Dusty plasmas
Abstract
This is the final report of a three-year, Laboratory-Directed Research and Development (LDRD) project at the Los Alamos National Laboratory (LANL). The objective of this project has been to develop a fundamental understanding of dusty plasmas at the Laboratory. While dusty plasmas are found in space in galactic clouds, planetary rings, and cometary tails, and as contaminants in plasma enhanced fabrication of microelectronics, many of their properties are only partially understood. Our work has involved both theoretical analysis and self-consistent plasma simulations to understand basic properties of dusty plasmas related to equilibrium, stability, and transport. Such an understanding can improve the control and elimination of plasma dust in industrial applications and may be important in the study of planetary rings and comet dust tails. We have applied our techniques to the study of charging, dynamics, and coagulation of contaminants in plasma processing reactors for industrial etching and deposition processes and to instabilities in planetary rings and other space plasma environments. The work performed in this project has application to plasma kinetics, transport, and other classical elementary processes in plasmas as well as to plasma waves, oscillations, and instabilities.
- Authors:
- Publication Date:
- Research Org.:
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE, Washington, DC (United States)
- OSTI Identifier:
- 266370
- Report Number(s):
- LA-UR-96-1341
ON: DE96010474; TRN: 96:016924
- DOE Contract Number:
- W-7405-ENG-36
- Resource Type:
- Technical Report
- Resource Relation:
- Other Information: PBD: [1996]
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 70 PLASMA PHYSICS AND FUSION; PLASMA; DUSTS; PROGRESS REPORT; COSMIC DUST; INTERSTELLAR SPACE; ANALYTICAL SOLUTION; NUMERICAL SOLUTION; PARTICLE SIZE; GLOW DISCHARGES
Citation Formats
Jones, M E, Winske, D, Keinigs, R, and Lemons, D. Dusty plasmas. United States: N. p., 1996.
Web. doi:10.2172/266370.
Jones, M E, Winske, D, Keinigs, R, & Lemons, D. Dusty plasmas. United States. https://doi.org/10.2172/266370
Jones, M E, Winske, D, Keinigs, R, and Lemons, D. 1996.
"Dusty plasmas". United States. https://doi.org/10.2172/266370. https://www.osti.gov/servlets/purl/266370.
@article{osti_266370,
title = {Dusty plasmas},
author = {Jones, M E and Winske, D and Keinigs, R and Lemons, D},
abstractNote = {This is the final report of a three-year, Laboratory-Directed Research and Development (LDRD) project at the Los Alamos National Laboratory (LANL). The objective of this project has been to develop a fundamental understanding of dusty plasmas at the Laboratory. While dusty plasmas are found in space in galactic clouds, planetary rings, and cometary tails, and as contaminants in plasma enhanced fabrication of microelectronics, many of their properties are only partially understood. Our work has involved both theoretical analysis and self-consistent plasma simulations to understand basic properties of dusty plasmas related to equilibrium, stability, and transport. Such an understanding can improve the control and elimination of plasma dust in industrial applications and may be important in the study of planetary rings and comet dust tails. We have applied our techniques to the study of charging, dynamics, and coagulation of contaminants in plasma processing reactors for industrial etching and deposition processes and to instabilities in planetary rings and other space plasma environments. The work performed in this project has application to plasma kinetics, transport, and other classical elementary processes in plasmas as well as to plasma waves, oscillations, and instabilities.},
doi = {10.2172/266370},
url = {https://www.osti.gov/biblio/266370},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Wed May 01 00:00:00 EDT 1996},
month = {Wed May 01 00:00:00 EDT 1996}
}