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Title: X-Ray Emission Cross Sections following Charge Exchange by Multiply-Charged Ions of Astrophysical Interest

Journal Article · · Journal of Physics: Conference Series, vol. 58, N/A, November 30, 2006, pp. 165

The CTMC method is used to calculate emission cross sections following charge exchange processes involving highly charged ions of astrophysical interest and typical cometary targets. Comparison is made to experimental data obtained on the EBIT-I machine at Lawrence Livermore National Laboratory LLNL for O{sup 8+} projectiles impinging on different targets at a collision energy of 10 eV/amu. The theoretical cross sections are used together with ion abundances measured by the Advanced Composition Explorer to reproduce cometary spectra. Discrepancies due to different estimated delays of solar wind events between the comet and the Earth-orbiting satellite are discussed.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
908097
Report Number(s):
UCRL-JRNL-229081; TRN: US0703615
Journal Information:
Journal of Physics: Conference Series, vol. 58, N/A, November 30, 2006, pp. 165, Vol. 58
Country of Publication:
United States
Language:
English

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