Published September 14, 2007
| Version v1
Journal article
Polarization of Heα Radiation due to Anisotropy of Fast-Electron Transport in Ultraintense-Laser-Produced Plasmas
Creators
- 1. Department of Energy Sciences, Tokyo Institute of Technology, Nagatsuta-cho 4259, Midori-ku, Yokohama, Kanagawa, 226-8502 (Japan)
- 2. Institute of Laser Engineering, Osaka University, Yamada-oka 2-6, Suita, Osaka, 565-0871 (Japan)
- 3. Physics Laboratory, School of Medicine, Kitasato University, Kitasato 1-15-1, Sagamihara, Kanagawa, 228-8555 (Japan)
- 4. Department of Applied Physics, Faculty of Engineering, University of Miyazaki, Gakuen Kibanadai-nishi 1-1, Miyazaki, 889-2192 (Japan)
Description
An atomic kinetics code is developed to gain insight into the generation of polarized Heα by fast electron transport relevant to fast ignition. The calculation predicts a very small polarization in the dense region (≥100 times the critical density) due to frequent elastic transitions between magnetic sublevels, while high polarization is observable in the low density region (≤10 times the critical density). It is inferred that fast electrons are collimated due to electromagnetic instability, resulting in the generation of anisotropic fast electrons along the propagation axis in the low density region
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 99
- Journal Issue
- 11
- Journal Page Range
- p. 115003-115003.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39050134
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ANISOTROPY; CHARGED-PARTICLE TRANSPORT; ELECTRONS; HELIUM; LASER-PRODUCED PLASMA; PLASMA INSTABILITY; POLARIZATION; THERMONUCLEAR IGNITION
- Descriptors DEC
- ELEMENTARY PARTICLES; ELEMENTS; FERMIONS; FLUIDS; GASES; INSTABILITY; LEPTONS; NONMETALS; PLASMA; RADIATION TRANSPORT; RARE GASES
Optional Information
- Notes
- (c) 2007 The American Physical Society