Bulletin of the American Physical Society
Fall 2024 Joint Meeting of the Texas Section of the APS, Texas Section of the AAPT & Zone 13 of the SPS
Thursday–Saturday, October 17–19, 2024; Southern Methodist University, Dallas, Texas
Session M01: Plenary III
11:00 AM–12:00 PM,
Saturday, October 19, 2024
Southern Methodist University
Room: Oren Auditorium
Chair: Hao-Yi Wu, Southern Methodist University
Abstract: M01.00001 : A Simple Goal: Complete Understanding of the (Dusty Plasma) Universe*
11:00 AM–11:30 AM
Presenter:
Lorin S Matthews
(Baylor University)
Author:
Lorin S Matthews
(Baylor University)
A complex, or dusty, plasma consists of tiny pieces of solid material a hundred times smaller than the width of a human hair immersed in a plasma environment. This talk gives a brief overview of dusty plasma experiments and numerical modeling of dust particle charging and transport in plasma environments. Understanding the charging and dynamics of dust is important to understanding our universe as well as exploring our solar system. Charged dust is the primary component of many beautiful astrophysical phenomena such as comet tails, planetary rings, protoplanetary disks, and noctilucent clouds. It can also be a problem. The Apollo astronauts found lunar dust a nuisance, obscuring visors and instrument readouts, degrading seals, and abrading materials. The Mars Rovers stopped working when their solar panels became covered with dust. Magnetically-confined fusion experiments create dust when plasma interacts with the walls, which can disrupt the fusion process. Insights into dusty plasma will contribute to producing clean energy in the future.
*Support for this work from the US Department of Energy, Office of Science, Office of Fusion Energy Sciences under awards DE-SC0021334 and DE-SC0024681, and National Science Foundation under awards PHY-2308742 and PHY-2308743.
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