An explanation of the apparent non-observation of 'near' plasma satellite emission lines in highly turbulent plasmas
- 1 February 1971
- journal article
- Published by IOP Publishing in Journal of Physics B: Atomic and Molecular Physics
- Vol. 4 (2) , L7-L10
- https://doi.org/10.1088/0022-3700/4/2/016
Abstract
Plasma satellite emission lines separated by twice the plasma frequency 2 omega p from allowed lines should often be stronger than the weaker (far) Baranger-Mozer omega p satellite of forbidden lines. Confusion between these features probably explains those observations in which the near Baranger-Mozer line has appeared to be anomalously weak relative to the far omega p satellite.Keywords
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