High-speed imaging of magnetized plasmas: when electron temperature matters
Simon Vincent, Vincent Dolique, Nicolas Plihon

TL;DR
This study demonstrates that electron temperature significantly influences high-speed imaging of magnetized plasmas, challenging the common assumption that light fluctuations directly represent plasma density variations.
Contribution
It provides a systematic comparison between high-speed camera imaging and direct plasma parameter measurements, highlighting the importance of electron temperature in interpreting plasma fluctuations.
Findings
Light intensity is not a reliable proxy for plasma density.
Electron temperature fluctuations are crucial for accurate interpretation of imaging data.
High-speed imaging fluctuations match an Arrhenius law incorporating density and temperature variations.
Abstract
High speed camera imaging is a powerful tool to probe the spatiotemporal features of unsteady processes in plasmas, usually assuming light fluctuations to be a proxy for the plasma density fluctuations. In this article, we systematically compare high speed camera imaging with simultaneous measurements of the plasma parameters -- plasma density, electron temperature, floating potential -- in a modestly magnetized Argon plasma column at low pressure (1 mTorr, magnetic fields ranging from 160 to 640~G). The light emission was filtered around ~nm, ~nm, ~nm. We show that the light intensity cannot be interpreted as a proxy for the plasma density and that the electron temperature cannot be ignored when interpreting high speed imaging, both for the time-averaged profiles and for the fluctuations. The features of plasma parameter fluctuations are investigated, with a…
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