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Diagnostics of the Solar Wind Plasma
2009The solar wind is a fully ionized plasma, coming from the outer atmosphere of the Sun, the so-called solar corona, which expands as a supersonic flow into the interplanetary medium [55]. The first observations indicating that the Sun might be emitting a wind were made by Biermann in 1946 of comet tails [1], which are observed to point away from the Sun.
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Microwave diagnostics of small plasma objects
Journal of Applied Physics, 2005Mikhail N Shneider, Miles R B
exaly
Analysis of the enthalpy probe technique for thermal plasma diagnostics
Review of Scientific Instruments, 1995Gervais Soucy
exaly
Diagnostics for plasma-based electron accelerators
Reviews of Modern Physics, 2018M C Downer, A Debus, U Schramm
exaly
Diagnostics of plasma reactive species and induced chemistry of plasma treated foods
Critical Reviews in Food Science and Nutrition, 2019Camila Augusto Perussello +2 more
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