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Collision strengths for the intercombination lines of S IIIThe collision strengths of intercombination lines of S III ions observed in the Io torus are calculated on the basis of data gathered by Voyager instruments, the IUE and the Faint Object Telescope. The doubly ionized ions are excited by electron impacts and move from the 3P2P(3) ground state to excited 3s3P3(1)PO, (1)DO, 3p3d(1)PO, and 3p4s(1)PO states. Excitational cross sections are calculated with a two-state close-coupling approximation for the energy range up to 1,000,000 K, with target states being represented by multiconfiguration interaction wave functions. The close-coupling approximation regarded as an accurate technique because of the dominance of the Coulomb factor in the ionized state. The wave function calculations are estimated to yield values accurate to within 30 percent. Further work is need to quantify the magnitude of error introduced by resonance contributions to the collision strengths.
Document ID
19860051040
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ho, Y. K.
(Louisiana State Univ. Baton Rouge, LA, United States)
Henry, R. J. W.
(Louisiana State University Baton Rouge, United States)
Date Acquired
August 12, 2013
Publication Date
April 15, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 303
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
86A35778
Funding Number(s)
CONTRACT_GRANT: NAGW-48
Distribution Limits
Public
Copyright
Other

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