Physics:Mercier criterion
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Short description: Plasma criteria
The Mercier criterion is a criterion for plasma used in the theoretical study of plasma instability. It was first proposed in 1954 by C. Mercier, who applied the perturbation method (in which [math]\displaystyle{ \omega =\frac {\partial } {\partial t} }[/math] represents the frequency[specify] and [math]\displaystyle{ \mathbf k = \frac {\partial} {\partial z} }[/math] is the z-direction of the unit vector) to the plasma mathematical model to compute calculations.[1][2]
References
- ↑ Bauer, Frances; Betancourt, Octavio; Garabedian, Paul (1984). Magnetohydrodynamic Equilibrium and Stability of Stellarators. New York, NY: Springer-Verlag New York. p. 22-27. doi:10.1007/978-1-4612-5240-5_5. ISBN 978-1-4612-9753-6. https://link.springer.com/chapter/10.1007/978-1-4612-5240-5_5.
- ↑ Mikhailovskii, A. B. (October 2017). Instabilities in a Confined Plasma. CRC Press. ISBN 978-1-351-43816-2. https://books.google.com/books?id=8pY4DwAAQBAJ&pg=PT94.
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