swahl@geomar_de
Member
Dear all
sorry for asking another question, but the following came up today in a discussion and it's essential for us to know for planning future experiments with CESM 1.2.0
We currently have a setup with the B_1955-2005_WACCM_CN compset. Questions:
- How is the O3 (ozone) dealt with in the radiation (camrt) code. Is the 3D structure from the MOZART chemistry used in the radiation calculations or are they any simplifications applied before doing the radiative transfer calculations? We looked extensively at the source code and came to the conclusion that the full 3D ozone information is used in the radiation calculation. Can someone confirm this?
- Is the a difference between upper (WACCM) and lower atmosphere (CAM) on how ozone is treated in the radiation?
- How does it work with the CO2? As the above compset contains a carbon cycle we do have 3D CO2 distribution which is reduced to (lat,lon) via " call calc_col_mean(state, co2, co2_col_mean)" in radiation.F90. So does the real 3D structure go into the radiation? (Or is just the value from the external GHG forcing file used (e.g. CO2 from ghg_rcp45_1960clim_c110503.nc in case one uses "climatological" CO2)?)
A simple yes/no answer is sufficient as we just want to make sure we got everything right.
sorry for asking another question, but the following came up today in a discussion and it's essential for us to know for planning future experiments with CESM 1.2.0
We currently have a setup with the B_1955-2005_WACCM_CN compset. Questions:
- How is the O3 (ozone) dealt with in the radiation (camrt) code. Is the 3D structure from the MOZART chemistry used in the radiation calculations or are they any simplifications applied before doing the radiative transfer calculations? We looked extensively at the source code and came to the conclusion that the full 3D ozone information is used in the radiation calculation. Can someone confirm this?
- Is the a difference between upper (WACCM) and lower atmosphere (CAM) on how ozone is treated in the radiation?
- How does it work with the CO2? As the above compset contains a carbon cycle we do have 3D CO2 distribution which is reduced to (lat,lon) via " call calc_col_mean(state, co2, co2_col_mean)" in radiation.F90. So does the real 3D structure go into the radiation? (Or is just the value from the external GHG forcing file used (e.g. CO2 from ghg_rcp45_1960clim_c110503.nc in case one uses "climatological" CO2)?)
A simple yes/no answer is sufficient as we just want to make sure we got everything right.