K-shell radiation physics in low- to moderate-atomic-number z-pinch plasmas on the Z accelerator
Dense z-pinches produced by 100 ns implosions of wire arrays or gas puffs produce substantial soft X-ray power. One class of z-pinch radiation sources includes low- to moderate-atomic-number K-shell radiators, such as aluminum and iron. These loads are designed for 1–10 keV K-shell X-ray generation,...
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Published in: | Journal of quantitative spectroscopy & radiative transfer Vol. 99; no. 1; pp. 341 - 348 |
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Abstract | Dense z-pinches produced by 100
ns implosions of wire arrays or gas puffs produce substantial soft X-ray power. One class of z-pinch radiation sources includes low- to moderate-atomic-number K-shell radiators, such as aluminum and iron. These loads are designed for 1–10
keV K-shell X-ray generation, and offer opportunities for crystal spectroscopy that can reveal fundamental properties of the plasma when studied using plasma spectroscopic modeling. Typically these plasmas are characterized by ion densities of
∼
10
20
cm
-
3
, diameters of 1–5
mm, electron temperatures up to several keV, and a range of opacities of the K-shell lines. Measurements from wire arrays on Sandia's 20
MA Z accelerator are presented along with collisional radiative and hydrodynamic simulations. The impact of opacity and 3D structure on non-LTE, non-diffusive radiation transport and X-ray production is discussed. |
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AbstractList | Dense z-pinches produced by 100
ns implosions of wire arrays or gas puffs produce substantial soft X-ray power. One class of z-pinch radiation sources includes low- to moderate-atomic-number K-shell radiators, such as aluminum and iron. These loads are designed for 1–10
keV K-shell X-ray generation, and offer opportunities for crystal spectroscopy that can reveal fundamental properties of the plasma when studied using plasma spectroscopic modeling. Typically these plasmas are characterized by ion densities of
∼
10
20
cm
-
3
, diameters of 1–5
mm, electron temperatures up to several keV, and a range of opacities of the K-shell lines. Measurements from wire arrays on Sandia's 20
MA Z accelerator are presented along with collisional radiative and hydrodynamic simulations. The impact of opacity and 3D structure on non-LTE, non-diffusive radiation transport and X-ray production is discussed. |
Author | Deeney, C. Velikovich, A.L. Safronova, A. Coverdale, C.A. Jones, B. LePell, P.D. Thornhill, J.W. Davis, J. Kantsyrev, V. Whitney, K.G. Clark, R.W. Maron, Y. McKenney, J.L. Apruzese, J.P. Oreshkin, V.I. |
Author_xml | – sequence: 1 givenname: B. surname: Jones fullname: Jones, B. email: bmjones@sandia.gov organization: Sandia National Laboratories, Albuquerque, NM 87185, USA 1 – sequence: 2 givenname: C. surname: Deeney fullname: Deeney, C. organization: Sandia National Laboratories, Albuquerque, NM 87185, USA 1 – sequence: 3 givenname: C.A. surname: Coverdale fullname: Coverdale, C.A. organization: Sandia National Laboratories, Albuquerque, NM 87185, USA 1 – sequence: 4 givenname: P.D. surname: LePell fullname: LePell, P.D. organization: Ktech Corporation, Albuquerque, NM 87123, USA – sequence: 5 givenname: J.L. surname: McKenney fullname: McKenney, J.L. organization: Sandia National Laboratories, Albuquerque, NM 87185, USA 1 – sequence: 6 givenname: J.P. surname: Apruzese fullname: Apruzese, J.P. organization: Naval Research Laboratory, Washington, DC 20375, USA – sequence: 7 givenname: J.W. surname: Thornhill fullname: Thornhill, J.W. organization: Naval Research Laboratory, Washington, DC 20375, USA – sequence: 8 givenname: K.G. surname: Whitney fullname: Whitney, K.G. organization: Naval Research Laboratory, Washington, DC 20375, USA – sequence: 9 givenname: R.W. surname: Clark fullname: Clark, R.W. organization: Naval Research Laboratory, Washington, DC 20375, USA – sequence: 10 givenname: A.L. surname: Velikovich fullname: Velikovich, A.L. organization: Naval Research Laboratory, Washington, DC 20375, USA – sequence: 11 givenname: J. surname: Davis fullname: Davis, J. organization: Naval Research Laboratory, Washington, DC 20375, USA – sequence: 12 givenname: Y. surname: Maron fullname: Maron, Y. organization: Faculty of Physics, Weizmann Institute of Science, 76100 Rehovot, Israel – sequence: 13 givenname: V. surname: Kantsyrev fullname: Kantsyrev, V. organization: Department of Physics, University of Nevada, Reno, NV 89557-0058, USA – sequence: 14 givenname: A. surname: Safronova fullname: Safronova, A. organization: Department of Physics, University of Nevada, Reno, NV 89557-0058, USA – sequence: 15 givenname: V.I. surname: Oreshkin fullname: Oreshkin, V.I. organization: High Current Electronics Institute, Tomsk, Siberia 634055, Russia |
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Snippet | Dense z-pinches produced by 100
ns implosions of wire arrays or gas puffs produce substantial soft X-ray power. One class of z-pinch radiation sources includes... |
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StartPage | 341 |
SubjectTerms | K-shell X-ray production and spectroscopy Opacity Z-pinch plasma |
Title | K-shell radiation physics in low- to moderate-atomic-number z-pinch plasmas on the Z accelerator |
URI | https://dx.doi.org/10.1016/j.jqsrt.2005.05.027 |
Volume | 99 |
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