Shifts of ionized-helium lines from electron collisions in dense plasmas
- 1 May 1983
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review A
- Vol. 27 (5) , 2566-2576
- https://doi.org/10.1103/physreva.27.2566
Abstract
The semiclassical impact-parameter method is used to calculate shifts of ionized helium lines in the first three spectral series caused by electrons in a plasma. These shifts together with opposite and smaller shifts due to ion quadrupole interactions are in agreement with observed shifts of lines corresponding to the Paschen series of hydrogen. Adding plasma polarization shifts according to the linearized Debye model to the shifts calculated here results in overestimates by a factor of 2 for the shifts of these lines. For lines corresponding to the Balmer series such addition may be consistent with measurements, while for the Lyman series all present theoretical models are found inadequate.Keywords
This publication has 20 references indexed in Scilit:
- Electron scattering contribution to the red shift of HeII lines in plasmaPhysics Letters A, 1981
- Stark broadening of visible neutral helium lines in a plasmaJournal of Quantitative Spectroscopy and Radiative Transfer, 1981
- Plasma Shifts of Hydrogenic-Ion LinesPhysical Review Letters, 1980
- Spectral Line Shifts Produced by Electron Collisions in HeII PlasmaJournal of the Physics Society Japan, 1980
- Quantum Scattering Theory of the Complex Level Shift of Spectral Lines in PlasmasProgress of Theoretical Physics, 1980
- Teopия acиммeтpии штaкoвcкиx пpoфилeй вoдopoдныx линий в плoтнoй плaзмeJournal of Quantitative Spectroscopy and Radiative Transfer, 1975
- Electron-Impact Broadening of Isolated Lines of Neutral Atoms in a Plasma. IPhysical Review B, 1969
- Measurement of Stark Profiles of Neutral and Ionized Helium and Hydrogen Lines from Shock-Heated Plasmas in Electromagnetic T TubesPhysical Review B, 1962
- Stark Broadening of Neutral Helium Lines in a PlasmaPhysical Review B, 1962
- The Statistics of the Gravitational Field Arising from a Random Distribution of Stars. I. The Speed of Fluctuations.The Astrophysical Journal, 1942