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Observations of High-Density Corrections to VUV Line-Wing Shapes in a Plasma with a Few Particles Per Debye Sphere

Published online by Cambridge University Press:  25 September 2017

E.A.M. Baker
Affiliation:
Blackett Laboratory, Imperial College, LondonSW7 2BZ
D.D. Burgess
Affiliation:
Blackett Laboratory, Imperial College, LondonSW7 2BZ

Extract

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Observations of high density effects on spectral line shapes are reported for neutral, singly- and doubly-ionized emitters in a dense plasma with a small number of particles per Debye sphere. The source used in these experiments was a well-diagnosed linear pinch,run in argon, producing a plasma with electron density between 0.5 x 1018 and 3 x 1018 cm–3, and temperature between 22,000 K and 27,000 K.

Satellite-like features observed in the wings of H I Lyman α are attributed to the influence of unbound quasimolecular states. A number of the satellites are apparently due to states of H–Ar+ (similar to two such Lyman α satellites observed by Preston 1977). However, it seems likely that at least one of the satellite features observed should be attributed to the influence of Ar++ perturbers. Such quasimolecular features might be expected to become increasingly important at higher densities, and for more highly-ionized perturbing ions.

Type
Research Article
Copyright
Copyright © Crown Research Institutes 1977