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 CO8: Dusty Plasmas, Sources, and Diagnostics
2:00 PM–5:00 PM,
Monday, November 5, 2018
OCC
Room: C120-122
Chair: Lorin Matthews, Baylor University
Abstract ID: BAPS.2018.DPP.CO8.1
Abstract: CO8.00001 : Aligned Chains within the PK-4 Environment*
2:00 PM–2:12 PM
Presenter:
Truell W Hyde
(CASPER, Baylor Univ)
Authors:
Truell W Hyde
(CASPER, Baylor Univ)
Lorin S Matthews
(CASPER, Baylor Univ)
Peter Hartmann
(Wigner Research Centre for Physics, CASPER, Baylor Univ)
Marlene Rosenberg
(University of California at San Diego)
Oleg F. Petrov
(Joint Institute for High Temperatures, Russian Academy of Sciences, CASPER, Baylor Univ)
Vladimir Nosenko
(DLR Institute of Material Physics in Space, Wessling, Germany, CASPER, Baylor Univ)
Jie Kong
(CASPER, Baylor Univ)
Ke Qiao
(CASPER, Baylor Univ)
Eva Kostadinova
(CASPER, Baylor Univ)
Jorge Carmona Reyes
(CASPER, Baylor Univ)
Complex plasmas have proven a versatile analog for the study of soft matter systems. On Earth, the streaming ion flow plays a major role in such systems, particularly in interparticle interactions and particle alignment. Since it is in general much weaker than other system forces, in terrestrial experiments its effects are partially masked by gravity obscuring the underlying physics. One way of avoiding this issue is through use of the PK-4 currently in operation on the International Space Station. [1]
This talk will discuss extended particle chain formation as observed in Campaigns 1 through 4 by the PK-4. Experimental observations will be compared to plasma discharge simulations as well as dust charging and interaction simulations. Data for the dust-dust and dust-plasma interaction will also be compared and the relationship between the phenomenon generally known as striations and dust particle behavior will be examined.
[1] M. Y. Pustylnik, et. al. Review of Scientific Instruments 87 (2016) 093505.*Support from NASA Grant number 1571701 and NSF Grant numbers 1414523,1707215, 174023 is gratefully acknowledged.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.CO8.1
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