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Particle velocity distribution in a three-dimensional dusty plasma under microgravity conditions
Conference proceeding   Open access   Peer reviewed

Particle velocity distribution in a three-dimensional dusty plasma under microgravity conditions

Bin Liu, J Goree, M. Y Pustylnik, H. M Thomas, V. E Fortov, A. M Lipaev, A. D Usachev, V. I Molotkov, O. F Petrov and M. H Thoma
AIP conference proceedings, Vol.1925(1)
DIVERSE WORLD OF DUSTY PLASMAS: Proceedings of the 8th International Conference on the Physics of Dusty Plasmas
01/05/2018
DOI: 10.1063/1.5020393
url
https://doi.org/10.1063/1.5020393View
Published (Version of record) Open Access

Abstract

The velocity distribution function of dust particles immersed in a plasma was investigated under microgravity conditions. A three-dimensional (3D) cloud of polymer microspheres was suspended in a neon plasma, in the PK-4 instrument onboard the International Space Station (ISS). These dust particles were tracked using video microscopy in a cross section of the 3D dust cloud. The velocity distribution function (VDF) is found to have a non-Maxwellian shape with high-energy tails; it is fit well by a combination of low-energy Maxwellian core and a high-energy non-Gaussian Kappa-distribution halo. Similar non-Maxwellian VDFs are typically observed in space plasmas.

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