Versions Compared

Key

  • This line was added.
  • This line was removed.
  • Formatting was changed.

Terminology

The CPDN OpenIFS@Home documentation uses slightly different terminology to what OpenIFS users might be used to.

OpenIFS@Home Ancillary Files

This refers to all the input files that the OpenIFS model needs to run:

  • initial data to start a forecast (normally obtained from ECMWF);
  • ifsdata and climate files (downloaded from the OpenIFS ftp site);
  • model namelist (only parts of the OpenIFS namelist can be uploaded, see below)

These ancillary files are uploaded in a zipped format to the CPDN repository.

Experiment information is read from the initial files GRIB metadata upon upload to the OpenIFS@Home repository and used to set the experiment id, date/time of forecast etc.

Experiment namelist

It's not possible to upload a complete model namelist to the OpenIFS@Home website. This is because some restrictions are necessary in order for the model to work correctly and efficiently when running on a volunteer's computer.

At the time of writing, the only part of the model namelist allowed to be uploaded is the 'NAMFPC', or 'FullPos' namelist, which controls all the model's output.  Even this is vetted by CPDN first to ensure the model does not produce more output than can be reasonably handled by the volunteer's computer and network for transfer of the results back to the CPDN database.

Apart from the model's NAMFPC output control namelist, the rest of the namelist is selected as a 'template' when the experiment on OpenIFS@Home is configured. Namelist experiment templates exist for different resolutions and different classes of experiments; for example 10 day NWP forecasts, seasonal forecasts etc. For more details please see the OpenIFS@Home dashboard and documentation, or contact the CPDN team directly.

Preparing Initial Files to Upload

The upload of initial files is made from the OpenIFS@Home OpenIFS@home Dashboard on the OpenIFS@Home portal. It expects the initial files to be laid out in a particular directory structure.

There are 3 types of permitted directory structures as illustrated in the diagram left. They correspond to whether multiple dates are present, and whether ensembles of initial data are being used.

File format

Following the directory layout below, create a gzipped tarfile of the data ready to be uploaded.

Code Block
languagebash
titleExample
% tar cvfz  hijc_2017041212.tgz   hijc

(a) Single date.

In this case the directory structure would be as following:

Code Block
% ls -R hijc     #  "hha4" is the experiment id in this example
hijc/2017041212:
ICMCLhijcINIT   ICMSHhijcINIT    specwavein         wam_subgrid_0
ICMGGhijcINIT   cdwavein         uwavein            wam_subgrid_1
ICMGGhijcINIUA  sfcwindin        wam_grid_tables    wam_subgrid_2


Info

There is no fort.4 or namelist file and no 'ecmwf' directory as is common in the files downloaded from the ECMWF provided initial model files.

(b) Multiple dates.

This case is an extension of (a) but with multiple sub-directories, one for each date. The example below shows two dates but it's possible to use many more.

Code Block
languagebash
% ls -R hijc     #  "hha4" is the experiment id in this example
hijc/2017041212:
ICMCLhijcINIT   ICMSHhijcINIT    specwavein         wam_subgrid_0
ICMGGhijcINIT   cdwavein         uwavein            wam_subgrid_1
ICMGGhijcINIUA  sfcwindin        wam_grid_tables    wam_subgrid_2

hijc/2017041300:
ICMCLhijcINIT   ICMSHhijcINIT    specwavein         wam_subgrid_0
ICMGGhijcINIT   cdwavein         uwavein            wam_subgrid_1
ICMGGhijcINIUA  sfcwindin        wam_grid_tables    wam_subgrid_2

(c) Ensemble of starts and multiple dates

This is the more complex case. Not only are there multiple dates but for each date there are multiple ensemble members.

The directory structure will now look like: <expid>/<date>/<ens>/.

The following examples shows two dates, each with 3 ensemble members. By convention, there is always a '000' member.

Code Block
languagebash
% ls -R h76y       # 'h76y' is the experiment id in this case
h76y:
2016092500

h76y/2016092500:
000
001
002

h76y/2016092500/000:
ICMCLh76yINIT    ICMSHh76yINIT    specwavein         wam_subgrid_0
ICMGGh76yINIT    cdwavein         uwavein            wam_subgrid_1
ICMGGh76yINIUA   sfcwindin        wam_grid_tables    wam_subgrid_2

h76y/2016092500/001:
ICMCLh76yINIT ......    # lines omitted for brevity

h76y:
2016092512:

h76y/2016092512:
000
001
002

h67y/2016092512/000:
ICMCLh76yINIT    ICMSHh76yINIT    specwavein         wam_subgrid_0
.....   # lines omitted for brevity


Info

In this case, to save space, make links between common files in each ensemble directory.

