Observations¶
The [observe] section configures synthetic observation generation. PROTEUS
can compute transit and eclipse depth spectra from the simulated atmospheric
state using the petitRADTRANS forward model.
The [accretion] section is reserved for late accretion modelling (not yet
implemented).
Synthetic observations [observe]¶
| Parameter | Type | Default | Description |
|---|---|---|---|
module |
str or none | "none" |
Observation module: petitRADTRANS or none (disabled) |
source |
str | "all" |
Composition source selection: all, outgas, profile, or offchem |
spectrum_type |
str | "both" |
Spectrum products to generate: both, transit, or eclipse |
remove_one_gas |
bool | true |
Generate leave-one-out spectra (<SPECIES>_removed/ppm columns) |
clip_vmr |
float | 1e-8 |
Minimum VMR below which a species is excluded from the radiative transfer |
reference_pressure |
float | 10 |
Reference pressure level used to set the planet radius baseline [bar] |
petitRADTRANS [observe.petitRADTRANS]¶
petitRADTRANS computes wavelength-dependent
transit and emission depths from the atmospheric composition and
temperature-pressure profile. Its opacity tables are read from
$FWL_DATA/prt/input_data (set via the FWL_DATA environment variable at
PROTEUS startup).
Composition sources¶
The atmospheric composition passed to petitRADTRANS is controlled by
observe.source:
all(default): compute spectra for all available sourcesoutgas,profile, oroffchem: compute spectra only for the selected source
Available source modes:
| Source | Description |
|---|---|
outgas |
Constant VMR with height from the outgassing module (helpfile *_vmr columns) |
profile |
Full vertical VMR profile from the climate module NetCDF output (*_vmr arrays) |
offchem |
Photochemical composition from the VULCAN offline chemistry output |
When observe.source = "all", unavailable sources are skipped automatically:
profile is skipped when atmos_clim.module = "dummy", and offchem is
skipped when atmos_chem.module is none.
When observe.source is set explicitly to profile or offchem, PROTEUS
raises an error if the required upstream module is unavailable.
The spectrum product set is controlled by observe.spectrum_type:
both(default): compute both transit and eclipse spectratransit: compute only transit spectraeclipse: compute only eclipse spectra
Supported line species¶
The following gases are searched for in the petitRADTRANS correlated-k
opacity table directory. A species is included only when its corresponding
opacity directory exists under input_data/opacities/lines/correlated_k/:
H2O, H2, CO2, CO, CH4, SO2, H2S, O2, N2, NH3, OH
The species whose opacity file has the broadest wavelength coverage is moved to the front of the line-species list before calling petitRADTRANS. This helps avoid opacity-table overlap issues in the forward-model initialisation.
Rayleigh and CIA species¶
Rayleigh scattering and collision-induced absorption (CIA) species are taken
from the constants defined in proteus.utils.constants
(prt_rayleigh_species, prt_cia_species) and are filtered to those present
in the actual gas mixture.
Profile interpolation¶
Before calling petitRADTRANS, the temperature and VMR profiles are interpolated onto a uniform 100-point log-spaced pressure grid using PCHIP splines. Temperature values are clipped to the range [100.5 K, 3999.5 K] to stay within petitRADTRANS table bounds. If the atmosphere profile is stored with decreasing pressure (surface first), it is reversed to ascending order before interpolation.
Leave-one-out species spectra¶
After computing the baseline spectrum (all species present), PROTEUS can optionally re-run petitRADTRANS once per line species, removing one species at a time. This produces additional spectrum columns in the output CSV that show the contribution of each individual gas to the total signal.
This behaviour is controlled by observe.remove_one_gas.
Set it to false to write baseline-only spectra.
Set observe.petitRADTRANS.silent = true to silence the opacity-loading
console messages emitted by petitRADTRANS when creating Radtrans objects.
See Output format for the CSV column layout.
Configuration options¶
| Parameter | Type | Default | Description |
|---|---|---|---|
line_opacity_mode |
str | "c-k" |
Opacity treatment: "c-k" (correlated-k, faster) or "lbl" (line-by-line, higher spectral resolution) |
include_rayleigh |
bool | true |
Include Rayleigh scattering contributions |
include_cia |
bool | true |
Include collision-induced absorption contributions |
silent |
bool | false |
Suppress petitRADTRANS stdout/stderr during Radtrans initialization |
Late accretion [accretion]¶
| Parameter | Type | Default | Description |
|---|---|---|---|
module |
str or none | none |
Late accretion module (reserved for future implementation) |
See also: Model description | Output format | Postprocessing