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Title: Laboratory astrophysics: Measurements of n = n{prime} to n = 2 line emission in Fe{sup 16+} to Fe{sup 23+}

Technical Report ·
DOI:https://doi.org/10.2172/238552· OSTI ID:238552
 [1]; ; ; ; ; ;  [2];  [3];  [4]
  1. Univ. of California, Berkeley, CA (United States). Space Sciences Lab.
  2. Lawrence Livermore National Lab., CA (United States). Dept. of Physics and Space Technology
  3. Auburn Univ., AL (United States). Dept. of Physics
  4. Columbia Univ., New York, NY (United States). Dept. of Physics

One of the dominant forms of astronomical line emission in the 6 {angstrom} to 18 {angstrom} spectral region is line emission produced by n = n{prime} to n = 2 transitions in Fe{sup 16+} to Fe{sup 23+} (i.e., Fe L-shell n-2 line emission). Using the Lawrence Livermore National Laboratory electron beam ion trap (EBIT) facility, the authors have carried out a number of measurements designed to address astrophysical issues concerning Fe L-shell line emission. Desired ions are produced and trapped using the nearly monoenergetic electron beam of EBIT. Trapped ions are collisionally excited and the resulting X-ray line emission detected using Bragg crystal spectrometers. They have recently completed a line survey of Fe L-shell 3-2 line emission. The line survey will allow a more reliable accounting of line blending in astronomical spectra. They have now begun a series of broadband, high resolution line ratio measurements. These measurements are designed to benchmark atomic calculations used in astronomical plasma emission codes and also for comparison with X-ray spectral observations of astronomical objects. Initial measurements have been carried out in Fe{sup 23+}. Preliminary results agree with distorted wave calculations to within 20% and better.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States)
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
238552
Report Number(s):
UCRL-JC-123517; CONF-960155-4; ON: DE96010823; CNN: Grant NASA NAGW-4185; TRN: AHC29612%%102
Resource Relation:
Conference: 10. American Physical Society (APS) topical conference on atomic processes and plasmas, San Francisco, CA (United States), 14-18 Jan 1996; Other Information: PBD: 5 Mar 1996
Country of Publication:
United States
Language:
English