[Model]
¶
This header defines the type of forward model (FM) that will be computed by TauREx3.
There are only four distinct forward model_type
:
transmission
Transmission forward model
emission
Emission forward model
directimage
Direct-image forward model
custom
User-type forward model, See Custom Types
Both emission and direct image also include an optional keyword ngauss
which
dictates the number of Gaussian quadrate points used in the integration. By default
this is set to ngauss=4
.
Contributions¶
Contributions define what processes in the atmosphere contribute to the optical depth. These contributions are defined as subheaders with the name of the header being the contribution to add into the forward model.Any forward model type can be augmented with these contributions.
Examples¶
Transmission spectrum with molecular absorption and CIA from H2-He
and H2-H2
:
[Model]
model_type = transmission
[[Absorption]]
[[CIA]]
cia_pairs = H2-He,He-He
Emission spectrum with molecular absorption, CIA and Rayleigh scattering:
[Model]
model_type = emission
ngauss = 4
[[Absorption]]
[[CIA]]
cia_pairs = H2-He,He-He
[[Rayleigh]]
The following sections give a list of available contributions
Molecular Absorption¶
[[Absorption]]
Adds molecular absorption to the forward model. Here the active molecules contribute to absorption. No other keywords are needed. No fitting parameters.
Collisionally Induced Absorption¶
[[CIA]]
Adds collisionally induced absorption to the forward model.
Requires cia_path
to be set. Both active and inactive
molecules can contribute.
No fitting parameters
Keywords¶
Variable |
Type |
Description |
|
|
List of molecular pairs. e.g. |
Rayleigh Scattering¶
[[Rayleigh]]
Adds Rayleigh scattering to the forward model. Both active and inactive molecules can contribute. No keywords or fitting parameters.
Optically thick clouds¶
[[SimpleClouds]]
or [[ThickClouds]]
A simple cloud model that puts a infinitely absorping cloud deck in the atmosphere.
Keywords¶
Variable |
Type |
Description |
|
|
Pressure of top of cloud-deck in Pa |
Fitting Parameters¶
Variable |
Type |
Description |
|
|
Pressure of top of cloud-deck in Pa |
Mie scattering (Lee)¶
[[LeeMie]]
Computes Mie scattering contribution to optical depth Formalism taken from: Lee et al. 2013, ApJ, 778, 97
Keywords¶
Variable |
Type |
Description |
|
|
Particle radius in um |
|
|
Extinction coefficient |
|
|
Mixing ratio in atmosphere |
|
|
Bottom of cloud deck in Pa |
|
|
Top of cloud deck in Pa |
Fitting Parameters¶
Parameter |
Type |
Description |
|
|
Particle radius in um |
|
|
Extinction coefficient |
|
|
Mixing ratio in atmosphere |
|
|
Bottom of cloud deck in Pa |
|
|
Top of cloud deck in Pa |
Mie scattering (BH)¶
[[BHMie]]
Computes a Mie scattering contribution using method given by Bohren & Huffman 2007
Keywords¶
Variable |
Type |
Description |
|
|
Particle radius in um |
|
|
Mixing ratio in atmosphere |
|
|
Bottom of cloud deck in Pa |
|
|
Top of cloud deck in Pa |
|
|
Path to molecule scattering parameters |
|
|
Type of mie cloud |
Fitting Parameters¶
Parameter |
Type |
Description |
|
|
Particle radius in um |
|
|
Mixing ratio in atmosphere |
|
|
Bottom of cloud deck in Pa |
|
|
Top of cloud deck in Pa |
Mie scattering (Flat)¶
[[FlatMie]]
Computes a flat absorbing region of the atmosphere across all wavelengths
Keywords¶
Variable |
Type |
Description |
|
|
Opacity value |
|
|
Bottom of absorbing region in Pa |
|
|
Top of absorbing region in Pa |
Fitting Parameters¶
Parameter |
Type |
Description |
|
|
Opacity value |
|
|
Bottom of absorbing region in Pa |
|
|
Top of absorbing region in Pa |