2006
DOI: 10.1103/physrevlett.97.035001
|View full text |Cite
|
Sign up to set email alerts
|

Opacity Measurements of a Hot Iron Plasma Using an X-Ray Laser

Abstract: The temporal evolution of the opacity of an iron plasma at high temperature (30-350 eV) and high density (0.001-0.2 g cm-3) has been measured using a nickel-like silver x-ray laser at 13.9 nm. The hot dense iron plasma was created in a thin (50 nm) iron layer buried 80 nm below the surface in a plastic target that was heated using a separate 80 ps pulse of 6-9 J, focused to a 100 microm diameter spot. The experimental opacities are compared with opacities evaluated from plasma conditions predicted using a flui… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
12
0

Year Published

2009
2009
2018
2018

Publication Types

Select...
5
5

Relationship

1
9

Authors

Journals

citations
Cited by 34 publications
(12 citation statements)
references
References 24 publications
0
12
0
Order By: Relevance
“…Although experiments can now recreate conditions that are similar in density and temperature to the conditions in the Sun's interior, they usually do not directly measure opacity over a broad X-ray energy range. They either measure the emission properties of the heated plasma and assume that emissivity and opacity are in equilibrium [281], or use non-tunable X-ray lasers [282]. Recent seminal experiments at Sandia's Z machine [238] measured the iron opacity at solar interior conditions higher than predicted at energies around 1 keV, which could explain discrepancies between solar models and helioseismic observations.…”
Section: Opacity In Hot Dense Plasmasmentioning
confidence: 99%
“…Although experiments can now recreate conditions that are similar in density and temperature to the conditions in the Sun's interior, they usually do not directly measure opacity over a broad X-ray energy range. They either measure the emission properties of the heated plasma and assume that emissivity and opacity are in equilibrium [281], or use non-tunable X-ray lasers [282]. Recent seminal experiments at Sandia's Z machine [238] measured the iron opacity at solar interior conditions higher than predicted at energies around 1 keV, which could explain discrepancies between solar models and helioseismic observations.…”
Section: Opacity In Hot Dense Plasmasmentioning
confidence: 99%
“…It is expected that the uniformity of the gain region could be increased significantly by tamping the Se target on both sides (by CH, for instance) [29]. With a seed pulse of 0.1I s intensity under the revised conditions, sub-100-fs pulses (∼80 fs) of slightly higher intensity (∼2 × 10 11 W cm −2 for the unfocussed beam) are predicted.…”
Section: Resultsmentioning
confidence: 99%
“…with h > 1) can exist in plasmas dominated by strong absorption features [13]. Previously transmission measurements of plasma-based EUV lasers have provided information on plasma opacity [14] and the rate of ablation of solid targets irradiated by optical lasers [15]. In an experiment by Edwards et al [15], the rate of laser ablation was measured from the transmission of the EUV laser through the ablated target using the observation that ablated plasma material becomes transparent, so that the target transmission is dominated only by absorption in the remaining solid target.…”
Section: Introductionmentioning
confidence: 98%