Short-scalelength plasma spectroscopy
Traditional x-ray plasma spectroscopy techniques employ long scalelength laser-produced plasmas in an attempt to moderate the density and temperature gradients present in the ablation plasma. These approaches have the disadvantages that the large plasma may lead to significant opacity effects, la...
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ndltd-UBC-oai-circle.library.ubc.ca-2429-29182018-01-05T17:31:08Z Short-scalelength plasma spectroscopy Forsman, Andrew Traditional x-ray plasma spectroscopy techniques employ long scalelength laser-produced plasmas in an attempt to moderate the density and temperature gradients present in the ablation plasma. These approaches have the disadvantages that the large plasma may lead to significant opacity effects, lasers having substantial power must be used and numerical simulations of the laser-produced plasma frequently must be used to interpret the data. As an alternative technique the use of short-scalelength plasmas as sources for x-ray spectroscopy have been investigated. High-resolution silicon K-shell spectra from a short-scalelength, laser-produced plasma have been obtained in temporally and spatially integrated measurements. Density-sensitive line-intensity ratios of the helium like satellites and that of the lithium-like satellites are employed simultaneously with temperature-sensitive line-intensity ratios between the helium and lithium-like satellites to assess their diagnostic value. A constant, uniform plasma model is used to interpret the data. It appears that the emission of dielectronic satellite lines is dominated by a region with a relatively well-defined density and temperature in the ablation zone. Science, Faculty of Physics and Astronomy, Department of Graduate 2008-12-15T23:44:54Z 2008-12-15T23:44:54Z 1992 1992-11 Text Thesis/Dissertation http://hdl.handle.net/2429/2918 eng For non-commercial purposes only, such as research, private study and education. Additional conditions apply, see Terms of Use https://open.library.ubc.ca/terms_of_use. 1678621 bytes application/pdf |
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English |
format |
Others
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Traditional x-ray plasma spectroscopy techniques employ long scalelength laser-produced
plasmas in an attempt to moderate the density and temperature gradients present in the
ablation plasma. These approaches have the disadvantages that the large plasma may
lead to significant opacity effects, lasers having substantial power must be used and
numerical simulations of the laser-produced plasma frequently must be used to interpret
the data. As an alternative technique the use of short-scalelength plasmas as sources
for x-ray spectroscopy have been investigated. High-resolution silicon K-shell spectra
from a short-scalelength, laser-produced plasma have been obtained in temporally and
spatially integrated measurements. Density-sensitive line-intensity ratios of the helium
like satellites and that of the lithium-like satellites are employed simultaneously with
temperature-sensitive line-intensity ratios between the helium and lithium-like satellites
to assess their diagnostic value. A constant, uniform plasma model is used to interpret
the data. It appears that the emission of dielectronic satellite lines is dominated by a
region with a relatively well-defined density and temperature in the ablation zone. === Science, Faculty of === Physics and Astronomy, Department of === Graduate |
author |
Forsman, Andrew |
spellingShingle |
Forsman, Andrew Short-scalelength plasma spectroscopy |
author_facet |
Forsman, Andrew |
author_sort |
Forsman, Andrew |
title |
Short-scalelength plasma spectroscopy |
title_short |
Short-scalelength plasma spectroscopy |
title_full |
Short-scalelength plasma spectroscopy |
title_fullStr |
Short-scalelength plasma spectroscopy |
title_full_unstemmed |
Short-scalelength plasma spectroscopy |
title_sort |
short-scalelength plasma spectroscopy |
publishDate |
2008 |
url |
http://hdl.handle.net/2429/2918 |
work_keys_str_mv |
AT forsmanandrew shortscalelengthplasmaspectroscopy |
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