The files that are typically the same are the:

  • Climate/boundary forcing file: ICMCL*
  • Wave model grid files: wam_grid_tables, wam_subgrid_*

By making links we have a structure that looks like (omitting some files listed above for clarity):

Code Block
% ls -lR h76y
.....
h76y/2016092500/000:
total 32032
-rw-r----- 1 nagc rd  3055416 Jun 13  2019 ICMCLh76yINIT
-rw-r----- 1 nagc rd  4489702 Jun 13  2019 ICMGGh76yINIT
-rw-r----- 1 nagc rd 15648820 Jun 13  2019 ICMGGh76yINIUA
-rw-r----- 1 nagc rd  9544080 Jun 13  2019 ICMSHh76yINIT
-rw-r----- 1 nagc rd  2546565 Jun 13  2019 cdwavein
-rw-r----- 1 nagc rd  6354333 Jun 13  2019 sfcwindin
-rw-r----- 1 nagc rd   493848 Jun 13  2019 specwavein
-rw-r----- 1 nagc rd  1138804 Jun 13  2019 uwavein
-rw-r----- 1 nagc rd  5384833 Jun 13  2019 wam_grid_tables
-rw-r----- 1 nagc rd   438485 Jun 13  2019 wam_subgrid_0
-rw-r----- 1 nagc rd   438485 Jun 13  2019 wam_subgrid_1
-rw-r----- 1 nagc rd   438485 Jun 13  2019 wam_subgrid_2

h76y/2016092500/001:
total 29144
lrwxrwxrwx 1 nagc rd       20 Jun 13  2019 ICMCLh76yINIT -> ../000/ICMCLh76yINIT
-rw-r----- 1 nagc rd  4487766 Jun 13  2019 ICMGGh76yINIT
-rw-r----- 1 nagc rd 15755898 Jun 13  2019 ICMGGh76yINIUA
-rw-r----- 1 nagc rd  9543716 Jun 13  2019 ICMSHh76yINIT
-rw-r----- 1 nagc rd  2546565 Jun 13  2019 cdwavein
-rw-r----- 1 nagc rd  6354333 Jun 13  2019 sfcwindin
-rw-r----- 1 nagc rd   493848 Jun 13  2019 specwavein
-rw-r----- 1 nagc rd  1138804 Jun 13  2019 uwavein
lrwxrwxrwx 1 nagc rd  5384833 Jun 13  2019 wam_grid_tables -> ../000/wam_grid_tables
lrwxrwxrwx 1 nagc rd   438485 Jun 13  2019 wam_subgrid_0 -> ../000/wam_subgrid_0
lrwxrwxrwx 1 nagc rd   438485 Jun 13  2019 wam_subgrid_1 -> ../000/wam_subgrid_1
lrwxrwxrwx 1 nagc rd   438485 Jun 13  2019 wam_subgrid_2 -> ../000/wam_subgrid_2

It can helpful to write a bash script to create these directory structures, check filesizes and links.

Search for available climate and ifsdata files

Normally all climate and ifsdata files will have been uploaded to CPDN for the supported resolutions.

To search what's available, go to the OpenIFS@Home Dashboard at: https://dev.cpdn.org/oifs_dashboard.php  (login if required)

Click on the 'search' button: .

ifsdata files

In the Type dropdown menu select 'ifsdata' to see the list of files available:

This will show a list similar to:

To find out more information and download the file if required, click on the blue link.

climate files

In the Type dropdown menu select 'climate_data' to generate a similar list:

This will show a similar list from which individual files can be selected for more information and downloaded if required.

Preparing climate and ifsdata to upload

Normally, this will not be necessary. All the climate and ifsdata needed to run OpenIFS on the OpenIFS@Home platform will have already been uploaded.

New files would be needed if you plan to use a modified or different set of boundary forcings e.g. a modified sea-surface temperature.

In this case, it's advised that you contact the CPDN support team for help and advice in preparing these files.





Panel
borderColorgray
borderWidth1
borderStyledotted
titleOn this page...

Table of Contents
indent15px


Panel
borderColorgray
borderWidth1
borderStyledotted
titlePages in this section...

Children Display
pageOpenIFS@Home OpenIFS@home / CPDN



Image RemovedImage AddedImage Removed


Image Added