diff --git a/LEM.png b/LEM.png deleted file mode 100644 index b8dff74ced2a27125756ced01db30ddcddd30c14..0000000000000000000000000000000000000000 Binary files a/LEM.png and /dev/null differ diff --git a/offlineRT/README.md b/offlineRT/README.md index 4e08ec14a240e985d862eb2b00f7c025438e3425..f02df4c4a26f695f422345c094bad62c3b6682b4 100644 --- a/offlineRT/README.md +++ b/offlineRT/README.md @@ -3,12 +3,14 @@ This directory contains scripts for pre- and post-processing of input and output * **input_for_libradtran.ipynb** This Jupyter notebook generates the input files for LibRadTran from ICON-LEM output files. * Subdirectories **c_cluster_solar/thermal_...** are for different radiative transfer calculations. + * List of radiative transfer calculations: + - c_cluster_solar/thermal_ipa3d: 1D radiative transfer calculations with Delta-Eddington two-stream solver and ice-optical parameterizations by Fu and Baum - c_cluster_solar/thermal_mystic: 3D and 1D radiative transfer calculations with the MYSTIC solver - c_cluster_solar/thermal_ipa3d_cg/dl: 1D radiative transfer calculations with the Delta-Eddington two-stream solver for NWP homogeneous grid-box clouds and homogeneous clouds with cloud fraction at a resolution of 2.5 km - solar/thermal_clear_sky: Clear-sky radiative transfer calculations with Delta-Eddington two-stream and MYSTIC solvers -* To run the offline radiative transfer calculations, run the bash script *'step1_makeInpFiles.sh' in the desired radiative transfer_subdirectory/ccSolar/thermal. This will automatically create input files for all subdomains and time steps to be used by the *'uvspec' program of LibRadtran.Finally, run *'submit_runs.sh' to distribute the runs to different nodes. The outputs are radiative heating rates written as ASCII files in the representative subdirectory. +* To run the offline radiative transfer calculations, run the bash script *'step1_makeInpFiles.sh'* in the desired radiative transfer_subdirectory/ccSolar/thermal. This will automatically create input files for all subdomains and time steps to be used by the *'uvspec'* program of LibRadtran.Finally, run *'submit_runs.sh'* to distribute the runs to different nodes. The outputs are radiative heating rates written as ASCII files in the representative subdirectory. * The python scripts **convert_libradtran_data_to_netcdf().py** process the all-sky and clear-sky radiative heating rate outputs from each radiative transfer calculation and merge the outputs from all subdomains to get the heating rates over the entire LEM domain and save the result as a netcdf file. diff --git a/sims/README.md b/sims/README.md index e5d824ad4d6f8dfeebfc9789f9fcb5258d0fd183..7d2e18b499033f50e842d88fb546870b8605c193 100644 --- a/sims/README.md +++ b/sims/README.md @@ -5,6 +5,7 @@ This directory contains the scripts for setting up the ICON model for both the b * The **preprocessing** subdirectory contains the scripts to prepare the initial and lateral boundary conditions from the ICON-NWP simulation for ICON-LEM simulations with DWD_ICON_tools and CDO. * The **runscript** subdirectory contains the ICON runscript for the baroclinic life cycle and large eddy model simulations. - - The baroclinic life cycle simulation (*LC1-channel-4000x9000km-2km-0002) follows the same model setup as in Keshtgar et al., 2023 (https://wcd.copernicus.org/articles/4/115/2023/). + + - The baroclinic life cycle simulation (*LC1-channel-4000x9000km-2km-0002*) follows the same model setup as in Keshtgar et al., 2023 (https://wcd.copernicus.org/articles/4/115/2023/). - The model setup procedure is described here: https://gitlab.phaidra.org/climate/keshtgar-etal-crh-cyclone-wcd2022/-/tree/main/blc_initial_conditions