Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1772487 | High Energy Density Physics | 2013 | 8 Pages |
Abstract
This paper is devoted to a theoretical description of the spectral absorption in warm dense plasmas, such as those involved in hohlraum-based opacity measurements. Dealing with complex spectra, when the effect of natural and experimental broadening, optical thickness and line overlap are taken into account, the calculation of plasma transmission becomes quite intricate. Taking as a working hypothesis a large experimental broadening, simple analytical formulas are obtained for this transmission. The formulas are checked by comparison to the exact convolution of various detailed spectra with a broadening profile. The current numerical method is then applied to the computation of transmission in Fe and Br plasmas, where opacity and line-overlap effects may be substantial.
Keywords
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Astronomy and Astrophysics
Authors
M. Poirier,