Published October 22, 2008
| Version v1
Journal article
X-ray Spectroscopy of Hot Dense Plasmas: Experimental Limits, Line Shifts and Field Effects
Creators
- 1. Institute of Physics, Academy of Sciences CR, Na Slovance 2, 18221 Prague (Czech Republic)
- 2. Dept. de Ingenieria Energetica-UNED, 28040 Madrid (Spain)
- 3. Physique Atomique dans les Plasmas Denses, LULI, UMR 7605, CNRS-CEA-Ecole Polytechnique- Universite Paris 6, 4 Place Jussieu, 75252 Paris Cedex 05 (France)
- 4. CELIA Universite Bordeaux-CEA, 33405 Talence (France)
- 5. Institut fuer Optik und Quantenelektronik, Friedrich-Schiller-Universitaet, 07743 Jena (Germany)
- 6. Physics Department, 206 Allison Laboratory, Auburn University, Auburn, AL 36849 (United States)
Description
High-resolution x-ray spectroscopy is capable of providing complex information on environmental conditions in hot dense plasmas. Benefiting from application of modern spectroscopic methods, we report experiments aiming at identification of different phenomena occurring in laser-produced plasma. Fine features observed in broadened profiles of the emitted x-ray lines and their satellites are interpreted using theoretical models predicting spectra modification under diverse experimental situations.
Additional details
Identifiers
- DOI
- 10.1063/1.3026477;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1058
- Journal Issue
- 1
- Journal Page Range
- p. 341-348
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 19. international conference on spectral line shapes
- Dates
- 15-20 Jun 2008
- Place
- Valladolid (Spain)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41002899
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- LASER-PRODUCED PLASMA; PLASMA DENSITY; PLASMA PRODUCTION; SPECTRAL SHIFT; X-RAY SPECTROSCOPY
- Descriptors DEC
- PLASMA; SPECTROSCOPY
Optional Information
- Notes
- (c) 2008 American Institute of Physics