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Absorption spectroscopy of mid and neighboring Z plasmas: Iron, nickel,copper and germanium
Opacities of four medium Z element plasmas (iron, nickel, copper and germanium) have been measured at the LULI-2000 facility in similar conditions: temperatures between 15 and 25 eV and densities between 2 and 10 mg/cm 3, in a wavelength range (8–18 Å) including the strong 2p–3d structures. Two lase...
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Published in: | High energy density physics 2009-09, Vol.5 (3), p.173-181 |
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Main Authors: | , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Opacities of four medium
Z element plasmas (iron, nickel, copper and germanium) have been measured at the LULI-2000 facility in similar conditions: temperatures between 15 and 25
eV and densities between 2 and 10
mg/cm
3, in a wavelength range (8–18
Å) including the strong 2p–3d structures.
Two laser beams from the LULI facility were used in the nanosecond-picosecond configuration. The NANO-2000 beam (at
λ
=
0.53
μm) heated a gold hohlraum with an energy between 30 and 150
J with a duration of 0.6
ns. Samples covering half a hohlraum hole were thus radiatively heated. The picosecond pulse PICO-2000 beam (at
λ
=
1.053
μm) has been used to produce a short (about 10
ps) X-ray backlighter in order to reduce time variations of temperatures and densities during the measurement. A crystal high-resolution spectrometer was used as the main diagnostic to record at the same time the non-absorbed and the absorbed backlighter spectra. Radiation temperatures were measured using a broadband spectrometer. 1D and 2D simulations have been performed in order to estimate hydrodynamic plasmas parameters.
The measured spectra have been compared with theoretical ones obtained using either the superconfiguration code SCO or the detailed term accounting code HULLAC. These comparisons allow us to check the modeling of the statistical broadening and of the spin-orbit splitting of the 2p–3d transitions and related effects such as the interaction between relativistic subconfigurations belonging to the same non-relativistic configuration. |
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ISSN: | 1574-1818 1878-0563 |
DOI: | 10.1016/j.hedp.2009.05.015 |