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Katrina Vermillion

Publications and source records attributed to Katrina Vermillion.

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Structural States of Filamentary Microgravity Dusty Plasma

This study investigates the filamentary structural states of microgravity dusty plasma using data from the Plasmakristall-4 (PK-4) facility on board the International Space Station. The dust particles in the PK-4 discharge are observed to form field-aligned filaments and nested (layered) structures in response to changes in the plasma conditions, neutral gas pressure, and externally applied electric field. This work explores the possibility that these filamentary dusty plasmas exhibit properties of liquid crystals. The structural characteristics of the dust clouds are studied for nine sets of pressure-current conditions using pair correlation functions calculated for particles (i) within individual filaments, (ii) within the central plane of the dust cloud, and (iii) within successive planes of the cloud (the 3D cloud). It is observed that, at low pressure ($\approx$30 Pa), the entire cloud is in a weakly crystalline state with similar coupling of particles within filaments and among neighboring filaments. At high pressure ($\approx$70 Pa), the order within filaments improves (enhanced crystalline behavior), while the degree of freedom of filaments to move with respect to each other increases (enhanced liquid behavior). Since neutral gas pressure in dusty plasma acts as inverse temperature, we argue that the structural changes observed with increasing pressure are analogous to a transition to a nematic liquid crystal state. It is further observed that the filaments exhibit alignment in nested surfaces for several pressure-current conditions, suggesting the possibility of a smectic liquid crystal state. These results are confirmed by molecular dynamics simulations of the dust and ions using the DRIAD (Dynamic Response of Ions And Dust) code.

physics.plasm-ph

Evolution of Ion Wake Characteristics with Experimental Conditions

Two-dimensional microparticle crystals can be formed in the sheath of a gas discharge plasma. Ions from the bulk plasma are accelerated in the sheath electric field, flowing past the grains to create a positive ion wake downstream from the grains. Interaction between the ion wake and neighboring grains creates additional coupling between oscillation modes and can trigger mode-coupling instability (MCI). Recent experiments have shown that at a fixed discharge power there are threshold pressures above and below which the monolayer always crystallizes or melts, respectively. The melting is due to MCI being triggered in the crystal monolayer, while the crystallization is due to the suppression of MCI by neutral damping in the fluid monolayer. The relationship between the discharge parameters and ion wake characteristics is unknown. A molecular dynamics simulation of ion dynamics and dust charging is used to self-consistently determine the dust charge and ion wake characteristics for different experimental conditions. It is found that the ion wake is strongly dependent on discharge pressure but not affected much by the discharge power.

physics.plasm-ph

Influence of Temporal Variations in Plasma Conditions on the Electric Potential Near Self-Organized Dust Chains

The self-organization of dust grains into stable filamentary dust structures (or "chains") largely depends on dynamic interactions between the individual charged dust grains and the complex electric potential arising from the distribution of charges within the local plasma environment. Recent studies have shown that the positive column of the gas discharge plasma in the Plasmakristall-4 (PK-4) experiment onboard the International Space Station (ISS) 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 by employing a molecular dynamics model of the dust and ions with boundary conditions supplied by a Particle-in-Cell with Monte Carlo collisions (PIC-MCC) 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. Comparison between simulated dust chains and experimental data from the PK-4 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.

physics.plasm-ph