Titlebook: An Introduction to Plasma Astrophysics and Magnetohydrodynamics; Marcel Goossens Book 2003 Springer Science+Business Media Dordrecht 2003

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書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics影響因子(影響力)




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics影響因子(影響力)學(xué)科排名




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics網(wǎng)絡(luò)公開度




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics被引頻次




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics被引頻次學(xué)科排名




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics年度引用




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics年度引用學(xué)科排名




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics讀者反饋




書目名稱An Introduction to Plasma Astrophysics and Magnetohydrodynamics讀者反饋學(xué)科排名

TRACE

發(fā)酵

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

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

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

細(xì)胞膜

致敬

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

針葉

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

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