Emission Line Spectra in the Soft X-Ray Region 20-75 (Angstrom)
Conference
·
OSTI ID:15002783
As part of a project to complete a comprehensive catalogue of astrophysically relevant emission lines in support of new-generation X-ray observatories using the Lawrence Livermore electron beam ion traps EBIT-I and EBIT-II, we studied emission lines of argon and sulfur in the soft X-ray and extreme ultraviolet region. Here we present observations of Ar IX through Ar XVI and S VII through S XIV between 20 and 75 {angstrom} to illustrate our work.
- Research Organization:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Organization:
- US Department of Energy (US)
- DOE Contract Number:
- W-7405-ENG-48
- OSTI ID:
- 15002783
- Report Number(s):
- UCRL-JC-149432; TRN: US0402365
- Resource Relation:
- Conference: Laboratory Astrophysics Workshop, NASA Ames, Moffett Field, CA (US), 05/01/2002--05/03/2002; Other Information: PBD: 18 Jun 2002
- Country of Publication:
- United States
- Language:
- English
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