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Titlebook: Lectures on Non-linear Plasma Kinetics; Vadim N. Tsytovich Book 1995 Springer-Verlag Berlin Heidelberg 1995 Astrophysics and space physics

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21#
發(fā)表于 2025-3-25 04:33:49 | 只看該作者
Plasma Maser Effect and Adiabatic Invariants in Non-linear Interactions,e themaser effect may be produced by the inverse population of particles which are participating in the non-linear interactions or by the inverse population of waves. We have discussed earlier that a plasma is a strongly non-linear state of matter, and that it may contain a large number of waves whi
22#
發(fā)表于 2025-3-25 07:49:23 | 只看該作者
Non-linear Interactions of Collective Oscillations and Waves with Particle Fluctuations, fluctuations. One cannot avoid the non-linear interactions of the turbulent and regular wave fields with the fields of these fluctuations and with the fluctuations in the index of refraction produced by the particle fluctuations. To complete the discussion of the non-linear kinetics we must conside
23#
發(fā)表于 2025-3-25 13:09:38 | 只看該作者
24#
發(fā)表于 2025-3-25 16:06:38 | 只看該作者
Some Remarks on Plasma Non-linear Kinetics in External Magnetic Fields. Conclusion,ound oscillations. However, for those collective modes we have tried to show as fully as possible what is known about their different non-linear interactions and non-linear kinetic processes. We have considered all that is known about all the interactions and relations between the various non-linear
25#
發(fā)表于 2025-3-25 21:45:09 | 只看該作者
Kinetics of Random Collective Excitations. Quasi-linear Interactions,a mathematical and from a physical point of view it is impossible to follow each particle separately. In fact, if all particles interact strongly with one another, chaos will ensue and any initial conditions will soon be forgotten: it is physically impossible to follow the trajectory of any individu
26#
發(fā)表于 2025-3-26 01:11:43 | 只看該作者
Fluctuations and Particle Collisions,t these fluctuations are closely connected with particle collisions in the plasma. We shall describe these relations in the present chapter and we shall show that collisions between particles in a plasma are quite different from collisions between particles in the absence of other plasma particles.
27#
發(fā)表于 2025-3-26 06:46:33 | 只看該作者
28#
發(fā)表于 2025-3-26 10:23:23 | 只看該作者
Plasma Maser Effect and Adiabatic Invariants in Non-linear Interactions,en in a turbulent state which results in the formation of small-scale inhomogeneities in the fields and in the particle distributions. These inhomogeneities are characteristic features of the plasma state of matter since a plasma is often turbulent.
29#
發(fā)表于 2025-3-26 12:45:21 | 只看該作者
Non-linear Interactions of Collective Oscillations and Waves with Particle Fluctuations,e a process connected with the emission by particles during collisions, which is nothing but bremsstrahlung. Since the cross-sections for collisions are significantly changed by collective processes in the plasma we may expect that the bremsstrahlung will also be significantly changed by collective
30#
發(fā)表于 2025-3-26 19:40:40 | 只看該作者
Collective Effects in Bremsstrahlung of Plasma Particles,ould bear in mind that the final result of absorption or amplification in a non-equibrium system is the result of the balance between stimulated bremsstrahlung absorption and stimulated bremsstrahlung emission.
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