This thesis explores Langmuir waves in a laboratory plasma and draws comparisons to solar wind turbulence. A dual-filament setup generates and perturbs a plasma (argon/helium), with Langmuir probes used to extract electron characteristics. A Vlasov–Poisson code simulates beam–plasma interactions and produces a k-spectrum for comparison. This research seeks to validate lab diagnostics against space-based probe data from missions like Parker Solar Probe.

Langmuir wave study in a laboratory plasma, a model for solar wind.

LEMONIDIS, OSCAR BRADMAN
2024/2025

Abstract

This thesis explores Langmuir waves in a laboratory plasma and draws comparisons to solar wind turbulence. A dual-filament setup generates and perturbs a plasma (argon/helium), with Langmuir probes used to extract electron characteristics. A Vlasov–Poisson code simulates beam–plasma interactions and produces a k-spectrum for comparison. This research seeks to validate lab diagnostics against space-based probe data from missions like Parker Solar Probe.
2024
Langmuir wave study in a laboratory plasma, a model for solar wind.
Langmuir Wave
Plasma
Solar Wind
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.12608/94344