Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...227..285m&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 227, no. 1, Jan. 1990, p. 285-288. Research supported by the Centre Franco-Ind
Astronomy and Astrophysics
Astrophysics
15
Configuration Interaction, Cosmic Plasma, Electron Impact, Electron States, Ground State, Wave Functions, Atomic Excitations, Fluorine, Maxwell-Boltzmann Density Function, Particle Collisions, Silicon
Scientific paper
The R-matrix method is used to calculate a large number of electron-impact excitation transitions from the ground state of the Si(5+) fluorine-like ion. Extensive configuration interaction wavefunctions are used to represent the lowest sixteen target states included in the calculation. Effective collision strengths have been calculated for electron temperatures in the range 10 to the 5th - 10 to the 6th K, by assuming a Maxwellian distribution for the velocities of the incident electrons.
Le Dourneuf M.
Mohan Man
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