切口
发表于 2025-3-21 17:28:01
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TRACE
发表于 2025-3-21 21:54:06
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发酵
发表于 2025-3-22 04:17:04
Franz Koenigsberger,Rolf Hackstein very short cyclotron time scale and the gyro-radius length scale. At the other end, it accurately describes the macroscopic behaviour of large astrophysical and fusion plasmas. The complexity arising from this wide range of plasma physics information makes it virtually impossible to solve the Boltz
很是迷惑
发表于 2025-3-22 05:13:34
Introduction,re (almost) everywhere in the universe and to point out that they are extremely complicated physical systems fundamentally different from classic neutral gases, especially when there is a magnetic field present. The hope is that the reader is convinced that plasmas are exciting physical objects that
治愈
发表于 2025-3-22 12:12:13
Fluid equations for mass, momentum and energy, very short cyclotron time scale and the gyro-radius length scale. At the other end, it accurately describes the macroscopic behaviour of large astrophysical and fusion plasmas. The complexity arising from this wide range of plasma physics information makes it virtually impossible to solve the Boltz
bizarre
发表于 2025-3-22 16:23:53
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细胞膜
发表于 2025-3-22 20:42:28
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致敬
发表于 2025-3-22 23:57:08
Basic plasma properties, range electromagnetic interaction between the charged particles. In this Chapter we shall study the two basic characteristics that are used in the definition of a plasma: quasi-neutrality and collective behaviour. We shall determine basic consequences arising from the long-range Coulomb interaction
针叶
发表于 2025-3-23 01:43:15
Fluid equations for mass, momentum and energy, plasmas are most accurately described by particle distribution functions in phase space. The spatial and temporal evolution of these distribution functions are governed by the Boltzmann equation (2.9). This is a partial differential equation in a 7-dimensional space. Chapman and Enskog were the fir
connoisseur
发表于 2025-3-23 06:32:59
Magnetohydrodynamics, Chapter do not form a closed set. The aim of this Chapter is to obtain closure. Let us recall that expressions for the anisotropic part of the stress tensor and for the flux of heat due to random motions are necessary but not sufficient for obtaining this goal. Inspection of the single-fluid equati