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
[S.l.] : American Institute of Physics (AIP)
Published 1989
ISSN: |
1089-7550
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Source: |
AIP Digital Archive
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Topics: |
Physics
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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.
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Type of Medium: |
Electronic Resource
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URL: |
_version_ | 1798289670440747008 |
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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 |