標題: Titlebook: Nonlinear MHD Waves and Turbulence; Proceedings of the W Thierry Passot,Pierre-Louis Sulem Conference proceedings 1999 Springer-Verlag Berl [打印本頁] 作者: 面臨 時間: 2025-3-21 19:09
書目名稱Nonlinear MHD Waves and Turbulence影響因子(影響力)
書目名稱Nonlinear MHD Waves and Turbulence影響因子(影響力)學科排名
書目名稱Nonlinear MHD Waves and Turbulence網(wǎng)絡公開度
書目名稱Nonlinear MHD Waves and Turbulence網(wǎng)絡公開度學科排名
書目名稱Nonlinear MHD Waves and Turbulence被引頻次
書目名稱Nonlinear MHD Waves and Turbulence被引頻次學科排名
書目名稱Nonlinear MHD Waves and Turbulence年度引用
書目名稱Nonlinear MHD Waves and Turbulence年度引用學科排名
書目名稱Nonlinear MHD Waves and Turbulence讀者反饋
書目名稱Nonlinear MHD Waves and Turbulence讀者反饋學科排名
作者: humectant 時間: 2025-3-21 22:44
https://doi.org/10.1007/3-540-47038-7Alfven waves; Dissipation; MHD; MHD turbulence; MHD waves; Magnetohydrodynamics; Plasma; astrophysics; magne作者: 知識 時間: 2025-3-22 03:04
978-3-642-08598-7Springer-Verlag Berlin Heidelberg 1999作者: negotiable 時間: 2025-3-22 08:12 作者: 勤勉 時間: 2025-3-22 09:18 作者: inspired 時間: 2025-3-22 13:05
Quasi-Two-Dimensional Hydrodynamics and Interaction of Vortex Tubes,This paper is long overdue. Most of the results presented here were obtained in 1986-87. Just a small portion of them (the equations for the dynamics of a pair of counter-rotating vortices and their self-similar solutions) were published in time - in 1988 [1]. The publication was very brief and did not include any details of the calculations.作者: Mechanics 時間: 2025-3-22 18:53 作者: Habituate 時間: 2025-3-22 22:48 作者: 支形吊燈 時間: 2025-3-23 05:11
,Nonlinear Phenomena Involving Dispersive Alfvén Waves,he generation of low-frequency turbulence and the modication of the background plasma density in the Earth’s ionosphere and magnetosphere, as well as to the large amplitude coherent nonlinear structures which are frequently observed in auroral plasmas.作者: 用不完 時間: 2025-3-23 08:53 作者: 碳水化合物 時間: 2025-3-23 12:50 作者: fodlder 時間: 2025-3-23 16:20 作者: 艱苦地移動 時間: 2025-3-23 21:34
Dynamics of Vortex and Magnetic Lines in Ideal Hydrodynamics and MHD,nt fluids. The Weber type transformation for ideal MHD gives the whole Lagrangian vector invariant. When this invariant is absent this transformation coincides with the Clebsch representation analog introduced in作者: Distribution 時間: 2025-3-23 22:39
Conference proceedings 1999s expanded versions of oral contributions pre- sented at this meeting, should be of interest for a large community of resear- chers in space plasmas and nonlinear sciences. Special effort was made to put the new results into perspective and to provide a detailed literature review. A main motivation 作者: 易達到 時間: 2025-3-24 05:39
,Nonlinear Phenomena Involving Dispersive Alfvén Waves, with small amplitude Alfvén waves and their relation with other low-frequency plasma modes in a uniform plasma. We then show that dispersive Alfvén waves can be excited either by electron beams or by high-frequency external pump waves. Finite amplitude dispersive Alfvén waves interact with the back作者: QUAIL 時間: 2025-3-24 08:54 作者: 啟發(fā) 時間: 2025-3-24 12:07
,Alfvén Wave Filamentation and Plasma Heating,equations are here derived to describe this phenomenon. They apply in different regimes, depending on the level of the dispersion with respect to the nonlinearity. The (scalar) nonlinear Schr?dinger equation, valid when the wave is strongly dispersive, allows the study of the influence of the coupli作者: 農(nóng)學 時間: 2025-3-24 16:30
,Nonlinear Quasiresonant Alfvén Oscillations in a One-Dimensional Magnetic Cavity,rced by the shear motion of its boundaries is studied. It is shown that, even in the case of strong nonlinearity, these oscillations can be represented, to leading order, by a sum of two solutions in the form of oppositely propagating waves with permanent shapes. An infinite set of nonlinear algebra作者: Hormones 時間: 2025-3-24 21:10
,On the Reflection of Alfvén Waves in the Inhomogeneous Solar Wind,) the mass density of the medium, (ii) strength and direction of the external magnetic field, (iii) of the mean flow velocity and (iv) of multiple ion species in the background. The effects (i) to (iv) are studied initially isolated and then in combination, causing the reflection of Alfvén waves, wh作者: 意外的成功 時間: 2025-3-25 02:25
