Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session JP11: Poster Session IV: Education and Outreach; Undergraduate or High School Research; Plasma technology, Fusion reactor Nuclear and Materials Science; Propulsion; Materials Interfaces (2:00pm-5:00pm)
Tuesday, November 6, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.JP11.78
Abstract: JP11.00078 : Self-consistent simulation of dust-plasma interactions in micro-gravity*
Presenter:
Dustin L Sanford
(CASPER, Baylor Univ)
Authors:
Dustin L Sanford
(CASPER, Baylor Univ)
Lorin Matthews
(CASPER, Baylor Univ)
Truell W Hyde
(CASPER, Baylor Univ)
A complex (dusty) plasma consists of ions, electrons, and micron-sized solid particles, commonly referred to as dust. An interesting aspect of complex plasma is its ability to self-organize into dust liquids, 2D and 3D dust crystal lattices and 1D dust chains. The resulting interaction between the dust and the flowing plasma creates an ion wakefield downstream from the dust, with the resulting positive space region modifying the interaction between the grains and contributing to the observed dynamics and equilibrium structure of the system.The PK4 experiment onboard the International Space Station allows for the investigation of the formation and dynamics of dust structures in microgravity, where the weak ion wakefield interactions play a larger role in determining the system dynamics. Here we present a molecular dynamics simulation capable of resolving the dynamics of extended dust structures on both ion and dust particle time scales. The results are compared with experimental data from the PK4 experiment.
*Support from NASA Grant number 1571701, and NSF Grant numbers 1414523, 1707215 and 174023 is gratefully acknowledged.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.JP11.78
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