The H(-) equilibrium using coupled rate equations for H(-), H, H(+), H2, and H2(+)

Details The H(-) equilibrium using coupled rate equations for H(-), H, H(+), H2, and H2(+) The H(-) equilibrium using coupled rate equations for H(-), H, H(+), H2, and H2(+)

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...93...23l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 93, June 1984, p. 23-35.

Statistics

Computation

7

Computational Astrophysics, Hydrogen Ions, Ion Production Rates, Radiative Transfer, Stellar Atmospheres, Stellar Composition, Continuous Spectra, H Lines, Interatomic Forces, Ion Charge, Ionization Coefficients, Negative Ions, Opacity, Reaction Kinetics, Stellar Spectra

Scientific paper

The authors formulate rate equations for the reaction network coupling H, H-, H+, H2, and H2+. They attempt to systematize the notation, and to write the equations in a form suitable for modern computational methods of handling the coupled rate equations and radiative transfer equations, for both dynamical and static atmospheres. The authors have accounted for more processes than are generally considered in most current work; some of these may have an impact on the equilibrium of H- (hence its opacity) and on charge conservation (hence the proton density) in the atmospheres of solar-type stars.

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