The Astrophysical Journal · 1946 · 98 citations · 0 references
Natural SciencesAstronomyPhysicsAstrophysicsSolar AstronomySpectroscopyAbsorption SpectroscopyAtomic Absorption SpectroscopyAtomic SpectraHydrogen AtomHydrogen Atom SpectrumHydrogen Atom Wave FunctionsSolar Absorption Lines
In this paper the contribution to the continuous absorption coefficient of the negative hydrogen ion by the free-free transitions is evaluated in terms of the matrix elements of the acceleration in the Hartree field of a hydrogen atom. The new coefficients are larger than the earlier determinations by factors ex- ceeding 10 over the entire range of wave lengths of astrophysical interest. Tables,of the continuous absorption coefficient of H, including both the bound-free and the free-free transitions for various temperatures (2520° ~ T ~ 10,0800) and wave lengths (X > 4000 A) are also provided. It is further shown that the new coefficients are sufficient to account for the solar continuous spectrum from X 4000 A to X 25,000 A