Soft x-ray spectra from a gas-puff z pinch

Nave, G. ; Challis, C. D. ; Dangor, A. E. ; Lunney, J. G.

[S.l.] : American Institute of Physics (AIP)
Published 1989
ISSN:
1089-7550
Source:
AIP Digital Archive
Topics:
Physics
Notes:
XUV and x-ray emission spectra of the elements carbon, oxygen, neon, and argon, in the spectral range 3–300 A(ring), generated in a gas-puff z pinch, are presented. The spectra are analyzed to give time-integrated measurements of the density, electron temperature, and dimensions of the imploded plasma and the "hot spots'' that often occur in the gas-puff pinch. In particular, dielectronic satellite lines are used to measure the electron density and temperature, and Stark broadening to measure electron density. The effect of optical depth is included.
Type of Medium:
Electronic Resource
URL:
_version_ 1798289670440747008
autor Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
autorsonst Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
book_url http://dx.doi.org/10.1063/1.342653
datenlieferant nat_lic_papers
hauptsatz hsatz_simple
identnr NLZ218696817
issn 1089-7550
journal_name Journal of Applied Physics
materialart 1
notes XUV and x-ray emission spectra of the elements carbon, oxygen, neon, and argon, in the spectral range 3–300 A(ring), generated in a gas-puff z pinch, are presented. The spectra are analyzed to give time-integrated measurements of the density, electron temperature, and dimensions of the imploded plasma and the "hot spots'' that often occur in the gas-puff pinch. In particular, dielectronic satellite lines are used to measure the electron density and temperature, and Stark broadening to measure electron density. The effect of optical depth is included.
package_name American Institute of Physics (AIP)
publikationsjahr_anzeige 1989
publikationsjahr_facette 1989
publikationsjahr_intervall 8014:1985-1989
publikationsjahr_sort 1989
publikationsort [S.l.]
publisher American Institute of Physics (AIP)
reference 65 (1989), S. 3385-3390
search_space articles
shingle_author_1 Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
shingle_author_2 Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
shingle_author_3 Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
shingle_author_4 Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
shingle_catch_all_1 Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
Soft x-ray spectra from a gas-puff z pinch
XUV and x-ray emission spectra of the elements carbon, oxygen, neon, and argon, in the spectral range 3–300 A(ring), generated in a gas-puff z pinch, are presented. The spectra are analyzed to give time-integrated measurements of the density, electron temperature, and dimensions of the imploded plasma and the "hot spots'' that often occur in the gas-puff pinch. In particular, dielectronic satellite lines are used to measure the electron density and temperature, and Stark broadening to measure electron density. The effect of optical depth is included.
1089-7550
10897550
American Institute of Physics (AIP)
shingle_catch_all_2 Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
Soft x-ray spectra from a gas-puff z pinch
XUV and x-ray emission spectra of the elements carbon, oxygen, neon, and argon, in the spectral range 3–300 A(ring), generated in a gas-puff z pinch, are presented. The spectra are analyzed to give time-integrated measurements of the density, electron temperature, and dimensions of the imploded plasma and the "hot spots'' that often occur in the gas-puff pinch. In particular, dielectronic satellite lines are used to measure the electron density and temperature, and Stark broadening to measure electron density. The effect of optical depth is included.
1089-7550
10897550
American Institute of Physics (AIP)
shingle_catch_all_3 Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
Soft x-ray spectra from a gas-puff z pinch
XUV and x-ray emission spectra of the elements carbon, oxygen, neon, and argon, in the spectral range 3–300 A(ring), generated in a gas-puff z pinch, are presented. The spectra are analyzed to give time-integrated measurements of the density, electron temperature, and dimensions of the imploded plasma and the "hot spots'' that often occur in the gas-puff pinch. In particular, dielectronic satellite lines are used to measure the electron density and temperature, and Stark broadening to measure electron density. The effect of optical depth is included.
1089-7550
10897550
American Institute of Physics (AIP)
shingle_catch_all_4 Nave, G.
Challis, C. D.
Dangor, A. E.
Lunney, J. G.
Soft x-ray spectra from a gas-puff z pinch
XUV and x-ray emission spectra of the elements carbon, oxygen, neon, and argon, in the spectral range 3–300 A(ring), generated in a gas-puff z pinch, are presented. The spectra are analyzed to give time-integrated measurements of the density, electron temperature, and dimensions of the imploded plasma and the "hot spots'' that often occur in the gas-puff pinch. In particular, dielectronic satellite lines are used to measure the electron density and temperature, and Stark broadening to measure electron density. The effect of optical depth is included.
1089-7550
10897550
American Institute of Physics (AIP)
shingle_title_1 Soft x-ray spectra from a gas-puff z pinch
shingle_title_2 Soft x-ray spectra from a gas-puff z pinch
shingle_title_3 Soft x-ray spectra from a gas-puff z pinch
shingle_title_4 Soft x-ray spectra from a gas-puff z pinch
sigel_instance_filter dkfz
geomar
wilbert
ipn
albert
source_archive AIP Digital Archive
timestamp 2024-05-06T08:04:30.583Z
titel Soft x-ray spectra from a gas-puff z pinch
titel_suche Soft x-ray spectra from a gas-puff z pinch
topic U
uid nat_lic_papers_NLZ218696817