Published January 21, 2009 | Version v1
Journal article

Planar Wire Array Dynamics and Radiation Scaling at Multi-MA Levels on the Saturn Pulsed Power Generator

  • 1. Sandia National Laboratories, PO Box 5800, Albuquerque, NM 87185 (United States)
  • 2. Department of Physics, University of Nevada, Reno, NV 89557 (United States)
  • 3. Laboratoire de Physique et Technologie des Plasmas, Laboratoire du Centre National de la Recherche Scientifique, Ecole Polytechnique, 91128 Palaiseau (France)
  • 4. Icarus Research, P.O. Box 30780, Bethesda, MD 20824-0780 (United States)

Description

Planar wire arrays are studied at 3-6 MA on the Saturn pulsed power generator as potential drivers of compact hohlraums for inertial confinement fusion studies. Comparison with zero-dimensional modeling suggests that there is significant trailing mass. The modeled energy coupled from the generator cannot generally explain the energy in the main x-ray pulse. Preliminary comparison at 1-6 MA indicates sub-quadratic scaling of x-ray power in a manner similar to compact cylindrical wire arrays. Time-resolved pinhole images are used to study the implosion dynamics.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1088
Journal Issue
1
Journal Page Range
p. 109-112
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
7. international conference on dense Z-pinches
Dates
12-21 Aug 2008
Place
Alexandria, VA (United States)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41005909
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CYLINDRICAL CONFIGURATION; IMPLOSIONS; INERTIAL CONFINEMENT; MASS; PLASMA DIAGNOSTICS; PULSES; SIMULATION; TIME RESOLUTION; WIRES; X RADIATION; X-RAY SPECTRA
Descriptors DEC
CONFIGURATION; CONFINEMENT; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; PLASMA CONFINEMENT; RADIATIONS; RESOLUTION; SPECTRA; TIMING PROPERTIES

Optional Information

Notes
(c) 2009 American Institute of Physics