The microwave reflection and noise emission (extraordinary mode) from cylindrical rare-gas (He, Ne, Ar) afterglow plasmas in an axial magnetic field is described. Reflection and noise emission are measured as a function of magnetic field near electron cyclotron resonance (ω ≈ ωc) with electron density as a parameter (ωp < ω). A broad peak, which shifts to lower values of ωc/ω) as electron density increases, is observed for (ωc/ω) ≤ 1. For all values of electron density a second sharp peak is found very close to cyclotron resonance in reflection measurements. This peak does not occur in the emission data. Calculations of reflection and emission using a theoretical model consisting of a one-dimensional, cold plasma slab with nonuniform electron density yield results in qualitative agreement with the observations. Both the experimental and theoretical results suggest that the broad, density-dependent peak involves resonance effects at the upper hybrid frequency (ωh2 = ωc2 + ωp2) of the plasma.
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Blum et al. (1969) studied this question.
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