Oscillator strengths and collision strengths for S V

Details Oscillator strengths and collision strengths for S V Oscillator strengths and collision strengths for S V

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...246.1040v&link_type=abstract

Astrophysical Journal, Part 1, vol. 246, June 15, 1981, p. 1040-1044.

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13

Atomic Collisions, Extreme Ultraviolet Radiation, Jupiter (Planet), Planetary Radiation, Electron Transitions, Ground State, Molecular Oscillators, Monatomic Molecules, Transition Probabilities, Wave Functions

Scientific paper

Observations of the optical extreme-ultraviolet spectrum of the Jupiter planetary system during the Voyager space mission revealed bright emission lines of some sulfur ions. The spectra of the torus at the orbit of Io are likely to contain S V lines. The described investigation provides oscillator strengths and collision strengths for the first four UV lines. The collision strengths from the ground state to four other excited states are also obtained. Use is made of a two-state calculation which is checked for convergence for some transitions by employing a three-state or a four-state approximation. Target wave functions for S V are calculated so that the oscillator strengths calculated in dipole length and dipole velocity approximations agree within 5%.

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