On the structure of plasma liners for plasma jet induced magnetoinertial fusion
- 1. Department of Applied Mathematics and Statistics, Stony Brook University, Stony Brook, New York 11794 (United States)
- 2. Computational Science Center, Brookhaven National Laboratory, Upton, New York 11973 (United States)
- 3. General Atomics, P.O. Box 85608, San Diego, California 92186-5608 (United States)
Description
The internal structure and self-collapse properties of plasma liners, formed by the merger of argon plasma jets, have been studied via 3-dimensional numerical simulations using the FronTier code. We have shown that the jets merger process is accomplished through a cascade of oblique shock waves that heat the liner and reduce its Mach number. Oblique shock waves and the adiabatic compression heating have led to the 10 times reduction of the self-collapse pressure of a 3-dimensional argon liner compared to a spherically symmetric liner with the same pressure and density profiles at the merging radius. We have also observed a factor of 10 variations of pressure and density in the leading edge of the liner along spherical surfaces close to the interaction with potential plasma targets. Such a non-uniformity of imploding plasma liners presents problems for the stability of targets during compression.
Additional details
Identifiers
- DOI
- 10.1063/1.4789887;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 20
- Journal Issue
- 2
- Journal Page Range
- p. 022704-022704.10
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44070436
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ADIABATIC COMPRESSION HEATING; ARGON; COMPUTERIZED SIMULATION; INTERACTIONS; MACH NUMBER; NUMERICAL ANALYSIS; PLASMA; PLASMA JETS; PLASMA SIMULATION; SHOCK WAVES; STABILITY; SURFACES; SYMMETRY; THREE-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- DIMENSIONLESS NUMBERS; ELEMENTS; FLUIDS; GASES; HEATING; MATHEMATICS; NONMETALS; PLASMA HEATING; RARE GASES; SIMULATION; VELOCITY
Optional Information
- Notes
- (c) 2013 American Institute of Physics