標(biāo)題: Titlebook: An Introduction to Plasma Astrophysics and Magnetohydrodynamics; Marcel Goossens Book 2003 Springer Science+Business Media Dordrecht 2003 [打印本頁(yè)] 作者: 切口 時(shí)間: 2025-3-21 17:28
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
作者: TRACE 時(shí)間: 2025-3-21 21:54 作者: 發(fā)酵 時(shí)間: 2025-3-22 04:17
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作者: 很是迷惑 時(shí)間: 2025-3-22 05:13
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作者: 治愈 時(shí)間: 2025-3-22 12:12
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作者: bizarre 時(shí)間: 2025-3-22 16:23 作者: 細(xì)胞膜 時(shí)間: 2025-3-22 20:42 作者: 致敬 時(shí)間: 2025-3-22 23:57
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作者: 針葉 時(shí)間: 2025-3-23 01:43
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作者: connoisseur 時(shí)間: 2025-3-23 06:32
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作者: Counteract 時(shí)間: 2025-3-23 10:21 作者: abnegate 時(shí)間: 2025-3-23 14:20
The solar wind,km s. at the Earth’s orbit caused a huge controversy in the astrophysical and geophysical communities. Parker’s theory was received with a great deal of skepticism, even disbelief. Fortunately for E. Parker, Russian and American satellites soon afterwards did indeed discover this fast streaming sola作者: 審問(wèn) 時(shí)間: 2025-3-23 19:04 作者: 煞費(fèi)苦心 時(shí)間: 2025-3-23 23:19
978-1-4020-1433-8Springer Science+Business Media Dordrecht 2003作者: 切掉 時(shí)間: 2025-3-24 02:38
Die Wechselwirkung der physischen Kr?fteut the focus is on basic concepts of plasma physics and on basic properties of plasmas. An average student in physics or mathematics at the K.U.Leuven does not know very much about plasma physics. He is not particularly worried by this lack of scientific knowledge as he happens to live in a corner o作者: 巨頭 時(shí)間: 2025-3-24 09:53
Franz Koenigsberger,Rolf Hackstein 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作者: NEG 時(shí)間: 2025-3-24 11:32
Franz Koenigsberger,Rolf Hackstein 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作者: 牛的細(xì)微差別 時(shí)間: 2025-3-24 18:02
,Das Gau?sche Divisionsverfahren, 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作者: 權(quán)宜之計(jì) 時(shí)間: 2025-3-24 21:17 作者: 觀察 時(shí)間: 2025-3-25 01:34
Jeannette Prinzessin zu Fürstenbergkm s. at the Earth’s orbit caused a huge controversy in the astrophysical and geophysical communities. Parker’s theory was received with a great deal of skepticism, even disbelief. Fortunately for E. Parker, Russian and American satellites soon afterwards did indeed discover this fast streaming sola作者: 是他笨 時(shí)間: 2025-3-25 03:24 作者: 陳列 時(shí)間: 2025-3-25 11:06 作者: nitroglycerin 時(shí)間: 2025-3-25 12:45 作者: 頭盔 時(shí)間: 2025-3-25 18:39
Basic plasma properties,haviour. We identify major plasma parameters that characterize the high-frequency behaviour associated with the dynamics of the electrons and the low-frequency behaviour associated with the dynamics of the ions.作者: 防銹 時(shí)間: 2025-3-25 23:04
Book 2003 encounter with plasmas, with a powerful plasma model that they can link to familiar classic fluid dynamics. The solar wind is studied as an example of hydrodynamics and MHD at work in solar physics and astrophysics. .作者: 脫離 時(shí)間: 2025-3-26 00:26 作者: Ordeal 時(shí)間: 2025-3-26 05:26
,Das Gau?sche Divisionsverfahren, 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 equations for a very simple case (3.42) revealed that there are more unknowns than equations.作者: atrophy 時(shí)間: 2025-3-26 11:28 作者: Aesthete 時(shí)間: 2025-3-26 13:22 作者: 沒有希望 時(shí)間: 2025-3-26 19:10 作者: ULCER 時(shí)間: 2025-3-26 23:53
Book 2003sics. On Earth they are essential for magnetic controlled thermonuclear fusion. ..This textbook collects lecture notes from a one-semester course taught at the K.U. Leuven to advanced undergraduate students in applied mathematics and physics. A particular strength of this book is that it provides a 作者: 人充滿活力 時(shí)間: 2025-3-27 02:12
,Das Gau?sche Divisionsverfahren,d-like behaviour of plasmas. Magneto-gravity waves will be absent for the present discussion. There are situations in solar and astrophysical plasmas where a gravitational force, either due to an external gravitational field or due to self-gravitation, has to be included in the mathematical analysis.作者: Aerate 時(shí)間: 2025-3-27 06:36 作者: Maximize 時(shí)間: 2025-3-27 10:29
8樓作者: Valves 時(shí)間: 2025-3-27 14:52
9樓作者: 燕麥 時(shí)間: 2025-3-27 20:27
9樓作者: ARCHE 時(shí)間: 2025-3-28 01:01
9樓作者: 踉蹌 時(shí)間: 2025-3-28 03:53
10樓作者: 善于 時(shí)間: 2025-3-28 08:45
10樓作者: Preamble 時(shí)間: 2025-3-28 13:19
10樓作者: 預(yù)知 時(shí)間: 2025-3-28 17:04
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