A method to perform a Mars experiment is described.
Following physical processes are used in this experiment.
This experiment requires data of distribution of surface properties and radiative property. So, the experiment is performed with the following 4 steps:
Here, we perform an experiment in practice/Mars-exp directory. Please create the directory and enter there as follows:
$ cd practice $ mkdir Mars-exp $ cd Mars-exp
Then, executable files and configuration files are copied as follows:
$ cp ../../src/main/dcpam_main ../../src/main/init_data ../../src/main/sst_data . $ cp ../../src/sample_nml/*.nml .
Note that you can perform an experiment in any directory by using executable files and configuration (namelist) files.
This experiment requires additional data, sea surface temperature, surface properties, sea ice density, and ozone distribution. Those data are prepared at following site.
Please download "sp_for_Mars_T21_MGS+MGS+cons.nc" and "lnactbl15m_2006-07-13.nc" from above site, and place those files at experimental directory.
At the last, run a experiment using "dcpam_main" and "dcpam_M_T21L32.nml". Resolution is T21L32. Integration time is 2 days. A restart data file, a restart data file of surface data, and some history data files are output.
$ ./dcpam_main -N=dcpam_M_T21L32.nml | tee Mars.log
If initial data, surface data, settings of experiments want to be changed, edit "init_data_M_T21L32.nml", "dcpam_M_T21L32.nml".