Time Evolution of Three-Dimensional Structural State in Microgravity Dusty Plasma
POSTER
Abstract
Dusty plasmas are collections of charged macroscopic particles (referred to as “dust”) in low temperature, weakly ionized plasma. As the dust grains collect charge from the free-moving electrons in the plasma cloud, they become negatively charged and are observed to organize in complex structural states. Here we analyze data from the Plasmakristall-4 microgravity dusty plasma experiment on board the International Space Station. Previous studies of dust clouds in the PK-4 experiment have suggested that anisotropic dust-dust interactions lead to the formation of exotic structural states reminiscent of liquid crystal states [1], such as smectic and nematic structures. We extend those previous studies for datasets that used improved temporal resolution through a reduced FOV and corresponding increased camera frame rate for better imaging and data. In these experiments, the clouds are trapped in the camera field of view using a polarity-switched axial electric field. The time evolution of the dusty plasma structural state is studied using pair correlation functions calculated for particles within the central plane of the dust cloud and within successive planes of the cloud (the 3D cloud).
[1] https://doi.org/10.48550/arXiv.2505.14576
[1] https://doi.org/10.48550/arXiv.2505.14576
Presenters
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Jacob Fries
University of Alabama in Huntsville, University of Alabama Huntsville
Authors
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Jacob Fries
University of Alabama in Huntsville, University of Alabama Huntsville
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Ransom H May
Columbus State University
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Katherine E Notbohm
University of Alabama in Huntsville
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Daniel C Nyatuame
Auburn University
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Jason Jenkins
University of Alabama Huntsville
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Evdokiya G Kostadinova
Auburn University
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Saikat Thakur
Auburn University
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David Robert Charles Goymer
Auburn University
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Bradley Andrew
Auburn University
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Diana Jiménez Martí
Baylor University
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Lorin S Matthews
Baylor University
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Truell W Hyde
Baylor University