... | ... | @@ -44,7 +44,7 @@ The `target_parameters` section handles the target (planet) settings. |
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- `use_gravity`
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- boolean
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- if True, uses equatorial gravity instead of mass to calculate gravity
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- e.g. `use_gravity = False`. In that case, the equatorial gravity at 1 bar will be derived from `target_equatorial_radius` and `target_mass`. If `True`, the equatorial gravity at 1 bar will be derived from `target_equatorial_gravity`.
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- e.g. `use_gravity = False`. In that case, the equatorial gravity at 1 bar is derived from `target_equatorial_radius` and `target_mass`. If `True`, the equatorial gravity at 1 bar is derived from `target_equatorial_gravity`.
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- `use_flattening`
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- boolean
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- if True, uses flattening instead of polar radius to calculate gravity
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... | ... | @@ -91,11 +91,11 @@ The `light_source_parameters` section handles the light source (star) settings. |
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- `use_irradiation`
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- boolean
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- if True, use irradiation instead of range to calculate the light source spectrum
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- e.g. `use_irradiation = False`. In that case, the irradiation will be calculated using `light_source_range`. If `True`, the distance between the light source and the target will be directly calculated from `use_light_source_spectrum`.
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- e.g. `use_irradiation = False`. In that case, the irradiation will be calculated using `light_source_range`. If `True`, the distance between the light source and the target will be calculated from `light_source_irradiation`.
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- `use_irradiation`
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- boolean
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- if True, use a spectrum for the light source instead of a black body
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- e.g. `use_light_source_spectrum = False`. In that case, the spectral irradiance of the target will be calculated from a black body. If `True`, the spectral irradiance will be read from `light_source_spectrum_file` and re-adapted so that the light source radiosity correspond to `light_source_effective_temperature`.
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- e.g. `use_light_source_spectrum = False`. In that case, the spectral irradiance of the target will be calculated from a black body. If `True`, the spectral irradiance is read from `light_source_spectrum_file` and re-adapted so that the light source radiosity correspond to `light_source_effective_temperature`.
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- `light_source_radius`
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- float
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- (m) radius of the light source
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... | ... | @@ -181,6 +181,7 @@ The `atmosphere_parameters` section handles the atmospheric settings. |
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- e.g. `pressure_min = 1e7`. Used only if `use_pressure_grid` is `False`.
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## species_parameters
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The `species_parameters` section handles the atmospheric elemental abundances, which absorbing species to include and the chemical mode (equilibrium or out-of-equilibrium).
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- `use_atmospheric_metallicity`
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- boolean
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- if True, use the atmospheric metallicity instead of the element/H ratios or the elements metallicity to get the elemental abundances
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... | ... | @@ -227,8 +228,26 @@ The `atmosphere_parameters` section handles the atmospheric settings. |
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- e.g. `vmr_profiles_file = 'vmr_example_ref.dat'`. The file must be in the `path_vmr_profiles` directory.
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## spectrum_parameters
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The `spectrum_parameters` section handles the spectral range and resolution of the calculated spectrum.
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- `wavenumber_min`
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- float
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- (cm-1) first wavenumber of the calculated spectrum
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- e.g. `wavenumber_min = 130`.
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- `wavenumber_max`
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- float
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- (cm-1) last wavenumber of the calculated spectrum
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- e.g. `wavenumber_min = 30130`.
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- `wavenumber_step`
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- float
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- (cm-1) wavenumber step of the calculated spectrum
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- e.g. `wavenumber_min = 200`.
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## clouds_parameters
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The `clouds_parameters` section handles the clouds settings.
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- `cloud_mode`
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- string
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- cloud mode ('fixedRadius'|'fixedSedimentation'|'fixedRadiusCondensation'|'fixedRadiusTime')
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- e.g. `eddy_mode = 'fixedSedimentation'`. `'fixedRadius'` mean that the mean cloud particle radius is constant within the pressure grid, set to the value of `cloud_particle_radius`. `'fixedSedimentation'` mean that mean cloud particle is calculated based on the value of `sedimentation_parameter` (see [Ackerman and Marley 2001](https://iopscience.iop.org/article/10.1086/321540/fulltext/52911.text.html)). `'AckermanConvective'` mean that Kzz is calculated using the method from Ackerman et al, but taking into account the convective flux. `'infinity'` is the same than AckermanConvective, but if `cloud_mode = 'fixedRadius'` (see [`clouds_parameters`](#clouds_parameters)), the cloud will extend to the top of the atmosphere (no sedimentation).
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## retrieval_parameters
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... | ... | |