Razumovskyy / VenusLW

K-terms for radiative transfer in Venus Atmosphere in longwave region

VenusLW

Getting k-distributions for radiative transfer in Venus Atmosphere in longwave region (10 - 6000 cm^-1). After running the executables one can obtain the next k-term in a given spectral band.

Note

• obtaining k-terms is an iterative process and requires running this programs several times.
• resulting parameterizations are strongly affected by input atmospheric profile and chosen spectroscopy (look in PTTables repository).

Prerequisites:

• Ubuntu 20.04 (or other Linux distro)
• gfortran compiler
• matplotlib (for plots)
• precalculated spectral PT-tables located in /srv/PT_TABLES/ directory. PT-tables should be available for CO₂, SO₂ and H₂O atmospheric components.

Building the project:

To build, type: ./make.sh in the terminal. Make sure you are in the root directory of the project.

Steps:

1. Fill the input file "band_settings.txt". Example (for the first channel):

   __1 M 10.0D0 200.0D0 H2 H2O_gas_profile.dat

2. Fill the file "channel_settings.txt". Set values of thresholds of absorption coeffcient for lower and upper atmospheric levels. Example:

   0.0 1 1e15 50

3. Run the executables

4. Run Python scripts plot_cooling.py, plot_flux_down.py, or plot_flux_up.py to plot cooling rates and upward/downward fluxes, to compare the accuracy of the obtained k-term (current channel number in band_settings.txt file).

5. If needed, repeat steps 1-4 with updated input values in channels_settings.txt file to get more accurate k-term.