Non-equilibrium scattering in the ultraviolet line haze and retarded hydrogen ionization at millimeter wavelengths are the two key obstacles for simulation-based solar irradiance modeling.
: 1989 , How deep can one see into the Sun? 124 ( 1 ), 15
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Non-Equilibrium Spectrum Formation Affecting Solar Irradiance
Non-equilibrium scattering in the ultraviolet line haze and retarded hydrogen ionization at millimeter wavelengths are the two key obstacles for simulation-based solar irradiance modeling.