Published May 1, 1995 | Version v1
Journal article

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

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.