Magnetic booster fast ignition macron accelerator
Description
A new fast ignition scheme was recently proposed where the ignition is done by the impact of a small solid projectile accelerated to velocities in excess of 108 cm/s, with the acceleration done in two steps: first, by laser ablation of a flyer plate, and second by injecting the flyer plate into a conical duct. The two principal difficulties of this scheme are as follows: first, the required large mass ratio for the laser ablation rocket propelled flyer plate, and second, the Rayleigh-Taylor instability of the flyer plate during its implosive compression in the conical duct. To overcome these difficulties, it is suggested to accelerate a projectile by a magnetic fusion booster stage, made up of a dense, wall-confined magnetized plasma brought to thermonuclear temperatures. After ignition, this plasma undergoes a thermonuclear excursion greatly increasing its pressure, resulting in the explosion of a weakened segment of the wall, with the segment becoming a fast moving projectile. The maximum velocity this projectile can reach is the velocity of sound of the booster stage plasma, which at a temperature of 108 K is of the order 108 cm/s
Additional details
Identifiers
- DOI
- 10.1063/1.2378631;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 13
- Journal Issue
- 11
- Journal Page Range
- p. 112702-112702.5
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38023344
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S36: MATERIALS SCIENCE; S43: PARTICLE ACCELERATORS;
- Descriptors DEI
- ABLATION; COMPRESSION; ELECTRON TEMPERATURE; ICF DEVICES; ION TEMPERATURE; LASERS; LIGHT TRANSMISSION; PARTICLE BEAM FUSION ACCELERATOR; PLASMA; PLASMA GUNS; RAYLEIGH-TAYLOR INSTABILITY; SOUND WAVES; THERMONUCLEAR IGNITION
- Descriptors DEC
- ACCELERATORS; INSTABILITY; THERMONUCLEAR DEVICES; TRANSMISSION
Optional Information
- Notes
- (c) 2006 American Institute of Physics