs_prod_gdas.20210420_00.gdas_pgrb2.tar
-rw-r-----    1 nwprod    rstprod  65121796608 Apr 22 02:56 com_gfs_prod_gdas.20210420_00.gdas_restart.tar
-rw-r--r--    1 nwprod    prod     18200814080 Apr 22 03:06 com_gfs_prod_gdas.20210420_00.gdaswave_keep.tar
-rw-r-----    1 nwprod    rstprod  13013076992 Apr 22 03:08 com_gfs_prod_gfs.20210420_00.gfs.tar
-rw-r--r--    1 nwprod    prod     62663230976 Apr 22 03:13 com_gfs_prod_gfs.20210420_00.gfs_flux.tar
-rw-r--r--    1 nwprod    prod     127932879360 Apr 22 03:47 com_gfs_prod_gfs.20210420_00.gfs_nca.tar
-rw-r--r--    1 nwprod    prod     138633526272 Apr 22 04:00 com_gfs_prod_gfs.20210420_00.gfs_ncb.tar
-rw-r--r--    1 nwprod    prod     140773240832 Apr 22 03:27 com_gfs_prod_gfs.20210420_00.gfs_pgrb2.tar
-rw-r--r--    1 nwprod    prod     61253672960 Apr 22 03:32 com_gfs_prod_gfs.20210420_00.gfs_pgrb2b.tar
-rw-r--r--    1 nwprod    prod     19702107136 Apr 22 03:34 com_gfs_prod_gfs.20210420_00.gfs_restart.tar
-rw-r--r--    1 nwprod    prod     18617610240 Apr 22 04:02 com_gfs_prod_gfs.20210420_00.gfswave_output.tar
-rw-r--r--    1 nwprod    prod     30737774592 Apr 22 04:05 com_gfs_prod_gfs.20210420_00.gfswave_raw.tar

The warm starts and other output from production are at C768 deterministic and C384 EnKF. The warm start files must be converted to your desired resolution(s) using chgres_cube if you wish to run a different resolution. If you are running a C768/C384 experiment you can use them as is.

What files should you pull for starting a new experiment with warm starts from production?

That depends on what mode you want to run...free-forecast or cycled. Whichever mode navigate to the top of your COMROT and pull the entirety of the tarball(s) listed below for your mode. The files within the tarball are already in the $CDUMP.$PDY/$CYC folder format expected by the system.

free-forecast

Two tarballs to pull:

File #1 (for starting cycle SDATE):

/NCEPPROD/hpssprod/runhistory/rhYYYY/YYYYMM/YYYYMMDD/com_gfs_prod_gfs.YYYYMMDD_CC.gfs_restart.tar

File #2 (for prior cycle GDATE=SDATE-06):

/NCEPPROD/hpssprod/runhistory/rhYYYY/YYYYMM/YYYYMMDD/com_gfs_prod_gdas.YYYYMMDD_CC.gdas_restart.tar

cycled

There are 18 tarballs to pull (9 for SDATE and 9 for GDATE (SDATE-06)):

HPSS path: /NCEPPROD/hpssprod/runhistory/rhYYYY/YYYYMM/YYYYMMDD/

Tarballs per cycle:

com_gfs_prod_gdas.YYYYMMDD_CC.gdas_restart.tar
com_gfs_prod_enkfgdas.YYYYMMDD_CC.enkfgdas_restart_grp1.tar
com_gfs_prod_enkfgdas.YYYYMMDD_CC.enkfgdas_restart_grp2.tar
com_gfs_prod_enkfgdas.YYYYMMDD_CC.enkfgdas_restart_grp3.tar
com_gfs_prod_enkfgdas.YYYYMMDD_CC.enkfgdas_restart_grp4.tar
com_gfs_prod_enkfgdas.YYYYMMDD_CC.enkfgdas_restart_grp5.tar
com_gfs_prod_enkfgdas.YYYYMMDD_CC.enkfgdas_restart_grp6.tar
com_gfs_prod_enkfgdas.YYYYMMDD_CC.enkfgdas_restart_grp7.tar
com_gfs_prod_enkfgdas.YYYYMMDD_CC.enkfgdas_restart_grp8.tar

Go to the top of your COMROT/ROTDIR and pull the contents of all tarballs there. The tarballs already contain the needed directory structure.

Warm starts (from pre-production parallels)

Recent pre-implementation parallel series was for GFS v16 (implemented March 2021). For the prior v15 (Q2FY19) see an additional table below.

