標(biāo)題: Titlebook: Cross-Magnetic Turbulent Diffusion of Charged Particles in a Weakly Ionized Plasma; Michio Matsumoto Book 1972 Westdeutscher Verlag GmbH, [打印本頁] 作者: HAG 時間: 2025-3-21 18:57
書目名稱Cross-Magnetic Turbulent Diffusion of Charged Particles in a Weakly Ionized Plasma影響因子(影響力)
書目名稱Cross-Magnetic Turbulent Diffusion of Charged Particles in a Weakly Ionized Plasma影響因子(影響力)學(xué)科排名
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書目名稱Cross-Magnetic Turbulent Diffusion of Charged Particles in a Weakly Ionized Plasma讀者反饋學(xué)科排名
作者: 流動性 時間: 2025-3-21 21:53 作者: 溫室 時間: 2025-3-22 01:51
Introduction,his 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..作者: 委屈 時間: 2025-3-22 05:06
Basic Consideration,ter 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作者: dilute 時間: 2025-3-22 10:32 作者: 一致性 時間: 2025-3-22 15:23 作者: 一致性 時間: 2025-3-22 20:48
Discussion,ot only by the density fluctuations, but also by the field fluctuations which result from the phase difference between ion and electron fluctuations. The turbulent correlation length λ. is much smaller than the wave lengths of current convective instability waves, but larger than the electron Debye 作者: FID 時間: 2025-3-23 01:04 作者: aesthetician 時間: 2025-3-23 03:35
Effect of small amplitude Fluctuations,e diffusion coefficients due to the fluctuations are small compared to those due to the Boltzmann type collisions even for strong magnetic fields . with S. = o. (10.～ 10.). For reason of studying the influence of the correlation functions it is usefull to begin with that easiest case.作者: 使更活躍 時間: 2025-3-23 05:33 作者: fastness 時間: 2025-3-23 11:14
Discussion,ons when the values . are not so small as shown in eq. (23). We will here discuss the values of A for the intermediate region between the small and large amplitude fluctuations by comparing with the succesive method of Kadomtsev.作者: hypertension 時間: 2025-3-23 17:28
Achtergrondinformatie en basisprincipesre determined by fourth order moments, the fourth order moments by next higher order ones, and so on. For a calculation, we must truncate this hierarchy. Then, we apply a method similar to Millionshchikov’s to the fourth order moments, mentioned before. The validity of this method will be discussed later.作者: 窗簾等 時間: 2025-3-23 22:02 作者: verdict 時間: 2025-3-23 22:20
Forschungsberichte des Landes Nordrhein-Westfalenhttp://image.papertrans.cn/d/image/240358.jpg作者: 吝嗇性 時間: 2025-3-24 04:52
Overview: 978-3-531-02282-6978-3-322-87851-9作者: pantomime 時間: 2025-3-24 07:54 作者: Interim 時間: 2025-3-24 14:28
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 affected by electric field fluctuations.作者: anchor 時間: 2025-3-24 18:52 作者: 花爭吵 時間: 2025-3-24 21:23
Basic Consideration,ter 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 affected by electric field fluctuations.作者: 臭了生氣 時間: 2025-3-25 01:44
Evalueren met beeldende middelenIf 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).作者: 賞心悅目 時間: 2025-3-25 05:41 作者: 收養(yǎng) 時間: 2025-3-25 07:47
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.作者: 宏偉 時間: 2025-3-25 11:47
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).作者: Matrimony 時間: 2025-3-25 18:20
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).作者: correspondent 時間: 2025-3-25 21:55
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.作者: 手段 時間: 2025-3-26 01:55
https://doi.org/10.1007/978-3-322-87851-9Debye length; Plasma; density; diffusion; electron; energy; experiment; magnetic field; particles; turbulence作者: 避開 時間: 2025-3-26 07:33 作者: Anticoagulants 時間: 2025-3-26 10:45
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..作者: Fulsome 時間: 2025-3-26 14:05
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作者: 現(xiàn)暈光 時間: 2025-3-26 20:16 作者: 占卜者 時間: 2025-3-26 22:33
Achtergrondinformatie en basisprincipeseffect which results from the diffusion along the magnetic field . (See the second term of eq. (31)). We consider the turbulent state in which the field fluctuations become stationary and homogeneous. This state corresponds to that of the positive column in strong magnetic fields with B several time作者: 背信 時間: 2025-3-27 04:52 作者: 創(chuàng)新 時間: 2025-3-27 08:21 作者: Popcorn 時間: 2025-3-27 11:29 作者: 教唆 時間: 2025-3-27 14:27 作者: Hamper 時間: 2025-3-27 20:32 作者: exhilaration 時間: 2025-3-28 00:28
der Hand. Dieses Buch wird Ihnen einiges darüber sagen, wie Sie genau das, was das "Verkaufen" so unangenehm macht, nicht mehr machen müssen. Warum? Weil Ihr potenzieller Kunde das für Sie tun wird - Sie dürfen ihn nur nicht daran hindern. Das bedeutet natürlich nicht, dass Sie gar nichts mehr tun m作者: flammable 時間: 2025-3-28 04:39 作者: 暗語 時間: 2025-3-28 09:48 作者: Spinal-Tap 時間: 2025-3-28 11:34
The Traditional Mediterranean Polycultural Landscape as Cultural Heritage: Its Origin and Historicalcesses. However, the pressure on these landscapes and their rapid transformation into more modern forms call out for a better knowledge of the more complex forms of traditional land use and relative landscapes. In this context, an identification and clarification of the role of such mixed and comple作者: Flatus 時間: 2025-3-28 18:30
Textbook 2019 Data is a related research area which studies how one can make RDF data available on the Web and interconnect it with other data with the aim of increasing its value for everybody. Knowledge Graphs have been shown useful not only for Web search (as demonstrated by Google, Bing, etc.) but also in ma作者: lesion 時間: 2025-3-28 21:01
