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Simulating Plasma Microwave Diagnostics
Journal of Scientific Computing, 2006The paper presents computational simulations of plasma diagnostics via microwave absorption, where the number density of the charge particles and its collision frequency with the neutral particles are measured basing on the microwave attenuation phenomenon.
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Plasma Diagnostics by Spectroscopic Methods
Applied Optics, 1967Spectroscopic techniques for the measurement of plasma parameters are reviewed for a range of temperatures up to 10(6) degrees K. Tables and figures of useful data have been prepared or have been collected from the literature for ready application to experimental measurements.
D, Robinson, P D, Lenn
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Plasma MicroRNA as a novel diagnostic
Clinica Chimica Acta, 2019MicroRNAs (miRNAs) are small, single-stranded, endogenous, non-coding RNAs necessary for proper gene expression. Their mechanism of action controls translation by base-pairing with target messenger RNA (mRNAs) thus leading to translation blockage or mRNA degradation.
Rafal Szelenberger +4 more
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Plasma diagnostics with Bernstein waves
Zeitschrift für angewandte Mathematik und Physik ZAMP, 1974Note: ZAMP 25, 677 (1974) Reference CRPP-CONF-1974-002 Record created on 2008-05-13, modified on 2017-05 ...
Bitter, M., Paris, P. J.
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RF techniques in plasma diagnostics
Plasma Physics and Controlled Fusion, 1998An overview is given on active and passive microwave diagnostics established on fusion experiments. The basic principles of the various techniques are briefly outlined and their limits as well as recent developments are discussed.
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INFRARED PLASMA DIAGNOSTICS WITH LASERS
Infrared Physics, 1976Abstract Infrared lasers have rendered possible measurements of plasma parameters in a range not accessible using either optical or microwave techniques. Diagnostic methods based on the refraction and scattering of radiation by free electrons are discussed.
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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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