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Title: Model of enhanced energy deposition in a Z-pinch plasma

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.874192· OSTI ID:20217079
 [1];  [1];  [1];  [1];  [2];  [3]
  1. Radiation Hydrodynamics Branch, Plasma Physics Division, Naval Research Laboratory, Washington, D.C. 20375 (United States)
  2. Advanced Power Technologies, Inc., Washington, D.C. 20037 (United States)
  3. Sandia National Laboratories, Albuquerque, New Mexico 87545 (United States)

In numerous experiments, magnetic energy coupled to strongly radiating Z-pinch plasmas exceeds the thermalized kinetic energy, sometimes by a factor of 2-3. An analytical model describing this additional energy deposition based on the concept of macroscopic magnetohydrodynamic (MHD) turbulent pinch heating proposed by Rudakov and Sudan [Phys. Reports 283, 253 (1997)] is presented. The pinch plasma is modeled as a foam-like medium saturated with toroidal ''magnetic bubbles'' produced by the development of surface m=0 Rayleigh-Taylor and MHD instabilities. As the bubbles converge to the pinch axis, their magnetic energy is converted to thermal energy of the plasma through pdV work. Explicit formulas for the average dissipation rate of this process and the corresponding contribution to the resistance of the load, which compare favorably to the experimental data and simulation results, are presented. The possibility of using this enhanced (relative to Ohmic heating) dissipation mechanism to power novel plasma radiation sources and produce high K-shell yields using long current rise time machines is discussed. (c) 2000 American Institute of Physics.

OSTI ID:
20217079
Journal Information:
Physics of Plasmas, Vol. 7, Issue 8; Other Information: PBD: Aug 2000; ISSN 1070-664X
Country of Publication:
United States
Language:
English