Titlebook: Cross-Magnetic Turbulent Diffusion of Charged Particles in a Weakly Ionized Plasma; Michio Matsumoto Book 1972 Westdeutscher Verlag GmbH,

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Achtergrondinformatie en basisprincipesBefore discussing the turbulent state, we examine the current convective instability, which was first studied by Kadomtsev..) His theory is based on the approximation of quasi-neutrality .. Now we take account of the effect of the ion temperature. We use the linearized eq. (9), in which the quasi-neutrality condition is not necessary.

宏偉

Steady State Cross-Magnetic Flow,If the microscopic state of the plasma at time t is completely determined by the well-known coordinates and velocities of particles, we can start from the Klimontovich equations for the phase densities Na (., ., t).

Matrimony

Hierarchy for the Moments of density Fluctuations,We derive an equation for the density fluctuations δ n. (., t) from the continuity and momentum equations which are constructed from eqs. (3) and (5).

correspondent

Current convective Instability,Before discussing the turbulent state, we examine the current convective instability, which was first studied by Kadomtsev..) His theory is based on the approximation of quasi-neutrality .. Now we take account of the effect of the ion temperature. We use the linearized eq. (9), in which the quasi-neutrality condition is not necessary.

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https://doi.org/10.1007/978-3-322-87851-9Debye length; Plasma; density; diffusion; electron; energy; experiment; magnetic field; particles; turbulence

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Hulpmiddelen in de samenwerkinghis problem theoretically. and experimentally.. In cases of weak turbulence, the ion diffusion coefficient D. is proportional to the electric field fluctuation energy or the mean square amplitude of density fluctuations..

Fulsome

R. Boniver,D. C. Alpini,G. Brugnoniter than the plasma frequencies π., where the subscript a stands for the type of the charged particles. Frequencies of the fluctuations are much less than V.. Hence, we assume that the charged particles have almost nearly a local Maxwellian velocity distribution. The charged particles are further af

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