... | ... | @@ -268,10 +268,22 @@ The `clouds_parameters` section handles the clouds settings. The cloud optical c |
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- list of floats
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- (kg.m-3) density of the clouds particles
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- e.g. `cloud_particle_density = 917, 1980`. The number of elements must match `n_clouds` (see [`atmosphere_parameters`](#atmosphere_parameters)).
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- `supersaturation_parameter`
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- list of floats
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- supersaturation parameter of the clouds
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- e.g. `supersaturation_parameter = 0.003, 0.003`.
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- `sticking_efficiency`
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- list of floats
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- sticking efficiency of the clouds
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- e.g. `sticking_efficiency = 1.0, 1.0`.
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- `reference_wavenumber`
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- list of floats
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- (cm-1) [for diagnostic] wavenumber for cloud optical depth output
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- 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)).
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- `load_cloud_profiles`
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- boolean
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- if True, use initial cloud profile defined in vmr_profiles_file
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- e.g. `load_cloud_profiles = False`.
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## retrieval_parameters
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The `retrieval_parameters` section handles the retrieval/inversion settings.
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... | ... | @@ -311,6 +323,10 @@ The `retrieval_parameters` section handles the retrieval/inversion settings. |
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- integer
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- number of iterations between 2 calls of the cloud physics
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- e.g. `cloud_iteration_interval = 4` mean that the cloud VMR is calculated with an interval of 4 iterations, i.e. every 5 iterations.
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- `n_burn_iterations`
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- integer
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- number of iterations before the end where all the physics is calculated at every iterations
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- e.g. `n_burn_iterations = 99`.
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- `retrieval_tolerance`
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- float
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- tolerance for the flux convergence (0 to use the iterations limits)
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... | ... | @@ -330,6 +346,10 @@ The `retrieval_parameters` section handles the retrieval/inversion settings. |
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## options
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The `options` section handles the output options settings.
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- `output_transmission_spectra`
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- boolean
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- if True, output the transmission spectra
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- 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).
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- `output_species_spectral_contributions`
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- boolean
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- if True, output the absorbers spectral contribution
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... | ... | @@ -342,6 +362,10 @@ The `options` section handles the output options settings. |
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- boolean
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- if True, output the thermal spectral contribution
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- 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.
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- `output_fluxes`
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- boolean
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- if True, output the radiosities without the effect of irradiance
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- e.g. `output_fluxes = True`. This enable the output of the fluxes (i.e. the radiosities without light source).
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- `output_hdf5`
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- boolean
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- if True, set the output format to HDF5
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... | ... | @@ -503,7 +527,7 @@ Structure of the file: |
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| ├── ...
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| └── gasn
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├── levels
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| ├── altitude <- (array float) atltitude in levels
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| ├── altitude <- (array float) altitude in levels
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| ├── delta_temperature_convection<- (array float) difference of temperature due to convection
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| ├── gradiant_temperature <- (array float) T gradiant
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| ├── is_convective <- (array integer) (0|1) if 1, convection is occurring at the level
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... | ... | @@ -516,6 +540,12 @@ Structure of the file: |
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| ├── temperature_adiabatic <- (array float) adiabatic temperature in levels
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| ├── temperature_uncertainty <- (array float) uncertainty on temperatures
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| └── temperature_uncertainty_b <- (array float) variant of the uncertainty on temperatures
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├── run_quality
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| ├── actual_internal_temperature <- (scalar float) actual T_int of the planet at the end of the run
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| ├── chi2_retrieval <- (scalar float) reduced chi2 of the retrieval
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| ├── delta_chi2_retrieval <- (scalar float) relative difference between the chi2 and the chi2 at the previous iteration.
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| ├── delta_temperature <- (array float) difference between the temperature and the temperature at the previous iteration.
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| └── 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).
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└── spectra
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├── emission
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| ├── contributions
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... | ... | |