標(biāo)題: Titlebook: Cosmic Electrodynamics; Electrodynamics and Gregory D. Fleishman,Igor N. Toptygin Book 2013 Springer Science+Business Media New York 2013 [打印本頁] 作者: 可樂 時間: 2025-3-21 18:26
書目名稱Cosmic Electrodynamics影響因子(影響力)
作者: sigmoid-colon 時間: 2025-3-21 21:28 作者: 美色花錢 時間: 2025-3-22 00:34
Nonlinear MHD Waves and Discontinuities,es often rise to large-amplitude perturbations, which cannot be fully accommodated by the linear theory and so require non-linear treatment. In this chapter we consider a number of important examples of the nonlinear waves—simple waves, solitons, and discontinuities—with the use of exact or approxim作者: Corporeal 時間: 2025-3-22 07:22 作者: 地名詞典 時間: 2025-3-22 11:34
Particle Transport in Turbulent Cosmic Media, distribution of heavy elements released by supernova explosions, dust particle distribution and evolution, propagation of energetic particles away from their sources, and many more. The particles under study can either be dynamically important for the entire system or play a passive role. In the la作者: angina-pectoris 時間: 2025-3-22 14:35 作者: angina-pectoris 時間: 2025-3-22 20:36
Emission Processes,ms of computing the Poynting vector flux through a closed infinitely distant surface surrounding the radiation source (Melrose 1980;Rybicki and Lightman 1986; Ginzburg 1987;Nagirner 2007b). In contrast, computing the emission from a plasma, which is an anisotropic, dispersive, and absorbing matter, 作者: exorbitant 時間: 2025-3-23 00:19
Radiation Transfer,thus, the radiation intensity, spectral distribution, polarization, and directivity can all vary in space and time. The theory of radiation transfer represents a broad field of the physics with numerous astrophysical applications (Chandrasekhar 1961;Mihalas 1978;Dolginov etal.1979;Ginzburg 1987; Nag作者: 六個才偏離 時間: 2025-3-23 03:59
Particle Acceleration in Astrophysical Media,arge Hadron collider (LHC) recently commissioned in Europe. These specially designed accelerating devices are needed because high-energy particles lose their energy very quickly due to interaction with matter and external fields and, thus, become thermally assimilated by the medium.作者: Diastole 時間: 2025-3-23 09:27 作者: 直言不諱 時間: 2025-3-23 11:22 作者: 巨碩 時間: 2025-3-23 16:58 作者: 伙伴 時間: 2025-3-23 18:04
Immobilism in the French Fourth RepublicDispersion of a medium is provided by a response of the particles composing the medium to an external electromagnetic field applied to the medium. To study the dispersion quantitatively we have to derive macroscopic equations describing averaged electromagnetic fields in the medium.作者: Cougar 時間: 2025-3-23 22:13
Plasma Dispersion: Linear Modes in the Plasma,Dispersion of a medium is provided by a response of the particles composing the medium to an external electromagnetic field applied to the medium. To study the dispersion quantitatively we have to derive macroscopic equations describing averaged electromagnetic fields in the medium.作者: ARCHE 時間: 2025-3-24 02:21
Nonlinear MHD Waves and Discontinuities,es often rise to large-amplitude perturbations, which cannot be fully accommodated by the linear theory and so require non-linear treatment. In this chapter we consider a number of important examples of the nonlinear waves—simple waves, solitons, and discontinuities—with the use of exact or approximate analytical methods.作者: Herd-Immunity 時間: 2025-3-24 07:01
Instability of MHD Motion and Astrophysical MHD Turbulence,cillate with some damping rate and so eventually dissipate. In astrophysics, however, there are numerous examples of the states, which are not stable. Instead, an instability takes place in many cases: small random perturbations of the macroscopic parameters rise at the expense of either mechanical or magnetic energy.作者: 神圣不可 時間: 2025-3-24 13:51
Particle Acceleration in Astrophysical Media,arge Hadron collider (LHC) recently commissioned in Europe. These specially designed accelerating devices are needed because high-energy particles lose their energy very quickly due to interaction with matter and external fields and, thus, become thermally assimilated by the medium.作者: 陪審團(tuán) 時間: 2025-3-24 15:28 作者: Antagonist 時間: 2025-3-24 19:05 作者: Prologue 時間: 2025-3-25 02:11
