Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-26T03:56:16.539Z Has data issue: false hasContentIssue false

Gas–puff Z pinches with strong axial magnetic fields

Published online by Cambridge University Press:  09 March 2009

F. S. Felber
Affiliation:
Jaycor P. O. Box 85154, San Diego, CA 92138
F. J. Wessel
Affiliation:
Jaycor P. O. Box 85154, San Diego, CA 92138
N. C. Wild
Affiliation:
Jaycor P. O. Box 85154, San Diego, CA 92138
H. U. Rahman
Affiliation:
Jaycor P. O. Box 85154, San Diego, CA 92138
A. Fisher
Affiliation:
University of California at Irvine, Irvine, CA 92717
C. M. Fowler
Affiliation:
Los Alamos National Laboratory, Los Alamos, NM 87545
M. A. Liberman
Affiliation:
Institute for Physical Problems, Moscow, 117334, U.S.S.R.
A. L. Velikovich
Affiliation:
Institute for Physical Problems, Moscow, 117334, U.S.S.R.

Abstract

Ultrahigh axial magnetic fields have been compressed and measured in a gas-puff Z pinch. A 0·5-MA, 2–cm-radius annular gas-puff Z pinch with a 3-minute repetition rate was imploded radially onto an axial seed field, causing the field to compress. Axial magnetic field compressions up to 180 and peak magnetic fields up to 1·6 MG were measured. Faraday rotation of an argon laser (515·4 nm) in a quartz fiber on axis was the principal magnetic field diagnostic. Other diagnostics included a nitrogen laser interferometer, x-ray diodes, and magnetic field probes.

The magnetic field compression results are consistent with simple snowplow and self-similar analytic models, which are presented. The axial magnetic fields strongly affect the Z pinch dynamics. Even small axial fields help stabilize the pinches, some of which exhibit several stable radial bounces during a current pulse.

The method of compressing axial fields in a gas-puff Z pinch is extrapolable to the order of 100 MG. Scaling laws are presented. Potential applications of ultrahigh axial fields in Z pinches are discussed for x-ray lasers, inertial confinement fusion, and collimated sources of gamma radiation.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1987

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Bogomolov, G. D., Velikovich, A. L., & Liberman, M. A., 1983 Ultrahigh Magnetic Fields,Proc. Third Int. Conf. on Megagauss Magnetic Field Generation and Related Topics, Novosibirsk, edited by Titov, V. M. and Shvetsov, G. A. (Nauka, Moscow, 1984), p. 232 (in Russian).Google Scholar
Felber, F. S., 1982 Phys. Fluids, 25, 643.CrossRefGoogle Scholar
Felber, F. S., 1983 Western Research Corporation Report WRC-676-V, (unpublished).Google Scholar
Felber, F. S., Liberman, M. A. & Velikovich, A. L., 1985. Appl. Phys. Lett. 46, 1043.CrossRefGoogle Scholar
Felber, F. S., Malley, M. M., & Wong, S. K., 1987 IEEE Particle Accelerator Conf.(Washington, D.C.,16–19 March 1987), Paper P16.Google Scholar
Liberman, M. A. & Velikovich, A. L., 1984 J. Plasma Phys. 31, 381.CrossRefGoogle Scholar
Rahman, H. U., Felber, F. S., Wessel, F. J., Liberman, M. A., & Velikovich, A. L., 1986 4th Int'l Conf. on Megagauss Magnetic Field Generation and Related Topics(Santa Fe, NM,14–17 July 1986); to be published by Plenum Press.Google Scholar
Shiloh, J., Fisher, A. & Rostoker, N., 1978 Phys. Rev. Lett. 40, 515.CrossRefGoogle Scholar
Wessel, F. J., Felber, F. S., Wild, N. C., Rahman, H. U., Fisher, A. & Ruden, E., 1986 Appl. Phys. Lett., 48, 1119.CrossRefGoogle Scholar