Published December 31, 2007
| Version v1
Journal article
Supersonic-Jet Experiments Using a High-Energy Laser
Creators
- 1. LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau (France)
- 2. Laboratoire de l'Univers et de ses Theories, Observatoire de Paris, CNRS, Universite Paris Diderot, Place Jules Janssen, 92190 Meudon (France)
- 3. CEA/DIF/DPTA BP 12, 91680 Bruyeres-le-Chatel (France)
- 4. Graduate School of Engineering, Osaka University, Suita, Osaka 565-0871 (Japan)
- 5. School of Chemistry, University of St Andrews, Purdie Blg, St Andrews KY16 9ST (United Kingdom)
- 6. Science Applications International Corporation, McLean, Virginia 22102 (United States)
- 7. Joint Institute for High Temperatures of RAS, Izhorskaya 13/19, Moscow, 125412 (Russian Federation)
Description
In this Letter, laboratory astrophysical jet experiments performed with the LULI2000 laser facility are presented. High speed plasma jets (150 km·s-1) are generated using foam-filled cone targets. Accurate experimental characterization of the plasma jet is performed by measuring its time evolution and exploring various target parameters. Key jet parameters such as propagation and radial velocities, temperature, and density are obtained. For the first time, the required dimensionless quantities are experimentally determined on a single-shot basis. Although the jets evolve in vacuum, most of the scaling parameters are relevant to astrophysical conditions
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 99
- Journal Issue
- 26
- Journal Page Range
- p. 265001-265001.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39050153
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ASTROPHYSICS; EVOLUTION; LASERS; PLASMA JETS; RADIAL VELOCITY
- Descriptors DEC
- PHYSICS; VELOCITY
Optional Information
- Notes
- (c) 2007 The American Physical Society