Immobilism in the French Fourth Republices often rise to large-amplitude perturbations, which cannot be fully accommodated by the linear theory and so require non-linear treatment. In this chapter we consider a number of important examples of the nonlinear waves—simple waves, solitons, and discontinuities—with the use of exact or approxim作者: Inertia 時間: 2025-3-25 05:46
Singapore’s Totalitarian Mass Societycillate with some damping rate and so eventually dissipate. In astrophysics, however, there are numerous examples of the states, which are not stable. Instead, an instability takes place in many cases: small random perturbations of the macroscopic parameters rise at the expense of either mechanical 作者: 過多 時間: 2025-3-25 07:38 作者: 周年紀(jì)念日 時間: 2025-3-25 13:11
Wood Pellet Production Standards,re listed in Table1.1. The characteristic spatial scales of these fields can be of the same order of or ever greater than the size of the object. These large-scale fields often coexist with small-scale fields varying on scales much shorter than the object size. The small-scale field is not necessari作者: 虛度 時間: 2025-3-25 18:57
Elizabeth Arnold,Chester Hanveyms of computing the Poynting vector flux through a closed infinitely distant surface surrounding the radiation source (Melrose 1980;Rybicki and Lightman 1986; Ginzburg 1987;Nagirner 2007b). In contrast, computing the emission from a plasma, which is an anisotropic, dispersive, and absorbing matter, 作者: Exposition 時間: 2025-3-25 21:23
https://doi.org/10.1007/978-3-319-74612-8thus, the radiation intensity, spectral distribution, polarization, and directivity can all vary in space and time. The theory of radiation transfer represents a broad field of the physics with numerous astrophysical applications (Chandrasekhar 1961;Mihalas 1978;Dolginov etal.1979;Ginzburg 1987; Nag作者: 序曲 時間: 2025-3-26 02:52 作者: Tartar 時間: 2025-3-26 06:18
Elizabeth Arnold,Chester Hanveyistic plasma component on top of nonrelativistic background plasma or drives the entire plasma to an ultrarelativistic state. A vivid example of the first option is the galactic and extragalactic (ultra-high-energy) cosmic rays (CRs), while the latter one includes ultrarelativistic pulsar winds or j作者: Cloudburst 時間: 2025-3-26 11:59 作者: 菊花 時間: 2025-3-26 14:40 作者: 隱語 時間: 2025-3-26 19:01 作者: 粗糙 時間: 2025-3-26 21:49 作者: 入伍儀式 時間: 2025-3-27 01:30 作者: Decongestant 時間: 2025-3-27 08:41
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/c/image/238876.jpg作者: Cursory 時間: 2025-3-27 12:54
https://doi.org/10.1007/978-1-4614-5782-4MHD examples; cosmic electrodynamics; galactic superbubble MHD; interstellar winds plasma; nonlinear sel作者: Corporeal 時間: 2025-3-27 14:32 作者: 陶醉 時間: 2025-3-27 19:36
Book 2013ined with new developments and the authors demarcate what is well established and what is still under debate. To book illustrates how apparently complicated phenomena can be addressed and understood using well-known physical principles and equations within appropriate approximations and simplificati作者: 弄皺 時間: 2025-3-27 22:34
Magnetohydrodynamics of the Cosmic Plasma,undamentals, so we just remind the equations and briefly discuss the meaning of the terms entering them without going into the detail too deeply. The relation of HD to the kinetic theory has been outlined in Sect. 1.3.作者: 原告 時間: 2025-3-28 04:07 作者: gruelling 時間: 2025-3-28 10:12 作者: offense 時間: 2025-3-28 13:31 作者: arabesque 時間: 2025-3-28 15:44
Elizabeth Arnold,Chester Hanveyrbitrary any longer, while set up by the plasma dispersion (see Chap.3). Then, the concept of the nonzero energy flux through an infinitely distant surface can only work in case of truly nonabsorbing matter, which is strictly speaking not the case for real media including astrophysical plasmas.作者: eardrum 時間: 2025-3-28 22:05
Dynamo Mechanism of Large-Scale Magnetic Field Generation,ution depends critically on the distribution of the magnetic energy over spatial and temporal scales, not on the magnetic field energy density alone. Therefore, study of the magnetic field over all available scales is needed to deeply understand astrophysical phenomena.作者: upstart 時間: 2025-3-29 01:12 作者: Factual 時間: 2025-3-29 04:58 作者: falsehood 時間: 2025-3-29 11:09