,Relativistic Alfvén Solitons and Acceleration of Cosmic Rays, those plasmas have specific properties that are presented in this paper. Nonlinear dynamics are different in a pair plasma and in proton dominated plasma. The nonlinear disturbances of Alfvén type are interesting to accelerate relativistic particles and the extension of Fermi acceleration to a rela作者: 表皮 時間: 2025-3-25 06:27
Reduced Models of Magnetohydrodynamic Turbulence in the Interstellar Medium and the Solar Wind,m of equations has been derived from the compressible magnetohydrodynamic (MHD) equations to describe turbulence in the interstellar medium and the solar wind. These equations apply to a plasma permeated by a spatially varying mean magnetic field when the plasma beta is of the order unity or less. I作者: 向前變橢圓 時間: 2025-3-25 08:09
,Alfvénic Turbulence and Wave Propagation in the Corona and Heliosphere,adial gradients in determining the variation of amplitude with distance. Some comments on the role of photospheric vorticity as a source for Alfvén waves are presented, 1-D and 2-D MHD couplings of the waves as they climb out of the coronal density gradient are described (parametric decay, sound wav作者: CRAMP 時間: 2025-3-25 14:42 作者: 扔掉掐死你 時間: 2025-3-25 19:29
Coherent Electrostatic Nonlinear Waves in Collisionless Space Plasmas,ions, magnetotail, etc) from di)erent space experiments. One of the striking results obtained in the recent years is that these waves are basically electrostatic and coherent, in the form of solitary structures (weak double layers and solitary waves having respectively a net and no net potential dro作者: minimal 時間: 2025-3-25 23:06 作者: 保全 時間: 2025-3-26 03:17 作者: ASSAY 時間: 2025-3-26 06:28
Shell Models for MHD Turbulence,teractions, the paper focuses on the most recent results concerning dynamical properties and intermittency of a model which is a generalization to MHD of the Gledzer-Yamada-Okhitani (GOY) model for hydrodynamic. Applications to astrophysical problems are also discussed.作者: follicle 時間: 2025-3-26 08:37
Dynamics of Vortex and Magnetic Lines in Ideal Hydrodynamics and MHD,fluids it is shown that the equations of motion for vorticity and magnetic field with the help of this transformation follow from the variational principle. By means of this representation it is possible to integrate the system of hydrodynamic type with the Hamiltonian . = Ω.r. It is also demonstrat作者: 雇傭兵 時間: 2025-3-26 15:20
Conference proceedings 1999of experts in plasma physics, fluid dynamics and applied mathematics. The aim of the meeting was to survey the current knowledge on two main topics: (i) propagation of plasma waves (like Alfven, whistler or ion-acoustic waves), their instabilities and the development of a nonlinear dynamics lea- din作者: molest 時間: 2025-3-26 19:56
,On the Reflection of Alfvén Waves in the Inhomogeneous Solar Wind,nts. Particular attention is given to singularities of the wave equation in the presence of mean flow e.g. critical layers where the mean flow velocity equals the Alfvén speed, and localized wave reflection may occur, as well as other changes in wave properties.作者: 自由職業(yè)者 時間: 2025-3-26 22:48
,Nonlinear Quasiresonant Alfvén Oscillations in a One-Dimensional Magnetic Cavity,ic equations for the Fourier coefficients of these solutions is derived. It is then reduced to a finite set of equations by trancation and solved analytically in the one-mode approximation and numerically in the general case. The comparison of the analytical and numerical results is carried out.作者: GUISE 時間: 2025-3-27 05:01
,Relativistic Alfvén Solitons and Acceleration of Cosmic Rays,tivistic plasma as an accelerating medium turns out to be far more efficient than in a non-relativistic plasma. If it happens in Nature, as suggested by some observations, a head on collision of relativistic Alfvén solitons is a very efficient event to accelerate cosmic rays.作者: 吝嗇性 時間: 2025-3-27 09:07 作者: 繼而發(fā)生 時間: 2025-3-27 11:59 作者: Detonate 時間: 2025-3-27 14:24
0075-8450 ure.Includes supplementary material: The workshop "Nonhnear MHD Waves and Turbulence" was held at the - servatoire de Nice, December 1-4, 1998 and brought together an international group of experts in plasma physics, fluid dynamics and applied mathematics. The aim of the meeting was to survey the cu作者: wangle 時間: 2025-3-27 17:55 作者: 同義聯(lián)想法 時間: 2025-3-27 23:47 作者: parasite 時間: 2025-3-28 03:45 作者: aesthetic 時間: 2025-3-28 09:34
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