Ion equilibrium for minor components in a thin plasma

Details Ion equilibrium for minor components in a thin plasma Ion equilibrium for minor components in a thin plasma

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...91..183l&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 91, no. 1, Nov. 1991, p. 183-196.

Astronomy and Astrophysics

Astrophysics

64

Metal Ions, Optical Thickness, Plasma Equilibrium, Abundance, Cosmic Plasma, Recombination Reactions, Solar Corona

Scientific paper

The ionization equilibrium of some cosmically less abundant elements (F, P, Cl, K, Ti, Cr, Mn, and Co) is computed. The computation is performed using the Shull and Van Steenberg (1982) approximations for the ionization, radiative, dielectronic, and autoionization rates. The fitting coefficients for the rates are given and the ion abundances are supplied for temperatures between 10 exp 5 and 10 exp 8 K.

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