skyscapes.physical_model.base#
Abstract physical-model interface for a planet’s radiative output.
Subclasses own whatever spectral-physics parameters describe “this kind of planet” (Lambertian, grid-interpolated, radiative-transfer, future thermal emission). The only invariant is a single hook that maps (phase_angle, star-planet distance, wavelength, planet radius) onto a contrast (flux ratio relative to the host star).
The planet radius is supplied as a method argument rather than a class
field – Rp_Rearth is a property of the planet, not the physical
model. Planet.contrast forwards self.Rp_Rearth to the physical
model at call time.
Classes#
Spectral-physics layer for a planet. |
Module Contents#
- class skyscapes.physical_model.base.AbstractPhysicalModel[source]#
Bases:
equinox.ModuleSpectral-physics layer for a planet.
Concrete subclasses own per-planet physical-model parameters (albedo, grid contrast cube, ExoJax composition, etc.). The host planet’s radius is supplied at call time via
contrast(..., Rp_Rearth=...).- abstractmethod contrast(phase_angle_rad, dist_AU, wavelength_nm, Rp_Rearth)[source]#
Return planet-to-star contrast.
- Args:
- phase_angle_rad: Star-planet-observer phase angle
beta, shape
(K, T)(matchingAbstractOrbit.propagate).
dist_AU: Star-planet distance, shape
(K, T). wavelength_nm: Wavelength, scalar or shape(W,). Rp_Rearth: Planet radius [Earth radii], shape(K,),supplied by the host
Planet.- phase_angle_rad: Star-planet-observer phase angle
- Returns:
Flux-ratio contrast, shape
(K, T).
- Parameters:
phase_angle_rad (jaxtyping.Array)
dist_AU (jaxtyping.Array)
wavelength_nm (jaxtyping.Array)
Rp_Rearth (jaxtyping.Array)
- Return type:
jaxtyping.Array