2021
DOI: 10.1088/1361-6595/abe7a1
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Influence of secondary electron emission on plasma-surface interactions in the low earth orbit environment

Abstract: The low earth orbit plasma experienced by exposed interconnect-dielectric junctions commonly found on spacecraft solar panel surfaces was modeled using a fully kinetic particle-in-cell (PIC) simulation of both ambient ions and electrons. From time-accurate simulations we observed that the plasma sheath had a formation time somewhere between the ion and electron time scales of 17 μs and 30 ps, respectively and electron and ion velocity distribution functions were observed to be highly non-Maxwellian. Comparison… Show more

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Cited by 9 publications
(1 citation statement)
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“…To satisfy the numerical validity of the time-explicit nature of the coupling between Poisson's equation and particle movement, we use a time-step, ∆t < 0.1ω −1 pe and grid cell-size, ∆x < λ D [21], where ω pe and λ D are the local electron plasma frequency and Debye length, respectively. The code CHAOS has previously been used in plume-plasma [2,3], and plasma-surface interaction [22] studies, and provides the multi-GPU scalability necessary for this study.…”
Section: Numerical Approach and General Plasma Conditionsmentioning
confidence: 99%
“…To satisfy the numerical validity of the time-explicit nature of the coupling between Poisson's equation and particle movement, we use a time-step, ∆t < 0.1ω −1 pe and grid cell-size, ∆x < λ D [21], where ω pe and λ D are the local electron plasma frequency and Debye length, respectively. The code CHAOS has previously been used in plume-plasma [2,3], and plasma-surface interaction [22] studies, and provides the multi-GPU scalability necessary for this study.…”
Section: Numerical Approach and General Plasma Conditionsmentioning
confidence: 99%