X-ray spectroscopy and imaging of stainless steel X-pinches with application to astrophysics

The European Physical Journal Special Topics - Tập 169 - Trang 155-158 - 2009
A. S. Safronova1, V. L. Kantsyrev1, A. A. Esaulov1, N. D. Ouart1, U. I. Safronova1, I. Shrestha1, K. M. Williamson1
1University of Nevada, Reno, USA

Tóm tắt

X-pinches are very good sources of x-rays and can be used for studying radiative properties of high density and temperature plasmas with scale from a few μm to several mm in size. An X-pinch is formed by the touch-crossing of two or more wires between the electrodes of a high-current pulsed-power generator. As a result of current quickly vaporizing and strongly ionizing the wire material, X-pinch yields short (few nsec) x-ray bursts from one or few bright plasma spots near the wire cross point. Other distinct features of X-pinches are strong electron beams, which make them attractive objects for x-ray spectropolarimetry, as well as plasmas jets for astrophysical applications. Recently, we spectroscopically studied x-ray L-shell and K-shell radiation from variety of X-pinches from different materials and load configurations. In the present work, the results of x-ray spectroscopy and imaging of X-pinches from stainless steel are presented. The application of these results to astrophysics is highlighted.

Tài liệu tham khảo

A.S. Safronova, V.L. Kantsyrev, N.D. Ouart, et al., JQSRT 99, 560 (2006)

V.L. Kantsyrev, A.S. Safronova, V.V. Ivanov, et al., JQSRT 99, 349 (2006)

V.L. Kantsyrev, A.S. Safronova, D.A. Fedin, et al., IEEE Trans. Plasma Sci. 34, 194 (2006)

A.S. Safronova, V.L. Kantsyrev, P. Neill, et al., Can. J. Phys. 86, 267 (2008)

K.J.H. Phillips, C.J. Greer, A.K. Bhatia, et al., Astron. Astroph. 324, 381 (1997)

S.V. Lebedev, J.P. Chittenden, F.N. Beg, et al., Astroph. J. 564, 113 (2002)

A.A. Esaulov, A.L. Velikovich, V.L. Kantsyrev, et al., Phys. Plasmas 13, 120701 (2006)

A.S. Safronova, V.L. Kantsyrev, A.A. Esaulov, et al., Phys. Plasmas 15, 033302 (2008)

A. Esaulov, Phys. Plasmas 13, 042506 (2006)

M.F. Gu, Can. J. Phys. 86, 675 (2008)

U.I. Safronova, et al., Phys. Rev. A 64, 012507 (2001)