A V Blant et al 2000 Plasma Sources Sci. Technol. 9 12 doi:10.1088/0963-0252/9/1/303
A V Blant
, O H Hughes
, T S Cheng
, S V Novikov
,
and C T Foxon![]()
We have made a detailed study of the optical spectroscopy of two different RF plasma sources used for the growth of GaN by molecular beam epitaxy. Our studies show that for both sources the predominant species present in the cavity are nitrogen atoms. The strongest optical emission occurs at 869 nm. We have also studied, in detail, the factors which influence the ion content of the flux. Two key parameters are the temperature of the wall of the cavity and the size of the holes in the aperture plate from which the species emerge into the vacuum. We have identified conditions under which the ion content can be made negligibly small and show that this results in films with improved optical properties.
52.50.Qt Plasma heating by radio-frequency fields; ICR, ICP, helicons
Issue 1 (February 2000)
Received 4 January 1999, in final form 3 September 1999
A V Blant et al 2000 Plasma Sources Sci. Technol. 9 12
T Koponen et al 2006 New J. Phys. 8 179
N Dunlop et al 1999 Distrib. Syst. Engng. 6 82
Peter R Hobson and John Watson 2002 J. Opt. A: Pure Appl. Opt. 4 S34
R Martínez-Herrero et al 2004 J. Opt. A: Pure Appl. Opt. 6 S64
Amir Karniel et al 2005 J. Neural Eng. 2 S250
T J Quinn 2001 Metrologia 38 89
F Ninio 1976 J. Phys. A: Math. Gen. 9 1281
M Modarres et al 1978 J. Phys. G: Nucl. Phys. 4 L127
W G Scaife 1974 J. Phys. D: Appl. Phys. 7 647