I. Peres et al., DEPENDENCE OF THE EMISSION CHARACTERISTICS OF MAGNETIZED SURFACE-WAVEPLASMAS ON THE AZIMUTHAL CONFIGURATION OF THE WAVE-FIELD, Journal of applied physics, 82(9), 1997, pp. 4211-4218
A 1D plasma-wave model initially developed for describing a plasma sus
tained by a surface wave in the azimuthally symmetric configuration (m
=0) was modified for simulating surface waves in the dipolar mode (m =
1). Using this model, it is shown that the maintenance limit for unma
gnetized plasmas in the symmetric mode, which, as was previously deter
mined, requires that the product of the wave frequency and the plasma
radius be smaller than 2 GHz cm, is no longer valid for magnetized pla
smas. Comparison of calculated and measured radial distributions of ar
gon atoms in a radiative excited state shows that changes observed in
this distribution when varying some of the operating conditions can be
explained by a switching of the discharge from one mode to the other.
Conditions for selection of the mode are derived from considerations
on wave propagation and power dissipation along the plasma column. (C)
1997 American Institute of Physics. [S0021-8979(97)03421-X].