Download CCSM3.0 User`s Guide - CESM | Community Earth System Model

3
OBTAINING CODE, SCRIPTS AND INPUT DATA
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Table 4: inputdata/ sub-directories
ocn/docn6/
ice/csim4/
ice/dice6/
lnd/clm2/inidata 2.1/ccsm
lnd/clm2/srfdata/csm
lnd/clm2/rtmdata
lnd/clm2/pftdata
lnd/clm2/rawdata
lnd/dlnd6
cpl/cpl6/
docn cycling data
csim data
dice cycling data
clm initial data
clm surface data
clm river-routing (RTM) data
clm pft-physiology data
clm raw data to create surface datasets at model resolution
dlnd cycling data
coupler data
The initial and boundary datasets for each component will be found in their respective subdirectories.
Because it could take up several Gigabytes of disk space depending upon the resolution of the input
datasets downloaded, the input data tar files should be untarred on a disk with sufficient space.
Along with the released input datasets, we are also providing an empty directory tree, inputdata user/, that has the same structure as inputdata/, but without any files. This tree is provided
for user-created input datasets. It should be untarred in a directory parallel to the inputdata/ directory. It should not be untarred under inputdata/. If the user intends to replace an existing inputdata/
dataset with their own customized dataset, the new dataset should be give a unique filename and
placed in the corresponding directory as the original inputdata/ file that it replaces. More details are
provided in section 6.12.
3.4
Testing the downloaded source code and data files
After downloading the model source code and data sets, users are strongly advised to validate
the download by running low-resolution tests described in section 7.3.1. T31 and gx3v5 data sets are
required to run the recommended test suite.