Update Documentation authored by Doriann Blain's avatar Doriann Blain
......@@ -268,10 +268,22 @@ The `clouds_parameters` section handles the clouds settings. The cloud optical c
- list of floats
- (kg.m-3) density of the clouds particles
- e.g. `cloud_particle_density = 917, 1980`. The number of elements must match `n_clouds` (see [`atmosphere_parameters`](#atmosphere_parameters)).
- `supersaturation_parameter`
- list of floats
- supersaturation parameter of the clouds
- e.g. `supersaturation_parameter = 0.003, 0.003`.
- `sticking_efficiency`
- list of floats
- sticking efficiency of the clouds
- e.g. `sticking_efficiency = 1.0, 1.0`.
- `reference_wavenumber`
- list of floats
- (cm-1) [for diagnostic] wavenumber for cloud optical depth output
- e.g. `reference_wavenumber = 1e4, 1e4`. Output the cloud opacities at this wavenumber. The number of elements must match `n_clouds` (see [`atmosphere_parameters`](#atmosphere_parameters)).
- `load_cloud_profiles`
- boolean
- if True, use initial cloud profile defined in vmr_profiles_file
- e.g. `load_cloud_profiles = False`.
## retrieval_parameters
The `retrieval_parameters` section handles the retrieval/inversion settings.
......@@ -311,6 +323,10 @@ The `retrieval_parameters` section handles the retrieval/inversion settings.
- integer
- number of iterations between 2 calls of the cloud physics
- e.g. `cloud_iteration_interval = 4` mean that the cloud VMR is calculated with an interval of 4 iterations, i.e. every 5 iterations.
- `n_burn_iterations`
- integer
- number of iterations before the end where all the physics is calculated at every iterations
- e.g. `n_burn_iterations = 99`.
- `retrieval_tolerance`
- float
- tolerance for the flux convergence (0 to use the iterations limits)
......@@ -330,6 +346,10 @@ The `retrieval_parameters` section handles the retrieval/inversion settings.
## options
The `options` section handles the output options settings.
- `output_transmission_spectra`
- boolean
- if True, output the transmission spectra
- e.g. `output_transmission_spectra = True`. This enable the output of the transmission spectrum, plus the contributions to the transmission spectrum if the output contribution options are set to True (see below).
- `output_species_spectral_contributions`
- boolean
- if True, output the absorbers spectral contribution
......@@ -342,6 +362,10 @@ The `options` section handles the output options settings.
- boolean
- if True, output the thermal spectral contribution
- e.g. `output_thermal_spectral_contribution = True`. This enable the output of the thermal contribution (i.e. without light source), which is useful to calculate e.g. the Bond albedo.
- `output_fluxes`
- boolean
- if True, output the radiosities without the effect of irradiance
- e.g. `output_fluxes = True`. This enable the output of the fluxes (i.e. the radiosities without light source).
- `output_hdf5`
- boolean
- if True, set the output format to HDF5
......@@ -503,7 +527,7 @@ Structure of the file:
| ├── ...
| └── gasn
├── levels
| ├── altitude <- (array float) atltitude in levels
| ├── altitude <- (array float) altitude in levels
| ├── delta_temperature_convection<- (array float) difference of temperature due to convection
| ├── gradiant_temperature <- (array float) T gradiant
| ├── is_convective <- (array integer) (0|1) if 1, convection is occurring at the level
......@@ -516,6 +540,12 @@ Structure of the file:
| ├── temperature_adiabatic <- (array float) adiabatic temperature in levels
| ├── temperature_uncertainty <- (array float) uncertainty on temperatures
| └── temperature_uncertainty_b <- (array float) variant of the uncertainty on temperatures
├── run_quality
| ├── actual_internal_temperature <- (scalar float) actual T_int of the planet at the end of the run
| ├── chi2_retrieval <- (scalar float) reduced chi2 of the retrieval
| ├── delta_chi2_retrieval <- (scalar float) relative difference between the chi2 and the chi2 at the previous iteration.
| ├── delta_temperature <- (array float) difference between the temperature and the temperature at the previous iteration.
| └── radiosity_actual_target_ratio <- (scalar float) ratio of the actual radiosity of the planet at the end of the run and the targeted radiosity (calculated with internal_temperature in input).
└── spectra
├── emission
| ├── contributions
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