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Probing a dusty magnetized plasma with self-excited dust-density waves

Benjamin Tadsen*, Franko Greiner, and Alexander Piel

  • IEAP, Christian-Albrechts-Universität, 24098 Kiel, Germany

  • *tadsen@physik.uni-kiel.de

Phys. Rev. E 97, 033203 – Published 14 March, 2018

DOI: https://doi.org/10.1103/PhysRevE.97.033203

Abstract

A cloud of nanodust particles is created in a reactive argon-acetylene plasma. It is then transformed into a dusty magnetized argon plasma. Plasma parameters are obtained with the dust-density wave diagnostic introduced by Tadsen et al. [Phys. Plasmas 22, 113701 (2015)]. A change from an open to a cylindrically enclosed nanodust cloud, which was observed earlier, can now be explained by a stronger electric confinement if a vertical magnetic field is present. Using two-dimensional extinction measurements and the inverse Abel transform to determine the dust density, a redistribution of the dust with increasing magnetic induction is found. The dust-density profile changes from being peaked around the central void to being peaked at an outer torus ring resulting in a hollow profile. As the plasma parameters cannot explain this behavior, we propose a rotation of the nanodust cloud in the magnetized plasma as the origin of the modified profile.

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