Self-organization of dust grains into stable filamentary dust structures (or “chains”) largely depends on dynamic interactions between individual charged dust grains and complex electric potential arising from the distribution of charges within a local plasma environment. Recent studies have shown that the positive column of the gas discharge plasma in the Plasmakristall-4 (PK-4) experiment at the International Space Station supports the presence of fast-moving ionization waves, which lead to variations of plasma parameters by up to an order of magnitude from the average background values. The highly variable environment resulting from ionization waves may have interesting implications for the dynamics and self-organization of dust particles, particularly concerning the formation and stability of dust chains. Here, we investigate the electric potential surrounding dust chains in the PK-4 experiment by employing a molecular dynamics model of the dust and ions with boundary conditions supplied by a particle-in-cell with Monte Carlo collision simulation of the ionization waves. The model is used to examine the effects of the plasma conditions within different regions of the ionization wave and compare the resulting dust structure to that obtained by employing the time-averaged plasma conditions. The comparison between simulated dust chains and experimental data from the PK-4 experiment shows that the time-averaged plasma conditions do not accurately reproduce observed results for dust behavior, indicating that more careful treatment of plasma conditions in the presence of ionization waves is required. It is further shown that commonly used analytic forms of the electric potential do not accurately describe the electric potential near charged dust grains under these plasma conditions.
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February 2022
Research Article|
February 17 2022
Influence of temporal variations in plasma conditions on the electric potential near self-organized dust chains
Katrina Vermillion
;
Katrina Vermillion
a)
1
CASPER, Baylor University
, One Bear Place 97316, Waco, Texas 76798-7316, USA
a)Author to whom correspondence should be addressed: katrina_vermillion1@baylor.edu
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Dustin Sanford;
Dustin Sanford
1
CASPER, Baylor University
, One Bear Place 97316, Waco, Texas 76798-7316, USA
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Lorin Matthews
;
Lorin Matthews
1
CASPER, Baylor University
, One Bear Place 97316, Waco, Texas 76798-7316, USA
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Peter Hartmann
;
Peter Hartmann
1
CASPER, Baylor University
, One Bear Place 97316, Waco, Texas 76798-7316, USA
2
Institute for Solid State Physics and Optics, Wigner Research Centre for Physics
, P.O. Box 49, H-1525 Budapest, Hungary
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Marlene Rosenberg;
Marlene Rosenberg
3
Department of Electrical and Computer Engineering, University of California at San Diego
, La Jolla, California 92093, USA
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Evdokiya Kostadinova
;
Evdokiya Kostadinova
1
CASPER, Baylor University
, One Bear Place 97316, Waco, Texas 76798-7316, USA
4
Department of Physics, Leach Science Center, Auburn University
, Auburn, Alabama 36849, USA
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Jorge Carmona-Reyes
;
Jorge Carmona-Reyes
1
CASPER, Baylor University
, One Bear Place 97316, Waco, Texas 76798-7316, USA
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Truell Hyde
;
Truell Hyde
1
CASPER, Baylor University
, One Bear Place 97316, Waco, Texas 76798-7316, USA
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Andrey M. Lipaev;
Andrey M. Lipaev
5
Joint Institute for High Temperatures, Russian Academy of Sciences
, Izhorskaya 13/19, 125412 Moscow, Russia
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Alexandr D. Usachev;
Alexandr D. Usachev
5
Joint Institute for High Temperatures, Russian Academy of Sciences
, Izhorskaya 13/19, 125412 Moscow, Russia
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Andrey V. Zobnin;
Andrey V. Zobnin
5
Joint Institute for High Temperatures, Russian Academy of Sciences
, Izhorskaya 13/19, 125412 Moscow, Russia
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Oleg F. Petrov
;
Oleg F. Petrov
5
Joint Institute for High Temperatures, Russian Academy of Sciences
, Izhorskaya 13/19, 125412 Moscow, Russia
6
Moscow Institute of Physics and Technology
, Institutsky Lane 9, Dolgoprudny, Moscow Region 141700, Russia
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Markus H. Thoma
;
Markus H. Thoma
7
I. Physikalisches Institut, Justus-Liebig-Universität Giessen
, Heinrich-Buff-Ring 16, 35392 Giessen Germany
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Mikhail Y. Pustylnik;
Mikhail Y. Pustylnik
8
Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Linder Höhe
, 51147 Cologne, Germany
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Hubertus M. Thomas
;
Hubertus M. Thomas
8
Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Linder Höhe
, 51147 Cologne, Germany
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Alexey Ovchinin
Alexey Ovchinin
9
Gagarin Research and Test Cosmonaut Training Center
, 141160 Star City, Moscow Region, Russia
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a)Author to whom correspondence should be addressed: katrina_vermillion1@baylor.edu
Phys. Plasmas 29, 023701 (2022)
Article history
Received:
October 14 2021
Accepted:
January 31 2022
Citation
Katrina Vermillion, Dustin Sanford, Lorin Matthews, Peter Hartmann, Marlene Rosenberg, Evdokiya Kostadinova, Jorge Carmona-Reyes, Truell Hyde, Andrey M. Lipaev, Alexandr D. Usachev, Andrey V. Zobnin, Oleg F. Petrov, Markus H. Thoma, Mikhail Y. Pustylnik, Hubertus M. Thomas, Alexey Ovchinin; Influence of temporal variations in plasma conditions on the electric potential near self-organized dust chains. Phys. Plasmas 1 February 2022; 29 (2): 023701. https://doi.org/10.1063/5.0075261
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