Results 111 to 120 of about 36,956 (161)
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Convection and wave-particle interactions

Journal of Atmospheric and Terrestrial Physics, 1978
Abstract We study, by means of the adiabatic invariants and Liouville's theorem, the deformation of the distribution functions of substorm injected particles in the magnetosphere. Assuming a steady-state convection process, we can obtain simple analytical expressions for the particle flux, the anisotropy and the growth rate of electromagnetic ...
Jacques Solomon, René Pellat
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Wave–Particles Interaction

2014
AbstractIn this Chapter an alternative derivation of the self-consistent Vlasov-Maxwell equations for wave-particles interaction is given. The analysis is carried out under a rigorous Hamiltonian framework and targeted to modeling the dynamics of the Free Electron Laser.
A. Campa   +3 more
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Wave-Particle Interactions

1984
Note: Magnetospheric studies of the interactions between plasma waves and particles have generally been performed using Gaussian units. To allow the material presented here to be conveniently used in conjunction with other published material on magnetospheric wave-particle interactions, we have not converted equations from the literature into MKS units.
L. R. Lyons, D. J. Williams
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Relativistic structure of stochastic wave–particle interaction

The Physics of Fluids, 1988
Stochastic interactions of charged particles with electrostatic waves propagating at arbitrary angles to an external magnetic field are studied based on a relativistic canonical Hamiltonian formalism. The present theory, however, is valid also for electromagnetic waves after a slight modification.
Akimoto, K., Karimabadi, H.
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New resonances in wave–particle interactions

Physics of Plasmas, 2023
One of the most characteristic features of relativistic particle dynamics at cyclotron resonances is the stepwise dependence of energy and momentum on time [V. A. Buts and A. G. Zagorodny, Phys. Plasmas 28(2), 022311 (2021)]. The reason for these steps is the phase synchronization of charged particles and waves. To describe other features, we introduce
V. A. Buts, A. G. Zagorodny
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Computational models for wave-particle interactions

Computer Physics Communications, 1986
Abstract A 2-D finite-element evolution Fokker-Planck code, BACCHUS, is presented. The originally current-drive version and a more recent bounce-averaged version are discussed in some detail. A 1 1 2 - D quasi-linear code, RUNAWAY, is also described, especially to elucidate the major difficulties arising when the wave-particle interaction ...
S. Succi   +5 more
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Wave–particle interactions in plasmas

Plasma Physics and Controlled Fusion, 2006
An overview of the interactions between waves and particles in plasmas is given. Interest is focused on cases where special particle populations, like energetic particle tails, interact with waves. The two basic, but inter-related, mechanisms through which waves and particles can exchange energy, resonance and stochastization are briefly illustrated ...
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Linear Wave-Particle Interactions

1998
Abstract Collisionless absorption of h.f. power is a remarkable property of hot plasmas, and it is of great theoretical interest to understand how it occurs. It also has practical importance, since the possibility of selective dissipation and thermalisation of h.f. waves with the appropriate frequency, phase velocity, and polarization is
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Gyroresonant Wave-Particle Interactions

1972
This review will be restricted to gyroresonant interactions. The basic processes of these interactions are discussed in the frame of the quasi-linear theory. Frequencies of interaction, anisotropy of the particle distribution function, and amplification and diffusion coefficients are computed for different types of interaction and different regions of ...
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Wave-particle interactions in hot plasmas

AIP Conference Proceedings, 2006
This overview talk focuses on the populations of particles which are transmitted through the nearly perpendicular termination shock from the solar wind to the heliosheath, and how they relax and excite waves in the heliosheath. The transmission process probably involves direct transmission of the very cold solar wind core.
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