Improved excitation rate coefficients for the N = 2 and N = 3 levels of CA XIX and Fe XXV including fine structure

Details Improved excitation rate coefficients for the N = 2 and N = 3 levels of CA XIX and Fe XXV including fine structure Improved excitation rate coefficients for the N = 2 and N = 3 levels of CA XIX and Fe XXV including fine structure

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apjs...59..183p&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 59, Oct. 1985, p. 183-195.

Astronomy and Astrophysics

Astrophysics

29

Calcium, Electron Scattering, Fine Structure, Iron, Oscillator Strengths, Transition Probabilities, Collision Parameters, Plasma Spectra, Tables (Data), X Ray Spectra

Scientific paper

Recently calculated collision strengths, including relativistic and resonance effects, are employed to compute Maxwellian averaged collision strengths for all 78 transitions involving the states 1 1S0, 2 3S1, 2 1S0, 2 3P0,1,2, 2 1P1, 3 3S1, 3 1S0, 3 3P0,1,2, and 3 1P1 and Ca XIX and Fe XXV. These rate parameters are tabulated at temperatures of interest in astrophysical and laboratory plasmas with radiation in the hard X-ray wavelength range.

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