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This paper presents fully kinetic particle simulations of plasma charging at lunar craters with the presence of lunar lander modules using the recently developed Parallel Immersed-Finite-Element Particle-in-Cell (PIFE-PIC) code. The computation model explicitly includes the lunar regolith layer on top of the lunar bedrock, taking into account the regolith layer thickness and permittivity as well as the lunar lander module in the simulation domain, resolving a nontrivial surface terrain or lunar lander configuration. Simulations were carried out to study the lunar surface and lunar lander module charging near craters at the lunar terminator region under mean and severe plasma environments. The lunar module’s position is also investigated to see its effect on the plasma charging relative to the craters. Differential surface charging was clearly resolved by the simulations. For the charging of a lunar lander module made of conducting materials, the results show a near-uniform potential close to that of its surrounding environment and moderate levels of local electric fields. Additionally, the risks associated with charging and discharging increase significantly under a more severe plasma charging environment as shown in the severe plasma environment cases.
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Kinetic simulations of dust grain charging in experimental plasma conditions
This paper presents fully-kinetic numerical investigations of the charging of spherical and irregular dust grains in the OML sheath regime and a stationary experimental plasma environment utilizing the Dusty Parallel Immersed-Finite-Element Particle-in-Cell (PIFE-PIC-D) framework. The simulations account for surface charging of the dust grains immersed in an stationary plasma environment. PIFE-PIC-D explicitly resolves the geometrical and material properties (permittivity) of each individual dust grain. The charge collection over time of each dust grain is investigated with varying size, irregularity, number of grains, spacing between dust grains, and permittivity. The charging behavior of a dust cluster is estimated by calculating its electron Debye length edge-to-edge separation to offer valuable insights into a dust cluster’s general charge dynamics. Lastly, unlike prior studies that focused solely on either fully conducting spheres or perfectly dielectric spheres, this work explores a more comprehensive range of permittivities for irregular dust grain aggregates.
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- Award ID(s):
- 2132655
- PAR ID:
- 10652103
- Publisher / Repository:
- Elsevier
- Date Published:
- Journal Name:
- Icarus
- Volume:
- 420
- Issue:
- C
- ISSN:
- 0019-1035
- Page Range / eLocation ID:
- 116212
- Subject(s) / Keyword(s):
- Dusty plasma, Dust charging, Kinetic simulations
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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- Free Publicly Accessible Full Text
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Accepted Manuscript1.0
- Journal Article:
- https://doi.org/10.1016/j.icarus.2024.116212
