Close category search window
 

Diagnostic characterization of a prepulsed carbon fiber Z pinch using spectral line intensity analyses

Sign In

Cookies must be enabled to login.After enabling cookies , please use refresh or reload or ctrl+f5 on the browser for the login options.

Formats Non-Member Member
$31 $31
Learn how you can qualify for the best price for this item!
Become an IEEE Member or Subscribe to
IEEE Xplore for exclusive pricing!
close button

puzzle piece

IEEE membership options for an individual and IEEE Xplore subscriptions for an organization offer the most affordable access to essential journal articles, conference papers, standards, eBooks, and eLearning courses.

Learn more about:

IEEE membership

IEEE Xplore subscriptions

4 Author(s)
Lorenz, A. ; The Blackett Laboratory, Imperial College of Science, Technology and Medicine, London SW7 2BZ, United Kingdom ; Peacock, N.J. ; OMullane, M.G. ; Neely, David

Your organization might have access to this article on the publisher's site. To check, click on this link:http://dx.doi.org/+10.1063/1.1149630 

Plasma formation and x-ray generation efficiency of a carbon fiber Z pinch are dramatically improved by means of an optimized current prepulse. In this article results are presented of time-integrated and also time-resolved electron temperature measurements using the optical line emission of the coronal plasma surrounding a still, cold fiber. Two phases of discharges with current prepulse are studied: the preionization phase only in which time-integrated spectra of C II–C IV emission are recorded and time resolution of the heating phase after onset of the main current pulse using C III and C IV line emission. Experimentally obtained, n=3–4, 3–3, line ratios are fitted with collisional radiative, ADAS computations of line intensity ratios as a function of electron temperature, density, ne and variable confinement, τ. All levels up to n=5 are included with the influence of higher levels also accounted for. Deviations from coronal balance give an effective value for the product eτ>. As a result, the electron temperature of the preionized coronal plasma is estimated at Te=5 eV at a density of ne≈1017cm-3. The temperature rises to about 12 eV at the same density after the start of the main current with prepulse. Similar analytic techniques are applied to time-integrated C V and C VI XUV resonance lines from the main pinch and give plasma parameters in accord with the x-ray continuum diagnostics. © 1999 American Institute of Physics.

Published in:
Review of Scientific Instruments  (Volume:70 ,  Issue: 2 )

Date of Publication: Feb 1999

Need Help?


IEEE Advancing Technology for Humanity About IEEE Xplore | Contact | Help | Terms of Use | Nondiscrimination Policy | Site Map | Privacy & Opting Out of Cookies

A not-for-profit organization, IEEE is the world's largest professional association for the advancement of technology.
© Copyright 2013 IEEE - All rights reserved. Use of this web site signifies your agreement to the terms and conditions.