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Ion collection by a sphere in a flowing plasma: 3. Floating potential and drag force

TLDR
In this paper, the interaction of an ion-collecting sphere at floating potential with a flowing collisionless plasma is investigated using the particle in cell code SCEPTIC, and the dependence of the floating potential on the flow velocity for a conducting sphere is found to agree very well with the orbital motion limited approximation, which ignores the asymmetry in the plasma potential.
Abstract
The interaction of an ion-collecting sphere at floating potential with a flowing collisionless plasma is investigated using the particle in cell code SCEPTIC. The dependence of the floating potential on the flow velocity for a conducting sphere is found to agree very well with the orbital motion limited approximation, which ignores the asymmetry in the plasma potential. But the charge, even on conducting spheres and at zero flow, is not well represented by using the standard expression for capacitance. Insulating spheres become asymmetrically charged because of ion collection asymmetry, and their total (negative) charge is considerably increased by flow. The collection flux asymmetry is documented for both conducting and insulating spheres and is not greatly different between them. The drag force upon the sphere is obtained from the code calculations. It shows reasonable agreement with appropriate analytic approximations. However, numerical discrepancies up to 20% are found, which are attributed to uncertainties in the analytical values.

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Citations
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Complex (dusty) plasmas: current status, open issues, perspectives

TL;DR: The field of complex (dusty) plasmas is reviewed in this paper, where the major types of experimental complex Plasmas are briefly discussed, including grain charging in different regimes, interaction between charged particles, and momentum exchange between different species.
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Colloquium : Fundamentals of dust-plasma interactions

TL;DR: In this paper, the underlying physics of different forces that act on a charged dust grain is reviewed, including wakefield and ion focusing effects and dipole-dipole interactions between unevenly charged dust rods.
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Complex plasmas: a laboratory for strong correlations

TL;DR: In this article, the authors give an overview on recent experimental and theoretical results in complex plasmas, including liquid-like behavior, crystal formation, structural and dynamic properties, which is expected that many of these effects will be of interest also to researchers in other fields where strong correlations play a prominent role.
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The Particle-In-Cell Method

TL;DR: In this paper, the authors summarize the recent work of an European-wide collaboration which has been ongoing since about one decade using Particle-in-Cell (PIC) methods in low temperature plasma physics.
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Complex plasma: dusts in plasma

TL;DR: In this article, some fundamental aspects of a complex system involving plasma particles and dust particles in a collective way are reviewed and possible applications are discussed, as well as possible applications of such systems.
References
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Book

Introduction to Dusty Plasma Physics

TL;DR: The book Introduction to Plasma Physics by Shukla and Mamun as discussed by the authors deals with various aspects of collective processes in dusty plasmas and provides a handbook on waves and instabilities in the coming years.
Book

Principles of Plasma Diagnostics

TL;DR: In this paper, the authors introduce a glossary of fast ions and fusion products, including fast ions, fast ion, and fast ion fusion products and their applications in the field of magnetic diagnostics.
Journal ArticleDOI

The Theory of Collectors in Gaseous Discharges

TL;DR: In this article, a cylindrical or spherical electrode (collector) immersed in an ionized gas is brought to a suitable potential, it becomes surrounded by a symmetrical space charge region or "sheath" of positive or of negative ions (or electrons).
Journal ArticleDOI

Dynamical friction. I. General considerations: the coefficient of dynamical friction

TL;DR: In this paper, it was shown that a star must experience dynamical friction, i.e., it must suffer from a systematic tendency to be decelerated in the direction of its motion.
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