What is it about?

Azimuthal surface waves are eigenmodes of cylindrical plasma–dielectric–metal structures both in the presence of and without an axial static magnetic field. They are actively studied due to possible applications in plasma electronics, nanotechnologies and biomedical diagnostics. Higher radial modes are known to propagate at higher frequencies and shorter wavelengths compared to those of the zeroth mode, a feature which is of interest for practical applications. To gain the advantage of the excitation of higher radial modes of azimuthal surface waves one has first to know their dispersion properties. This paper generalizes the results of earlier papers by including a static axial magnetic field and considering the higher radial modes. The presence of the constant axial magnetic field removes the degeneracy in the wave spectrum with respect to the sign of the azimuthal wavenumber.

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Why is it important?

It contains a brief overview of studying azimuthal electromagnetic waves, I particular, of surface type; as well as studying (both analytical and numerical) of their dispersion properties in the case of higher radial harmonics.

Perspectives

The knowledge of the dispersion properties helps in studying the wave excitation and application in physics of gas discharges.

Igor Girka
V. N. Karazin Kharkiv National University, Ukraine

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This page is a summary of: Higher radial modes of azimuthal surface waves in magnetoactive cylindrical plasma waveguides, Journal of Plasma Physics, November 2018, Cambridge University Press,
DOI: 10.1017/s0022377818001101.
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