CESM2 and E3SM variables used for diagnosing westerly wind events
Data files
Oct 18, 2023 version files 5.08 GB
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CESM2_rlut_tauu_tauv_ua.tar.gz
1.76 GB
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E3SM_rlut_tauu_tauv_ua.tar.gz
3.32 GB
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README.md
2.32 KB
Abstract
This data set contains variables needed to identify and evaluate westerly wind events (WWEs) in a simulation using the Community Earth System Model version 2 (CESM2) and a simulation using the Energy Exascale Earth System Model (E3SM). The CESM2 simulation was a historical run from 1980–1999 that was restarted from the CMIP6 historical simulation. The E3SM was a 400-year pre-industrial simulation from which we analyzed the last 39 years. Only those last 39 years are included in the E3SM files.
For both the CESM2 and E3SM simulations, meridionally-averaged zonal wind stress from 2.5°S – 2.5°N filtered from 5–90 days was used to identify westerly wind events in the Pacific Ocean (120°E – 280°E). Events were defined as patches of zonal wind stress in the time-longitude plane with zonal wind stress values of 0.04 Nm-2 or larger that lasted at least 5 days and were at least 10° longitude long. Meridional wind stress was also used along with the zonal wind stress to make spatiotemporal composite wind-stress vectors across all WWEs for each model. Outgoing longwave radiation (OLR) was also used as a proxy for convection. Again spatiotemporal composites were made of OLR centered on WWEs for each model. Finally, 1000-mb zonal wind speed was used to determine if WWEs defined by 5-90 day filtered zonal wind stress actually correspond to unfiltered westerly wind speeds.
These simulations were part of a larger set of simulations used to evalute the fidelity of WWEs in CMIP6 simulations through a variety of model diagnostics. WWEs are important to air-sea feedbacks as they can initiate ocean Kelvin waves that then propagate eastward altering the thermodynamic structure of the upper ocean. Most importantly, these WWE-generated Kelvin waves can play an important role in El Nino Southern Oscillation dynamics.
https://doi.org/10.5061/dryad.63xsj3v88
There is a .tar.gz file for both the CESM2 and E3SM variables that were used to diagnose westerly wind events in each simulation. Af the tar files are unpacked there will be 4 directories that contain files for zonal and meridional wind stress, outgoing longwave radiation, and 1000-mb zonal wind speed.
Description of the data and file structure
The CESM2_rlut_tauu_tauv_ua.tar.gz file contains the following directories and files when unpacked, where each file contains one 3D variable with 64°lat x 288° lon and 7301 days. An ncdump on each file will show the metadata.
rlut -> CESM2.0_B1850.cam.h1.FLUT.30S-30N.00010101-00210101.nc
The rlut variable is the outgoing longwave radiation (W/m2)
tauu -> CESM2.0_B1850.cam.h1.TAUX.30S-30N.00010101-00210101.nc
The tauu variable is the zonal wind stress (N/m2)
tauv -> CESM2.0_B1850.cam.h1.TAUY.30S-30N.00010101-00210101.nc
The tauv variable is the meridional wind stress (N/m2)
ua -> level1000mb -> CESM2.0_BHIST.cam.h1.U1000.30S-30N.00010101-00210101.time_bnds.nc
The ua variable is the 1000-mb zonal wind speed (m/s)
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The E3SM_rlut_tauu_tauv_ua.tar.gz file contains the following directories and files when unpacked, where each file contains one 3D variable with 60°lat x 360° lon and 14235 days. An ncdump on each file will show the metadata.
rlut -> CESM2.0_B1850.cam.h1.FLUT.30S-30N.00010101-00210101.nc
The rlut variable is the outgoing longwave radiation (W/m2)
tauu -> CESM2.0_B1850.cam.h1.TAUX.30S-30N.00010101-00210101.nc
The tauu variable is the zonal wind stress (N/m2)
tauv -> CESM2.0_B1850.cam.h1.TAUY.30S-30N.00010101-00210101.nc
The tauv variable is the meridional wind stress (N/m2)
ua -> level1000mb -> ua_timeNOTrecordDim -> E3SM.ctrl.ua000.0362-0400.2p5NSavg.nc
The ua variable is the 1000-mb zonal wind speed (m/s) averaged between 2.5°S-2.5°N, so the latitude dimension has been dropped
Code/Software
Python 3.8 was used to analyze this data
