Electron impact excitation cross sections for O III

Details Electron impact excitation cross sections for O III Electron impact excitation cross sections for O III

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26as...40..259g&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 40, May 1980, p. 259-261.

Astronomy and Astrophysics

Astrophysics

1

Atomic Excitations, Electron Impact, Inelastic Scattering, Oxygen Ions, Wave Functions, Astrophysics, Born Approximation, Cross Sections, Ground State, Oscillators

Scientific paper

An analytic atomic independent particle model is used to generate wave functions for the valence and excited states of O III; the relevance of the model to astrophysical processes (particularly in the solar corona and chromosphere) is considered. These wave functions are used along with the Born approximation and the LS coupling scheme to calculate generalized oscillator strengths and integrated cross sections from threshold to 1 keV for the electron impact excitation of O III from the ground state 2p2(3P0) to the excited states 3s, 4s, 5s, 3p, 4p, 3d, 4d, and 5d.

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