  • What resolution are warm-starts available for? Warm-start ICs are saved at the resolution the model was run at (C768/C384) and can only be used to run at the same resolution combination. If you need to run a different resolution you will need to make your own cold-start ICs. See cold start section above.
  • What dates have warm-start files saved? Unfortunately the frequency changed enough during the runs that it’s not easy to provide a definitive list easily.
  • What files? All warm-starts are saved in separate tarballs which include “restart” in the name. You need to pull the entirety of each tarball, all files included in the restart tarballs are needed.
  • Where are these tarballs? See below for the location on HPSS for each v16 pre-implementation parallel.
  • What tarballs do I need to grab for my experiment? Tarballs from two cycles are required. The tarballs are listed below, where $CDATE is your starting cycle and $GDATE is one cycle prior.
    • Free-forecast:
      • ../$CDATE/gfs_restarta.tar
      • ../$GDATE/gdas_restartb.tar
    • Cycled w/EnKF:
      • ../$CDATE/gdas_restarta.tar
      • ../$CDATE/enkfgdas_restarta_grp##.tar (where ## is 01 through 08) (note, older tarballs may include a period between enkf and gdas: "enkf.gdas")
      • ../$GDATE/gdas_restartb.tar
      • ../$GDATE/enkfgdas_restartb_grp##.tar (where ## is 01 through 08) (note, older tarballs may include a period between enkf and gdas: "enkf.gdas")
  • Where do I put the warm-start initial conditions? Extraction should occur right inside your COMROT. You may need to rename the enkf folder (enkf.gdas.$PDY -> enkfgdas.$PDY).

GFSv16 (March 2021) Pre-Implementation Parallel HPSS Locations

Time Period Parallel Name Archive Location on HPSS
(/NCEPDEV/emc-global/5year/emc.glopara/...)
2019050106 ~ 2019060100 v16retro0e .../WCOSS_D/gfsv16/v16retro0e/yyyymmddhh
2019060106 ~ 2019083118 v16retro1e .../WCOSS_D/gfsv16/v16retro1e/yyyymmddhh
2019090100 ~ 2019110918 v16retro2e .../WCOSS_D/gfsv16/v16retro2e/yyyymmddhh
2019111000 ~ 2020122200 v16rt2 .../WCOSS_D/gfsv16/v16rt2/yyyymmddhh
2020122206 ~ implementation v16rt2n .../WCOSS_D/gfsv16/v16rt2n/yyyymmddhh

GFSv15 (Q2FY19) Pre-Implementation Parallel HPSS Locations

Time Period Parallel Name Archive Location on HPSS
(/NCEPDEV/emc-global/5year/...)
Real-time
(05/25/2018 ~ 06/12/2019)
prfv3rt1 .../emc.glopara/WCOSS_C/Q2FY19/prfv3rt1
2017/2018 Winter/Spring
(11/25/2017 ~ 05/31/2018)
fv3q2fy19retro1 .../Fanglin.Yang/WCOSS_DELL_P3/Q2FY19/fv3q2fy19retro1
2017 Summer/Fall Part 1
(05/25//2017 ~ 08/31/2017)
fv3q2fy19retro2 .../emc.glopara/WCOSS_C/Q2FY19/fv3q2fy19retro2
2017 Summer/Fall Part 2
(08/02//2017 ~ 11/30/2017)
fv3q2fy19retro2 .../Fanglin.Yang/WCOSS_DELL_P3/Q2FY19/fv3q2fy19retro2
2016/2017 Winter/Spring
(11/25/2016 ~ 05/31/2017)
fv3q2fy19retro3 .../Fanglin.Yang/WCOSS_DELL_P3/Q2FY19/fv3q2fy19retro3
2016 Summer/Fall Part 1
(5/22/2016 ~ 08/25/2016)
fv3q2fy19retro4 .../emc.glopara/WCOSS_C/Q2FY19/fv3q2fy19retro4
2016 Summer/Fall Part 2
(08/17//2016 ~ 11/30/2016)
fv3q2fy19retro4 .../emc.glopara/WCOSS_DELL_P3/Q2FY19/fv3q2fy19retro4
2015/2016 Winter/Spring
(11/25/2015 ~ 05/31/2016)
fv3q2fy19retro5 .../emc.glopara/WCOSS_DELL_P3/Q2FY19/fv3q2fy19retro5
2015 Summer/Fall
(5/03/2015 ~ 11/30/2015)
fv3q2fy19retro6 .../emc.glopara/WCOSS_DELL_P3/Q2FY19/fv3q2fy19retro6