Published May 2006 | Version v1
Journal article

Study of X-ray photoionized Fe plasma and comparisons with astrophysical modeling codes

  • 1. Lawrence Livermore National Laboratory, Livermore, CA 94551 (United States)
  • 2. Department of Pure and Applied Physics, Queen's University Belfast, BT7 1NN (United Kingdom)
  • 3. Sandia National Laboratory, Albuquerque, NM, 37185 (United States)
  • 4. Department of Physics, Clarendon Laboratory, Parks Road, Oxford OX1 3PU (United Kingdom)

Description

The charge state distributions of Fe, Na and F are determined in a photoionized laboratory plasma using high-resolution X-ray spectroscopy. Independent measurements of the density and radiation flux indicate the ionization parameter ξ in the plasma reaches values ξ=20-25ergcms-1 under near steady-state conditions. A curve-of-growth analysis, which includes the effects of velocity gradients in a one-dimensional expanding plasma, fits the observed line opacities. Absorption lines are tabulated in the wavelength region 8-17A. Initial comparisons with a number of astrophysical X-ray photoionization models show reasonable agreement

Additional details

Identifiers

DOI
10.1016/j.jqsrt.2005.05.057;
PII
S0022-4073(05)00188-3;

Publishing Information

Journal Title
Journal of Quantitative Spectroscopy and Radiative Transfer
Journal Volume
99
Journal Issue
1-3
Journal Page Range
p. 712-729
ISSN
0022-4073
CODEN
JQSRAE

Optional Information

Copyright
Copyright (c) 2005 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.