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
Similar Records
Cometary X-ray emission: theoretical cross sections following charge exchange by multiply charged ions of astrophysical interest
X-ray emission cross sections following charge exchange by multiply charged ions of astrophysical interest
X-Ray Emission Cross Sections following Charge Exchange by Multiply-Charged Ions of Astrophysical Interest
Journal Article
·
Tue Feb 13 00:00:00 EST 2007
· Canadian Journal of Physics
·
OSTI ID:908097
X-ray emission cross sections following charge exchange by multiply charged ions of astrophysical interest
Journal Article
·
Wed Feb 15 00:00:00 EST 2006
· Physical Review. A
·
OSTI ID:908097
X-Ray Emission Cross Sections following Charge Exchange by Multiply-Charged Ions of Astrophysical Interest
Journal Article
·
Mon Sep 19 00:00:00 EDT 2005
· Physical Review A, vol. 73, N/A, September 23, 2005, pp. 022723
·
OSTI ID:908097