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Building Langmuir Probes and Emissive Probes for Plasma Potential Measurements in Low Pressure, Low Temperature Plasmas
Published on: May 25, 2021
Peter H Yoon1, Rodrigo A López2, Chadi S Salem3
1Institute for Physical Science and Technology, University of Maryland, College Park, MD 20742, USA.
Quiet-time solar wind electrons exhibit non-thermal velocity distributions, explained by whistler-mode turbulence. This turbulence couples with fluctuations, forming kappa-like distributions observed in space plasma.
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