petitRADTRANS.opacities.hminus#

Functions#

`get_non_cia_gas_continuum_contributions`()
`compute_h_minus_free_free_xsec`(wavelengths, ...)	Calculate the H- free-free cross-section in units of cm^2 per H per e- pressure (in cgs).
`compute_h_minus_bound_free_xsec`(wavelengths_bin_edges)	Calculate the H- bound-free cross-section in units of cm^2 per H-, as defined on page 155 of
`compute_h_minus_opacities`(mass_fractions, pressures, ...)	Calculate the H- opacity.
`compute_non_cia_gas_induced_continuum_opacities`(...)

Module Contents#

petitRADTRANS.opacities.hminus.get_non_cia_gas_continuum_contributions()#

petitRADTRANS.opacities.hminus.compute_h_minus_free_free_xsec(wavelengths, temperatures, electron_partial_pressure)#

Calculate the H- free-free cross-section in units of cm^2 per H per e- pressure (in cgs). Source: “The Observation and Analysis of Stellar Photospheres” by David F. Gray, p. 156

Args:: wavelengths: (angstrom) temperatures: electron_partial_pressure:

Returns:

petitRADTRANS.opacities.hminus.compute_h_minus_bound_free_xsec(wavelengths_bin_edges)#

Calculate the H- bound-free cross-section in units of cm^2 per H-, as defined on page 155 of “The Observation and Analysis of Stellar Photospheres” by David F. Gray

Args:: wavelengths_bin_edges: (angstrom)

Returns:

petitRADTRANS.opacities.hminus.compute_h_minus_opacities(mass_fractions, pressures, temperatures, frequencies, frequency_bins_edges, mean_molar_masses, **kwargs)#: Calculate the H- opacity.

petitRADTRANS.opacities.hminus.compute_non_cia_gas_induced_continuum_opacities(gas_continuum_contributors, mass_fractions, pressures, temperatures, frequencies, frequency_bins_edges, mean_molar_masses, **kwargs)#