effective_temperature
effective_temperature¶
- frei.effective_temperature(grid, spec, dtaus, final_temps)[source]¶
Compute effective temperature of an atmosphere given the outputs from
emit.This is the mean of the effective temperatures computed from Milne’s solution and the Stefan-Boltzmann law.
- Parameters
grid (Grid) – Wavelength, pressure and temperature grid
spec (Spectrum1D) – Emission spectrum
dtaus (ndarray) – Change in optical depth in final iteration
final_temps (Quantity) – Temperature grid in the final iteration