Hostname: page-component-848d4c4894-wg55d Total loading time: 0 Render date: 2024-05-21T15:50:28.094Z Has data issue: false hasContentIssue false
  • English
  • Français

Stability of Luminous Discharges in Strong Fields

Published online by Cambridge University Press:  19 July 2016

Gregory Benford
Gregory Benford*
Affiliation:
Department of Physics University of California, Irvine Irvine, CA 92717

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

I show that a common thermal instability of conventional plasma discharges does not occur if plasma turbulence impedes current flow. Normally, thermal discharges drain current into a single hotter filament, because classical Coulomb resistance falls as a filament heats. Anomalous resistance reverses this, stabilizing the circuit. Only small levels of turbulence are needed.

Type
7. Magnetic Fields in Galactic Nuclei
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 401 - 402
Copyright
Copyright © Kluwer 1990 

References

Benford, Gregory, 1988, Ap. J. 333, 735.CrossRefGoogle Scholar
Blandford, R., in IAU Symposium 136, ed. by Morris, Mark, Kluwer, Boston, p. 652.Google Scholar
Heyvaerts, J., Norman, C. and Pudritz, R., 1988, Ap. J. 333, 718.CrossRefGoogle Scholar