ACCESS-ESM1.5
Release: 1.2
Getting started
Updates
UM code update for controling orbital parameters at runtime #115, #116
Include reduced “spinup” diagnostic profiles suitable for long spin-up and paleoclimate simulations #105, #106
Include basin mask ocean input file for proper saving of basin specific diagnostics #101, #102
Change processor decomposition for better performance #109, #110
Fix incorrectly saved atmosphere variable
2,290 TOTAL DOWNWARD PAR FLUX AT SURFACE
#107, #108
Compress large CICE log files #532
Prevent simulations from using incorrect sea ice restarts #539
Updated netCDF file names for converted atmosphere output #93
CASA-CNP variables are correctly named in the netCDF conversion #157
Notes
- Orbital parameters can now be set at runtime in the UM
namelist
files. Instructions on controlling them are available here. - The new “spinup” diagnostic profiles produce a reduced amount of model output and are designed for long spin-up simulations. Please see this post for details on the variables saved.
- Basin specific ocean diagnostics (such as
temp_merid_flux_gyre_atlantic
) are now correctly saved. Please see this topic for details on the previous issues. - Increasing the number of processors allocated to the atmosphere by 48 cores was found to reduce the typical runtime by 10% with a negligible cost in SU usage. Large variations in walltimes were observed due to potential system-wide issues, however under typical circumstances the updated processor decomposition
- The new configurations use the updated um2nc version 1.1.0 for converting atmosphere outputs to netCDF. The new version produces netCDF filenames containing more information on dates and data frequencies. For example,
aiihca.paa1jan
andaiihca.pea1jan
are now namedaiihca.pa-010101_mon.nc
andaiihca.pe-010101_dai.nc
. This change in behaviour can be disabled by loading the olderpayu/1.1.5
in theUM_conversion_job.sh
job script.
Limitations
Maximum model run-time of 1 year per queue submission
Not directly compatible with equivalent CLEX
payu
configurations
Known Issues
Ice diagnostics measuring a rate are incorrect
Occasional extreme sea-ice thickness in isolated grid cells
The historical forcing configuration does not reproduce CMIP6 r20 due to an error in the ancillaries for that experiment
Model configurations do not reproduce equivalent CMIP6 simulations, possibly due to differences in model executables. Details on the impacts of this will be documented shortly.
Credits
ACCESS-ESM1.5 was developed by CSIRO (Ziehn T, Chamberlain MA, Law RM, Lenton A, Bodman RW, Dix M, Stevens L, Wang YP, Srbinovsky J, 2020: The Australian Earth System Model: ACCESS-ESM1.5. Journal of Southern Hemisphere Earth Systems Science 70 , 193–214, https://doi.org/10.1071/ES19035)
payu
configurations were adapted from work by The Centre of Excellence for Climate Extremes (CLEX)
Model build infrastructure @paulleopardi @harshula @TommyGatti
Configuration development and testing @spencerwong @paulleopardi @MartinDix @anton @minghangli @dougiesquire @Aidan
Related
payu
development @jo-basevi @spencerwong @anton
Model post-processing @bend @spencerwong @MartinDix @atteggiani
Testing and deployment infrastructure @TommyGatti @jo-basevi @Aidan
Documentation @spencerwong @atteggiani @Aidan @jasmeen_kaur
Support
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If you have specific questions about this release follow the guidelines for requesting support from ACCESS-NRI .
If you have questions about access-esm create a topic in Earth System and tag it with access-esm. If you require assistance follow the guidelines for requesting help.
Resources
- How to run the model: Run ACCESS-ESM - ACCESS-Hive
- Model configuration repository: GitHub - ACCESS-NRI/access-esm1.5-configs: Standard ACCESS-ESM1.5 configurations released and supported by ACCESS-NRI
- Model configuration releases: Releases · ACCESS-NRI/access-esm1.5-configs · GitHub
- Model version releases: Releases · ACCESS-NRI/ACCESS-ESM1.5 · GitHub
- Model paper: CSIRO PUBLISHING | Journal of Southern Hemisphere Earth Systems Science.