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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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11#
發(fā)表于 2025-3-23 13:37:41 | 只看該作者
Vadim N. Tsytovichria is an obvious feature, and abnormal hair has been reported in argininosuccinic aciduria, citrullinaemia, argininaemia, homocystinuria, tyrosinaemia, Hartnup disease, and others. Before the mechanism of protein synthesis was clearly understood, it was considered possible that excess of an amino a
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發(fā)表于 2025-3-23 17:07:56 | 只看該作者
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發(fā)表于 2025-3-23 22:55:45 | 只看該作者
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發(fā)表于 2025-3-24 04:31:17 | 只看該作者
Kinetics of Random Collective Excitations. Quasi-linear Interactions,tion turn out to be far from simple to answer. Let us accept that a typical plasma state is a state where many collective oscillations are excited at a level which is sufficiently high for their interaction to be non-linear. In that case it is reasonable to use for these collective oscillations a ki
16#
發(fā)表于 2025-3-24 08:06:35 | 只看該作者
Fluctuations and Particle Collisions,istical fluctuations in a plasma when there are no external fields or strong collective oscillations. At first sight these two problems are unrelated but, in fact, they are related to one another. In discussing fluctuations when there are no fields present we shall consider the case of an arbitrary
17#
發(fā)表于 2025-3-24 13:14:46 | 只看該作者
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發(fā)表于 2025-3-24 15:01:57 | 只看該作者
19#
發(fā)表于 2025-3-24 19:02:24 | 只看該作者
Non-linear Modulational Interactions,ar interactions is larger than the difference in the frequencies of the interacting waves. The physics of this interaction consists in the modulation of the plasma parameters by one of the interacting waves which leads to the above-mentioned frequency broadening and to interactions with other waves.
20#
發(fā)表于 2025-3-24 23:56:50 | 只看該作者
Dissipative Structures and Strong Langmuir Turbulence,tive structures. Many problems of strong turbulence are still being studied. However, this field of research is so important that it needs a special discussion. At the present time the majority of the important physical concepts are clear, but the details of the formation of strong turbulence and it
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