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Title: Background measurement methods for opacity experiments conducted at the Z facility

Journal Article · · Review of Scientific Instruments
DOI: https://doi.org/10.1063/5.0057225 · OSTI ID:1894606

Laboratory experiments typically test opacity models by measuring spectrally resolved transmission of a sample using bright backlight radiation. A potential problem is that any unaccounted background signal contaminating the spectrum will artificially reduce the inferred opacity. Methods developed to measure background signals in opacity experiments at the Sandia Z facility are discussed. Preliminary measurements indicate that backgrounds are 9%–11% of the backlight signal at wavelengths less than 10 Å. Background is thus a relatively modest correction for all Z opacity data published to date. Future work will determine how important background is at longer wavelengths.

Research Organization:
Sandia National Laboratories (SNL-NM), Albuquerque, NM (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
NA0003525
OSTI ID:
1894606
Report Number(s):
SAND2022-13485J; 710460
Journal Information:
Review of Scientific Instruments, Journal Name: Review of Scientific Instruments Journal Issue: 8 Vol. 92; ISSN 0034-6748
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English

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Conceptual design of initial opacity experiments on the national ignition facility journal January 2017
A higher-than-predicted measurement of iron opacity at solar interior temperatures journal December 2014
Diagnosis of x-ray heated Mg/Fe opacity research plasmas journal November 2008
Experimental investigation of opacity models for stellar interior, inertial fusion, and high energy density plasmas journal May 2009
Control and diagnosis of temperature, density, and uniformity in x-ray heated iron/magnesium samples for opacity measurements journal May 2014
Absorption experiments on x-ray-heated mid- Z constrained samples journal November 1996
Systematic Study of L -Shell Opacity at Stellar Interior Temperatures journal June 2019
Iron-Plasma Transmission Measurements at Temperatures Above 150 eV journal December 2007
Numerical investigations of potential systematic uncertainties in iron opacity measurements at solar interior temperatures journal June 2017

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