Laboratory Observations of Plasma Satellites on the2P14D1and2P34D3Lines of Helium

Abstract
During the implosion phase of a low-density θ pinch in helium preheated to Te1 eV at Ne5×1013 cm3, the He I 2P14D1 and 2P34D3 lines show satellites displaced away from the forbidden 2PnF transitions by 0.3-0.6 Å. These satellites are identified with those predicted by Baranger and Mozer as due to the effects of nonthermal longitudinal plasma oscillations on atomic spectra.

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