Non-maxwellian plasma electrons in the inversion population of Ne-like ions
- 1. Department of Physics and Astronomy, Brigham Young University, Provo, UT 84602 (United States)
- 2. Institute of Spectroscopy of Russian Academy of Science, Troitsk, Moscow Region, 142092 (Russian Federation)
Description
Level populations and line intensities are calculated for a pure Ne-like argon plasma showing their dependence on plasma parameters (electron temperature, density, plasma column diameter, electron energy distribution, etc.). It is shown that intensity ratios for 2-3 resonance transitions in the Ne-like ion can be used for plasma diagnostics. These intensity ratios are sensitive enough to detect the fraction of suprahot electrons in the plasma. Suprahot electrons cause a strong inversion effect for highly excited levels, e.g., 15:2p3p [J=0], 29:2s3s [J=0]. For these levels, collisional excitation strengths are large at almost any energy of impact electron above threshold. The inversion changes in time with a maximum at t∼80 psec at an electron density of ne∼8x1018 cm-3. The inversion increases with electron energy
Additional details
Identifiers
- DOI
- 10.1063/1.47928;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 332
- Journal Issue
- 1
- Journal Page Range
- p. 393-398
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- X-ray lasers 1994
- Acronym
- 4. international colloquium
- Dates
- 15-20 May 1994
- Place
- Williamsburg, VA (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40032432
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ARGON IONS; ELECTRON DENSITY; ELECTRON SPECTRA; ELECTRON TEMPERATURE; ELECTRONS; EXCITATION; EXCITED STATES; MULTICHARGED IONS; PLASMA; PLASMA DENSITY; PLASMA DIAGNOSTICS; RESONANCE
- Descriptors DEC
- CHARGED PARTICLES; ELEMENTARY PARTICLES; ENERGY LEVELS; ENERGY-LEVEL TRANSITIONS; FERMIONS; IONS; LEPTONS; SPECTRA
Optional Information
- Notes
- (c) 1994 American Institute of Physics.